NASA

4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Daniel Velásquez, ingeniero de operaciones de la NASA, a la izquierda, revisa el sistema Mobile Vertipad Sensor Package como parte del proyecto de pruebas Air Mobility Pathways en el Centro de Investigación de Vuelo Armstrong de la NASA en Edwards, California, el 17 de octubre de 2023.NASA/Steve Freeman Read this story in English here. Nacido y criado en Perú, Daniel Velásquez se estableció en los Estados Unidos cuando tenía 10 años. Aunque esa decisión fue una gran transición para su familia, también le creó muchas oportunidades. Ahora Velásquez es ingeniero de operaciones del proyecto Pathfinders de Movilidad Aérea de la NASA en el Centro de Investigación de Vuelo Armstrong de la NASA en Edwards, California. Velásquez desarrolla ensayos de vuelo para aeronaves eléctricas de despegue y aterrizaje vertical (eVTOL, por sus siglas en inglés), poniendo a prueba específicamente su rendimiento durante varias fases del vuelo, como el rodaje, el despegue, el crucero, la aproximación y el aterrizaje. Se interesó en el centro Armstrong de la NASA debido a su legado en el avance de la investigación de vuelo y a su contribución al programa del Transbordador Espacial. “Formar parte de un centro con una historia tan rica en el apoyo a las misiones espaciales y la aeronáutica avanzada fue una motivación importante para mí,” dice Velásquez. “Uno de los mayores hitos de mi carrera ha sido la oportunidad de conocer (virtualmente) y colaborar con un astronauta en un posible proyecto de la NASA.” Daniel Velásquez se encuentra junto al letrero de la entrada principal del Centro de Investigación de Vuelo Armstrong de la NASA en Edwards, California.Daniel Velásquez Velásquez está increíblemente orgulloso de su origen latino por su rica cultura, su fuerte sentido de comunidad y la conexión a sus padres. “Mis padres son mi mayor inspiración. Sacrificaron mucho para asegurarse de que mis hermanos y yo pudiéramos tener éxito, dejando atrás la comodidad de su hogar y su familia en Perú para darnos mejores oportunidades,” dice Velásquez. “Su esfuerzo y dedicación me motivan cada día. Todo lo que hago es para honrar sus sacrificios y demostrarles que sus esfuerzos no fueron un vano. Todo mi éxito se lo debo a ellos.” Velásquez comenzó su carrera en la NASA en 2021 como un pasante en el Programa de Pasantías Pathways mientras estudiaba ingeniería aeroespacial en la Universidad Rutgers en New Brunswick, New Jersey. A través de ese programa, el aprendió sobre un software de modelado eVTOL que se llama Diseño y Análisis de Aeronaves de Alas Giratorias de la NASA y creó una guía de ayuda que otros ingenieros de la NASA pudieran consultar cuando trabajaban con el software. Al mismo tiempo, también es un sargento primero de la Reserva del Ejército de EE. UU. y es responsable de supervisar el entrenamiento y el desarrollo de los soldados subalternos durante las reuniones mensuales. Planifica, crea y presenta clases para que los soldados se mantengan al día y refinen sus habilidades, a la vez que supervisa los ejercicios prácticos, las revisiones posteriores de acción y recopila lecciones aprendidas durante los entrenamientos. Daniel Velásquez se graduó en la Universidad Rutgers en mayo de 2023 mientras trabajaba como pasante en la NASA. Aquí está posando con el horizonte de Nueva York al fondo.Daniel Velásquez “Este trabajo es diferente de lo que hago día a día en la NASA, pero me ha ayudado a convertirme en una persona más franca,” dice. “Ser capaz de conversar con una variedad de personas y poder hacerlo bien es una habilidad que adquirí y refiné mientras servía a mi país.” Velásquez explica que nunca imaginó trabajar para la NASA, ya que era algo que sólo había visto en las películas y en la televisión, pero está muy orgulloso de trabajar para la agencia después de todo el trabajo duro y los sacrificios que lo llevaron hasta aquí. “Estoy increíblemente orgulloso de trabajar cada día con algunas de las personas más motivadas y dedicadas en la industria.” Share Details Last Updated Oct 16, 2024 EditorDede DiniusContactElena Aguirreelena.aguirre@nasa.govLocationArmstrong Flight Research Center Related TermsArmstrong Flight Research CenterAir Mobility Pathfinders projectHispanic Heritage MonthNASA en españolPeople of ArmstrongPeople of NASA Explore More 3 min read Sacrifice and Success: NASA Engineer Honors Family Roots Article 23 mins ago 6 min read Christine Knudson Uses Earthly Experience to Study Martian Geology Geologist Christine Knudson works with the Curiosity rover to explore Mars — from about 250… Article 7 hours ago 3 min read NASA Spotlight: Felipe Valdez, an Inspiring Engineer Article 2 days ago Keep Exploring Discover More Topics From NASA Armstrong Flight Research Center Hispanic Heritage Month NASA en español Explora el universo y descubre tu planeta natal con nosotros, en tu idioma. Armstrong People View the full article

24 Min Read The Marshall Star for October 16, 2024 Liftoff! NASA’s Europa Clipper Sails Toward Ocean Moon of Jupiter NASA’s Europa Clipper has embarked on its long voyage to Jupiter, where it will investigate Europa, a moon with an enormous subsurface ocean that may have conditions to support life. The spacecraft launched at 11:06 a.m. CDT on Oct. 14 aboard a SpaceX Falcon Heavy rocket from Launch Pad 39A at NASA’s Kennedy Space Center. A SpaceX Falcon Heavy rocket carrying NASA’s Europa Clipper spacecraft lifts off from Launch Complex 39A at the agency’s Kennedy Space Center at 11:06 a.m. CDT on Oct. 14. After launch, the spacecraft plans to fly by Mars in February 2025, then back by Earth in December 2026, using the gravity of each planet to increase its momentum. With help of these “gravity assists,” Europa Clipper will achieve the velocity needed to reach Jupiter in April 2030.Credit: NASA/Kim Shiflett The largest spacecraft NASA ever built for a mission headed to another planet, Europa Clipper also is the first NASA mission dedicated to studying an ocean world beyond Earth. The spacecraft will travel 1.8 billion miles on a trajectory that will leverage the power of gravity assists, first to Mars in four months and then back to Earth for another gravity assist flyby in 2026. After it begins orbiting Jupiter in April 2030, the spacecraft will fly past Europa 49 times. “Congratulations to our Europa Clipper team for beginning the first journey to an ocean world beyond Earth,” said NASA Administrator Bill Nelson. “NASA leads the world in exploration and discovery, and the Europa Clipper mission is no different. By exploring the unknown, Europa Clipper will help us better understand whether there is the potential for life not just within our solar system, but among the billions of moons and planets beyond our Sun.” Approximately five minutes after liftoff, the rocket’s second stage fired up and the payload fairing, or the rocket’s nose cone, opened to reveal Europa Clipper. About an hour after launch, the spacecraft separated from the rocket. Ground controllers received a signal soon after, and two-way communication was established at 12:13 p.m. with NASA’s Deep Space Network facility in Canberra, Australia. Mission teams celebrated as initial telemetry reports showed Europa Clipper is in good health and operating as expected. “We could not be more excited for the incredible and unprecedented science NASA’s Europa Clipper mission will deliver in the generations to come,” said Nicky Fox, associate administrator, Science Mission Directorate at NASA Headquarters. “Everything in NASA science is interconnected, and Europa Clipper’s scientific discoveries will build upon the legacy that our other missions exploring Jupiter – including Juno, Galileo, and Voyager – created in our search for habitable worlds beyond our home planet.” The main goal of the mission is to determine whether Europa has conditions that could support life. Europa is about the size of our own Moon, but its interior is different. Information from NASA’s Galileo mission in the 1990s showed strong evidence that under Europa’s ice lies an enormous, salty ocean with more water than all of Earth’s oceans combined. Scientists also have found evidence that Europa may host organic compounds and energy sources under its surface. If the mission determines Europa is habitable, it may mean there are more habitable worlds in our solar system and beyond than imagined. “We’re ecstatic to send Europa Clipper on its way to explore a potentially habitable ocean world, thanks to our colleagues and partners who’ve worked so hard to get us to this day,” said Laurie Leshin, director, NASA’s Jet Propulsion Laboratory (JPL). “Europa Clipper will undoubtedly deliver mind-blowing science. While always bittersweet to send something we’ve labored over for years off on its long journey, we know this remarkable team and spacecraft will expand our knowledge of our solar system and inspire future exploration.” In 2031, the spacecraft will begin conducting its science-dedicated flybys of Europa. Coming as close as 16 miles to the surface, Europa Clipper is equipped with nine science instruments and a gravity experiment, including an ice-penetrating radar, cameras, and a thermal instrument to look for areas of warmer ice and any recent eruptions of water. As the most sophisticated suite of science instruments NASA has ever sent to Jupiter, they will work in concert to learn more about the moon’s icy shell, thin atmosphere, and deep interior. To power those instruments in the faint sunlight that reaches Jupiter, Europa Clipper also carries the largest solar arrays NASA has ever used for an interplanetary mission. With arrays extended, the spacecraft spans 100 feet from end to end. With propellant loaded, it weighs about 13,000 pounds. In all, more than 4,000 people have contributed to Europa Clipper mission since it was formally approved in 2015. “As Europa Clipper embarks on its journey, I’ll be thinking about the countless hours of dedication, innovation, and teamwork that made this moment possible,” said Jordan Evans, project manager, JPL. “This launch isn’t just the next chapter in our exploration of the solar system; it’s a leap toward uncovering the mysteries of another ocean world, driven by our shared curiosity and continued search to answer the question, ‘are we alone?’” Europa Clipper’s three main science objectives are to determine the thickness of the moon’s icy shell and its interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission’s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet. Managed by Caltech in Pasadena, California, JPL leads the development of the Europa Clipper mission in partnership with the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, for NASA’s Science Mission Directorate. The main spacecraft body was designed by APL in collaboration with JPL and NASA’s Goddard Space Flight Center, Marshall Space Flight Center, and Langley Research Center. The Planetary Missions Program Office at Marshall executes program management of the Europa Clipper mission. NASA’s Launch Services Program, based at NASA Kennedy, managed the launch service for the Europa Clipper spacecraft. › Back to Top Staying the Course: 30 Years of NASA’s Student Rover Challenge Get ready, get set, and let’s go take a look back at NASA’s 2024 Human Exploration Rover Challenge! Watch as talented student teams from around the world gather in Huntsville for the 30th annual competition to push the boundaries of innovation and engineering. These student teams piloted their human-powered rovers over simulated lunar and Martian terrain for a chance at winning an award during this Artemis student challenge. From jaw-dropping triumphs to unexpected setbacks, this year’s competition was a thrilling ride from start to finish. Buckle up and enjoy the ride as you witness the future of space exploration unfold! The challenge is managed by NASA’s Southeast Regional Office of STEM Engagement at the agency’s Marshall Space Flight Center. Learn more about the challenge. › Back to Top Black Hole Destroys Star, Goes After Another, NASA Missions Find NASA’s Chandra X-ray Observatory and other telescopes have identified a supermassive black hole that has torn apart one star and is now using that stellar wreckage to pummel another star or smaller black hole, as described in our latest press release. This research helps connect two cosmic mysteries and provides information about the environment around some of the bigger types of black holes. This artist’s illustration shows a disk of material (red, orange, and yellow) that was created after a supermassive black hole (depicted on the right) tore apart a star through intense tidal forces.X-ray: NASA/CXC/Queen’s Univ. Belfast/M. Nicholl et al.; Optical/IR: PanSTARRS, NSF/Legacy Survey/SDSS; Illustration: Soheb Mandhai / The Astro Phoenix; Image Processing: NASA/CXC/SAO/N. Wolk This artist’s illustration shows a disk of material (red, orange, and yellow) that was created after a supermassive black hole (depicted on the right) tore apart a star through intense tidal forces. Over the course of a few years, this disk expanded outward until it intersected with another object – either a star or a small black hole – that is also in orbit around the giant black hole. Each time this object crashes into the disk, it sends out a burst of X-rays detected by Chandra. The inset shows Chandra data (purple) and an optical image of the source from Pan-STARRS (red, green, and blue). In 2019, an optical telescope in California noticed a burst of light that astronomers later categorized as a “tidal disruption event”, or TDE. These are cases where black holes tear stars apart if they get too close through their powerful tidal forces. Astronomers gave this TDE the name of AT2019qiz. Meanwhile, scientists were also tracking instances of another type of cosmic phenomena occasionally observed across the Universe. These were brief and regular bursts of X-rays that were near supermassive black holes. Astronomers named these events “quasi-periodic eruptions,” or QPEs. This latest study gives scientists evidence that TDEs and QPEs are likely connected. The researchers think that QPEs arise when an object smashes into the disk left behind after the TDE. While there may be other explanations, the authors of the study propose this is the source of at least some QPEs. In 2023, astronomers used both Chandra and Hubble to simultaneously study the debris left behind after the tidal disruption had ended. The Chandra data were obtained during three different observations, each separated by about 4 to 5 hours. The total exposure of about 14 hours of Chandra time revealed only a weak signal in the first and last chunk, but a very strong signal in the middle observation. From there, the researchers used NASA’s Neutron Star Interior Composition Explorer (NICER) to look frequently at AT2019qiz for repeated X-ray bursts. The NICER data showed that AT2019qiz erupts roughly every 48 hours. Observations from NASA’s Neil Gehrels Swift Observatory and India’s AstroSat telescope cemented the finding. The ultraviolet data from Hubble, obtained at the same time as the Chandra observations, allowed the scientists to determine the size of the disk around the supermassive black hole. They found that the disk had become large enough that if any object was orbiting the black hole and took about a week or less to complete an orbit, it would collide with the disk and cause eruptions. This result has implications for searching for more quasi-periodic eruptions associated with tidal disruptions. Finding more of these would allow astronomers to measure the prevalence and distances of objects in close orbits around supermassive black holes. Some of these may be excellent targets for the planned future gravitational wave observatories. The paper describing these results appears in the Oct. 9 issue of the journal Nature. The first author of the paper is Matt Nicholl of Queen’s University Belfast in Ireland. NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts. › Back to Top Revealing the Hidden Universe with Full-shell X-ray Optics at Marshall The study of X-ray emission from astronomical objects reveals secrets about the universe at the largest and smallest spatial scales. Celestial X-rays are produced by black holes consuming nearby stars, emitted by the million-degree gas that traces the structure between galaxies, and can be used to predict whether stars may be able to host planets hospitable to life. X-ray observations have shown that most of the visible matter in the universe exists as hot gas between galaxies and have conclusively demonstrated that the presence of “dark matter” is needed to explain galaxy cluster dynamics, that dark matter dominates the mass of galaxy clusters, and that it governs the expansion of the cosmos. A composite X-ray/Optical/Infrared image of the Crab Pulsar. The X-ray image from the Chandra X-ray Observatory (blue and white), reveals exquisite details in the central ring structures and gas flowing out of the polar jets. Optical light from the Hubble Space Telescope (purple) shows foreground and background stars as pinpoints of light. Infrared light from the Spitzer Space Telescope (pink) traces cooler gas in the nebula. Finally, magnetic field direction derived from X-ray polarization observed by the Imaging X-ray Polarimetry Explorer is shown as orange lines.Magnetic field lines: NASA/Bucciantini et al; X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Infrared: NASA-JPL-Caltech X-ray observations also enable us to probe mysteries of the universe on the smallest scales. X-ray observations of compact objects such as white dwarfs, neutron stars, and black holes allow us to use the universe as a physics laboratory to study conditions that are orders of magnitude more extreme in terms of density, pressure, temperature, and magnetic field strength than anything that can be produced on Earth. In this astrophysical laboratory, researchers expect to reveal new physics at the subatomic scale by conducting investigations such as probing the neutron star equation of state and testing quantum electrodynamics with observations of neutron star atmospheres. At NASA’s Marshall Space Flight Center, a team of scientists and engineers is building, testing, and flying innovative optics that bring the universe’s X-ray mysteries into sharper focus. Unlike optical telescopes that create images by reflecting or refracting light at near-90-degree angles (normal incidence), focusing X-ray optics must be designed to reflect light at very small angles (grazing incidence). At normal incidence, X-rays are either absorbed by the surface of a mirror or penetrate it entirely. However, at grazing angles of incidence, X-rays reflect very efficiently due to an effect called total external reflection. In grazing incidence, X-rays reflect off the surface of a mirror like rocks skipping on the surface of a pond. A classic design for astronomical grazing incidence optics is the Wolter-I prescription, which consists of two reflecting surfaces, a parabola and hyperbola (see figure below). This optical prescription is revolved around the optical axis to produce a full-shell mirror (i.e., the mirror spans the full circumference) that resembles a gently tapered cone. To increase the light collecting area, multiple mirror shells with incrementally larger diameters and a common focus are fabricated and nested concentrically to comprise a mirror module assembly (MMA). Focusing optics are critical to studying the X-ray universe because, in contrast to other optical systems like collimators or coded masks, they produce high signal-to-noise images with low background noise. Two key metrics that characterize the performance of X-ray optics are angular resolution, which is the ability of an optical system to discriminate between closely spaced objects, and effective area, which is the light collecting area of the telescope, typically quoted in units of cm2. Angular resolution is typically measured as the half-power diameter (HPD) of a focused spot in units of arcseconds. The HPD encircles half of the incident photons in a focused spot and measures the sharpness of the final image; a smaller number is better. Schematic of a full-shell Wolter-I X-ray optic mirror module assembly with five concentrically nested mirror shells. Parallel rays of light enter from the left, reflect twice off the reflective inside surface of the shell (first off the parabolic segment and then off the hyperbolic segment), and converge at the focal plane.NASA Marshall has been building and flying lightweight, full-shell, focusing X-ray optics for over three decades, always meeting or exceeding angular resolution and effective area requirements. Marshall utilizes an electroformed nickel replication technique to make these thin full-shell X-ray optics from nickel alloy. X-ray optics development at Marshall began in the early 1990s with the fabrication of optics to support NASA’s Advanced X-ray Astrophysics Facility (AXAF-S) and then continued via the Constellation-X technology development programs. In 2001, Marshall launched a balloon payload that included two modules each with three mirrors, which produced the first focused hard X-ray images of an astrophysical source by imaging Cygnus X-1, GRS 1915, and the Crab Nebula. This initial effort resulted in several follow-up missions over the next 12 years and became known as the High Energy Replicated Optics (HERO) balloon program. In 2012, the first of four sounding rocket flights of the Focusing Optics X-ray Solar Imager (FOXSI) flew with Marshall optics onboard, producing the first focused images of the Sun at energies greater than 5 keV. In 2019 the Astronomical Roentgen Telescope X-ray Concentrator (ART-XC) instrument on the Spectr-Roentgen-Gamma Mission launched with seven Marshall-fabricated X-ray MMAs, each containing 28 mirror shells. ART-XC is currently mapping the sky in the 4-30 keV hard X-ray energy range, studying exotic objects like neutron stars in our own galaxy as well as active galactic nuclei, which are spread across the visible universe. In 2021, the Imaging X-ray Polarimetry Explorer (IXPE), flew and is now performing extraordinary science with a Marshall-led team using three, 24-shell MMAs that were fabricated and calibrated in-house. Most recently, in 2024, the fourth FOXSI sounding rocket campaign launched with a high-resolution Marshall MMA. The optics achieved 9.5 arcsecond HPD angular resolution during pre-flight test with an expected 7 arcsecond HPD in gravity-free flight, making this the highest angular resolution flight observation made with a nickel-replicated X-ray optic. Currently Marshall is fabricating an MMA for the Rocket Experiment Demonstration of a Soft X-ray (REDSoX) polarimeter, a sounding rocket mission that will fly a novel soft X-ray polarimeter instrument to observe active galactic nuclei. The REDSoX MMA optic will be 444 mm in diameter, which will make it the largest MMA ever produced by MSFC and the second largest replicated nickel X-ray optic in the world. The ultimate performance of an X-ray optic is determined by errors in the shape, position, and roughness of the optical surface. To push the performance of X-ray optics toward even higher angular resolution and achieve more ambitious science goals, Marshall is currently engaged in a fundamental research and development effort to improve all aspects of full-shell optics fabrication. Scientists Wayne Baumgartner, left, crouched, and Nick Thomas, left, standing, calibrate an IXPE MMA in the Marshall 100 m Beamline. Scientist Stephen Bongiorno, right, applies epoxy to an IXPE shell during MMA assembly.NASA Given that these optics are made with the electroformed nickel replication technique, the fabrication process begins with creation of a replication master, called the mandrel, which is a negative of the desired optical surface. First, the mandrel is figured and polished to specification, then a thin layer of nickel alloy is electroformed onto the mandrel surface. Next, the nickel alloy layer is removed to produce a replicated optical shell, and finally the thin shell is attached to a stiff holding structure for use. Each step in this process imparts some degree of error into the final replicated shell. Research and development efforts at Marshall are currently concentrating on reducing distortion induced during the electroforming metal deposition and release steps. Electroforming-induced distortion is caused by material stress built into the electroformed material as it deposits onto the mandrel. Decreasing release-induced distortion is a matter of reducing adhesion strength between the shell and mandrel, increasing strength of the shell material to prevent yielding, and reducing point defects in the release layer. Additionally, verifying the performance of these advanced optics requires world-class test facilities. The basic premise of testing an optic designed for X-ray astrophysics is to place a small, bright X-ray source far away from the optic. If the angular size of the source, as viewed from the optic, is smaller than the angular resolution of the optic, the source is effectively simulating X-ray starlight. Due to the absorption of X-rays by air, the entire test facility light path must be placed inside a vacuum chamber. At the center, a group of scientists and engineers operate the Marshall 100-meter X-ray beamline, a world-class end-to-end test facility for flight and laboratory X-ray optics, instruments, and telescopes. As per the name, it consists of a 100-meter-long vacuum tube with an 8-meter-long, 3-meter-diameter instrument chamber and a variety of X-ray sources ranging from 0.25 – 114 keV. Across the street sits the X-Ray and Cryogenic Facility (XRCF), a 527-meter-long beamline with an 18-meter-long, 6-meter-diameter instrument chamber. These facilities are available for the scientific community to use and highlight the comprehensive optics development and test capability that Marshall is known for. Within the X-ray astrophysics community there exist a variety of angular resolution and effective area needs for focusing optics. Given its storied history in X-ray optics, Marshall is uniquely poised to fulfill requirements for large or small, medium- or high-angular-resolution X-ray optics. To help guide technology development, the astrophysics community convenes once per decade to produce a decadal survey. The need for high-angular-resolution and high-throughput X-ray optics is strongly endorsed by the National Academies of Sciences, Engineering, and Medicine report, Pathways to Discovery in Astronomy and Astrophysics for the 2020s.In pursuit of this goal, Marshall is continuing to advance the state of the art in full-shell optics. This work will enable the extraordinary mysteries of the X-ray universe to be revealed. › Back to Top Hubble, New Horizons Team Up for a Simultaneous Look at Uranus NASA’s Hubble Space Telescope and New Horizons spacecraft simultaneously set their sights on Uranus recently, allowing scientists to make a direct comparison of the planet from two very different viewpoints. The results inform future plans to study like types of planets around other stars. NASA’s Hubble Space Telescope (left) and NASA’s New Horizon’s spacecraft (right) image the planet Uranus.NASA, ESA, STScI, Samantha Hasler (MIT), Amy Simon (NASA-GSFC), New Horizons Planetary Science Theme Team; Image Processing: Joseph DePasquale (STScI), Joseph Olmsted (STScI) Astronomers used Uranus as a proxy for similar planets beyond our solar system, known as exoplanets, comparing high-resolution images from Hubble to the more-distant view from New Horizons. This combined perspective will help scientists learn more about what to expect while imaging planets around other stars with future telescopes. “While we expected Uranus to appear differently in each filter of the observations, we found that Uranus was actually dimmer than predicted in the New Horizons data taken from a different viewpoint,” said lead author Samantha Hasler of the Massachusetts Institute of Technology in Cambridge and New Horizons science team collaborator. Direct imaging of exoplanets is a key technique for learning about their potential habitability, and offers new clues to the origin and formation of our own solar system. Astronomers use both direct imaging and spectroscopy to collect light from the observed planet and compare its brightness at different wavelengths. However, imaging exoplanets is a notoriously difficult process because they’re so far away. Their images are mere pinpoints and so are not as detailed as the close-up views that we have of worlds orbiting our Sun. Researchers can also only directly image exoplanets at “partial phases,” when only a portion of the planet is illuminated by their star as seen from Earth. Uranus was an ideal target as a test for understanding future distant observations of exoplanets by other telescopes for a few reasons. First, many known exoplanets are also gas giants similar in nature. Also, at the time of the observations, New Horizons was on the far side of Uranus, 6.5 billion miles away, allowing its twilight crescent to be studied – something that cannot be done from Earth. At that distance, the New Horizons view of the planet was just several pixels in its color camera, called the Multispectral Visible Imaging Camera. On the other hand, Hubble, with its high resolution, and in its low-Earth orbit 1.7 billion miles away from Uranus, was able to see atmospheric features such as clouds and storms on the day side of the gaseous world. “Uranus appears as just a small dot on the New Horizons observations, similar to the dots seen of directly imaged exoplanets from observatories like Webb or ground-based observatories,” Hasler said. “Hubble provides context for what the atmosphere is doing when it was observed with New Horizons.” The gas giant planets in our solar system have dynamic and variable atmospheres with changing cloud cover. How common is this among exoplanets? By knowing the details of what the clouds on Uranus looked like from Hubble, researchers can verify what is interpreted from the New Horizons data. In the case of Uranus, both Hubble and New Horizons saw that the brightness did not vary as the planet rotated, which indicates that the cloud features were not changing with the planet’s rotation. In this image, two three-dimensional shapes, top, of Uranus are compared to the actual views of the planet from NASA’s Hubble Space Telescope, bottom left, and NASA’s New Horizon’s spacecraft, bottom right. Comparing high-resolution images from Hubble to the smaller view from New Horizons offers a combined perspective that will help researchers learn more about what to expect while imaging planets around other stars with future observatories. NASA, ESA, STScI, Samantha Hasler (MIT), Amy Simon (NASA-GSFC), New Horizons Planetary Science Theme Team; Image Processing: Joseph DePasquale (STScI), Joseph Olmsted (STScI) However, the importance of the detection by New Horizons has to do with how the planet reflects light at a different phase than what Hubble, or other observatories on or near Earth, can see. New Horizons showed that exoplanets may be dimmer than predicted at partial and high phase angles, and that the atmosphere reflects light differently at partial phase. NASA has two major upcoming observatories in the works to advance studies of exoplanet atmospheres and potential habitability. “These landmark New Horizons studies of Uranus from a vantage point unobservable by any other means add to the mission’s treasure trove of new scientific knowledge, and have, like many other datasets obtained in the mission, yielded surprising new insights into the worlds of our solar system,” added New Horizons principal investigator Alan Stern of the Southwest Research Institute. NASA’s upcoming Nancy Grace Roman Space Telescope, set to launch by 2027, will use a coronagraph to block out a star’s light to directly see gas giant exoplanets. NASA’s Habitable Worlds Observatory, in an early planning phase, will be the first telescope designed specifically to search for atmospheric biosignatures on Earth-sized, rocky planets orbiting other stars. “Studying how known benchmarks like Uranus appear in distant imaging can help us have more robust expectations when preparing for these future missions,” concluded Hasler. “And that will be critical to our success.” Launched in January 2006, New Horizons made the historic flyby of Pluto and its moons in July 2015, before giving humankind its first close-up look at one of these planetary building block and Kuiper Belt object, Arrokoth, in January 2019. New Horizons is now in its second extended mission, studying distant Kuiper Belt objects, characterizing the outer heliosphere of the Sun, and making important astrophysical observations from its unmatched vantage point in distant regions of the solar system. The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA. The Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, built and operates the New Horizons spacecraft and manages the mission for NASA’s Science Mission Directorate. Southwest Research Institute, based in San Antonio and Boulder, Colorado, directs the mission via Principal Investigator Alan Stern and leads the science team, payload operations and encounter science planning. New Horizons is part of NASA’s New Frontiers program, managed by NASA’s Marshall Space Flight Center. › Back to Top Crew-8 Awaits Splashdown; Expedition 72 Stays Focused on Science Four International Space Station crew members continue waiting for their departure date as mission managers monitor weather conditions off the coast of Florida. The rest of the Expedition 72 crew stayed focused Oct. 14 on space biology and lab maintenance aboard the orbital outpost. The SpaceX Dragon Freedom spacecraft is pictured through the window of the SpaceX Dragon Endeavour spacecraft with a vivid green and pink aurora below.NASA NASA and SpaceX mission managers are watching unfavorable weather conditions off the Florida coast right now for the splashdown of the SpaceX Crew-8 mission with NASA astronauts Matthew Dominick, Mike Barratt, and Jeanette Epps, and Roscosmos cosmonaut Alexander Grebenkin. The homebound quartet spent Oct. 14 mostly relaxing while also continuing departure preps. Mission teams are currently targeting Dragon Endeavour’s undocking for no earlier than 2:05 a.m. CDT on Oct. 18. The Crew-8 foursome is in the seventh month of their space research mission that began on March 3. The other seven orbital residents will stay aboard the orbital outpost until early 2025. NASA astronaut Don Pettit is scheduled to return to Earth first in February with Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner aboard the Soyuz MS-26 crew ship. Next, station Commander Suni Williams and flight engineer Butch Wilmore are targeted to return home aboard SpaceX Dragon Freedom with SpaceX Crew-9 Commander Nick Hague, all three NASA astronauts, and Roscosmos cosmonaut Aleksandr Gorbunov. Williams had a light duty day Oct. 14 disassembling life support gear before working out for a cardio fitness study. Wilmore installed a new oxygen recharge tank and began transferring oxygen into tanks located in the Quest airlock. Hague collected his blood and saliva samples for incubation and cold stowage to learn how microgravity affects cellular immunity. Pettit also had a light duty day servicing biology hardware including the Cell Biology Experiment Facility, a research incubator with an artificial gravity generator, and the BioLab, which supports observations of microbes, cells, tissue cultures and more. The Huntsville Operations Support Center (HOSC) at NASA’s Marshall Space Flight Center provides engineering and mission operations support for the space station, the CCP, and Artemis missions, as well as science and technology demonstration missions. The Payload Operations Integration Center within HOSC operates, plans, and coordinates the science experiments onboard the space station 365 days a year, 24 hours a day. The first flight of Sierra Space’s Dream Chaser to the space station is now scheduled for no earlier than May 2025 to allow for completion of spacecraft testing. Dream Chaser, which will launch atop a ULA (United Launch Alliance) Vulcan rocket and later glide to a runway landing at NASA’s Kennedy Space Center, will carry cargo to the orbiting laboratory and stay on board for approximately 45 days on its first mission. Learn more about station activities by following the space station blog. › Back to Top View the full article

The Progress Pride flag is seen flying at the Mary W. Jackson NASA Headquarters Building, June 9, 2022, in Washington.Credits: NASA/Joel Kowsky NASA is announcing the relaunch of the NASA Acquisition Innovation Launchpad (NAIL), a framework to drive innovation and modernize acquisition processes across the agency, after piloting the program for a year. NASA spends approximately $21 billion or 85% of its budget on acquiring goods and services. Managed by NASA’s Office of Procurement, the NAIL was established to identify ways to manage risk-taking and encourage innovation through the submission, review, and approval of ideas from anyone who engages in the acquisition process. Since launching last year, the goal of the NAIL has been to build an innovation-focused culture that can produce ideas from team members in the Office of Procurement or across the agency, as well as from industry. “The success of the NAIL inaugural year has laid a strong foundation for the future,” said Karla Smith Jackson, deputy chief acquisition officer and assistant administrator for the Office of Procurement. Over the past year, the NAIL has achieved numerous milestones, allowing NASA to approach various procurement challenges and implement diverse solutions. Key accomplishments include improving procurement processes and technological automations and developing an industry feedback forum. The program update will leverage industry’s feedback to continue fostering innovative solutions and optimize the agency’s procurement efforts. As NASA’s Office of Procurement embarks on fiscal year 2025, the NAIL relaunch will use information from the program’s pilot year to focus on the following priorities: Providing additional engagement opportunities for the agency’s network of innovators Enhancing the framework to improve internal outcomes for the agency Promoting procurement success stories Investing in talent and technology “We are incredibly proud of the program’s achievements and are even more excited about the opportunities ahead with the relaunch,” said Kameke Mitchell, NAIL chair and director for the Procurement Strategic Operations Division. “We encourage everyone to get involved and make fiscal year 2025 a standout year for innovation.” In addition to programmatic updates, NAIL’s program manager, Brittney Chappell, will lead new engagements and framework enhancements moving forward. “I am thrilled to step into this role and lead the program, using everything our team has learned from the last year,” said Chappell. “Together with internal and external stakeholders, we will turn bold ideas into impactful solutions that drive real change.” To collaborate or share innovative ideas, reach out to the NAIL Procurement team at hq-op-nail@mail.nasa.gov. For more information about the NAIL framework, visit: https://www.nasa.gov/procurement-nail-framework Share Details Last Updated Oct 16, 2024 LocationNASA Headquarters Related TermsNASA HeadquartersDoing Business with NASA View the full article

4 Min Read NASA to Embrace Commercial Sector, Fly Out Legacy Relay Fleet An artist's concept of commercial and NASA space relays. Credits: NASA/Morgan Johnson NASA is one step closer on its transition to using commercially owned and operated satellite communications services to provide future near-Earth space missions with increased service coverage, availability, and accelerated science and data delivery.     As of Friday, Nov. 8, the agency’s legacy TDRS (Tracking and Data Relay Satellite) system, as part of the Near Space Network, will support only existing missions while new missions will be supported by future commercial services.    “There have been tremendous advancements in commercial innovation since NASA launched its first TDRS satellite more than 40 years ago,” said Kevin Coggins, deputy associate administrator of NASA’s SCaN (Space Communications and Navigation) program. “TDRS will continue to provide critical support for at least the next decade, but now is the time to embrace commercial services that could enhance science objectives, expand experimentation, and ultimately provide greater opportunities for discovery.”    TDRS will continue to provide critical support for at least the next decade, but now is the time to embrace commercial services." Kevin Coggins Deputy Associate Administrator for NASA’s SCaN Just as NASA has adopted commercial crew, commercial landers, and commercial transport services, the Near Space Network, managed by NASA’s SCaN, will leverage private industry’s vast investment in the Earth-based satellite communications market, which includes communications on airplanes, ships, satellite dish television, and more. Now, industry is developing a new space-based market for these services, where NASA plans to become one of many customers, bolstering the domestic space industry.    NASA’s Communications Services Project is working with industry through funded Space Act Agreements to develop and demonstrate commercial satellite communications services that meet the agency’s mission needs, and the needs of other potential users.    In 2022, NASA provided $278.5 million in funding to six domestic partners so they could develop and demonstrate space relay communication capabilities.  Inmarsat Government Inc. Kuiper Government Solutions (KGS) LLC SES Government Solutions Space Exploration Technologies (SpaceX) Telesat U.S. Services LLC Viasat Incorporated Read More About the CSP Partners An artist’s concept of commercial relay satellites. NASA/Morgan Johnson A successful space-based commercial service demonstration would encompass end-to-end testing with a user spacecraft for one or more of the following use cases: launch support, launch and early operations phase, low and high data rate routine missions, terrestrial support, and contingency services. Once a demonstration has been completed, it is expected that the commercial company would be able to offer their services to government and commercial users.    NASA also is formulating non-reimbursable Space Act Agreements with members of industry to exchange capability information as a means of growing the domestic satellite communications market. The Communications Services Project currently is partnered with Kepler Communications US Inc. through a non-reimbursable Space Act Agreement.    As the agency and the aerospace community expand their exploration efforts and increase mission complexity, the ability to communicate science, tracking, and telemetry data to and from space quickly and securely will become more critical than ever before. The goal is to validate and deliver space-based commercial communications services to the Near Space Network by 2031, to support future NASA missions.   NASA’s Tracking and Data Relay System  While TDRS will not be accepting new missions, it won’t be retiring immediately. Current TDRS users, like the International Space Station, Hubble Space Telescope, and many other Earth- and universe-observing missions, will still rely on TDRS until the mid-2030s. Each TDRS spacecraft’s retirement will be driven by individual health factors, as the seven active TDRS satellites are expected to decline at variable rates.     To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video An artist's concept of the International Space Station using NASA’s Tracking and Data Relay Satellite (TDRS) fleet to transmit data to Earth. NASA The TDRS fleet began in 1983 and consists of three generations of satellites, launching over the course of 40 years. Each successive generation of TDRS improved upon the previous model, with additional radio frequency band support and increased automation.    The first TDRS was designed for a mission life of 10 years, but lasted 26 years before it was decommissioned in 2009. The last in the third generation – TDRS-13 –was launched Aug. 18, 2017.   The TDRS constellation has been a workhorse for the agency, enabling significant data transfer and discoveries.”   DAve Israel Near Space Network Chief Architect “Each astronaut conversation from the International Space Station, every picture you’ve seen from Hubble Space Telescope, Nobel Prize-winning science data from the COBE satellite, and much more has flowed through TDRS,” said Dave Israel, Near Space Network chief architect. “The TDRS constellation has been a workhorse for the agency, enabling significant data transfer and discoveries.”   NASA’s Tracking and Data Relay Satellite 13 (TDRS-13) atop an Atlas V rocket at NASA’s Kennedy Space Center in Florida before launch. NASA/Tony Gray and Sandra Joseph The Near Space Network and the Communications Services Project are funded by NASA’s SCaN (Space Communications and Navigation) program office at NASA Headquarters in Washington. The network is operated out of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and the Communications Services Project is managed out of NASA’s Glenn Research Center in Cleveland. Share Details Last Updated Oct 16, 2024 EditorGoddard Digital TeamContactKatherine Schauerkatherine.s.schauer@nasa.govMolly KearnsLocationGoddard Space Flight Center Related TermsCommunicating and Navigating with MissionsGlenn Research CenterGoddard Space Flight CenterSpace Communications & Navigation ProgramThe Future of Commercial SpaceTracking and Data Relay Satellite (TDRS) Explore More 4 min read Communications Services Project Article 7 months ago 5 min read Wideband Technology Article 9 months ago 3 min read NASA Seeks Commercial Near Space Network Services NASA is seeking commercial communication and navigation service providers for the Near Space Network. Article 2 years ago View the full article

Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 3 min read Sols 4334-4335: Planning with Popsicles — A Clipper Celebration! This image was taken by Left Navigation Camera aboard NASA’s Mars rover Curiosity on Sol 4329 — Martian day 4,329 of the Mars Science Laboratory mission — on Oct. 10, 2024, at 05:35:08 UTC. NASA/JPL-Caltech Earth planning date: Monday, Oct. 14, 2024 Today was an unusually exciting day during tactical planning on the Curiosity mission because it intersected with a momentous event in space exploration: the launch of Europa Clipper from Kennedy Space Center. Even though the launch window occurred right in the middle of our morning planning meetings, at 9:06 a.m. PDT to be specific, today’s Tactical Uplink Lead and Science Operations Working Group Chair agreed it would be OK for the entire tactical team to take a 15-minute pause to turn on NASA TV and watch the launch together. Down the hall the Perseverance rover tactical team had decided the same, and for a few moments, the two teams paused their planning and watched together in anticipation as the countdown ticked down to T-0. Many of my close friends and co-workers had worked for years — some for decades — to make this mission a reality, and it was amazing to watch the enormous rocket carrying the Clipper spacecraft leap off the pad knowing how hard it was to get to this point. I cannot wait for the mission’s discoveries once it reaches Jupiter’s watery moon Europa! In true JPL tradition, we of course had to commemorate the event with some sweet frozen treats on-lab. Back when Curiosity landed, we had a full fridge of ice cream that was kept stocked for the first 90 sols of the mission. (Eating ice cream cones at 2 in the morning is a core memory of mine from those early days in our mission.) Today, in a clever nod to Europa’s icy surface, we celebrated with some even icier sweets: fruit and coffee popsicles to anyone on-lab. I chose coffee of course; the caffeine was great to help me get through a busy day of planning for Curiosity! On Mars, things with our rover are going well. We completed our mega ~50-meter drive (about 164 feet) over the weekend, which took Curiosity further north along the western side of Gediz Vallis channel. Our plan today is a “touch and go,” which means we’ll do contact science with APXS and MAHLI on a block in front of us named “Dollar Lake,” some remote sensing, including ChemCam LIBS of a target named “Cape Horn” and a couple Mastcam mosaics, followed by a drive to the north. We’ll continue to follow the western side of Gediz Vallis channel as we descend slightly down Mount Sharp, until we reach a location where we are able to head west towards a more easily traversable valley, and then restart our ascent. What a fun day of planning today. Congratulations to everyone involved helping Europa Clipper reach this incredible milestone, and go Clipper go! Written by Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory Share Details Last Updated Oct 16, 2024 Related Terms Blogs Explore More 4 min read Sols 4331-4333: Today’s Rover ABC – Aurora, Backwards Driving, and Chemistry, with a Side of Images Article 3 days ago 3 min read Sols 4329-4330: Continuing Downhill Article 5 days ago 3 min read Sols 4327-4328: On the Road Again Article 7 days ago Keep Exploring Discover More Topics From NASA Mars Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited… All Mars Resources Explore this collection of Mars images, videos, resources, PDFs, and toolkits. Discover valuable content designed to inform, educate, and inspire,… Rover Basics Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a… Mars Exploration: Science Goals The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four… View the full article

Hubble Space Telescope Home NASA’s Hubble Sees a… Hubble Space Telescope Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts E-books Lithographs Fact Sheets Glossary Posters Hubble on the NASA App More Online Activities 3 Min Read NASA’s Hubble Sees a Stellar Volcano NASA’s Hubble Space Telescope captures a spectacular view the star R Aquarii. Credits: NASA, ESA, Matthias Stute , Margarita Karovska , Davide De Martin (ESA/Hubble), Mahdi Zamani (ESA/Hubble) NASA’s Hubble Space Telescope has provided a dramatic and colorful close-up look at one of the most rambunctious stars in our galaxy, weaving a huge spiral pattern among the stars. Located approximately 700 light-years away, a binary star system called R Aquarii undergoes violent eruptions that blast out huge filaments of glowing gas. The twisted stellar outflows make the region look like a lawn sprinkler gone berserk. This dramatically demonstrates how the universe redistributes the products of nuclear energy that form deep inside stars and jet back into space. R Aquarii belongs to a class of double stars called symbiotic stars. The primary star is an aging red giant and its companion is a compact burned-out star known as a white dwarf. The red giant primary star is classified as a Mira variable that is over 400 times larger than our Sun. The bloated monster star pulsates, changes temperature, and varies in brightness by a factor of 750 times over a roughly 390-day period. At its peak the star is blinding at nearly 5,000 times our Sun’s brightness. This NASA Hubble Space Telescope image features the binary star system R Aquarii. NASA, ESA, Matthias Stute , Margarita Karovska , Davide De Martin (ESA/Hubble), Mahdi Zamani (ESA/Hubble) When the white dwarf star swings closest to the red giant along its 44-year orbital period, it gravitationally siphons off hydrogen gas. This material accumulates on the dwarf star’s surface until it undergoes spontaneous nuclear fusion, making that surface explode like a gigantic hydrogen bomb. After the outburst, the fueling cycle begins again. This outburst ejects geyser-like filaments shooting out from the core, forming weird loops and trails as the plasma emerges in streamers. The plasma is twisted by the force of the explosion and channeled upwards and outwards by strong magnetic fields. The outflow appears to bend back on itself into a spiral pattern. The plasma is shooting into space over 1 million miles per hour – fast enough to travel from Earth to the Moon in 15 minutes! The filaments are glowing in visible light because they are energized by blistering radiation from the stellar duo. Hubble first observed the star in 1990. R Aquarii was resolved into two very bright stars separated by about 1.6 billion miles. The ESA/Hubble team now has made a unique timelapse of R Aquarii’s dynamic behavior, from observations spanning from 2014 to 2023. Across the five images, the rapid and dramatic evolution of the binary star and its surrounding nebula can be seen. The binary star dims and brightens due to strong pulsations in the red giant star. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video This video features five frames spanning from 2014 to 2023 of R Aquarii. These frames show the brightness of the central binary changing over time due to strong pulsations in the red giant star. The central structures spiral outward due to their interaction with material previously ejected by the binary. This timelapse highlights the value of Hubble’s high resolution optical observations in the changing universe, known as time-domain astronomy. NASA, ESA, Matthias Stute , Margarita Karovska , Davide De Martin , Mahdi Zamani , N. Bartmann (ESA/Hubble) The scale of the event is extraordinary even in astronomical terms. Space-blasted material can be traced out to at least 248 billion miles from the stars, or 24 times our solar system’s diameter. Images like these and more from Hubble are expected to revolutionize our ideas about such unique stellar “volcanoes” as R Aquarii. The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA. Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, MD claire.andreoli@nasa.gov Ray Villard Space Telescope Science Institute, Baltimore, MD Bethany Downer ESA/Hubble Share Details Last Updated Oct 16, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms Astrophysics Astrophysics Division Binary Stars Goddard Space Flight Center Hubble Space Telescope Science Mission Directorate Stars The Universe Keep Exploring Discover More Topics From Hubble Hubble Space Telescope Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe. The Death Throes of Stars From colliding neutron stars to exploding supernovae, Hubble reveals new details of some of the mysteries surrounding the deaths of… Exploring the Birth of Stars Hubble Focus: The Lives of Stars NASA’s Hubble Space Telescope team has released a new e-book called “Hubble Focus: The Lives of Stars.” This e-book highlights… View the full article

Name: Christine Knudson Title: Geologist Formal Job Classification: Research Assistant Organization: Planetary Environments Laboratory, Science Directorate (Code 699) Christine Knudson is a geologist at NASA’s Goddard Space Flight Center in Greenbelt, Md. She began graduate school in August 2012, the same month that NASA’s Curiosity rover landed on Mars. “It is very exciting to be part of the rover team and to be involved in an active Mars mission,” she says. “On days when we’re downlinking science data and I’m on shift, I am one of the first people to see data from an experiment done on Mars!”Courtesy of Christine Knudsen What do you do and what is most interesting about your role here at Goddard? I am a geologist doing both laboratory and field work, primarily focusing on Mars analog research. I work on the Curiosity rover as part of the Sample Analysis at Mars (SAM) instrument team. Why did you become a geologist? As a child, I always loved being outside and I was really interested in all things related to the Earth. In college, I figured out that I wanted to be a geologist after taking an introduction to geology course. I wanted to learn more about the Earth and its interior, specifically volcanism. What is your educational background? In 2012, I received a B.S. in geology and environmental geoscience from Northern Illinois University. In August 2012, the same month that Curiosity landed on Mars, I started graduate school and in December 2014, I received a M.S. in geology from the same university. I focused on igneous geochemistry, investigating the pre-eruptive water contents of a Guatemalan volcano. Why did you come to Goddard? I came to Goddard in February 2015 to perform laboratory analyses of Mars analog materials, rock and mineral samples, from Earth, that the Curiosity rover and spectral orbiters have also identified on Mars. It is very exciting to be part of the rover team and to be involved in an active Mars mission. What is a highlight of your work as a laboratory geologist doing Mars analog research? Using laboratory analyses to interpret data we are getting back from Curiosity is incredibly exciting! I perform evolved gas analysis to replicate the analyses that the SAM instrument does on the rover. Curiosity scoops sand or drills into the rocks at stops along its drive through Gale Crater on Mars, then dumps the material into a small cup within the SAM instrument inside the rover. The rock is heated in a small oven to about 900 C [about 1650 F], and the instrument captures the gases that are released from the sample as it is heated. SAM uses a mass spectrometer to identify the different gases, and that tells us about the minerals that make up the rock. We do the same analyses on rocks and minerals in our lab to compare to the SAM analyses. The other instruments on Curiosity also aid in the identification of the rocks, minerals, and elements present in this location on the Martian surface. I also serve as a payload downlink lead for the SAM instrument. I check on the science and engineering data after we perform an experiment on Mars. On the days I’m on shift, I check to make sure that our science experiments finish without any problems, and that the instrument is “healthy,” so that the rover can continue driving and begin the science that is planned for the next sol. On days when we’re downlinking science data and I’m on shift, I am one of the first people to see data from an experiment done on Mars! What is some of the coolest field work you have done? I have done Mars analog field work in New Mexico, Hawaii, and Iceland. The field work in Hawaii is exciting because one of our field sites was inside a lava tube on Mauna Loa. We expect that there are lava tubes on Mars, and we know that the interior of the tubes would likely be better shielded from solar radiation, which might allow for the preservation of organic markers. Scientifically, we’re interested in characterizing the rocks and minerals inside lava tubes to understand how the interior differs from the surface over time and to investigate differences in elemental availability as an accessible resource for potential life. Learning about these processes on Earth helps us understand what might be possible on Mars too. “The field work in Hawaii is exciting because one of our field sites was inside a lava tube on Mauna Loa,” Knudson says. “We expect that there are lava tubes on Mars, and we know that the interior of the tubes would likely be better shielded from solar radiation, which might allow for the preservation of organic markers.”Courtesy of Christine Knudson I use handheld versions of laboratory instruments, some of which were miniaturized and made to fit on the Curiosity rover, to take in situ geochemical measurements — to learn what elements are present in the rocks and in what quantities. We also collect samples to analyze in the laboratory. I also love Hawaii because the island is volcanically active. Hawaii Volcano National Park is incredible! A couple years ago, I was able to see the lava lake from an ongoing eruption within the crater of Kīlauea volcano. The best time to see the lava lake is at night because the glowing lava is visible from multiple park overlooks. As a Mars geologist, what most fascinates you about the Curiosity rover? When Curiosity landed, it was the largest rover NASA had ever sent to Mars: It’s about the size of a small SUV, so landing it safely was quite the feat! Curiosity also has some of the first science instruments ever made to operate on another planet, and we’ve learned SO much from those analyses. Curiosity and the other rovers are sort of like robotic geologists exploring Mars. Working with the Curiosity rover allows scientists to do geology on Mars — from about 250 million miles away! Earth analogs help us to understand what we are seeing on Mars, since that “field site” is so incredibly far away and inaccessible to humans at this time. What do you do for fun? I spend most of my free time with my husband and two small children. We enjoy family hikes, gardening, and both my boys love being outside as much as I do. I also enjoy yoga, and I crochet: I make hats, blankets, and I’m starting a sweater soon. What is your “six-word memoir”? A six-word memoir describes something in just six words. Nature-lover. Mom. Geologist. Cat-enthusiast. Curious. Snack-fiend. By Elizabeth M. Jarrell NASA’s Goddard Space Flight Center, Greenbelt, Md. Conversations With Goddard is a collection of Q&A profiles highlighting the breadth and depth of NASA’s Goddard Space Flight Center’s talented and diverse workforce. The Conversations have been published twice a month on average since May 2011. Read past editions on Goddard’s “Our People” webpage. Share Details Last Updated Oct 16, 2024 EditorRob GarnerContactRob Garnerrob.garner@nasa.govLocationGoddard Space Flight Center Related TermsThe Solar SystemCuriosity (Rover)MarsMars Science Laboratory (MSL)People of GoddardPeople of NASA Explore More 7 min read Michael Thorpe Studies Sediment from Source to Sink Sedimentary and planetary geologist Michael Thorpe finds the stories rocks have to tell, those on… Article 9 months ago 5 min read Casey Honniball: Finding Her Space in Lunar Science Article 7 months ago 3 min read Malika Graham: Helping NASA Bring Mars Back to Earth Article 3 years ago View the full article

7 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Juvenile black, white, and yellow-striped Bluehead wrasse fish dart in and out of a dead colony of pillar coral (Dendrogyra cylindrus), now covered in various algae, in the waters of Playa Melones, Puerto Rico. NASA Ames/Milan Loiacono Coral reefs cover only 1% of the ocean floor, but support an estimated 25% of all marine life in the ocean, earning them the moniker ‘rainforest of the sea.’ They also play a critical role for coastal communities; preventing coastal erosion, protecting coastlines from hurricane damage, and generating $36 billion in annual income worldwide. We asked Juan Torres-Pérez, a research scientist and coral reef expert at NASA Ames Research Center, about the science behind coral reefs, and the role they play in both marine ecosystems and human communities. What is the difference between a reef, coral, and a coral reef? Reef Reefs are ridge-like structures, either natural or artificial. “A reef by definition is a structure that provides some relief above the ocean floor,” Torres-Pérez said. “It could be something man-made: you can pile a bunch of car tires, and then they get colonized by different organisms. Or it could be natural: a small hill on top of the ocean floor in which the primary framework is a rock.” Corals Corals are animals from the phylum Cnidaria, typically found along tropical coastlines. They comprise hundreds to thousands of living organisms called polyps, each only a few millimeters in diameter. Each polyp has its own body and a mouth with stinging tentacles to capture food such as plankton and small fish. The polyps grow together until they form a colony, and it is this colony that we recognize as a coral. There are two types of coral: hard corals and soft corals. Hard corals, also known as stony corals or more formally as Scleractinians, secrete calcium carbonate to form a hard skeleton; it is this type of coral that form a coral reefs. Soft corals, also known as Alcyonacea, are fleshy and bendable, often resembling trees or fans. Juvenile black, white, and yellow-striped Bluehead wrasse fish dart in and out of a reef, composed of yellow fire coral (Millepora complanate, back left), branching finger coral (Porites furcate, front left), and various species of sea rods and sea fans. This coral reef sits in the waters of Playa Melones, Puerto Rico. NASA Ames/Milan Loiacono The colorful appearance of corals comes from the microscopic algae that live inside coral cells, called zooxanthellae. These algae perform photosynthesis, bringing vital food and nutrients to the corals. “The majority of the products from photosynthesis, about 80 to 90%, pass on to the coral, and then the coral uses those for its own metabolism,” said Torres-Pérez. “This is why corals are usually found in shallow waters: because these organisms need the sunlight to photosynthesize.” Coral Reefs A coral reef is a term used to describe the collective structure of hard corals that help shape a coral reef ecosystem. “A coral reef is a reef whose main structure is made by living organisms, in this case corals,” said Torres-Pérez. “A coral reef will always be a reef, but not all reefs are coral reefs.” The largest coral reef in the world is Australia’s Great Barrier Reef, which is over 1,000 miles long and covers around 133,000 square miles. Why are coral reefs important? Healthy coral reefs play a crucial role in providing coastal protection, habitats for marine life, and even key ingredients for potential new medicines. “Coral reef ecosystems provide habitat for thousands of species, from unicellular organisms like bacteria or some phytoplankton communities, to large organisms like sharks, groupers or snappers, and reptiles like sea turtles,” Torres-Pérez said. Corals act as a protective barrier during big storm events such as typhoons or hurricanes and have proven to be 97% effective in preventing damage to the natural and built environment. As coral reefs have been damaged in recent decades, coastal flooding and erosion have increased, causing significant damage to coastal communities. Many communities depend on coral reefs as a resource to sustain their livelihoods. “These are critical ecosystems, not only in terms of the whole biodiversity of the planet but because they also provide sustenance for millions of people, especially in island nations,” Torres-Pérez said. Coral reefs also support fisheries (fish caught for commercial, recreational, or subsistence purposes), recreational activities, and educational purposes. Scientists have been exploring coral as a new ingredient source for some medicines. They have discovered that a chemical from coral can be extracted to create antibiotics that are effective against bacteria resistant to other types of antibiotics. These ingredients are replicated in a lab, eliminating the need to continuously harvest and harm corals. What are some current threats to coral reefs? According to a 2020 report produced by the Global Coral Reef Monitoring Network (GCRMN), 14% of the world’s coral reefs have been lost since 2009. In the wake of the 2023-2024 global coral bleaching event, that number is expected to increase. Map showing sea surface temperatures in March, 2022 near the Great Barrier Reef in Australia. The darker red colors indicate an in increase in sea surface temperature. Coral bleaching is caused by increasing ocean temperatures. As water temperatures rise, it causes corals to expel their zooxanthellae, leaving behind a bone-white shell and depriving the coral of its main food source. “Eventually what happens is that the coral is too weak to compete with other organisms, like filamentous algae, that can overgrow the coral and eventually kill the whole colony,” said Torres-Pérez. Other threats to coral reefs come from human activity, such as pollution or physical damage. “Increases in sedimentation from poor land management get deposited into the reefs,” said Torres-Pérez, citing urban stormwater runoff and deforestation as two examples of sedimentation. Coral sedimentation is the deposition and accumulation of sediments, like fine sands or mud, on a reef. This clouds the waters, blocking critical sunlight and reducing the ability of zooxanthellae to photosynthesize. Another human-caused threat to corals is eutrophication, the unnatural increase of nutrients in the water. “Eutrophication provides grounds for the development of filamentous algae, which grows much faster than corals,” said Torres-Pérez. Some of these excess nutrients in the water come from sewage released into coastal waters or runoff of agricultural fertilizers into the ocean. The algae feed off the excess nutrients and grow into massive blooms, which suppress the growth of corals. Cyanobacteria overgrowth crowds the water of Playa Melones, Puerto Rico, likely caused by an on-land source of pollution leeching excess nutrients into the water. In the background float students and instructors from the NASA OCEANOS internship.NASA Ames/Milan Loiacono Moreover, Torres-Pérez pointed out that human-caused physical damage to reefs can result from mechanical damage, such as ship anchors being thrown onto corals. Some fishing techniques, like deep water trawling (dragging fishing nets along the sea floor), can also damage reefs by pulling and tearing corals away from their bases. On a more individual scale, coral damage can also result from being stepped on by humans, or accumulated trash left behind by beach-goers. What is being done to protect coral, at NASA and beyond? Many coral reefs in the world are still unclassified, unexplored, or yet to be discovered. NASA’s NeMO-Net hopes to change that. Torres-Pérez, who is a Co-Investigator for NeMO-Net, described how the citizen science project functions like an interactive mobile video game, allowing anyone to identify corals. “Users can characterize different components of a coral reef based on 2D [and 3D] images of a coral reef,” said Torres-Pérez. “which goes into a machine learning component.” The information from these classifications is fed into a scientific model and helps NASA both classify and assess the health of coral reefs around the world. To learn more about NeMO-Net and how to get involved, check out their website. In 2022, Torres-Pérez founded OCEANOS (Ocean Community Engagement and Awareness using NASA Earth Observations and Science for Hispanic/Latino Students), a program aimed at bringing oceanography and STEM opportunities to the next generation of Hispanic/Latino students in Puerto Rico. During the program, students build and test their own low-cost optical sensors, test data in a phytoplankton lab, replant coral reefs, and create storymap presentations of their work. “We want students to feel confident and capable to pursue STEM careers,” Torres-Pérez said, “and we want them to become agents of change in their community to share the importance of preserving the ocean.” OCEANOS PI Juan Torres-Pérez delivers the opening address of the 2023 final presentations to a crowded room at the EcoExploratorio: el Museo de Ciencias de Puerto Rico.NASA Ames/Milan Loiacono Outside of NASA, Torres-Pérez is an active member of the U.S. Coral Reef Task Force (USCRTF); an interagency body established in 1998 from Executive Order 13089: Coral Reef Protection that aims to preserve, protect, and restore coral reef ecosystems. Resources to Learn More To learn more about coral reefs and how they are monitored, Torres-Pérez recommends checking out resources from the National Oceanic and Atmospheric Administration (NOAA), which has a section on their website dedicated to corals. One notable coral reef resource from NOAA is their Coral Reef Watch website, which monitors sea surface temperatures on global and local scales. The website serves government and non-governmental agencies with their data products, which are used to monitor and predict climate impacts on coral reefs worldwide. Written by: Katera Lee, NASA Ames Research Center Share Details Last Updated Oct 15, 2024 Related TermsGeneralEarth ScienceEarth Science Division Explore More 2 min read $1.5 Million Awarded at Watts on the Moon Finals Article 5 hours ago 1 min read NASA Glenn Connects with Morehead State University Article 5 hours ago 15 min read OpenET: Balancing Water Supply and Demand in the West Article 1 day ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

Researchers verified that 3D micro-computed tomography scans can map the orientation of plant roots in space and used the method to demonstrate that carrots grown in actual and simulated microgravity both had random root orientation. These findings suggest that simulated microgravity offers a reliable and more affordable tool for studying plant adaptation to spaceflight. MULTI-TROP evaluated the role of gravity and other factors on plant growth. Plant roots grow downward in response to gravity on Earth, but in random directions in microgravity, which is a challenge for developing plant growth facilities for space. Results from this investigation could help address this challenge, advancing efforts to grow plants for food and other uses on future space missions as well as improving plant cultivation on Earth. Preflight image of the BIOKON facility used to grow carrots for MULTI-TROP. Kayser Italia For climate model simulations, researchers developed four parameters of electrical discharges from thunderclouds that produce visual emissions known as Blue LUminous Events or BLUEs. BLUEs are thought to affect regional atmospheric chemistry and climate. The parameters reported by this study could inform models that help test the global and regional effects of thunderstorm corona discharges, including how their geographic distribution and global occurrence rate will change as the atmosphere warms. ASIM, an investigation from ESA (European Space Agency), studies high-altitude lightning in thunderstorms and the role it plays in Earth’s atmosphere and climate. Scientists need to understand processes occurring in Earth’s upper atmosphere to determine how lightning is connected to Earth’s climate and weather so they can develop better atmospheric models to guide weather and climate predictions. Lightning in a thunderstorm off the coast of Africa as seen from the International Space Station. NASA/Matthew Dominick A technique to detect sounds generated by the inner ear could be used as a non-invasive tool for monitoring changes in fluid pressure in the head during spaceflight. Increased fluid pressure in the head that occurs in microgravity can cause visual impairment and may also affect the middle and inner ear. Insight into fluid pressure changes could help scientists develop ways to protect astronauts from these effects. The ESA and ASI investigation Acoustic Diagnostics monitored hearing function in astronauts on long-term missions using otoacoustic emissions (sounds generated by the inner ear in response to specific tones). Researchers compared these measurements before and during flight to indirectly detect changes in fluid pressure in the head. Different body position and fit of the ear probes affected results of the test and the authors note that these issues need to be addressed. NASA astronaut Drew Morgan participates in a hearing test for the Acoustic Diagnostics investigation. ESA (European Space Agency)/Luca ParmitanoView the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Dr. Rickey Shyne is responsible for leading a staff of approximately 1,100 engineers and scientists.Credit: NASA Dr. Rickey J. Shyne, director of Research and Engineering at NASA’s Glenn Research Center in Cleveland, has been named one of Crain’s Cleveland Business’ 2024 Notable Black Leaders. Shyne is responsible for leading a staff of approximately 1,100 engineers and scientists, and managing research and development in propulsion, communications, power, and materials and structures for extreme environments in support of the agency’s missions. He is on the board of Southwest General Health Center and a former board member of Cleveland Engineering Society. Crain’s Notable Black Leaders represent all industries and communities. From magnates to mentors, they are working to enrich their companies, communities and city. Nominees must serve in a senior leadership role at their company or organization; have at least five years of experience in their field; and demonstrate significant accomplishments within their industry, professional organizations, and civic and community groups. They must live and work in the Northeast Ohio area. Shyne is featured in the Crain’s September 30 issue, online and in print. Return to Newsletter Explore More 2 min read Ohio State Marching Band Performs Tribute to NASA Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University Article 15 mins ago 1 min read Visitors Explore NASA at Ingenuity Fest Article 15 mins ago View the full article

2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Orbital Mining Corporation took second place in NASA’s Watts on the Moon Challenge. Left to right: Rob Button, deputy chief of NASA Glenn’s Power Division; three members of the team; Mary Wadel, NASA director of Technology Integration and Partnerships; and NASA astronaut Stephen Bowen. Credit: NASA/Sara Lowthian-Hanna Great Lakes Science Center, home of the visitor center for NASA’s Glenn Research Center in Cleveland, hosted the final phase of NASA’s Watts on the Moon Challenge on Sept. 20. NASA astronaut Stephen Bowen attended to help acknowledge the top winners. NASA awarded a total of $1.5 million to two U.S. teams for their novel technology solutions addressing energy distribution, management, and storage as part of the challenge. The innovations from this challenge aim to support NASA’s Artemis missions, which will establish a long-term human presence on the Moon. This two-phase competition challenged U.S. innovators to develop breakthrough technologies that could enable long-duration Moon missions to advance the nation’s lunar exploration goals. The winning teams are: First Prize ($1 million): Team H.E.L.P.S. (High Efficiency Long-Range Power Solution) from University of California, Santa Barbara , won the grand prize for their hardware solution, which featured the lowest mass and highest efficiency of all competitors. Second prize ($500,000): Orbital Mining Corporation, a space technology startup in Golden, Colorado, earned the second prize for its hardware solution that also successfully completed the 48-hour test with high performance. Four teams were invited to refine their hardware and deliver full system prototypes in the  final stage of the competition, and three finalist teams completed their technology solutions for demonstration and assessment at NASA Glenn. The University of California (UC), Santa Barbara, took first place in NASA’s Watts on the Moon Challenge. Left to right: Mary Wadel, NASA director of Technology Integration and Partnerships; Rob Button, deputy chief of NASA Glenn’s Power Division; UC Santa Barbara team members; and NASA astronaut Stephen Bowen. Credit: NASA/Sara Lowthian-Hanna NASA Glenn’s Mary Wadel, director of Technology Integration and Partnerships, recognized the work involved to bring this challenge to its conclusion. Rob Button, deputy chief of Glenn’s Power Division and his team of experts, formulated and executed the challenge and oversaw testing. The technologies were the first power transmission and energy storage prototypes to be tested by NASA in a vacuum chamber mimicking the freezing temperature and absence of pressure found at the permanently shadowed regions of the Lunar South Pole. The Watts on the Moon Challenge is a NASA Centennial Challenge led by NASA Glenn. As the agency’s lead center for power systems technologies, NASA Glenn has been involved in the Watts on the Moon Challenge from its inception. Return to Newsletter Explore More 1 min read NASA Glenn Connects with Morehead State University Article 15 mins ago 15 min read OpenET: Balancing Water Supply and Demand in the West Article 20 hours ago 3 min read NASA Activates Resources to Help Assess Impacts from Hurricane Milton Article 3 days ago View the full article

2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) The Ohio State University Marching Band pays tribute to NASA with a NASA worm logo formation. Credit: NASA/Brian Newbacher The Ohio State University (OSU) teamed up with NASA’s Glenn Research Center in Cleveland for a multi-faceted tribute to NASA on Sept 21. During a home football game against Marshall University, OSU’s Marching Band recognized the agency with a NASA-themed halftime show, in-game salute, and tribute to Glenn and two alums who play significant roles in NASA’s spaceflight operations. NASA Glenn Center Director Dr. Jimmy Kenyon and NASA employees and Ohio State alums Jeff and Molly Radigan are recognized by more than 100,000 fans in Ohio Stadium. Credit: NASA/Brian Newbacher The event kicked off in the morning during the Skull Session (pep rally) at St. John Arena on OSU’s campus. Public Address Announcer Wes Clark talked with Center Director Dr. Jimmy Kenyon, who shared information about Glenn and thanked OSU for the honor. During a special spotlight, Kenyon and OSU alums who now work at NASA’s Kennedy Space Center – Jeff Radigan, a NASA flight director, and Molly Radigan, deputy chief of Space Flight Systems – came onto the field to be recognized. The Ohio State University Marching Band pays tribute to NASA while in formation of an astronaut on the Moon. Credit: NASA/Brian Newbacher At halftime, a special astronaut video from the International Space Station introduced the NASA-themed show. The band then blasted off with its space-themed performance that included several songs — from “Fly Me to the Moon” to “Starman.” The talented band members marched in formations that included an astronaut and spaceship blasting off, garnering excitement for NASA and cheers from the audience. Back to Newsletter Explore More 1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University Article 15 mins ago 1 min read Visitors Explore NASA at Ingenuity Fest Article 15 mins ago View the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Dr. Benjamin Malphrus, executive director of the Space Science Center at Morehead State University, left, listens as NASA Glenn Center Director Dr. Jimmy Kenyon talks about NASA’s exploration efforts.Credit: Morehead State University NASA’s Glenn Research Center Director Dr. Jimmy Kenyon met with students and faculty at Morehead State University (MSU) in Kentucky on Sept. 19. Kenyon provided the keynote address on the topic of NASA’s exploration efforts and regional economic impact during the ASTRA-Con (Appalachian Space Technology & Research Advancement Conference). He also moderated a panel, which included Blue Origin’s Orbital Reef Lead Dr. Randy Lillard, MSU’s Dr. Pamela Clark (formerly of NASA’s Jet Propulsion Laboratory and Goddard Space Flight Center), and Glenn European Service Module Manager Logan Larson. Morehead State University (MSU)’s Dr. Benjamin Malphrus, right, shows NASA Glenn Center Director Dr. Jimmy Kenyon and others on tour the anechoic (echo-free) chamber used in support of MSU’s 21-meter Deep Space Network. Credit: Morehead State University Dr. Benjamin Malphrus, executive director of the Space Science Center at MSU, provided Kenyon, along with House Appropriations Subcommittee Chairman Hal Rogers’ staff and members of industry, with a tour of the space center and its capabilities. Kenyon learned about MSU’s space systems engineering program where students gain hands-on experience designing, constructing, and testing satellites before they launch into space. Members of NASA Glenn’s Technology Transfer Office also staffed an informative exhibit during the conference. Return to Newsletter Explore More 1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader Article 14 mins ago 2 min read $1.5 Million Awarded at Watts on the Moon Finals Article 14 mins ago 2 min read Ohio State Marching Band Performs Tribute to NASA Article 14 mins ago View the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA’s Jamie Richey shares opportunities for the public to engage with NASA during the Cleveland Ingenuity Fest 2024: Take Flight. Credit: NASA/Debbie Welch NASA’s Glenn Research Center participated in the Cleveland Ingenuity Fest 2024: Take Flight on Sept. 27-29. Ingenuity Fest, held at the 300,000-square-foot Hamilton Collaborative, features artwork, musicians, dancers, poets, and performances of all types. It also highlights maker and innovator exhibits, fine art, and more. NASA Glenn’s staff shared opportunities for the community to engage directly with NASA through prize challenges, crowdsourcing, and citizen science. Through these platforms, the public can make an impact on NASA’s mission by providing innovative solutions to address the agency’s needs. NASA Graphics and Visualization Lab’s Nikhita Kalluri shows visitors NASA’s advanced visualization technology during the Cleveland Ingenuity Fest 2024: Take Flight. Credit: NASA/Debbie Welch Guests learned about the agency’s mission to send the first woman and first person of color to the Moon through the Artemis program, experienced virtual reality visualizations showing NASA’s work with radioisotope power systems, and learned about the effects of drag on an aircraft using a mini wind tunnel. The Graphics and Visualization Lab showcased NASA’s advanced visualization technology to provide innovative solutions for the agency and the scientific community. Return to Newsletter Explore More 1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader Article 14 mins ago 2 min read Ohio State Marching Band Performs Tribute to NASA Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University Article 15 mins ago View the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) The Harvest Moon refers to the nearest full Moon to the autumnal equinox. The Moon appeared full for about three days last month from the evening of Monday, Sept. 16, through Thursday morning, Sept. 19. The brightest Moon was on Sept. 17. NASA’s Glenn Research Center photographers captured images of this supermoon as it shone across Cleveland. Here’s how they described it: “Complex.” Sara Lowthian-Hanna captured this composite image of the Moon above a Guardians of Traffic statue near downtown Cleveland. The Sept. 17 Harvest Moon had a lot going on: it was full, a supermoon, and experienced a partial lunar eclipse (when the Earth’s shadow falls upon the Moon’s surface). Credit: NASA/Sara Lowthian-Hanna “Shy.” Quentin Schwinn patiently waited for the Moon to peek out from behind clouds above the hangar at NASA’s Glenn Research Center. He took this shot just as a plane whizzed in front of the face of the Moon. Credit: NASA/Quentin Schwinn “Epic.” Jef Janis captured this shot of the Moon above the colorfully illuminated Rock & Roll Hall of Fame in downtown Cleveland. Credit: NASA/Jef Janis “Dramatic.” Jordan Salkin took this up-close image of wispy aircraft contrails crossing the face of the Moon. Credit: NASA/Jordan Salkin Return to Newsletter Explore More 1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader Article 14 mins ago 2 min read Ohio State Marching Band Performs Tribute to NASA Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University Article 15 mins ago View the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Artemis II crew members (left to right) Reid Wiseman, Christina Koch, and Jeremy Hansen share information about themselves and their mission during a town hall at NASA’s Glenn Research Center in Cleveland. Credit: NASA/Sara Lowthian-Hanna Three of the four astronauts who will venture around the Moon on Artemis II, the first crewed flight paving the way for future lunar surface missions, visited NASA’s Glenn Research Center in Cleveland, Sept. 10-11. NASA Glenn is an integral part of the development of the Orion spacecraft and a leader in propulsion, power, and communications research. Commander Reid Wiseman  and Mission Specialists  Christina Koch and Jeremy Hansen (Canadian Space Agency) discussed their upcoming mission and hosted a question-and-answer session during town hall events at Lewis Field in Cleveland and NASA’s Neil Armstrong Test Facility in Sandusky, Ohio. Victor Glover, who was unable to attend, is the pilot and fourth crew member. Both events included tours and recognition of employees who have contributed to the success of Artemis missions. Artemis II crew members Reid Wiseman, Christina Koch, and Jeremy Hansen (left to right, wearing blue flight suits) and other NASA personnel look down into the stainless-steel vacuum chamber in the In-Space Propulsion Facility at NASA’s Neil Armstrong Test Facility in Sandusky, Ohio. This is the world’s only facility capable of testing full-scale upper stage launch vehicles and rocket engines under simulated high-altitude conditions.Credit: NASA/Sara Lowthian-Hanna The Artemis II crew will lift off on an approximately 10-day mission from Launch Complex 39B at NASA’s Kennedy Space Center in Florida, blazing beyond Earth’s grasp atop the agency’s mega Moon rocket. The crew will check out Orion’s systems and perform a targeting demonstration test relatively close to Earth before venturing around the Moon.  Back to Newsletter Explore More 1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader Article 14 mins ago 2 min read Ohio State Marching Band Performs Tribute to NASA Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University Article 15 mins ago View the full article

4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Science in Space: October 2024 Cultures around the world celebrate Halloween on Oct 31. In many places, in addition to people wearing costumes and eating candy, this day is associated with spooky decorating using fake blood, skeletons, flies, and spiders, some of them glow-in-the-dark. Crew members on the International Space Station have been known to indulge in a bit of dressing up and candy consumption to mark the day, and the research they conduct year-round occasionally involves these iconic Halloween themes. No tricks, just treats. JAXA astronaut Koichi Wakata and NASA astronauts Frank Rubio, Nicole Mann, and Josh Cassada dressed up for Halloween 2022.NASA A current investigation, Megakaryocytes Flying-One or MeF1, investigates how components of real blood known as megakaryocytes and platelets develop and function during spaceflight. Megakaryocytes are large cells found in bone marrow and platelets are pieces of these cells. Both play important roles in blood clotting and immune response. Results could improve understanding of changes in inflammation, immune responses, and clot formation in spaceflight and on the ground. Creepy crawlies Fake spiders and flies are popular Halloween decorations (and fodder for fun pranks). Several investigations on the space station have used real ones. Fruit Fly Lab-02 used fruit flies, Drosophila melanogaster, to examine the cellular and genetic mechanisms that affect heart health during spaceflight. The flies experienced several effects on cardiac function, including changes in muscle fibers, that could be a fundamental response of heart muscles to microgravity. MVP Fly-01 looked at how spaceflight affects immune function and resulting changes to the nervous system of the same type of flies, along with the value of artificial gravity as a countermeasure. Researchers found that artificial gravity provided some protection to physical changes to the central nervous system from spaceflight. Spiders, Fruit Flies and Directional Plant Growth (CSI-05) compared the weaving characteristics of golden orb-web spiders on the space station and the ground. Under natural conditions, the spiders build asymmetric webs with the hub near the upper edge, where they wait for prey. In microgravity, most but not all webs were quite symmetric, although webs built when the lights were on were more asymmetric and the spiders waited facing away from the lights. This could mean that in the absence of gravity, the spiders orient to the direction of light. A golden-orb weaver and its web on the space station.NASA Bad to the bones Everyone needs healthy bones and skeletons, and not just on Halloween. But spaceflight and aging on Earth can cause loss of bone mass. Space station research has looked at the mechanisms behind this loss as well as countermeasures such as exercise and nutrition. Bisphosphonates as a Countermeasure to Bone Loss examined whether a medication that blocks the breakdown of bone, in conjunction with the routine in-flight exercise program, protected crew members from bone mineral density loss during spaceflight. The research found that it did reduce loss, which in turn reduced the occurrence of kidney stones in crew members. Assessment of the Effect of Space Flight on Bone (TBone) studied how spaceflight affects bone quality using a high-resolution bone scan technique. Researchers found incomplete recovery of bone strength and density in the tibia (a bone in the lower leg), comparable to a decade or more of terrestrial age-related bone loss. The work also highlighted the relationship between length of a mission and bone loss and suggested that pre-flight markers could identify crew members at greatest risk. In a merging of blood and bones, CSA’s Marrow looked at whether microgravity has a negative effect on bone marrow and the blood cells it produces. Decreased production of red blood cells can lead to a condition called space anemia. Findings related to the expression of genes involved in red blood cell formation and those related to bone marrow adipose or fat tissue, which stores energy and plays a role in immune function, could contribute to development of countermeasures. Marrow results also suggested that the destruction of red blood cells (known as hemolysis) is a primary effect of spaceflight and contributes to anemia. Bad news for vampires. ESA astronaut Thomas Pesquet storing Marrow samples in MELFI.NASA It glows in the dark Fluorescence – a cool effect at a ghoulish party – also is a common tool in scientific research, enabling researchers to see physical and genetic changes. The space station has special microscopes for observing glow-in-the-dark samples. For Medaka Osteoclast 2, an investigation from JAXA (Japan Aerospace Exploration Agency), researchers genetically modified translucent Medaka fish with fluorescent proteins to help them observe cellular and genetic changes the fish experience during spaceflight. One analysis revealed a decrease in the mineral density of bones in the throat and provided insights into the mechanisms behind these changes. A translucent Medaka fish with fluorescent proteins showing its bone structure.Philipp Keller, Stelzer Group, EMBL Biorock, an investigation from ESA (European Space Agency), examined how microgravity affects the interaction between rocks and microbes and found little effect on microbial growth. This result suggests that microbial-supported bioproduction and life support systems can perform in reduced gravity such as that on Mars, which would be a perfect place for an epic Halloween celebration. Preflight fluorescence microscopy image of a biofilm for the Biorock experiment.NASA Keep Exploring Discover More Topics From NASA International Space Station Space Station Research and Technology Space Station Research Results Station Benefits for Humanity View the full article

6 min read NASA, NOAA: Sun Reaches Maximum Phase in 11-Year Solar Cycle In a teleconference with reporters on Tuesday, representatives from NASA, the National Oceanic and Atmospheric Administration (NOAA), and the international Solar Cycle Prediction Panel announced that the Sun has reached its solar maximum period, which could continue for the next year. The solar cycle is a natural cycle the Sun goes through as it transitions between low and high magnetic activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South poles swapping places every decade — and the Sun transitions from being calm to an active and stormy state. Visible light images from NASA’s Solar Dynamics Observatory highlight the appearance of the Sun at solar minimum (left, Dec. 2019) versus solar maximum (right, May 2024). During solar minimum, the Sun is often spotless. Sunspots are associated with solar activity and are used to track solar cycle progress. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683. NASA/SDO Images from NASA’s Solar Dynamics Observatory highlight the appearance of the Sun at solar minimum (left, December 2019) versus solar maximum (right, May 2024). These images are in the 171-angstrom wavelength of extreme ultraviolet light, which reveals the active regions on the Sun that are more common during solar maximum. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683. NASA/SDO NASA and NOAA track sunspots to determine and predict the progress of the solar cycle — and ultimately, solar activity. Sunspots are cooler regions on the Sun caused by a concentration of magnetic field lines. Sunspots are the visible component of active regions, areas of intense and complex magnetic fields on the Sun that are the source of solar eruptions. “During solar maximum, the number of sunspots, and therefore, the amount of solar activity, increases,” said Jamie Favors, director, Space Weather Program at NASA Headquarters in Washington. “This increase in activity provides an exciting opportunity to learn about our closest star — but also causes real effects at Earth and throughout our solar system.” The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. Credits: Beth Anthony/NASA Solar activity strongly influences conditions in space known as space weather. This can affect satellites and astronauts in space, as well as communications and navigation systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity has led to increased aurora visibility and impacts on satellites and infrastructure in recent months. During May 2024, a barrage of large solar flares and coronal mass ejections (CMEs) launched clouds of charged particles and magnetic fields toward Earth, creating the strongest geomagnetic storm at Earth in two decades — and possibly among the strongest displays of auroras on record in the past 500 years. May 3–May 9, 2024, NASA’s Solar Dynamics Observatory observed 82 notable solar flares. The flares came mainly from two active regions on the Sun called AR 13663 and AR 13664. This video highlights all flares classified at M5 or higher with nine categorized as X-class solar flares. Credit: NASA “This announcement doesn’t mean that this is the peak of solar activity we’ll see this solar cycle,” said Elsayed Talaat, director of space weather operations at NOAA. “While the Sun has reached the solar maximum period, the month that solar activity peaks on the Sun will not be identified for months or years.” Scientists will not be able to determine the exact peak of this solar maximum period for many months because it’s only identifiable after they’ve tracked a consistent decline in solar activity after that peak. However, scientists have identified that the last two years on the Sun have been part of this active phase of the solar cycle, due to the consistently high number of sunspots during this period. Scientists anticipate that the maximum phase will last another year or so before the Sun enters the declining phase, which leads back to solar minimum. Since 1989, the Solar Cycle Prediction Panel — an international panel of experts sponsored by NASA and NOAA — has worked together to make their prediction for the next solar cycle. Solar cycles have been tracked by astronomers since Galileo first observed sunspots in the 1600s. Each solar cycle is different — some cycles peak for larger and shorter amounts of time, and others have smaller peaks that last longer. Sunspot number over the previous 24 solar cycles. Scientists use sunspots to track solar cycle progress; the dark spots are associated with solar activity, often as the origins for giant explosions — such as solar flares or coronal mass ejections — which can spew light, energy, and solar material out into space. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683. NOAA’s Space Weather Prediction Center “Solar Cycle 25 sunspot activity has slightly exceeded expectations,” said Lisa Upton, co-chair of the Solar Cycle Prediction Panel and lead scientist at Southwest Research Institute in San Antonio, Texas. “However, despite seeing a few large storms, they aren’t larger than what we might expect during the maximum phase of the cycle.” The most powerful flare of the solar cycle so far was an X9.0 on Oct. 3 (X-class denotes the most intense flares, while the number provides more information about its strength). NOAA anticipates additional solar and geomagnetic storms during the current solar maximum period, leading to opportunities to spot auroras over the next several months, as well as potential technology impacts. Additionally, though less frequent, scientists often see fairly significant storms during the declining phase of the solar cycle. The Solar Cycle 25 forecast, as produced by the Solar Cycle 25 Prediction Panel. Sunspot number is an indicator of solar cycle strength — the higher the sunspot number, the stronger the cycle. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683. NOAA’s Space Weather Prediction Center NASA and NOAA are preparing for the future of space weather research and prediction. In December 2024, NASA’s Parker Solar Probe mission will make its closest-ever approach to the Sun, beating its own record of closest human-made object to the Sun. This will be the first of three planned approaches for Parker at this distance, helping researchers to understand space weather right at the source. NASA is launching several missions over the next year that will help us better understand space weather and its impacts across the solar system. Space weather predictions are critical for supporting the spacecraft and astronauts of NASA’s Artemis campaign. Surveying this space environment is a vital part of understanding and mitigating astronaut exposure to space radiation. NASA works as a research arm of the nation’s space weather effort. To see how space weather can affect Earth, please visit NOAA’s Space Weather Prediction Center, the U.S. government’s official source for space weather forecasts, watches, warnings, and alerts. By Abbey Interrante NASA’s Goddard Space Flight Center, Greenbelt, Md. Media Contact: Sarah Frazier, NASA’s Goddard Space Flight Center, Greenbelt, Md. sarah.frazier@nasa.gov About the Author Abbey Interrante Share Details Last Updated Oct 15, 2024 Related Terms Goddard Space Flight Center Heliophysics Heliophysics Division Parker Solar Probe (PSP) Solar Science Sunspots The Sun The Sun & Solar Physics Explore More 3 min read Eclipse Megamovie Coding Competition Article 5 hours ago 2 min read ESA/NASA’s SOHO Spies Bright Comet Making Debut in Evening Sky The Solar and Heliospheric Observatory (SOHO) has captured images of the second-brightest comet to ever pass… Article 4 days ago 2 min read Hubble Spots a Grand Spiral of Starbursts Article 4 days ago Keep Exploring Discover More Topics From NASA Sunspots Solar Storms and Flares Solar storms and flares are eruptions from the Sun that can affect us here on Earth. Sun Parker Solar Probe On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona… View the full article

SpaceX A SpaceX Falcon Heavy rocket carrying NASA’s Europa Clipper spacecraft lifts off from NASA’s Kennedy Space Center in Florida on Monday, Oct. 14, 2024. Europa Clipper is the first mission designed to conduct a detailed study of Jupiter’s moon Europa to determine if it currently has habitable conditions. The spacecraft will travel 1.8 billion miles (2.9 billion km) to reach Jupiter in April 2030. It will orbit Jupiter and conduct 49 close flybys of Europa. Follow Europa Clipper’s journey in NASA’s Eyes on the Solar System app. Image credit: SpaceX View the full article

6 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) A natural color view from Cassini of Saturn with its Titan moon in the foreground in August 2012. Titan’s diameter is 50% larger than Earth’s moon.Credit: NASA NASA’s ambitious Cassini mission to Saturn in the late 1990s was one of the agency’s greatest accomplishments, providing unprecedented revelations about the esoteric outer planet and its moons. The complex undertaking was also a tremendous, yet bittersweet, achievement for the Lewis Research Center (today, NASA’s Glenn Research Center in Cleveland), which oversaw the rockets that propelled Cassini to Saturn. Cassini brought a close to over 35 years of Lewis’ management of NASA’s launch vehicles. Cassini Mission: 5 Things to Know About NASA Lewis’ Last Launch 1. NASA Lewis Launched the Largest and Most Complex Deep-Space Mission to Date In the early 1980s, NASA began planning the first-ever in-depth study of the planet Saturn. The mission would use the Cassini orbiter designed by NASA’s Jet Propulsion Laboratory in Southern California and the European Space Agency’s Huygens lander. It was one of the heaviest and most complex interplanetary spacecraft ever assembled. Cassini’s plutonium power system and intricate flight path further complicated the mission. NASA Lewis was responsible for managing the launches of government missions involving the Centaur upper stage and the Atlas and Titan boosters. Cassini’s 6-ton payload forced Lewis to use the U.S. Air Force’s three-stage Titan IV, the most powerful vehicle available, and pair it with the most advanced version of the Centaur, referred to as G-prime. The Titan IV shroud in the Space Power Facility in October 1990. It was only the second test since the world-class facility had been brought back online after over a decade in standby conditions.Credit: NASA/Quentin Schwinn 2. Lewis Performed Hardware Testing for the Cassini Launch One of NASA Lewis’ primary launch responsibilities was integrating the payload and upper stages with the booster. This involved balancing weight requirements, providing adequate insulation for Centaur’s cryogenic propellants, determining correct firing times for the stages, and ensuring that that the large shroud, which encapsulated both the upper stage and payload, jettisoned cleanly after launch. By the time of Cassini, the center had been testing shrouds (including the Titan III fairing) in simulated space conditions for over 25 years. NASA’s Space Power Facility possesses the world’s largest vacuum chamber and was large enough to accommodate the Titan IV’s 86-foot-tall, 16-foot-diameter fairing. In the fall of 1990, the shroud was installed in the chamber, loaded with weights that simulated the payload, and subjected to atmospheric pressures found at an altitude of 72 miles. The system was successfully separated in less than half a second. Using simulated Cassini and Centaur vehicles, NASA engineers also redesigned a thicker thermal blanket that would protect Cassini’s power system from acoustic vibrations during liftoff. Members of NASA Lewis’ Launch Vehicle Directorate pose with a Centaur model in May 1979 to mark the 50th successful launch of the Atlas/Centaur.Credit: NASA/Martin Brown 3. Lewis Personnel Assisted with the Launch In late August 1997, a group of NASA Lewis engineers traveled to NASA’s Kennedy Space Center in Florida to make final preparations for the Cassini launch, working with Air Force range safety personnel at Patrick Air Force Base to ensure a safe launch under all circumstances. After an aborted launch two days earlier, the vehicle was readied for another attempt in the evening of October 14. Lewis personnel took stations in the Launch Vehicle Data Center inside Hangar AE to monitor the launch vehicle’s temperature, pressure, speed, trajectory, and vibration during the launch. The weather was mild, and the countdown proceeded into the morning hours of October 15 without any major issues. At 4:43 a.m. EDT, Titan’s first stage and the two massive solid rocket motors roared to life, and the vehicle rose into the dark skies over Florida. The Lewis launch team monitored the flight as the vehicle exited Earth’s atmosphere, Titan burned through its stages, and Centaur sent Cassini out of Earth orbit and on its 2-billion-mile journey to Saturn. After a successful spacecraft separation, Lewis’ responsibilities were complete. The launch had gone exceedingly well. This illustration depicts the Cassini orbiter with the Huygens lander descending to the Titan moon (left) and Saturn in the background.Credit: NASA 4. Cassini-Huygens Brought a Close to Decades of Lewis Launch Operations Cassini-Huygens was NASA Lewis’ 119th and final launch, and it brought to a close the center’s decades of launch operations. The center had been responsible for NASA’s upper-stage vehicles since the fall of 1962. The primary stages were the Agena, which had 28 successful launches, and Centaur, which has an even more impressive track record and remains in service today. While Lewis continued to handle vehicle integration and other technical issues for launches of NASA payloads, in the 1980s, NASA began transferring launch responsibilities to commercial entities. In the mid-1990s, NASA underwent a major realignment that consolidated all launch vehicle responsibilities at NASA Kennedy. So it was with mixed emotions that around 20 Lewis employees and retirees gathered at the Cleveland center in the early morning hours of Oct. 15, 1997, to watch the Cassini launch. The group held its cheers for 40 minutes after liftoff until Lewis’ responsibilities concluded for the last time with the safe separation of Cassini from Centaur. “In many ways, this is the end of an era, across the agency and, in particular, here at Lewis,” noted one engineer from the Launch Vehicle and Transportation Office. The Titan IV/Centaur lifts off from Launch Complex 40 at Cape Canaveral on Oct. 15, 1997. NASA Lewis engineers were monitoring the launch from Hangar AE, roughly 3.5 miles to the south. Credit: NASA 5. Cassini Made Groundbreaking Discoveries That Inform Today’s NASA Missions Cassini’s seven-year voyage to Saturn included flybys of Venus (twice), Earth, and Jupiter so that the planets’ gravitational forces could accelerate the spacecraft. Cassini entered Saturn’s orbit in June 2004 and began relaying data and nearly half a million images back to Earth. Huygens separated from the spacecraft and descended to the surface of the Saturn’s largest moon, Titan, in January 2005. It was the first time a vehicle ever landed on a celestial body in the outer solar system. Cassini went on to make plunges into the planet’s upper atmosphere and through Saturn’s rings. Scientific information on the mysterious planet, its moons, and rings led to the publication of nearly 4,000 technical papers. After over 13 years and nearly 300 orbits, on Sept. 15, 2017, NASA intentionally sent Cassini plummeting into the atmosphere where it burned up, ending its remarkable mission. NASA engineers used their experiences from the Cassini mission to help design the Europa Clipper, which is intended to perform flybys of Jupiter’s moon Europa. Europa Clipper launched on Oct. 14. Keep Exploring Read the “Sending Cassini to Saturn” Series from NASA Glenn Visit NASA’s Cassini-Huygens Website Visit the European Space Agency’s Cassini-Huygens Website Watch NASA Coverage of the Cassini Launch See NASA Glenn’s Historic Centaur Rocket Display Explore More 24 min read NASA Celebrates Hispanic Heritage Month 2024 Article 4 days ago 3 min read Pioneering NASA Astronaut Health Tech Thwarts Heart Failure Article 4 days ago 8 min read Kathryn Sullivan: The First American Woman to Walk in Space Article 5 days ago View the full article

5 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) This mosaic from ESA’s Euclid space telescope contains 260 observations in visible and infrared light. It covers 132 square degrees, or more than 500 times the area of the full Moon, and is 208 gigapixels. This is 1% of the wide survey that Euclid will capture during its six-year mission.ESA/Euclid/Euclid Consortium/NASA, CEA Paris-Saclay, image processing by J.-C. Cuillandre, E. Bertin, G. Anselmi. CC BY-SA 3.0 IGO This section of the Euclid mosaic is zoomed in 36 times, revealing the core of galaxy cluster Abell 3381, 470 million light-years from Earth. The image, made using both visible and infrared light, shows galaxies of different shapes and sizes, including elliptical, spiral, and dwarf galaxies.ESA/Euclid/Euclid Consortium/NASA, CEA Paris-Saclay, image processing by J.-C. Cuillandre, E. Bertin, G. Anselmi. CC BY-SA 3.0 IGO This image shows an area of the Euclid mosaic zoomed in 150 times. The combination of visible and infrared light reveals galaxies that are interacting with each other in cluster Abell 3381, 470 million light-years away from Earth. ESA/Euclid/Euclid Consortium/NASA, CEA Paris-Saclay, image processing by J.-C. Cuillandre, E. Bertin, G. Anselmi. CC BY-SA 3.0 IGO The location and actual size of the newly released Euclid mosaic is highlighted in yellow on a map of the entire sky captured by ESA’s Planck mission and a star map from ESA’s Gaia mission. ESA/Euclid/Euclid Consortium/NASA; ESA/Gaia/DPAC; ESA and the Planck Collaboration. CC BY-SA 3.0 IGO With contributions from NASA, the mission will map a third of the sky in order to study a cosmic mystery called dark energy. ESA (the European Space Agency) has released a new, 208-gigapixel mosaic of images taken by Euclid, a mission with NASA contributions that launched in 2023 to study why the universe is expanding at an accelerating rate. Astronomers use the term “dark energy” in reference to the unknown cause of this accelerated expansion. The new images were released at the International Astronautical Congress in Milan on Oct. 15. The mosaic contains 260 observations in visible and infrared light made between March 25 and April 8 of this year. In just two weeks, Euclid covered 132 square degrees of the southern sky — more than 500 times the area of the sky covered by a full Moon. The mosaic accounts for 1% of the wide survey Euclid will conduct over six years. During this survey, the telescope observes the shapes, distances, and motions of billions of galaxies out to a distance of more than 10 billion light-years. By doing this, it will create the largest 3D cosmic map ever made. https://www.youtube.com/watch?v=86ZCsUfgLRQ Dive into a snippet of the great cosmic atlas being produced by the ESA Euclid mission. This video zooms in on a 208-gigapixel mosaic containing about 14 million galaxies and covering a portion of the southern sky more than 500 times the area of the full Moon as seen from Earth. Credit: ESA/Euclid/Euclid Consortium/NASA, CEA Paris-Saclay, image processing by J.-C. Cuillandre, E. Bertin, G. Anselmi; ESA/Gaia/DPAC; ESA/Planck Collaboration This first piece of the map already contains around 100 million stars and galaxies. Some 14 million of these galaxies could be used by Euclid to study the hidden influence of dark energy on the universe. “We have already seen beautiful, high-resolution images of individual objects and groups of objects from Euclid. This new image finally gives us a taste of the enormity of the area of sky Euclid will cover, which will enable us to take detailed measurements of billions of galaxies,” said Jason Rhodes, an observational cosmologist at NASA’s Jet Propulsion Laboratory in Southern California who is the U.S. science lead for Euclid and principal investigator for NASA’s Euclid dark energy science team. Galaxies Galore Even though this patch of space shows only 1% of Euclid’s total survey area, the spacecraft’s sensitive cameras captured an incredible number of objects in great detail. Enlarging the image by a factor of 600 reveals the intricate structure of a spiral galaxy in galaxy cluster Abell 3381, 470 million light-years away. This section of the Euclid mosaic is zoomed in 600 times. A single spiral galaxy is visible in great detail within cluster Abell 3381, 470 million light-years away from us. Data from both the visible and infrared light instruments on Euclid are included. ESA/Euclid/Euclid Consortium/NASA, CEA Paris-Saclay, image processing by J.-C. Cuillandre, E. Bertin, G. Anselmi. CC BY-SA 3.0 IGO “What really strikes me about these new images is the tremendous range in physical scale,” said JPL’s Mike Seiffert, project scientist for the NASA contribution to Euclid. “The images capture detail from clusters of stars near an individual galaxy to some of the largest structures in the universe. We are beginning to see the first hints of what the full Euclid data will look like when it reaches the completion of the prime survey.” Visble as well are clouds of gas and dust located between the stars in our own galaxy. Sometimes called “galactic cirrus” because they look like cirrus clouds at Earth, these clouds can be observed by Euclid’s visible-light camera because they reflect visible light from the Milky Way. The mosaic released today is taste of what’s to come from Euclid. The mission plans to release 53 square degrees of the Euclid survey, including a preview of the Euclid Deep Field areas, in March 2025 and to release its first year of cosmology data in 2026. NASA’s forthcoming Nancy Grace Roman mission will also study dark energy — in ways that are complementary to Euclid. Mission planners will use Euclid’s findings to inform Roman’s dark energy work. Scheduled to launch by May 2027, Roman will study a smaller section of sky than Euclid but will provide higher-resolution images of millions of galaxies and peer deeper into the universe’s past, providing complementary information. In addition, Roman will survey nearby galaxies, find and investigate planets throughout our galaxy, study objects on the outskirts of our solar system, and more. More About Euclid Euclid is a European mission, built and operated by ESA, with contributions from NASA. The Euclid Consortium — consisting of more than 2,000 scientists from 300 institutes in 15 European countries, the United States, Canada, and Japan — is responsible for providing the scientific instruments and scientific data analysis. ESA selected Thales Alenia Space as prime contractor for the construction of the satellite and its service module, with Airbus Defence and Space chosen to develop the payload module, including the telescope. Euclid is a medium-class mission in ESA’s Cosmic Vision Programme. Three NASA-supported science teams contribute to the Euclid mission. In addition to designing and fabricating the sensor-chip electronics for Euclid’s Near Infrared Spectrometer and Photometer (NISP) instrument, JPL led the procurement and delivery of the NISP detectors as well. Those detectors, along with the sensor chip electronics, were tested at NASA’s Detector Characterization Lab at Goddard Space Flight Center in Greenbelt, Maryland. The Euclid NASA Science Center at IPAC (ENSCI), at Caltech in Pasadena, California, will archive the science data and support U.S.-based science investigations. JPL is a division of Caltech. For more information about Euclid go to: https://www.nasa.gov/mission_pages/euclid/main/index.html For more information about Roman, go to: https://roman.gsfc.nasa.gov News Media Contacts Calla Cofield Jet Propulsion Laboratory, Pasadena, Calif. 626-808-2469 calla.e.cofield@jpl.nasa.gov ESA Media Relations media@esa.int 2024-141 Share Details Last Updated Oct 15, 2024 Related TermsEuclidAstrophysicsDark EnergyDark MatterGalaxiesJet Propulsion LaboratoryThe Universe Explore More 8 min read Revealing the Hidden Universe with Full-shell X-ray Optics at NASA MSFC The study of X-ray emission from astronomical objects reveals secrets about the Universe at the… Article 2 hours ago 5 min read Journey to a Water World: NASA’s Europa Clipper Is Ready to Launch Article 2 days ago 6 min read Can Life Exist on an Icy Moon? NASA’s Europa Clipper Aims to Find Out Article 3 days ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

NASA Administrator Bill Nelson talks to the agency’s workforce during his first State of NASA event Wednesday, June 2, 2021, at NASA Headquarters Mary W. Jackson Building in Washington. NASA/Bill Ingalls Continuing his efforts to deepen international collaboration and promote the peaceful use of space, NASA Administrator Bill Nelson will travel to Romania and Bulgaria, beginning Thursday, Oct. 17. Both countries have signed the Artemis Accords, a set of commonsense principles to commit to the peaceful exploration of space. Nelson will meet with key government and space officials in each country, including Marcel Ciolacu, Romania’s prime minister, and Rumen Radev, president of Bulgaria. In Romania, Nelson will engage with Bogdan-Gruia Ivan, minister of research, innovation and digitization, and Daniel Crunțeanu, general director of the Romanian Space Agency (ROSA). He also will visit Romanian science and technology institutions to learn about the country’s science facilities. In Bulgaria, Nelson will meet with Dr. Rosen Karadimov, minister of innovation and growth, and visit the country’s only satellite builder, which is producing satellites for organizations globally. During his travels to both countries, Nelson will discuss the importance of international partnerships and collaboration in space, including the transatlantic relationships to NASA. Nelson also will meet with students to highlight the benefits science, technology, engineering, and mathematics education and their roles as members of the Artemis Generation. For more information about NASA’s international partnerships, visit: https://www.nasa.gov/oiir -end- Meira Bernstein Headquarters, Washington 202-615-1747 meira.b.bernstein@nasa.gov Share Details Last Updated Oct 15, 2024 EditorRoxana BardanLocationNASA Headquarters Related TermsBill NelsonOffice of International and Interagency Relations (OIIR) View the full article

Making the most of a solar eclipse demands attention to detail. Do you have what it takes? NASA’s Eclipse Megamovie project launched a new coding competition, and they need your help to organize images from the April 8, 2024 total solar eclipse. This is your chance to make a lasting contribution to solar science! The Eclipse Megamovie project asked volunteers to take photos of the total solar eclipse that took place on April 8, 2024 to discover the secret lives of solar jets and plumes. Many jets and plumes seem to disappear or change from the time they are formed on the Sun to when they move out into the solar wind. Thanks to the efforts of over 145 citizen scientists, more than 1 terabyte of photographs were collected and are now being analyzed. These images will help scientists track disappearing jets and plumes, shedding light on how these solar events impact space weather and our understanding of the Sun’s outer atmosphere. One of the standout volunteers in the Eclipse Megamovie project is Hy Tran, a citizen scientist who earned praise from the science team for his detailed feedback and mentorship of fellow volunteers. “We love working with volunteers like Hy,” said Eclipse Megamovie scientist Hannah Hellman. “They bring passion, experience, and technological knowledge to our projects.” Superstar volunteer Hy Tran helps mentor other eclipse chasers. You can join the Eclipse Megamovie project now by taking part in a coding competition! Tran’s day job is in metrology—the science of measurement (not to be confused with meteorology!). “In my professional life,” said Tran, “I support a measurement standards and calibration program, so we live by having good procedures!” He also volunteers in technical societies, focusing on standards development, engineering, and technology education. Outside of work, Hy mentors and serves as a local leader in science/technology/engineering/mathematics (STEM) outreach. He loves woodturning and dabbles in amateur astrophotography and underwater photography. The technical challenges of participating in eclipse science projects so far have hit his sweet spot. Although it will be a while until the next eclipse, the Eclipse Megamovie team still needs your help. Join volunteers like Hy and participate in their coding competition! Your mission is to create the most accurate sorting machine that categorizes a solar eclipse photograph into a specific solar eclipse phase. Not only will your code help organize the massive amounts of data collected, but you’ll also have the chance to win some prizes. Prizes for the Competition First Place: Image-stabilized binoculars with solar filters, a feature on the Eclipse Megamovie website, an Eclipse Megamovie Team Patch, a NASA calendar, an Eclipse Megamovie sticker, and a First Prize Certificate. Second and Third Place: A feature on the Eclipse Megamovie website, an Eclipse Megamovie Team Patch, a NASA calendar, an Eclipse Megamovie sticker, and a certificate. Think you’ve got the skills to tackle this challenge? Visit the Eclipse Megamovie project website to sign up today! For more information, visit the Eclipse Megamovie page at Kaggle: http://kaggle.com/competitions/eclipse-megamovie. Facebook logo @DoNASAScience @DoNASAScience Share Details Last Updated Oct 15, 2024 Related Terms Citizen Science Eclipses Heliophysics Explore More 2 min read ESA/NASA’s SOHO Spies Bright Comet Making Debut in Evening Sky The Solar and Heliospheric Observatory (SOHO) has captured images of the second-brightest comet to ever pass… Article 4 days ago 2 min read Sail Along with NASA’s Solar Sail Tech Demo in Real-Time Simulation Article 5 days ago 3 min read Four Asteroids Named After NASA Volunteers Article 7 days ago View the full article

The study of X-ray emission from astronomical objects reveals secrets about the Universe at the largest and smallest spatial scales. Celestial X-rays are produced by black holes consuming nearby stars, emitted by the million-degree gas that traces the structure between galaxies, and can be used to predict whether stars may be able to host planets hospitable to life. X-ray observations have shown that most of the visible matter in the universe exists as hot gas between galaxies and have conclusively demonstrated that the presence of “dark matter” is needed to explain galaxy cluster dynamics, that dark matter dominates the mass of galaxy clusters, and that it governs the expansion of the cosmos. X-ray observations also enable us to probe mysteries of the Universe on the smallest scales. X-ray observations of compact objects such as white dwarfs, neutron stars, and black holes allow us to use the Universe as a physics laboratory to study conditions that are orders of magnitude more extreme in terms of density, pressure, temperature, and magnetic field strength than anything that can be produced on Earth. In this astrophysical laboratory, researchers expect to reveal new physics at the subatomic scale by conducting investigations such as probing the neutron star equation of state and testing quantum electrodynamics with observations of neutron star atmospheres. At NASA’s Marshall Space Flight Center, a team of scientists and engineers is building, testing, and flying innovative optics that bring the Universe’s X-ray mysteries into sharper focus. A composite X-ray/Optical/Infrared image of the Crab Pulsar. The X-ray image from the Chandra X-ray Observatory (blue and white), reveals exquisite details in the central ring structures and gas flowing out of the polar jets. Optical light from the Hubble Space Telescope (purple) shows foreground and background stars as pinpoints of light. Infrared light from the Spitzer Space Telescope (pink) traces cooler gas in the nebula. Finally, magnetic field direction derived from X-ray polarization observed by the Imaging X-ray Polarimetry Explorer is shown as orange lines. Magnetic field lines: NASA/Bucciantini et al; X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Infrared: NASA-JPL-Caltech Unlike optical telescopes that create images by reflecting or refracting light at near-90-degree angles (normal incidence), focusing X-ray optics must be designed to reflect light at very small angles (grazing incidence). At normal incidence, X-rays are either absorbed by the surface of a mirror or penetrate it entirely. However, at grazing angles of incidence, X-rays reflect very efficiently due to an effect called total external reflection. In grazing incidence, X-rays reflect off the surface of a mirror like rocks skipping on the surface of a pond. A classic design for astronomical grazing incidence optics is the Wolter-I prescription, which consists of two reflecting surfaces, a parabola and hyperbola (see figure below). This optical prescription is revolved around the optical axis to produce a full-shell mirror (i.e., the mirror spans the full circumference) that resembles a gently tapered cone. To increase the light collecting area, multiple mirror shells with incrementally larger diameters and a common focus are fabricated and nested concentrically to comprise a mirror module assembly (MMA). Focusing optics are critical to studying the X-ray universe because, in contrast to other optical systems like collimators or coded masks, they produce high signal-to-noise images with low background noise. Two key metrics that characterize the performance of X-ray optics are angular resolution, which is the ability of an optical system to discriminate between closely spaced objects, and effective area, which is the light collecting area of the telescope, typically quoted in units of cm2. Angular resolution is typically measured as the half-power diameter (HPD) of a focused spot in units of arcseconds. The HPD encircles half of the incident photons in a focused spot and measures the sharpness of the final image; a smaller number is better. Schematic of a full-shell Wolter-I X-ray optic mirror module assembly with five concentrically nested mirror shells. Parallel rays of light enter from the left, reflect twice off the reflective inside surface of the shell (first off the parabolic segment and then off the hyperbolic segment), and converge at the focal plane. NASA MSFC NASA Marshall Space Flight Center (MSFC) has been building and flying lightweight, full-shell, focusing X-ray optics for over three decades, always meeting or exceeding angular resolution and effective area requirements. MSFC utilizes an electroformed nickel replication (ENR) technique to make these thin full-shell X-ray optics from nickel alloy. X-ray optics development at MSFC began in the early 1990s with the fabrication of optics to support NASA’s Advanced X-ray Astrophysics Facility (AXAF-S) and then continued via the Constellation-X technology development programs. In 2001, MSFC launched a balloon payload that included two modules each with three mirrors, which produced the first focused hard X-ray (>10 keV) images of an astrophysical source by imaging Cygnus X-1, GRS 1915, and the Crab Nebula. This initial effort resulted in several follow-up missions over the next 12 years, and became known as the High Energy Replicated Optics (HERO) balloon program. In 2012, the first of four sounding rocket flights of the Focusing Optics X-ray Solar Imager (FOXSI) flew with MSFC optics onboard, producing the first focused images of the Sun at energies greater than 5 keV. In 2019 the Astronomical Roentgen Telescope X-ray Concentrator (ART-XC) instrument on the Spectr-Roentgen-Gamma Mission launched with seven MSFC-fabricated X-ray MMAs, each containing 28 mirror shells. ART-XC is currently mapping the sky in the 4-30 keV hard X-ray energy range, studying exotic objects like neutron stars in our own galaxy as well as active galactic nuclei, which are spread across the visible universe. In 2021, the Imaging X-ray Polarimetry Explorer (IXPE), flew and is now performing extraordinary science with an MSFC-led team using three, 24-shell MMAs that were fabricated and calibrated in-house. Most recently, in 2024, the fourth FOXSI sounding rocket campaign launched with a high-resolution MSFC MMA. The optics achieved 9.5 arcsecond HPD angular resolution during pre-flight test with an expected 7 arcsecond HPD in gravity-free flight, making this the highest angular resolution flight observation made with a nickel-replicated X-ray optic. Currently MSFC is fabricating an MMA for the Rocket Experiment Demonstration of a Soft X-ray (REDSoX) polarimeter, a sounding rocket mission that will fly a novel soft X-ray polarimeter instrument to observe active galactic nuclei. The REDSoX MMA optic will be 444 mm in diameter, which will make it the largest MMA ever produced by MSFC and the second largest replicated nickel X-ray optic in the world. Scientists Wayne Baumgartner (left, crouched) and Nick Thomas (left, standing) calibrate an IXPE MMA in the MSFC 100 m Beamline. Scientist Stephen Bongiorno (right) applies epoxy to an IXPE shell during MMA assembly. NASA MSFC The ultimate performance of an X-ray optic is determined by errors in the shape, position, and roughness of the optical surface. To push the performance of X-ray optics toward even higher angular resolution and achieve more ambitious science goals, MSFC is currently engaged in a fundamental research and development effort to improve all aspects of full-shell optics fabrication. Given that these optics are made with the Electroformed Nickel Replication technique, the fabrication process begins with creation of a replication master, called the mandrel, which is a negative of the desired optical surface. First, the mandrel is figured and polished to specification, then a thin layer of nickel alloy is electroformed onto the mandrel surface. Next, the nickel alloy layer is removed to produce a replicated optical shell, and finally the thin shell is attached to a stiff holding structure for use. Each step in this process imparts some degree of error into the final replicated shell. Research and development efforts at MSFC are currently concentrating on reducing distortion induced during the electroforming metal deposition and release steps. Electroforming-induced distortion is caused by material stress built into the electroformed material as it deposits onto the mandrel. Decreasing release-induced distortion is a matter of reducing adhesion strength between the shell and mandrel, increasing strength of the shell material to prevent yielding, and reducing point defects in the release layer. Additionally, verifying the performance of these advanced optics requires world-class test facilities. The basic premise of testing an optic designed for X-ray astrophysics is to place a small, bright X-ray source far away from the optic. If the angular size of the source, as viewed from the optic, is smaller than the angular resolution of the optic, the source is effectively simulating X-ray starlight. Due to the absorption of X-rays by air, the entire test facility light path must be placed inside a vacuum chamber. At MSFC, a group of scientists and engineers operate the Marshall 100-meter X-ray beamline, a world-class end-to-end test facility for flight and laboratory X-ray optics, instruments, and telescopes. As per the name, it consists of a 100-meter-long vacuum tube with an 8-meter-long, 3-meter-diameter instrument chamber and a variety of X-ray sources ranging from 0.25 – 114 keV. Across the street sits the X-Ray and Cryogenic Facility (XRCF), a 527-meter-long beamline with an 18-meter-long, 6-meter-diameter instrument chamber. These facilities are available for the scientific community to use and highlight the comprehensive optics development and test capability that Marshall is known for. Within the X-ray astrophysics community there exist a variety of angular resolution and effective area needs for focusing optics. Given its storied history in X-ray optics, MSFC is uniquely poised to fulfill requirements for large or small, medium- or high-angular-resolution X-ray optics. To help guide technology development, the astrophysics community convenes once per decade to produce a decadal survey. The need for high-angular-resolution and high-throughput X-ray optics is strongly endorsed by the National Academies of Sciences, Engineering, and Medicine report, Pathways to Discovery in Astronomy and Astrophysics for the 2020s.In pursuit of this goal, MSFC is continuing to advance the state of the art in full-shell optics. This work will enable the extraordinary mysteries of the X-ray universe to be revealed. Project Leads Dr. Jessica Gaskin and Dr. Stephen Bongiorno, NASA Marshall Space Flight Center (MSFC) Sponsoring Organizations The NASA Astrophysics Division supports this work primarily through the Internal Scientist Funding Model Direct Work Package and competed solicitations. This work is also supported by the Heliophysics Division through competed solicitations, as well as by directed work from other government entities. Share Details Last Updated Oct 15, 2024 Related Terms Astrophysics Astrophysics Division Marshall Astrophysics Marshall Space Flight Center Science-enabling Technology Technology Highlights Explore More 2 min read Hubble Spots a Grand Spiral of Starbursts Article 4 days ago 6 min read NASA’s Hubble, New Horizons Team Up for a Simultaneous Look at Uranus Article 6 days ago 4 min read NASA’s Hubble Watches Jupiter’s Great Red Spot Behave Like a Stress Ball Article 6 days ago View the full article

The Power and Promise of NASA’s International Partnerships