NASA

Artist’s rendering of a potentially habitable super-Earth orbiting a star called HD 20794. Illustration credit: Gabriel Pérez Díaz, SMM (IAC) The Discovery A possible “super-Earth” orbits a relatively close, Sun-like star, and could be a habitable world – but one of extreme temperature swings, from scorching heat to deep freeze. Key Facts The newly confirmed planet is the outermost of three detected so far around a star called HD 20794, just 20 light-years from Earth. Its 647-day orbit is comparable to Mars in our solar system. But this planet’s orbit is highly eccentric, stretched into an oval shape. That brings the planet close enough to the star to experience runaway heating for part of its year, then carries it far enough away to freeze any potential water on its surface. The planet has been bouncing between these extremes roughly every 300 days – perhaps for billions of years. Details The planet spends a good chunk of its year in the “habitable zone” around its star, the orbital distance that would allow liquid water to form on the surface under the right atmospheric conditions. But because of its eccentric orbit, it moves to a distance interior to the inner edge of the habitable zone when closest to the star, and outside the outer edge when farthest away. At its closest, the planet’s distance from the star is comparable to Venus’s distance from the Sun; at its farthest point, it is nearly twice the distance from Earth to the Sun. The planet is possibly rocky, like Earth, but could be a heftier version – about six times as massive as our home planet. Star HD 20794 and its posse of possible planets have been extensively studied, but the international team of astronomers that confirmed the outer planet, led by Nicola Nari of Light Bridges S.L. and the Instituto de Astrofisica de Canarias, examined more than 20 years worth of data to pin down all three planets’ orbits and likely masses. The scientists relied on data from two ground-based, precision instruments: HARPS, the High Accuracy Radial velocity Planet Searcher in La Silla, Chile, and ESPRESSO, the Echelle Spectrograph for Rocky Exoplanets and Stable Spectroscopic Observations in Paranal, Chile. Both instruments, connected to powerful telescopes, measure tiny shifts in the light spectrum of stars, caused by the gravity of planets tugging the star back and forth as they orbit. But such tiny shifts in the star’s spectrum also can be caused by imposters – spots, flares, or other activity on the star’s surface, carried along as the star rotates and masquerading as orbiting planets. The science team spent years painstakingly analyzing the spectrum shifts, or “radial velocity” data, for any sign of background noise or even jitters from the instruments themselves. They confirmed the reputation of HD 20794 as a fairly quiet star, not prone to outbursts that might be confused for signs of orbiting planets. Fun Facts The elliptically orbiting super-Earth appears to be an ideal target for future space-based telescopes designed to search for habitable worlds, seeking possible signs of life. High on the list is NASA’s Habitable Worlds Observatory, which will someday examine the atmospheres of Earth-sized planets around Sun-like stars. When launched in the decades ahead, the observatory would spread the light from such planets into a spectrum to determine which gases are present – including those that might reveal some form of life. The relative closeness of HD 20974, only 20 light-years away, its brightness, and its low level of surface activity – not to mention the third planet’s wild temperature swings – could make this system a prime candidate for scrutiny by HWO. The Discoverers The international science team that confirmed the eccentric super-Earth was led by researcher Nicola Nari of the Light Bridges S.L. and the Instituto de Astrofisica de Canarias, and included Dr. Michael Cretignier of the University of Oxford, who first picked up the potential planet’s signal in 2022. Their paper, “Revisiting the multi-planet system of the nearby star HD 20794,” was published online by the journal, Astronomy and Astrophysics, in January 2025. View the full article

2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) This was a magical revelation for the Greeks and the Egyptians, who were able to see from the motions of the stars and the way the Sun moved. They saw the way the Sun’s shadow worked in different places. And they figured, well, that’s only possible if the Earth is round. And they took that information and it extended into the time of the great mariners that explored our Earth by ships. They made the first orbit of Earth by sea, and they knew the Earth was round, allowing them to go across one ocean and come back home the other way. If the Earth were flat, they would have sailed off the end. And so we knew that. But then, at the dawn of the space age, in the late 50s and 60s, we were able to see for ourselves that our beautiful home is a gorgeous round object known as a sphere. And that was really special. It put ourselves into context of our solar system and our universe. We have a big round Sun and a beautiful round Earth and a round Mars. And today we use the roundness of Earth, the spherical Earth, to use methods in space geodesy to figure out where we are, where we’re going. I haven’t been lost in years. That’s pretty good. What’s happening to the Earth, what’s happening to our oceans as we take the pulse of our planet and consider other worlds beyond as we explore those. So as we get ready to go back to the Moon with women and men and explore other worlds, the roundness of our solar system and our universe is a special thing. And we should embrace that as we understand why our planet isn’t flat. [END VIDEO TRANSCRIPT] Full Episode List Full YouTube Playlist Share Details Last Updated Mar 11, 2025 Related TermsEarthScience Mission DirectorateThe Solar System Explore More 2 min read Hubble Unveils a Glittering View of Sh2-284 A tiny fraction of the stellar nursery known as Sh2-284 is visible in this glittering,… Article 3 days ago 3 min read Hubble Jams With A Cosmic Guitar Arp 105 is a dazzling ongoing merger between an elliptical galaxy and a spiral galaxy… Article 3 days ago 2 min read Hubble Spies a Spectacular Starburst Galaxy Sweeping spiral arms extend from NGC 4536, littered with bright blue clusters of star formation… Article 3 days ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

How Do We Know the Earth Isn't Flat? We Asked a NASA Expert

A chevron nozzle is installed on NASA’s Learjet for a mid-March 2001 flight test at Lorain Country Airport to verify that in an emergency, the aircraft could be flown using only the experimental engine. Credit: NASA/Marvin Smith Shortly after dawn on March 27, 2001, NASA pilot Bill Rieke took off from an airfield just outside of Phoenix in NASA’s blue-and-white Learjet 25 and flew low over a series of microphones for the first flight test of a groundbreaking NASA technology. On one of the plane’s engines was an experimental jagged-edged nozzle that researchers at Glenn Research Center in Cleveland had discovered made aircraft significantly quieter. These initial flight tests were an important step toward using these “chevron nozzles” on modern aircraft, lowering noise levels for communities. NASA Glenn has been exploring ways of reducing engine noise since the first jet airliners appeared in the 1950s. New turbofan engines in the 1960s were quieter, but the expansion of the overall airline industry meant that noise was still an issue. With the introduction of noise-limiting mandates in the 1970s, NASA and engine manufacturers embarked on a decades-long search for technologies to lower noise levels. NASA researchers discovered that the military’s use of rectangular notches, or tabs, along an engine nozzle’s exit – to help disguise a jet fighter’s infrared signature – could also reduce engine noise by helping mix the hot air from the engine core and the cooler air blowing through the engine fan. In the 1990s, Glenn researcher Dennis Huff and his colleagues discovered that a serrated, or sawtooth, shape, referred to as a chevron, offered more promise. Dennis Huff explains chevron nozzles, seen on a table, to U.S. Senator George Voinovich and other visitors inside the Aero-Acoustic Propulsion Laboratory facility in 2006. Huff was head of NASA Glenn Research Center’s Acoustics Branch at this point.Credit: NASA/Marvin Smith NASA contracted with General Electric and Pratt & Whitney to develop an array of tab and chevron designs to be analyzed in Glenn’s unique Aero-Acoustic Propulsion Laboratory (AAPL). Extensive testing in the spring of 1997 showed the possibilities for reducing noise with these types of nozzles. Engine manufacturers were impressed with the findings but wary of any technology that might impact performance. So, in 1998, NASA funded engine tests of the 14 most promising designs. The tests revealed the chevron nozzle had a negligible 0.25% reduction of thrust. It was a major development for jet noise research. In September 2000, Glenn’s Flight Operations Branch was contacted about the logistics of flight-testing chevron nozzles on the center’s Learjet 25 to verify the ground tests and improve computer modeling. Nothing further came of the request, however, until early the next year when Huff informed Rieke, chief of Flight Operations, that the researchers would like to conduct flight tests in late March—with just eight weeks to prepare. Glenn’s Acoustics Branch worked with colleagues at NASA’s Langley Research Center in Hampton, Virginia, and the Arizona-based engine manufacturer Honeywell on the effort. They planned to conduct testing at Estrella Sailport just outside of Phoenix from March 26 to 28, 2001. Bill Rieke and Ellen Tom with the chevron nozzle installed on the Learjet. NASA Glenn Research Center’s small Flight Operations team was heavily involved with icing research and solar cell calibration flights during this period, so arrangements were made for Tom, a Federal Aviation Administration pilot, to assist with the chevron flights. Credit: Courtesy of Bill Rieke With the required safety and design reviews, the eight-week target date would be difficult to meet for any test flight, but this one was particularly challenging as it involved modifications to the engine nacelle. While the special nozzle engineers created for the flights would allow them to switch between a six- and a 12-chevron design during testing, it also got hot quickly. This necessitated the installation of new sensors, rewiring of fire alarm cables, and the presence of an onboard test engineer to monitor the temperatures. The short turnaround also required expedited efforts to obtain flight plan approvals, verify the plane’s airworthiness, and perform normal maintenance activities. Despite the challenges, Rieke and a small team delivered the Learjet to Estrella on March 25, as planned. The next day was spent coordinating with the large Langley and Honeywell team and acquiring baseline noise data. The pilots idled the unmodified engine as the Learjet flew over three perpendicular rows of microphones at an altitude of 500 feet and speed of 230 miles per hour. View from below as NASA Glenn Research Center’s Learjet 25 passes overhead at the Estrella airfield with the experimental chevron nozzle visible on the left wing.Credit: Courtesy of Bill Rieke The flight patterns were repeated over the next two days while alternately using the two variations of the chevron nozzle. The researchers anecdotally reported that there was no perceptible noise reduction as the aircraft approached, but significant reductions once it passed. Recordings supported these observations and showed that sideline noise was reduced, as well. The flights of the Learjet, which was powered by a variation of GE’s J-85 turbojet, were complemented by Honeywell’s turbofan-powered Falcon 20 aircraft. These flights ultimately confirmed the noise reduction found in earlier AAPL tests. Overall, the flight tests were so successful that just over a year later the FAA began certifying GE’s CF34–8, the first commercial aircraft engine to incorporate chevron technology. The engine was first flown on a Bombardier CRJ900 in 2003. Continued studies by both NASA and industry led to the improved designs and the incorporation of chevrons into larger engines, such as GE’s GEnx. According to Huff, the chevron’s three-decibel noise decrease was analogous to the difference between running two lawnmowers and one. Their comparatively easy integration into engine design and minimal effect on thrust made the chevron a breakthrough in noise-reduction technology. In 2002, NASA presented an innovation award to the Glenn, Langley, and Honeywell team that carried out the flights. Today, airliners such as the 737 MAX and 787 Dreamliner use chevron nozzles to lower noise levels for communities near airports. Explore More 3 min read NASA Selects Three University Teams to Participate in Flight Research Article 6 hours ago 2 min read NASA Marks 110 Years Since Founding of Predecessor Organization Article 1 week ago 3 min read NASA’s X-59 Completes Electromagnetic Testing Article 2 weeks ago View the full article

This video sparkles with synthetic supernovae from the OpenUniverse project, which simulates observations from NASA’s upcoming Nancy Grace Roman Space Telescope. More than a million exploding stars flare into visibility and then slowly fade away. The true brightness of each transient event has been magnified by a factor of 10,000 for visibility, and no background light has been added to the simulated images. The pattern of squares shows Roman’s full field of view.Credit: NASA’s Goddard Space Flight Center and M. Troxel The universe is ballooning outward at an ever-faster clip under the power of an unknown force dubbed dark energy. One of the major goals for NASA’s upcoming Nancy Grace Roman Space Telescope is to help astronomers gather clues to the mystery. One team is setting the stage now to help astronomers prepare for this exciting science. “Roman will scan the cosmos a thousand times faster than NASA’s Hubble Space Telescope can while offering Hubble-like image quality,” said Rebekah Hounsell, an assistant research scientist at the University of Maryland-Baltimore county working at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and a co-principal investigator of the Supernova Cosmology Project Infrastructure Team preparing for the mission’s High-Latitude Time-Domain Survey. “We’re going to have an overwhelming amount of data, and we want to make it so scientists can use it from day one.” Roman will repeatedly look at wide, deep regions of the sky in near-infrared light, opening up a whole new view of the universe and revealing all sorts of things going bump in the night. That includes stars being shredded as they pass too close to a black hole, intense emissions from galaxy centers, and a variety of stellar explosions called supernovae. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video This data sonification transforms a vast simulation of a cosmic survey from NASA’s upcoming Nancy Grace Roman Space Telescope into a symphony of stellar explosions. Each supernova’s brightness controls its volume, while its color sets its pitch –– redder, more distant supernovae correspond to deep, low tones while bluer, nearer ones correspond to higher frequencies. The sound in stereo mirrors their locations in the sky. The result sounds like celestial wind chimes, offering a way to “listen” to cosmic fireworks. Credit: NASA’s Goddard Space Flight Center, M. Troxel, SYSTEM Sounds (M. Russo, A. Santaguida) Cosmic Radar Guns Scientists estimate around half a dozen stars explode somewhere in the observable universe every minute. On average, one of them will be a special variety called type Ia that can help astronomers measure the universe. These explosions peak at a similar intrinsic brightness, allowing scientists to find their distances simply by measuring how bright they appear. Scientists can also study the light of these supernovae to find out how quickly they are moving away from us. By comparing how fast they’re receding at different distances, scientists will trace cosmic expansion over time. Using dozens of type Ia supernovae, scientists discovered that the universe’s expansion is accelerating. Roman will find tens of thousands, including very distant ones, offering more clues about the nature of dark energy and how it may have changed throughout the history of the universe. “Roman’s near-infrared view will help us peer farther because more distant light is stretched, or reddened, as it travels across expanding space,” said Benjamin Rose, an assistant professor at Baylor University in Waco, Texas, and a co-principal investigator of the infrastructure team. “And opening a bigger window, so to speak, will help us get a better understanding of these objects as a whole,” which would allow scientists to learn more about dark energy. That could include discovering new physics, or figuring out the universe’s fate. The People’s Telescope Members of the planning team have been part of the community process to seek input from scientists worldwide on how the survey should be designed and how the analysis pipeline should work. Gathering public input in this way is unusual for a space telescope, but it’s essential for Roman because each large, deep observation will enable a wealth of science in addition to fulfilling the survey’s main goal of probing dark energy. Rather than requiring that many individual scientists submit proposals to reserve their own slice of space telescope time, Roman’s major surveys will be coordinated openly, and all the data will become public right away. “Instead of a single team pursuing one science goal, everyone will be able to comb through Roman’s data for a wide variety of purposes,” Rose said. “Everyone will get to play right away.” This animation shows a possible tiling pattern of part of NASA’s Nancy Grace Roman Space Telescope’s High Latitude Time-Domain Survey. The observing program, which is being designed by a community process, is expected to have two components: wide (covering 18 square degrees, a region of sky as large as about 90 full moons) and deep (covering about 5.5 square degrees, about as large as 25 full moons). This animation shows the deeper portion, which would peer back to when the universe was about 500 million years old, less than 4 percent of its current age of 13.8 billion years.Credit: NASA’s Goddard Space Flight Center This Is a Drill NASA plans to announce the survey design for Roman’s three core surveys, including the High-Latitude Time-Domain Survey, this spring. Then the planning team will simulate it in its entirety. “It’s kind of like a recipe,” Hounsell said. “You put in your observing strategy — how many days, which filters — and add in ‘spices’ like uncertainties, calibration effects, and the things we don’t know so well about the instrument or supernovae themselves that would affect our results. We can inject supernovae into the synthetic images and develop the tools we’ll need to analyze and evaluate the data.” Scientists will continue using the synthetic data even after Roman begins observing, tweaking all aspects of the simulation and correcting unknowns to see which resulting images best match real observations. Scientists can then fine-tune our understanding of the universe’s underlying physics. “We assume that all supernovae are the same regardless of when they occurred in the history of the universe, but that might not be the case,” Hounsell said. “We’re going to look further back in time than we’ve ever done with type Ia supernovae, and we’re not completely sure if the physics we understand now will hold up.” There are reasons to suspect they may not. The very first stars were made almost exclusively of hydrogen and helium, compared to stars today which contain several dozen elements. Those ancient stars also lived in very different environments than stars today. Galaxies were growing and merging, and stars were forming at a furious pace before things began calming down between about 8 and 10 billion years ago. “Roman will very dramatically add to our understanding of this cosmic era,” Rose said. “We’ll learn more about cosmic evolution and dark energy, and thanks to Roman’s large deep view, we’ll get to do much more science too with the same data. Our work will help everyone hit the ground running after Roman launches.” For more information about the Roman Space Telescope visit www.nasa.gov/roman. The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory and Caltech/IPAC in Southern California, the Space Telescope Science Institute in Baltimore, and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California. By Ashley Balzer NASA’s Goddard Space Flight Center, Greenbelt, Md. Media contact: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, Md. 301-286-1940 Explore More 7 min read NASA’s Roman and ESA’s Euclid Will Team Up To Investigate Dark Energy Article 2 years ago 7 min read NASA’s Roman Mission to Probe Cosmic Secrets Using Exploding Stars Article 4 years ago 4 min read NASA Successfully Joins Sunshade to Roman Observatory’s ‘Exoskeleton’ Article 4 weeks ago Share Details Last Updated Mar 11, 2025 EditorAshley BalzerContactAshley Balzerashley.m.balzer@nasa.govLocationGoddard Space Flight Center Related TermsNancy Grace Roman Space TelescopeDark EnergyGoddard Space Flight CenterStarsThe Universe View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA / Lillian Gipson NASA has selected three university teams to help solve 21st century aviation challenges that could transform the skies above our communities. As part of NASA’s University Leadership Initiative (ULI), both graduate and undergraduate students on faculty-led university teams will contribute directly to real-world flight research while gaining hands-on experience working with partners from other universities and industry. By combining faculty expertise, student innovation, and industry experience, these three teams will advance NASA’s vision for the future of 21st century aviation. koushik datta NASA Project Manager This is NASA’s eighth round of annual ULI awards. Research topics include: New aviation systems for safer, more efficient flight operations Improved communications frequency usage for more effective and reliable information transfer Autonomous flight capabilities that could advance research in areas such as NASA’s Advanced Air Mobility mission “By combining faculty expertise, student innovation, and industry experience, these three teams will advance NASA’s vision for the future of 21st century aviation,” said Koushik Datta, NASA University Innovation project manager at the Agency’s Ames Research Center in California. This eighth round of annual ULI selections would lead to awards totaling up to $20.7 million for the three teams during the next three years. For each team, the proposing university will serve as lead. The new ULI selections are: Florida Institute of Technology, Melbourne, Florida The team will create a framework for developing trustworthy increasingly autonomous aviation safety systems, such as those that could potentially employ artificial intelligence and machine learning. Team members include: The Pennsylvania State University in University Park; North Carolina Agricultural and Technical State University in Greensboro; University of Florida in Gainesville; Stanford University in California; Santa Fe Community College in New Mexico; and the companies Collins Aerospace of Charlotte in North Carolina; and ResilienX of Syracuse, New York. University of Colorado Boulder This team will investigate tools for understanding and leveraging the complex communications environment of collaborative, autonomous airspace systems. Team members include: Massachusetts Institute of Technology in Cambridge; The University of Texas at El Paso; University of Colorado in Colorado Springs; Stanford University in California; University of Minnesota Twin Cities in Minneapolis, North Carolina State University in Raleigh; University of California inSanta Barbara; El Paso Community College in Texas; Durham Technical Community College in North Carolina; the Center for Autonomous Air Mobility and Sensing research partnership; the company Aurora Flight Sciences, a Boeing Company, in Manassas, Virginia; and the nonprofit Charles Stark Draper Laboratory in Cambridge, Massachusetts. Embry-Riddle Aeronautical University, Daytona Beach, Florida This team will research continuously updating, self-diagnostic vehicle health management to enhance the safety and reliability of Advanced Air Mobility vehicles. Team members include: Georgia Institute of Technology in Atlanta; The University of Texas at Arlington; University of Southern California in Los Angeles; the company Collins Aerospace of Charlotte, North Carolina; and the Argonne National Laboratory. NASA’s ULI is managed by the agency’s University Innovation project, which also includes the University Student Research Challenge and the Gateways to Blue Skies competition. Watch the NASA Aeronautics solicitations page for the announcement of when the next opportunity will be to submit a proposal for consideration during the next round of ULI selections. About the AuthorJohn GouldAeronautics Research Mission DirectorateJohn Gould is a member of NASA Aeronautics' Strategic Communications team at NASA Headquarters in Washington, DC. He is dedicated to public service and NASA’s leading role in scientific exploration. Prior to working for NASA Aeronautics, he was a spaceflight historian and writer, having a lifelong passion for space and aviation. Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More 2 min read NASA Marks 110 Years Since Founding of Predecessor Organization Article 1 week ago 3 min read NASA’s X-59 Completes Electromagnetic Testing Article 2 weeks ago 4 min read NASA University Research Program Makes First Award to a Community College Project Article 2 weeks ago Keep Exploring Discover More Topics From NASA Missions Artemis Aeronautics STEM Explore NASA’s History Share Details Last Updated Mar 10, 2025 EditorJim BankeContactSteven Holzsteven.m.holz@nasa.gov Related TermsUniversity Leadership InitiativeAeronauticsFlight InnovationTransformative Aeronautics Concepts ProgramUniversity Innovation View the full article

SPHEREx and PUNCH Launch (Official NASA Broadcast)

5 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Artist’s concept of drones flying in an urban environment near large city skyscrapers.NASA / Maria Werries Remotely piloted aircraft could transform the way we transport people and goods and provide our communities with better access to vital services, like medical supply deliveries and efficient transportation. NASA’s Pathfinding for Airspace with Autonomous Vehicles (PAAV) subproject is working with partners to safely integrate remote air cargo and air taxi aircraft into our national airspace alongside traditional crewed aircraft. These new types of vehicles could make air cargo deliveries and air travel more affordable and accessible to communities across the country. The Need The United States large air cargo fleet is expected to grow significantly through 2044 to meet cargo demand, according to the Federal Aviation Administration (FAA). However, pilot shortages exacerbated by early retirements and crew reductions implemented during the coronavirus outbreak continue to present a challenge to the air cargo industry. In the future, one pilot could potentially manage multiple aircraft remotely. This could help meet the rising demand for air cargo operations, mitigate pilot shortages and costs, and increase the number of daily air cargo deliveries. Additionally, remotely piloted air taxis could reduce travel time for passengers and alleviate traffic congestion because they could avoid crowded roads and highways. Identifying the Technical Challenges Commercial companies are investing in autonomous technologies to enable remote air cargo deliveries and air taxi operations. NASA is working with the industry along the way to identify the unique technical challenges that must be overcome to safely put these new types of aircraft into routine operation. The agency has identified several challenges that need to be addressed for safe and scalable remote operations. Among these challenges are airspace integration, avoiding airborne and ground-based hazards, and resilient communication technologies. The main difference between conventional crewed aircraft and remotely piloted aircraft is the location of the pilot. Remote pilots operate aircraft from a control station on the ground instead of the cockpit. This means remote pilots will need new automation and decision support systems for operating the aircraft since they can’t rely on their eyes and view from the cockpit. Since remote pilots are on the ground, they need a reliable communications link that allows remote pilots to interact with the aircraft and maintain command and control. If the command-and-control capabilities are lost, an autonomous system would need to take over to make sure the uncrewed aircraft can fly and land safely, according to NASA researchers. Adequate software and procedures must be in place to safely manage off-nominal losses of the command-and-control capabilities. Air Traffic Control may help keep the uncrewed aircraft’s path clear from some traffic during takeoff and landing, while onboard automation technologies would need to avoid all other traffic, fly the aircraft along a known path, and check to ensure the runway is clear to land. A significant related challenge is that pilots are typically responsible for looking out the window for nearby aircraft and remaining well clear of them. Since the remote pilot is not in the aircraft, they will need an electronic detect and avoid system. Detect and avoid systems rely on information, sensors, and algorithms to help the remotely piloted aircraft remain clear of other aircraft. Some detect and avoid configurations are expected to use ground surveillance systems for detecting nearby air traffic at lower altitudes. These systems could improve overall situational awareness of traffic near the airport by providing a more comprehensive picture of live traffic. Additionally, automation and decision support tools could help remote pilots with other responsibilities that typically require pilot decisions from the cockpit, like integrating with traffic at non-towered airports. Implementing Solutions To address these challenges and others, NASA researchers are working with industry partners to research and test technologies, concepts, and airspace procedures that will enable remotely piloted operations. For example, industry is developing automated taxi, takeoff, and landing capabilities to help integrate remotely piloted aircraft operating at busy airports. These technologies could enable aircraft to navigate and integrate with other airport traffic autonomously, following standard routes and air traffic control commands for safe sequencing and spacing between other aircraft. Automated hazard detection would enable the aircraft to identify potential conflicts or hazards and take corrective actions without input from a remote pilot. This would ensure the aircraft safely navigates the airport environment even if the remote pilot is supervising multiple aircraft or their response is delayed. NASA researchers are beginning to test emerging technologies for remotely piloted aircraft operations with commercial partners. The goal is to help mature technical standards and assist in the development of certification requirements anrtd procedures required to integrate remotely piloted operations into the airspace. NASA aims to bridge technical and regulatory gaps through these industry partnerships involving research, testing, and development. Ultimately, NASA hopes to enable pilots to remotely fly multiple large aircraft to airports across the country at once, more efficiently transporting people and goods. This could enable carriers to meet rising air travel and transport demands in a safe, affordable, scalable way and expand access to new communities. PAAV is a subproject under NASA’s Air Traffic Management Exploration project within the agency’s Aeronautics Research Mission Directorate. Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More 4 min read NASA Kicks off Testing Campaign for Remotely Piloted Cargo Flights Article 2 months ago 2 min read NASA Flight Rerouting Tool Curbs Delays, Emissions Article 3 months ago 3 min read NASA Moves Drone Package Delivery Industry Closer to Reality Article 3 months ago Keep Exploring Discover More Topics From NASA Missions Artemis Aeronautics STEM Explore NASA’s History View the full article

3 Min Read NASA, Partners to Conduct Space Station Research During Expedition 73 NASA NASA astronauts are gearing up for a scientific mission aboard the International Space Station. Expedition 73 NASA astronauts Nichole Ayers and Anne McClain, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov will launch in March as part of the agency’s SpaceX Crew-10 mission. NASA astronaut Jonny Kim will join the crew when he launches aboard the Roscosmos Soyuz MS-27 spacecraft in April alongside Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky. Read more about some of the microgravity research planned by NASA and its partners: Subjects for human research NASA Astronauts often serve as test subjects, submitting blood and other samples for research. NASA astronaut Anne McClain is pictured submitting a sample on a previous mission with assistance from CSA (Canadian Space Agency) astronaut David Saint-Jacques. McClain will participate in NASA’s Complement of Integrated Protocols for Human Exploration Research investigation, or CIPHER, a suite of integrated studies on physiological and psychological changes seen in space. Results could provide valuable insights for future deep space missions. Testing lunar navigation NASA When Expedition 73 astronauts engage with students worldwide via the ISS Ham Radio program, researchers will use the ham radio hardware to test software for the Navigation and Communication Testbed (NAVCOM) that could help shape future lunar navigation. Researchers from the investigation recently launched a related study to the Moon aboard Firefly’s Blue Ghost to help bridge existing Earth navigation with emerging lunar-specific solutions. Advancing fire safety NASA Expedition 73 is scheduled to conduct a Material Ignition and Suppression Test (SoFIE-MIST), testing material flammability in microgravity. This research could improve fire safety on future missions, contributing to models used to select materials for space facilities and helping to determine the best ways to extinguish fires in space. Keeping blood flowing Angelo Taibi/ASI Expedition 73 crew members will participate in Drain Brain 2.0, which examines how blood flows from the brain to the heart in microgravity using this plethysmograph, a device that can record the volume of blood drainage from the skull. Results could identify which processes in the body compensate for the lack of gravity, helping to ensure proper blood flow for astronauts on future missions and people with cardiovascular issues on Earth. The International Space Station is a convergence of science, technology, and human innovation that enables research not possible on Earth. For more than 24 years, NASA has supported a continuous U.S. human presence aboard the orbiting laboratory, through which astronauts have learned to live and work in space for extended periods of time. The space station is a springboard for developing a low Earth economy and NASA’s next great leaps in exploration, including missions to the Moon under Artemis and, ultimately, human exploration of Mars. Learn more about the International Space Station, its research, and its crew, at: https://www.nasa.gov/station Keep Exploring Discover More Topics From NASA Space Station Research and Technology Humans In Space Space Station Research Results Human Research Program Share Details Last Updated Mar 10, 2025 Related TermsISS ResearchInternational Space Station (ISS) View the full article

On March 6, 1985, NASA’s newest space shuttle, Atlantis, made its public debut during a rollout ceremony at the Rockwell International manufacturing plant in Palmdale, California. Under construction for three years, Atlantis joined NASA’s other three space-worthy orbiters, Columbia, Challenger, and Discovery, and atmospheric test vehicle Enterprise. Officials from NASA, Rockwell, and other organizations attended the rollout ceremony. By the time NASA retired Atlantis in 2011, it had flown 33 missions in a career spanning 26 years and flying many types of missions envisioned for the space shuttle. The Visitor Center at NASA’s Kennedy Space Center in Florida has Atlantis on display. Space shuttle Atlantis under construction at Rockwell International’s Palmdale, California, plant in 1984. Credit/NASA. Atlantis during the rollout ceremony in Palmdale. Credit/NASA. Workers truck Atlantis from Palmdale to NASA’s Dryden, now Armstrong, Flight Research Center. Credit/NASA. On Jan. 25, 1979, NASA announced the names of the first four space-worthy orbiters – Columbia, Challenger, Discovery, and Atlantis. Like the other vehicles, NASA named Atlantis after an historical vessel of discovery and exploration – the Woods Hole Oceanographic Institute’s two-masted research ship Atlantis that operated from 1930 to 1966. On Jan. 29, NASA signed the contract with Rockwell International of Downey, California, to build and deliver Atlantis. Construction began in March 1980 and finished in April 1984. Nearly identical to Discovery but with the addition of hardware to support the cryogenic Centaur upper stage then planned to deploy planetary spacecraft in 1986, plans shelved following the Challenger accident. After a year of testing, workers prepared Atlantis for its public debut. Atlantis arrives at NASA’s Dryden, now Armstrong, Flight Research Center to prepare for its cross-country ferry flight. Credit/NASA. Atlantis during an overnight stop at Ellington Air Force Base, now Ellington Field, in Houston. Credit/NASA. Atlantis arrives at NASA’s Kennedy Space Center in Florida.Credit/NASA. Three days after the rollout ceremony, workers trucked Atlantis 36 miles overland to NASA’s Dryden, now Armstrong, Flight Research Center at Edwards Air Force Base in California’s Mojave Desert, for final preparations for its cross-country ferry flight. In the Mate Demate Device, workers placed Atlantis atop the Shuttle Carrier Aircraft, a modified Boeing 747, to begin the ferry flight. The duo left Edwards on April 12, the fourth anniversary of the first space shuttle flight. Following an overnight stop at Houston’s Ellington Air Force Base, now Ellington Field, Atlantis arrived at NASA’s Kennedy Space Center in Florida on April 13. Atlantis following its first rollout to Launch Pad 39A. Credit/NASA. The flight readiness firing of Atlantis’ three main engines.Credit/NASA. Liftoff of Atlantis on its first mission, STS-51J. Credit/NASA. Four months later, on Aug. 12, workers towed Atlantis from the processing facility to the assembly building and mated it to an external tank and twin solid rocket boosters. The entire stack rolled out to Launch Pad 39A on Aug. 30 in preparation for the planned Oct. 3 launch of the STS-51J mission. As with any new orbiter, on Sept. 13 NASA conducted a 20-second Flight Readiness Firing of Atlantis’ three main engines. On Sept. 16, the five-person crew participated in a countdown demonstration test, leading to an on time Oct. 3 launch. Atlantis had joined the shuttle fleet and begun its first mission to space. Space shuttle Atlantis in the Visitor Center at NASA’s Kennedy Space Center in Florida. Credit/NASA. Over the course of its 33 missions spanning more than 26 years, Atlantis flew virtually every type of mission envisioned for the space shuttle, including government and commercial satellite deployments, deploying spacecraft to visit interplanetary destinations, supporting scientific missions, launching and servicing scientific observatories such as the Hubble Space Telescope, performing crew rotations and resupplying the Mir space station, and assembling and maintaining the International Space Station. Atlantis flew the final mission of the shuttle program, STS-135, in July 2011. The following year, NASA transported Atlantis to the Kennedy Visitor Center for public display. Explore More 7 min read 40 Years Ago: Space Shuttle Discovery Makes its Public Debut Article 1 year ago 14 min read 40 Years Ago: STS-4, Columbia’s Final Orbital Flight Test Article 3 years ago 6 min read 45 Years Ago: Space Shuttle Enterprise Makes its Public Debut Article 3 years ago View the full article

Photo Credit: United Launch Alliance Photo Credit: United Launch Alliance Photo Credit: United Launch Alliance Photo Credit: NASA/Skip Williams NASA received the upper stage for the agency’s Artemis II SLS (Space Launch System) rocket on Mar. 4 supplied by Boeing and United Launch Alliance (ULA). Known as the interim cryogenic propulsion stage, it arrived at the Multi Payload Processing Facility (MPPF) at NASA’s Kennedy Space Center in Florida. The upper stage traveled to the spaceport from ULA’s Delta Operations Center at Cape Canaveral Space Force Station. While at the MPPF, technicians will fuel the SLS upper stage with hydrazine for its reaction control system before transporting it to the center’s Vehicle Assembly Building for integration with SLS rocket elements atop mobile launcher 1. The rocket’s solid rocket booster segments are already assembled for launch and the core stage soon will be integrated, as will the launch vehicle stage adapter. The upper stage will be mated to the adapter. The four-story propulsion system is powered by an RL10 engine, which will provide Orion with the boost it needs to orbit Earth twice before venturing toward the Moon. Photo Credit: United Launch Alliance and NASA/Skip Williams View the full article

NASA/JPL-Caltech/UCLA/MPS/DLR/IDA NASA’s Dawn spacecraft took this image of Ceres’ south polar region on May 17, 2017. Launched on Sept. 27, 2007, Dawn was NASA’s first truly interplanetary spaceship. The mission featured extended stays at two extraterrestrial bodies: giant asteroid Vesta and dwarf planet Ceres, both in the debris-strewn main asteroid belt between Mars and Jupiter. The spacecraft’s name was meant to present a simple view of the mission’s purpose: to provide information on the dawn of the solar system. The three principal scientific drivers for the mission were to capture the earliest moments in the origin of the solar system, determine the nature of the building blocks from which the terrestrial planets formed, and contrast the formation and evolution of two small planets that followed very different evolutionary paths. Dawn completed the first order exploration of the inner solar system, addressed NASA’s goal of understanding the origin and evolution of the solar system, and complemented investigations of Mercury, Earth, and Mars. Dawn’s mission ended on Nov. 1, 2018, after two extended missions. Follow Dawn’s journey from Earth to deep space through the words of mission director and chief engineer, Dr. Marc Rayman. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA View the full article

The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) Jessica Kong, Josh Alwood, and Sam Kim. Their commitment to the NASA mission represents the entrepreneurial spirit, technical expertise, and collaborative disposition needed to explore this world and beyond. Space Science and Astrobiology Star: Jessica Kong Jessica Kong is serving as the Facility Service Manager (FSM) for the Astrobiology and Life Science Lab building for the Exobiology Branch while the FSM is away on parental leave. She has applied her expertise as a chemist to connect seamlessly and effectively with N239 staff, and safety, and facility personnel, as well as to coordinate repairs and building shutdowns while minimizing disruption to laboratory research. Space Biosciences Star: Josh Alwood Josh Alwood is a researcher for the Space Biosciences Research Branch, focusing on bone biology and biomechanics, reproductive biology, and the nervous system. His pioneering research on molecular mechanisms of skeletal adaptation during spaceflight has advanced the development of countermeasures to protect astronaut health on long-duration missions. Earth Science Star: Sam Kim Sam Kim, a systems administrator and deputy project manager with the Earth Science Project Office (ESPO), serves many roles and excels in each one of them. During the 2024 ASIA-AQ field mission, Sam deployed for over two months as a key member of the advanced staging team at each of the mission’s four overseas field sites, ensuring that the facilities were ready for the arrival of the ASIA-AQ science and instrument team, while still performing his mission-critical role as systems administrator. View the full article

Explore This Section Webb News Latest News Latest Images Blog (offsite) Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 6 Min Read NASA’s Webb Peers Deeper into Mysterious Flame Nebula This collage of images from the Flame Nebula shows a near-infrared light view from NASA’s Hubble Space Telescope on the left, while the two insets at the right show the near-infrared view taken by NASA’s James Webb Space Telescope. Credits: NASA, ESA, CSA, M. Meyer (University of Michigan), A. Pagan (STScI) The Flame Nebula, located about 1,400 light-years away from Earth, is a hotbed of star formation less than 1 million years old. Within the Flame Nebula, there are objects so small that their cores will never be able to fuse hydrogen like full-fledged stars—brown dwarfs. Brown dwarfs, often called “failed stars,” over time become very dim and much cooler than stars. These factors make observing brown dwarfs with most telescopes difficult, if not impossible, even at cosmically short distances from the Sun. When they are very young, however, they are still relatively warmer and brighter and therefore easier to observe despite the obscuring, dense dust and gas that comprises the Flame Nebula in this case. NASA’s James Webb Space Telescope can pierce this dense, dusty region and see the faint infrared glow from young brown dwarfs. A team of astronomers used this capability to explore the lowest mass limit of brown dwarfs within the Flame Nebula. The result, they found, were free-floating objects roughly two to three times the mass of Jupiter, although they were sensitive down to 0.5 times the mass of Jupiter. “The goal of this project was to explore the fundamental low-mass limit of the star and brown dwarf formation process. With Webb, we’re able to probe the faintest and lowest mass objects,” said lead study author Matthew De Furio of the University of Texas at Austin. Image A: Flame Nebula: Hubble and Webb Observations This collage of images from the Flame Nebula shows a near-infrared light view from NASA’s Hubble Space Telescope on the left, while the two insets at the right show the near-infrared view taken by NASA’s James Webb Space Telescope. Much of the dark, dense gas and dust, as well as the surrounding white clouds within the Hubble image, have been cleared in the Webb images, giving us a view into a more translucent cloud pierced by the infrared-producing objects within that are young stars and brown dwarfs. Astronomers used Webb to take a census of the lowest-mass objects within this star-forming region. The Hubble image on the left represents light at wavelengths of 1.05 microns (filter F105W) as blue, 1.3 microns (F130N) as green, and 1.39 microns (F129M) as red. The two Webb images on the right represent light at wavelengths of 1.15 microns and 1.4 microns (filters F115W and F140M) as blue, 1.82 microns (F182M) as green, 3.6 microns (F360M) as orange, and 4.3 microns (F430M) as red. NASA, ESA, CSA, M. Meyer (University of Michigan), A. Pagan (STScI) Smaller Fragments The low-mass limit the team sought is set by a process called fragmentation. In this process large molecular clouds, from which both stars and brown dwarfs are born, break apart into smaller and smaller units, or fragments. Fragmentation is highly dependent on several factors with the balance between temperature, thermal pressure, and gravity being among the most important. More specifically, as fragments contract under the force of gravity, their cores heat up. If a core is massive enough, it will begin to fuse hydrogen. The outward pressure created by that fusion counteracts gravity, stopping collapse and stabilizing the object (then known as a star). However, fragments whose cores are not compact and hot enough to burn hydrogen continue to contract as long as they radiate away their internal heat. “The cooling of these clouds is important because if you have enough internal energy, it will fight that gravity,” says Michael Meyer of the University of Michigan. “If the clouds cool efficiently, they collapse and break apart.” Fragmentation stops when a fragment becomes opaque enough to reabsorb its own radiation, thereby stopping the cooling and preventing further collapse. Theories placed the lower limit of these fragments anywhere between one and ten Jupiter masses. This study significantly shrinks that range as Webb’s census counted up fragments of different masses within the nebula. “As found in many previous studies, as you go to lower masses, you actually get more objects up to about ten times the mass of Jupiter. In our study with the James Webb Space Telescope, we are sensitive down to 0.5 times the mass of Jupiter, and we are finding significantly fewer and fewer things as you go below ten times the mass of Jupiter,” De Furio explained. “We find fewer five-Jupiter-mass objects than ten-Jupiter-mass objects, and we find way fewer three-Jupiter-mass objects than five-Jupiter-mass objects. We don’t really find any objects below two or three Jupiter masses, and we expect to see them if they are there, so we are hypothesizing that this could be the limit itself.” Meyer added, “Webb, for the first time, has been able to probe up to and beyond that limit. If that limit is real, there really shouldn’t be any one-Jupiter-mass objects free-floating out in our Milky Way galaxy, unless they were formed as planets and then ejected out of a planetary system.” Image B: Low Mass Objects within the Flame Nebula in Infrared Light This near-infrared image of a portion of the Flame Nebula from NASA’s James Webb Space Telescope highlights three low-mass objects, seen in the insets to the right. These objects, which are much colder than protostars, require the sensitivity of Webb’s instruments to detect them. These objects were studied as part of an effort to explore the lowest mass limit of brown dwarfs within the Flame Nebula. The Webb images represent light at wavelengths of 1.15 microns and 1.4 microns (filters F115W and F140M) as blue, 1.82 microns (F182M) as green, 3.6 microns (F360M) as orange, and 4.3 microns (F430M) as red. NASA, ESA, CSA, STScI, M. Meyer (University of Michigan) Building on Hubble’s Legacy Brown dwarfs, given the difficulty of finding them, have a wealth of information to provide, particularly in star formation and planetary research given their similarities to both stars and planets. NASA’s Hubble Space Telescope has been on the hunt for these brown dwarfs for decades. Even though Hubble can’t observe the brown dwarfs in the Flame Nebula to as low a mass as Webb can, it was crucial in identifying candidates for further study. This study is an example of how Webb took the baton—decades of Hubble data from the Orion Molecular Cloud Complex—and enabled in-depth research. “It’s really difficult to do this work, looking at brown dwarfs down to even ten Jupiter masses, from the ground, especially in regions like this. And having existing Hubble data over the last 30 years or so allowed us to know that this is a really useful star-forming region to target. We needed to have Webb to be able to study this particular science topic,” said De Furio. “It’s a quantum leap in our capabilities between understanding what was going on from Hubble. Webb is really opening an entirely new realm of possibilities, understanding these objects,” explained astronomer Massimo Robberto of the Space Telescope Science Institute. This team is continuing to study the Flame Nebula, using Webb’s spectroscopic tools to further characterize the different objects within its dusty cocoon. “There’s a big overlap between the things that could be planets and the things that are very, very low mass brown dwarfs,” Meyer stated. “And that’s our job in the next five years: to figure out which is which and why.” These results are accepted for publication in The Astrophysical Journal Letters. Image C (Animated): Flame Nebula (Hubble and Webb Comparison) This animated image alternates between a Hubble Space Telescope and a James Webb Space Telescope observation of the Flame Nebula, a nearby star-forming nebula less than 1 million years old. In this comparison, three low-mass objects are highlighted. In Hubble’s observation, the low-mass objects are hidden by the region’s dense dust and gas. However, the objects are brought out in the Webb observation due to Webb’s sensitivity to faint infrared light. NASA, ESA, CSA, Alyssa Pagan (STScI) The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency). Downloads Click any image to open a larger version. View/Download all image products at all resolutions for this article from the Space Telescope Science Institute. Media Contacts Laura Betz – laura.e.betz@nasa.gov NASA’s Goddard Space Flight Center, Greenbelt, Md. Matthew Brown – mabrown@stsci.edu Space Telescope Science Institute, Baltimore, Md. Christine Pulliam – cpulliam@stsci.edu Space Telescope Science Institute, Baltimore, Md. Related Information More Webb News More Webb Images Webb Science Themes Webb Mission Page Learn more about brown dwarf discoveries Related For Kids What is the Webb Telescope? SpacePlace for Kids En Español Ciencia de la NASA NASA en español Space Place para niños Keep Exploring Related Topics James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Universe Universe Stories Stars Stories Share Details Last Updated Mar 10, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms James Webb Space Telescope (JWST) Astrophysics Brown Dwarfs Goddard Space Flight Center Science & Research Star-forming Nebulae The Universe View the full article

Will you design the zero gravity indicator (ZGI) that accompanies the Artemis II mission around the Moon? If your design is one of the most compelling and resonates with the global community and the Artemis II astronauts, your design might fly into space aboard the Orion spacecraft and you could win US$1225. Zero gravity indicators are small items carried aboard spacecraft that provide a visual indicator for when a spacecraft has reached the weightlessness of microgravity. A plush Snoopy doll was the ZGI for the Artemis I mission. For that uncrewed mission, Snoopy floated around, tethered inside the vehicle to indicate when the Orion spacecraft had reached space. For this Challenge, we’re asking creatives from all over the world to design a new ZGI to be fabricated by NASA’s Thermal Blanket Lab and launched into space aboard the Artemis II mission. Award: $23,275 in total prizes Open Date: March 7, 2025 Close Date: May 27, 2025 For more information, visit: https://www.freelancer.com/contest/Moon-Mascot-NASA-Artemis-II-ZGI-Design-Challenge-2527909/details View the full article

Challenges to measuring space-induced brain changes CSA (Canadian Space Agency) astronaut David Saint-Jacques undergoes an MRI for Wayfinding. CSA Researchers found that an upward shift in the brain during spaceflight makes it hard to distinguish different types of tissue, causing errors in determining changes in brain volume. Previous studies have interpreted these changes as evidence of adaptation to space. This finding suggests that unique methods are needed to analyze astronaut brain structure. Wayfinding, a CSA (Canadian Space Agency) investigation, looked at how the brain adapts to space and readapts after return to normal gravity using a variety of assessments, including neuroimaging. The researchers propose that previous data could be reanalyzed based on the errors identified by this paper. Catching micrometeoroids JAXA’s (Japan Aerospace Exploration Agency) Tanpopo panels were mounted on the Exposed Experiment Handrail Attachment Mechanism (ExHAM) at top center of this image. JAXA/Takuya Onishi An impact track made by a micrometeoroid on a panel outside the International Space Station contained iron and orthopyroxene crystals. This finding, along with previous studies, suggests that micrometeoroids containing these elements are abundant in low Earth orbit and more measurements are needed to determine their origins and potential for carrying life. At least 90% of meteoroids at one astronomical unit or AU (93 million miles or the distance between Earth and the Sun) do not reach Earth’s surface, so investigating those in low Earth orbit is key to understanding their nature. The JAXA (Japan Aerospace Exploration Agency) Tanpopo experiment placed blocks of a special gel outside the station to capture solid microparticles to test the theory that they could transport life among celestial bodies. Most meteoroids at one AU may have originated from Jupiter family comets. View the full article

James Gentile always wanted to fly. As he prepared for an appointment to the U.S. Air Force Academy to become a pilot, life threw him an unexpected curve: a diagnosis of Type 1 diabetes. His appointment was rescinded. With his dream grounded, Gentile had two choices—give up or chart a new course. He chose the latter, pivoting to aerospace engineering. If he could not be a pilot, he would design the flight simulations that trained those who could. Official portrait of James Gentile. NASA/Robert Markowitz As a human space vehicle simulation architect at NASA’s Johnson Space Center in Houston, Gentile leads the Integrated Simulation team, which supports the Crew Compartment Office within the Simulation and Graphics Branch. He oversees high-fidelity graphical simulations that support both engineering analysis and flight crew training for the Artemis campaign. His team provides critical insight into human landing system vendor designs, ensuring compliance with NASA’s standards. They also develop human-in-the-loop simulations to familiarize teams with the challenges of returning humans to the lunar surface, optimizing design and safety for future space missions. “I take great pride in what I have helped to build, knowing that some of the simulations I developed have influenced decisions for the Artemis campaign,” Gentile said. One of the projects he is most proud of is the Human Landing System CrewCo Lander Simulation, which helps engineers and astronauts tackle the complexities of lunar descent, ascent, and rendezvous. He worked his way up from a developer to managing and leading the project, transforming a basic lunar lander simulation into a critical tool for the Artemis campaign. What began as a simple model in 2020 is now a key training asset used in multiple facilities at Johnson. The simulation evaluates guidance systems and provides hands-on piloting experience for lunar landers. James Gentile in the Simulation Exploration and Analysis Lab during a visit with Apollo 16 Lunar Module Pilot Charlie Duke. From left to right: Katie Tooher, Charlie Duke, Steve Carothers, Mark Updegrove, and James Gentile. NASA/James Blair Before joining Johnson as a contractor in 2018, Gentile worked in the aviation industry developing flight simulations for pilot training. Transitioning to the space sector was challenging at first, particularly working alongside seasoned professionals who had been part of the space program for years. “I believe my experience in the private sector has benefited my career,” he said. “I’ve been able to bring a different perspective and approach to problem-solving that has helped me advance at Johnson.” Gentile attributes his success to never being afraid to speak up and ask questions. “You don’t always have to be the smartest person in the room to make an impact,” he said. “I’ve been able to show my value through my work and by continuously teaching myself new skills.” As he helps train the Artemis Generation, Gentile hopes to pass on his passion for aerospace and simulation development, inspiring others to persevere through obstacles and embrace unexpected opportunities. “The most important lessons I’ve learned in my career are to build and maintain relationships with your coworkers and not to be afraid to step out of your comfort zone,” he said. James Gentile with his son at NASA’s Johnson Space Center during the 2024 Bring Youth to Work Day. His journey did not go as planned, but in the end, it led him exactly where he was meant to be—helping humanity take its next giant leap. “I’ve learned that the path to your goals may not always be clear-cut, but you should never give up on your dreams,” Gentile said. View the full article

Explore Hubble 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 Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read Hubble Unveils a Glittering View of Sh2-284 Hubble’s infrared view of emission nebula Sh2-284 provides a glimpse of the brilliant young stars hidden within clouds of gas and dust. Credit: NASA, ESA, and M. Andersen (European Southern Observatory – Germany); Processing: Gladys Kober (NASA/Catholic University of America) Download this image A tiny fraction of the stellar nursery known as Sh2-284 is visible in this glittering, star-filled NASA Hubble Space Telescope image. This immense region of gas and dust is the birthing place of stars, which shine among the clouds. Bright clusters of newborn stars glow pink in infrared light, and clouds of gas and dust, resembling puffy cumulus clouds, are dotted with dark knots of denser dust. This image shows an infrared view from Hubble, giving an excellent view of the stars that might otherwise be obscured by Sh2-284’s clouds. Unlike visible light, infrared wavelengths can travel through clouds of gas and dust, providing a glimpse of the stars forming within the obscuring clouds. The nebula is shaped by a young central star cluster, Dolidze 25 (not visible in the Hubble image), whose stars range from 1.5 to 13 million years old (our Sun, in contrast, is 4.6 billion years old). The cluster blasts out ionizing winds and radiation, pushing at the gas and dust of the nebula and carving out intricate shapes and pillars, as seen in detail here. This ionizing radiation gives Sh2-284 its classification as an HII region, an emission nebula consisting primarily of ionized hydrogen. An emission nebula like Sh2-284 glows with its own light as stars within or nearby energize its gas with a flood of intense ultraviolet radiation. The ground-based image (top) of M24 shows the location of the Hubble view (bottom). The European Southern Observatory’s visible-light image shows prominent clouds of gas and dust, while the Hubble image’s infrared vision highlights the stars within and behind the clouds. Ground-based image: ESO/VPHAS+ Team; Hubble image: NASA, ESA, and M. Andersen (European Southern Observatory – Germany); Processing: Gladys Kober (NASA/Catholic University of America) Sh2-284 is also a low-metallicity region, which means it is poor in elements heavier than hydrogen and helium. These conditions mimic the early universe, when matter was mostly helium and hydrogen and heavier elements were just beginning to form via nuclear fusion within massive stars. Hubble took these images as part of an effort to examine how low metallicity influences stellar formation and how this would apply to the early universe. Sh2-284 resides 15,000 light-years away at the end of an outer spiral arm of our Milky Way galaxy, in the constellation Monoceros. Explore More Hubble’s Nebulae Exploring the Birth of Stars Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, MD claire.andreoli@nasa.gov Share Details Last Updated Mar 08, 2025 Location NASA Goddard Space Flight Center Related Terms Hubble Space Telescope Astrophysics Astrophysics Division Emission Nebulae Goddard Space Flight Center Nebulae Star-forming Nebulae 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. Hubble’s Cosmic Adventure Hubble’s Night Sky Challenge Hubble’s 35th Anniversary View the full article

Explore Hubble 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 Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 3 min read Hubble Jams With A Cosmic Guitar Elliptical galaxy NGC 3561B (upper left) and spiral galaxy NGC 3561A (lower right) form a shimmering guitar shape in the ongoing merger known collectively as Arp 105. NASA, ESA and M. West (Lowell Observatory); Processing: Gladys Kober (NASA/Catholic University of America) Arp 105 is a dazzling ongoing merger between an elliptical galaxy and a spiral galaxy drawn together by gravity, characterized by a long, drawn out tidal tail of stars and gas more than 362,000 light-years long. The immense tail, which extends beyond this image from NASA’s Hubble Space Telescope, was pulled from the two galaxies by their gravitational interactions and is embedded with star clusters and dwarf galaxies. The distinctively shaped arrangement of galaxies and tail gives the grouping its nickname: The Guitar. The gravitational dance between elliptical galaxy NGC 3561B and spiral galaxy NGC 3561A creates a wealth of fascinating colliding galaxy features. A long lane of dark dust emerging from the elliptical galaxy ends in, and may be feeding, a bright blue area of star formation on the base of the guitar known as Ambartsumian’s Knot. Ambartsumian’s Knot is a tidal dwarf galaxy, a type of star-forming system that develops from the debris in tidal arms of interacting galaxies. Two more bright blue areas of star formation are obvious in the Hubble image at the edges of the distorted spiral galaxy. The region to the left in the spiral galaxy is likely very similar to Ambartsumian’s Knot, a knot of intense star formation triggered by the merger. The region to the right is still under investigation ― it could be part of the collision, but its velocity and spectral data (indicating distance) are different from the rest of the system, so it may be a foreground galaxy. Thin, faint tendrils of gas and dust are just barely visible stretching between and connecting the two galaxies. These tendrils are particularly interesting to astronomers since they may help define the timescale of the evolution of this collision. A multitude of more-distant background galaxies are visible around and even through this merging duo. The bright blue blob of stars to the left of Ambartsumian’s Knot may be a particularly bright background galaxy. Arp 105 is one of the brightest objects in the crowded galaxy cluster Abell 1185 in the constellation Ursa Major. Abell 1185, located around 400 million light-years away, is a chaotic cluster of at least 82 galaxies, many of which are interacting, as well as a number of wandering globular clusters that are not gravitationally attached to any particular galaxy. This Hubble image was taken as part of a study of the ongoing creation of galactic and intergalactic stellar populations in Abell 1185. Explore More Hubble’s Galaxies Galaxy Details and Mergers Hubble Focus E-Book: Galaxies through Space and Time Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli (claire.andreoli@nasa.gov) NASA’s Goddard Space Flight Center, Greenbelt, MD Share Details Last Updated Mar 08, 2025 Editor NASA Hubble Mission Team Location NASA Goddard Space Flight Center Related Terms Goddard Space Flight Center Astrophysics Astrophysics Division Elliptical Galaxies Hubble Space Telescope Interacting Galaxies Spiral Galaxies 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. Hubble’s Partners in Science Hubble’s Night Sky Challenge Hubble’s Galaxies View the full article

Explore Hubble 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 Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read Hubble Spies a Spectacular Starburst Galaxy Starburst spiral NGC 4536 is bright with blue clusters of star formation and pink clumps of ionized hydrogen. NASA, ESA, and J. Lee (Space Telescope Science Institute); Processing: Gladys Kober (NASA/Catholic University of America) Sweeping spiral arms extend from NGC 4536, littered with bright blue clusters of star formation and red clumps of hydrogen gas shining among dark lanes of dust. The galaxy’s shape may seem a little unusual, and that’s because it’s what’s known as an “intermediate galaxy”: not quite a barred spiral, but not exactly an unbarred spiral, either ― a hybrid of the two. NGC 4536 is also a starburst galaxy, in which star formation is happening at a tremendous rate that uses up the gas in the galaxy relatively quickly, by galactic standards. Starburst galaxies can happen due to gravitational interactions with other galaxies or ― as seems to be the case for NGC 4536 ― when gas is packed into a small region. The bar-like structure of NGC 4536 may be driving gas inwards toward the nucleus, giving rise to a crescendo of star formation in a ring around the nucleus. Starburst galaxies birth lots of hot blue stars that burn fast and die quickly in explosions that unleash intense ultraviolet light (visible in blue), turning their surroundings into glowing clouds of ionized hydrogen, called HII regions (visible in red). NGC 4536 is approximately 50 million light-years away in the constellation Virgo. It was discovered in 1784 by astronomer William Herschel. Hubble took this image of NGC 4536 as part of a project to study galactic environments to understand connections between young stars and cold gas, particularly star clusters and molecular clouds, throughout the local universe. Download the image Explore More Hubble’s Galaxies Galaxy Details and Mergers Hubble Focus E-Book: Galaxies through Space and Time Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, MD claire.andreoli@nasa.gov Share Details Last Updated Mar 08, 2025 Location NASA Goddard Space Flight Center Related Terms Hubble Space Telescope Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Spiral Galaxies 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. Hubble’s Cosmic Adventure Hubble’s Night Sky Challenge Hubble’s 35th Anniversary View the full article

Explore Hubble 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 Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read Hubble Examines Stars Ensconced in a Cocoon of Gas NGC 460 is an open cluster of stars within a greater collection of nebulae and star clusters known as the N83-84-85 complex. NASA, ESA, and C. Lindberg (The Johns Hopkins University); Processing: Gladys Kober (NASA/Catholic University of America) Download this image An open cluster of stars shines through misty, cocoon-like gas clouds in this Hubble Space Telescope image of NGC 460. NGC 460 is located in a region of the Small Magellanic Cloud, a dwarf galaxy that orbits the Milky Way. This particular region contains a number of young star clusters and nebulae of different sizes ― all likely related to each other. The clouds of gas and dust can give rise to stars as portions of them collapse, and radiation and stellar winds from those hot, young bright stars in turn shape and compress the clouds, triggering new waves of star formation. The hydrogen clouds are ionized by the radiation of nearby stars, causing them to glow. The NGC 460 star cluster resides in one of the youngest parts of this interconnected complex of stellar clusters and nebulae, which is also home to a number of O-type stars: the brightest, hottest and most massive of the normal, hydrogen-burning stars (called main-sequence stars) like our Sun. O-type stars are rare ― out of more than 4 billion stars in the Milky Way, only about 20,000 are estimated to be O-type stars. The area that holds NGC 460, known as N83, may have been created when two hydrogen clouds in the region collided with one another, creating several O-type stars and nebulae. Open clusters like NGC 460 are made of anywhere from a few dozen to a few thousand stars loosely knitted together by gravity. Open clusters generally contain young stars, which may migrate outward into their galaxies as time progresses. NGC 460’s stars may someday disperse into the Small Magellanic Cloud, one of the Milky Way’s closest galactic neighbors at about 200,000 light-years away. Because it is both close and bright, it offers an opportunity to study phenomena that are difficult to examine in more distant galaxies. Six overlapping observations from a study of the gas and dust between stars, called the interstellar medium, were combined to create this Hubble image. The study aims to understand how gravitational forces between interacting galaxies can foster bursts of star formation. This highly detailed 65 megapixel mosaic includes both visible and infrared wavelengths. Download the 400 MB file and zoom in to see some of the intricacies captured by Hubble. Explore More Hubble’s Star Clusters Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, MD claire.andreoli@nasa.gov Share Details Last Updated Mar 08, 2025 Location NASA Goddard Space Flight Center Related Terms Hubble Space Telescope Astrophysics Astrophysics Division Goddard Space Flight Center Magellanic Clouds Star Clusters 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. Hubble’s Cosmic Adventure Hubble’s Night Sky Challenge Hubble’s 35th Anniversary View the full article

NASA’s SpaceX Crew-9 Scientific Mission Aboard the Space Station

NASA’s Worm logo is displayed in front of the agency’s headquarters in Washington.Credit: NASA For the 13th straight year, NASA has earned the title of Best Place to Work in the Federal Government – large agency – from the Partnership for Public Service. The ranking reflects employee satisfaction and workplace elements across the agency while executing NASA’s mission to explore the unknown and discover new knowledge for the benefit of humanity. “NASA’s greatest asset has always been its people – those who rise to the challenge of leading in air and space,” said NASA acting Administrator Janet Petro. “This recognition reflects a culture of collaboration, innovation, and excellence that fuels our mission every day and defines NASA as the best place to work in the federal government. I’m honored to lead this remarkable team as we continue benefiting humanity and inspiring the world in the process.” Throughout 2024, NASA’s workforce supported the agency’s groundbreaking accomplishments, including landing new science and technology on the Moon with an American company for the first time and launching a new mission to study Jupiter’s icy moon Europa. NASA teams also collaborated to maintain more than 24 years of continuous human exploration and scientific research aboard the International Space Station and unveiled its supersonic quiet aircraft. The agency also shared the wonder of a total eclipse with millions of Americans, conducted the final flight of its Ingenuity helicopter on Mars, and announced the newest class of Artemis Generation astronauts. With the release of its latest Economic Impact Report, NASA demonstrated how its work impacts the U.S. economy, creates value to society, and returns investment to taxpayers. The Partnership for Public Service began to compile the Best Places to Work rankings in 2003 to analyze federal employee’s viewpoints of leadership, work-life balance, and other factors of their job. A formula is used to evaluate employee responses to a federal survey, dividing submissions into four groups: large, midsize, and small agencies, in addition to their subcomponents. Read about the Best Places to Work for 2024 online. To learn more about NASA’s missions, visit: https://www.nasa.gov -end- Share Details Last Updated Mar 07, 2025 Related TermsPeople of NASALife at NASAMissionsNASA Centers & Facilities View the full article

6 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Ahead of launch, NASA’s SPHEREx is enclosed in a payload fairing at Vandenberg Space Force Base on March 2. The observatory is stacked atop the four small satellites that make up the agency’s PUNCH mission.NASA/BAE Systems/Benjamin Fry NASA’s latest space observatory is targeting a March 8 liftoff, and the agency’s PUNCH heliophysics mission is sharing a ride. Here’s what to expect during launch and beyond. In a little over a day, NASA’s SPHEREx space telescope is slated to launch from Vandenberg Space Force Base in California aboard a SpaceX Falcon 9 rocket. The observatory will map the entire celestial sky four times in two years, creating a 3D map of over 450 million galaxies. In doing so, the mission will provide insight into what happened a fraction of a second after the big bang, in addition to searching interstellar dust for the ingredients of life, and measuring the collective glow from all galaxies, including ones that other telescopes cannot easily detect. The launch window opens at 7:09:56 p.m. PST on Saturday, March 8, with a target launch time of 7:10:12 p.m. PST. Additional opportunities occur in the following days. Launching together into low Earth orbit, NASA’s SPHEREx and PUNCH missions will study a range of topics from the early universe to our nearest star. NASA/JPL-Caltech Sharing a ride with SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) is NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere), a constellation of four small satellites that will map the region where the Sun’s outer atmosphere, the corona, transitions to the solar wind, the constant outflow of material from the Sun. For the latest on PUNCH, visit the blog: https://blogs.nasa.gov/punch What SPHEREx Will Do The SPHEREx observatory detects infrared light — wavelengths slightly longer than what the human eye can see that are emitted by warm objects including stars and galaxies. Using a technique called spectroscopy, SPHEREx will separate the infrared light emitted by hundreds of millions of stars and galaxies into 102 individual colors — the same way a prism splits sunlight into a rainbow. Observing those colors separately can reveal various properties of objects, including their composition and, in the case of galaxies, their distance from Earth. No other all-sky survey has performed spectroscopy in so many wavelengths and on so many sources. The mission’s all-sky spectroscopic map can be used for a wide variety of science investigations. In particular, SPHEREx has its sights set on a phenomenon called inflation, which caused the universe to expand a trillion-trillionfold in a fraction of a second after the big bang. This nearly instantaneous event left an impression on the large-scale distribution of matter in the universe. The mission will map the distribution of more than 450 million galaxies to improve scientists’ understanding of the physics behind this extreme cosmic event. SPHEREx Fact Sheet Additionally, the space telescope will measure the total glow from all galaxies, including ones that other telescopes cannot easily detect. When combined with studies of individual galaxies by other telescopes, the measurement of this overall glow will provide a more complete picture of how the light output from galaxies has changed over the universe’s history. At the same time, spectroscopy will allow SPHEREx to seek out frozen water, carbon dioxide, and other key ingredients for life. The mission will provide an unprecedented survey of the location and abundance of these icy compounds in our galaxy, giving researchers better insight into the interstellar chemistry that set the stage for life. Launch Sequence But, first, SPHEREx has to get into space. Prelaunch testing is complete on the spacecraft’s various systems, and it’s been encapsulated in the protective nose cone, or payload fairing, atop the SpaceX Falcon 9 rocket that will get it there from Vandenberg’s Space Launch Complex-4 East. NASA’s SPHEREx mission will lift off from Space Launch Complex-4 East at Vanden-berg Space Force Base in California aboard a SpaceX Falcon 9 rocket, just as the Sur-face Water and Ocean Topography mission, shown here, did in December 2022. NASA/Keegan Barber A little more than two minutes after the Falcon 9 lifts off, the main engine will cut off. Shortly after, the rocket’s first and second stages will separate, followed by second-stage engine start. The reusable first stage will then begin its automated boost-back burn to the launch site for a propulsive landing. Once the rocket is out of Earth’s atmosphere, about three minutes after launch, the payload fairing that surrounds the spacecraft will separate into two halves and fall back to Earth, landing in the ocean. Roughly 41 minutes after launch, SPHEREx will separate from the rocket and start its internal systems so that it can point its solar panel to the Sun. After this happens, the spacecraft can establish communications with ground controllers at NASA’s Jet Propulsion Laboratory in Southern California, which manages the mission for the agency. This milestone, called acquisition of signal, should happen about three minutes after separation. About 52 minutes after liftoff, PUNCH should separate as well from the Falcon 9. Both spacecraft will be in a Sun-synchronous low Earth orbit, where their position relative to the Sun remains the same throughout the year. Each approximately 98-minute orbit allows the SPHEREx telescope to view a 360-degree strip of the celestial sky. As Earth’s orbit around the Sun progresses, that strip slowly advances, enabling SPHEREx to image almost the entire sky in six months. For PUNCH, the orbit provides a clear view in all directions around the Sun. About four days after launch, SPHEREx should eject the protective cover over its telescope lens. The observatory will begin science operations a little over a month after launch, once the telescope has cooled down to its operating temperature and the mission team has completed a series of checks. NASA’s Launch Services Program, based out of the agency’s Kennedy Space Center in Florida, is providing the launch service for SPHEREx and PUNCH. For more information about the SPHEREx mission, visit: https://www.jpl.nasa.gov/missions/spherex More About SPHEREx SPHEREx is managed by NASA JPL for the agency’s Astrophysics Division within the Science Mission Directorate at NASA Headquarters in Washington. BAE Systems (formerly Ball Aerospace) built the telescope and the spacecraft bus. The science analysis of the SPHEREx data will be conducted by a team of scientists located at 10 institutions in the U.S., two in South Korea, and one in Taiwan. Data will be processed and archived at IPAC at Caltech, which manages JPL for NASA. The mission’s principal investigator is based at Caltech with a joint JPL appointment. The SPHEREx dataset will be publicly available at the NASA-IPAC Infrared Science Archive. Get the SPHEREx Press Kit How to Watch March 8 SPHEREx Launch 6 Things to Know About SPHEREx Why NASA’s SPHEREx Will Make ‘Most Colorful’ Cosmic Map Ever NASA’s SPHEREX Space Telescope Will Seek Life’s Ingredients News Media Contacts Karen Fox / Alise Fisher NASA Headquarters, Washington 202-358-1600 / 202-358-2546 karen.c.fox@nasa.gov / alise.m.fisher@nasa.gov Calla Cofield, SPHEREx Jet Propulsion Laboratory, Pasadena, Calif. 626-808-2469 calla.e.cofield@jpl.nasa.gov Sarah Frazier, PUNCH Goddard Space Flight Center, Greenbelt, Md. 202-853-7191 sarah.frazier@nasa.gov 2025-033 Share Details Last Updated Mar 07, 2025 Related TermsSPHEREx (Spectro-Photometer for the History of the Universe and Ices Explorer)AstrophysicsExoplanetsGalaxiesHeliophysicsJet Propulsion LaboratoryPolarimeter to Unify the Corona and Heliosphere (PUNCH)The Big BangThe Milky WayThe Search for LifeThe SunThe Universe Explore More 5 min read NASA Webb Wows With Incredible Detail in Actively Forming Star System High-resolution near-infrared light captured by NASA’s James Webb Space Telescope shows extraordinary new detail and… Article 6 hours ago 2 min read Hubble Spies a Spiral in the Water Snake This NASA/ESA Hubble Space Telescope image of a vibrant spiral galaxy called NGC 5042 resides… Article 8 hours ago 5 min read NASA Turns Off 2 Voyager Science Instruments to Extend Mission Article 2 days ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

Intuitive Machines’ IM-2 captured an image March 6, 2025, after landing in a crater from the Moon’s South Pole. The lunar lander is on its side about 820 feet from the intended landing site, Mons Mouton. In the center of the image between the two lander legs is the Polar Resources Ice Mining Experiment 1 suite, which shows the drill deployed.Credit: Intuitive Machines Shortly after touching down inside a crater on the Moon, carrying NASA technology and science on its IM-2 mission, Intuitive Machines collected some data for the agency before calling an early end of mission at 12:15 a.m. CST Friday. As part of the company’s second Moon delivery for NASA under the agency’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign, the IM-2 mission included a drill to bring lunar soil to the surface and a mass spectrometer to look for the presence of volatiles, or gases, that could one day help provide fuel or breathable oxygen to future Artemis explorers. Planned to land at Mons Mouton, IM-2 touched down at approximately 11:30 a.m. March 6, more than 1,300 feet (400 meters) from its intended landing site. Intuitive Machines said images collected later confirmed the lander was on its side, preventing it from fully operating the drill and other instruments before its batteries were depleted. The IM-2 mission landed closer to the lunar South Pole than any previous lander. “Our targeted landing site near the lunar South Pole is one of the most scientifically interesting, and geographically challenging locations, on the Moon,” said Nicky Fox, associate administrator for science at NASA Headquarters in Washington. “Each success and setback are opportunities to learn and grow, and we will use this lesson to propel our efforts to advance science, exploration, and commercial development as we get ready for human exploration of Mars.” The Nova-C lander, named Athena, captured and transmitted images of the landing site before activating the technology and science instruments. Among the data collected, NASA’s PRIME-1 (Polar Resources Ice Mining Experiment 1) suite, which includes the lunar drill known as TRIDENT (The Regolith and Ice Drill for Exploring New Terrain), successfully demonstrated the hardware’s full range of motion in the harsh environment of space. The Mass Spectrometer Observing Lunar Operations (MSOLO) as part of the PRIME-1 suite of instruments, detected elements likely due to the gases emitted from the lander’s propulsion system. “While this mission didn’t achieve all of its objectives for NASA, the work that went into the payload development is already informing other agency and commercial efforts,” said Clayton Turner, associate administrator for space technology, NASA Headquarters. “As we continue developing new technologies to support exploration of the Moon and Mars, testing technologies in-situ is crucial to informing future missions. The CLPS initiative remains an instrumental method for achieving this.” Despite the lander’s configuration, Intuitive Machines, which was responsible for launch, delivery, and surface operations under its CLPS contract, was able to complete some instrument checkouts and collect 250 megabytes of data for NASA. “Empowering American companies to deliver science and tech to the Moon on behalf of NASA both produces scientific results and continues development of a lunar economy,” said Joel Kearns, deputy associate administrator for Exploration in the Science Mission Directorate at NASA Headquarters. “While we’re disappointed in the outcome of the IM-2 mission, we remain committed to supporting our commercial vendors as they navigate the very difficult task of landing and operating on the Moon.” NASA’s Laser Retroreflector Array, a passive instrument meant to provide a reference point on the lunar surface and does not power on, will remain affixed to the top deck of the lander. Although Intuitive Machines’ Nova-C Hopper and Nokia’s 4G/LTE Tipping Point technologies, funded in part by NASA, were only able to complete some objectives, they provided insight into maturing technologies ready for infusion into a commercial space application including some checkouts in flight and on the surface. Intuitive Machines’ IM-2 mission launched at 6:16 p.m., Feb. 26, aboard a SpaceX Falcon 9 rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida. Intuitive Machines has two more deliveries on the books for NASA in the future, with its IM-3 mission slated for 2026, and IM-4 mission in 2027. To date, five vendors have been awarded a total of 11 lunar deliveries under CLPS and are sending more than 50 instruments to various locations on the Moon, including the Moon’s far side and South Pole region. CLPS contracts are indefinite-delivery/indefinite-quantity contracts with a cumulative maximum contract value of $2.6 billion through 2028. Learn more about NASA’s CLPS initiative at: https://www.nasa.gov/clps -end- Cheryl Warner / Jasmine Hopkins Headquarters, Washington 202-358-1600 cheryl.m.warner@nasa.gov / jasmine.s.hopkins@nasa.gov Natalia Riusech / Nilufar Ramji Johnson Space Center, Houston 281-483-5111 nataila.s.riusech@nasa.gov / nilufar.ramji@nasa.gov Share Details Last Updated Mar 07, 2025 LocationNASA Headquarters Related TermsCommercial Lunar Payload Services (CLPS)ArtemisEarth's MoonScience & ResearchScience Mission DirectorateSpace Technology Mission Directorate View the full article