NASA

As any urban dweller who has lived through a heat wave knows, a shady tree can make all the difference. But what happens when there’s no shade available? A recent study in Nature Communications used NASA satellite data to identify a major gap in global resilience to climate change: cities in the Global South have far less green space — and therefore less cooling capacity — than cities in the Global North. The terms Global North and Global South were used in the study to distinguish developed countries (mostly in the Northern Hemisphere) from developing nations (mostly in the Southern Hemisphere). Cities tend to be hotter than nearby rural areas because of the urban heat island effect. Heat-trapping dark surfaces such as sidewalks, buildings, and roads absorb heat from the Sun’s rays, which raises the temperature of the city. Extreme heat poses serious health threats for urban residents, including dehydration, heat stroke, and even death. Though not a cure-all, greenery provides shade and releases moisture into the air, cooling the surroundings. “Cities can strategically prioritize developing new green spaces in areas that have less green space,” said Christian Braneon, a climate scientist at NASA’s Goddard Institute for Space Studies in New York who was not affiliated with this study. “Satellite data can be really helpful for this.” The Operational Land Imager (OLI) on the NASA and U.S. Geological Survey’s Landsat 8 satellite captured this natural color image of Sanaa, Yemen, on June 8, 2024. Sanaa, which has a hot, dry climate and little green space, had the second-lowest cooling capacity of 500 cities studied in a paper recently published in the journal Nature Communications. Wanmei Liang, NASA Earth Observatory An international team of researchers led by Yuxiang Li, a doctoral student at Nanjing University, analyzed the 500 largest cities in the world to compare their cooling capacities. They used data from the Landsat 8 satellite, jointly managed by NASA and the U.S. Geological Survey, to determine how effective green space was at cooling each city. First, they calculated the average land surface temperature for the hottest month of 2018 for each city, as well as the average of the hottest months from 2017 to 2019. Next, the researchers used a metric called the Normalized Difference Vegetation Index (NDVI) to map how much green space each city had. The NDVI relies on the fact that healthy vegetation absorbs red light and reflects infrared light: the ratio of these wavelengths can show the density of healthy vegetation in a given satellite image. Researchers found that cities in the Global South have just 70% of the greenery-related cooling capacity of cities in the Global North. The green spaces in an average Global South city cool the temperature by about 4.5 F (2.5 C). In an average Global North city, that cooling capacity is 6.5 F (3.6 C). This compounds an existing problem: cities in the South tend to be at lower latitudes (that is, nearer to the Equator), which are predicted to see more heat extremes in the coming years. “It’s already clear that Global South countries will be impacted by heat waves, rising temperatures, and climatic extremes more than their Global North counterparts,” said Chi Xu, a professor of ecology at Nanjing University and a co-author of the study. The Global South has less capacity to adapt to heat because air conditioning is less common and power outages are more frequent. Why do cities in the Global South struggle to stay cool? Cities in the Global South tend to have less green space than cities in the Global North. This mirrors studies of the disparities within cities, sometimes referred to as the “luxury effect”: wealthier neighborhoods tend to have more green space than poorer neighborhoods. “Wealthier cities also have more urban green spaces than the poorest cities,” Chi said. It’s unlikely that urban planners can close the gap between the study’s worst-performing city (Mogadishu, Somalia) and the best-performing one (Charlotte, North Carolina). Mogadishu is a dense city with a dry climate that limits vegetation growth. Still, there’s a lot that each city can learn from its neighbors. Within a given region, the researchers identified the city with the greatest cooling capacity and used that as a goal. They calculated the difference between the best-performing city in the region and every city nearby to get the potential additional cooling capacity. They found that cities’ average cooling capacity could be increased substantially — to as much as 18 F (10 C) — by systematically increasing green space quantity and quality. “How you utilize green space is really going to vary depending on the climate and the urban environment you’re focused on,” said Braneon, whose research at NASA focuses on climate change and urban planning. Greener cities in the U.S. and Canada have lower population densities. However, fewer people per square mile isn’t necessarily good for the environment: residents in low-density cities rely more on cars, and their houses tend to be bigger and less efficient. Braneon noted that there’s a suite of solutions beyond just planting trees or designating parks: Cities can increase cooling capacity by creating water bodies, seeding green roofs, and painting roofs or pavement lighter colors to reflect more light. With a global study like this, urban planners can compare strategies for cities within the same region or with similar densities. “For newly urbanized areas that aren’t completely built out, there’s a lot of room to still change the design,” Braneon said. By Madeleine Gregory NASA’s Goddard Space Flight Center, Greenbelt, Md. Share Details Last Updated Nov 26, 2024 Editor Rob Garner Contact Rob Garner rob.garner@nasa.gov Location Goddard Space Flight Center Related Terms Climate Change Earth Goddard Institute for Space Studies Goddard Space Flight Center Landsat Landsat 8 / LDCM (Landsat Data Continuity Mission) View the full article

The Texas Art Education Association hosted its annual conference from Nov. 14–16 at Moody Gardens Hotel & Convention Center in Galveston, Texas, drawing nearly 3,000 educators, administrators, and artists. This year’s theme, “Cosmic Connections: SPACE, the Last Frontier and the Element of Art,” celebrated the fusion of creativity and space exploration, with NASA’s Johnson Space Center participating for the first time to inspire the Artemis Generation art educators. Johnson Space Center volunteers Raul Tijerina (left), building graphics lead for the International Space Station Program; Gary Johnson (middle), technical manager in NASA’s International Space Station Mission Integration and Operations Office; and Christian Getteau, Imagery Integration and Multimedia producer with the Human Space Flight Technical Integration Contract, participate in the NASA booth at the Texas Art Education Association annual conference held Nov. 14–16 at Moody Gardens Hotel & Convention Center in Galveston, Texas.NASA From astronauts crafting in orbit to collaborative art projects on Earth, NASA continues to showcase how creativity can capture the wonder of the cosmos. This event allowed educators to connect with NASA, explore teaching resources, and discover innovative ways to merge the arts with science and space exploration in their classrooms. Johnson volunteers pose with an astronaut spacesuit at the Texas Art Education Association conference.NASA/Sumer Loggins “We have seen our astronauts bring the art of painting, music, photography, and more to orbit aboard the space shuttle and the International Space Station,” said Gary Johnson, NASA’s International Space Station Mission Integration and Operations Office technical manager. “Our mission is to inspire the next generation of artists and explorers to capture the beauty of space through any medium they choose.” “Everyone has a place at NASA,” added Raul Tijerina, International Space Station Program building graphics lead. “This collaboration celebrates the diversity of talents needed to explore the universe, including those who bring ideas to life through art.” NASA’s inflatable mascot, Cosmo, greets attendees and poses for photos during the art car show at the conference. NASA Guests immersed themselves in a variety of stellar experiences, including interacting with NASA’s inflatable mascot, Cosmo, taking selfies at the NASA booth, and viewing artwork that shares the past and celebrates the future of space exploration. The nonprofit SciArt Exchange provided teachers with details about its space art competitions, aimed at sparking curiosity across all ages. These competitions include the Project Mars Competition, where adults compete to have their artwork featured at Johnson, and the Moon Youth Art Competition, which highlights lunar-themed creations from students around the world. Attendees also explored infographics and had the chance to download NASA’s Spot the Station app to track the orbiting laboratory in real-time. NASA astronaut Michael Foreman (middle left) and Gordon Andrews, a strategic communications specialist for the International Space Station Program, pose with attendees following a space-themed presentation.NASA Gordon Andrews, a strategic communications specialist for the International Space Station Program, and NASA astronaut Michael Foreman introduced the Spacesuit Art Project to conference attendees. They shared the documentary “Space for Art,” which chronicles the project’s mission to inspire hope, courage, and healing through art. Andrews and Foreman discussed their experiences working on the project with retired NASA astronaut Nicole Stott, the first person to watercolor in space, and the Space for Art Foundation. Foreman shared stories from his time in space and posed for photos with guests. Andrews also presented to the Visual Art Administrators of Texas, a group of over 200 Texas education leaders. The film played at NASA’s booth, showcasing how the initiative brings hope to children undergoing pediatric cancer treatment by inviting them to create colorful spacesuit artwork. Each suit—Hope, Courage, Unity, Victory, Dreamer, Exploration, Beyond, and Infinity—embodies the resilience and imagination of its creators. Four of these spacesuits have journeyed to and from the microgravity laboratory, inspiring children to dream big as they view their artwork in orbit. By raising awareness about pediatric cancer and promoting art therapy worldwide, the project demonstrates the powerful connection between space exploration and the human spirit. The NASA booth featured the Spacesuit Art Project, showcasing a Flat Stanley of NASA astronaut Nicole Stott, the first person to watercolor in space, alongside spacesuits painted by pediatric patients.NASA Texas’ first Space Force Junior Reserve Officers’ Training Corps cadets—the only program of its kind in Texas and one of just 10 in the nation—participated in the event, as well. As a NASA rendition of the National Anthem played in the background, the cadets from Klein High School inspired the next generation of dreamers and doers to reach for the stars. Texas’ first Space Force Junior Reserve Officers’ Training Corps cadets from Klein High School participate in the ceremony as a NASA rendition of the National Anthem plays in the background. NASA The conference also featured three murals that will be added to the art collection in Johnson’s building 4 south. The art installation project began in 2022 when Johnson and Tijerina collaborated with Texas high school art programs to create space-themed murals for display at the center. With the help of their teachers, students brainstormed ideas and painted the murals together before visiting Johnson to install them and experience a guided walk-through of NASA’s facilities. Led by their shared passion for artistic expression and space exploration, the students bring color, wonder, and creativity to the walls at Johnson. The initiative is part of a long-term effort to engage with students locally and globally to ignite the imagination of all and enhance the visual work environment for Johnson employees. “Absolute Equality: Breaking Boundaries” by Reginald C. Adams, symbolizes unity and humanity’s collective future in space exploration. The artwork titled “Absolute Equality: Breaking Boundaries,” by artist Reginald C. Adams, will be one of the latest installations in building 4 south. The piece envisions humanity’s shared future, symbolizing unity and the possibilities of interplanetary exploration. Adams was a keynote speaker for the conference, and when he learned about the mural project, he wanted to contribute to the initiative. The two figures are enclosed within a shared helmet, representing a collective vision for the future of space exploration. The patterns surrounding them signify technology’s role in connecting humanity across cultural and societal divides. La Marque High School students, art teacher Joan Finn, and artist Cheryl Evans painted a mural highlighting the interconnected roles in space exploration. A collaborative piece by La Marque High School art students, art teacher Joan Finn, and artist Cheryl Evans depicted the interconnected roles of visionaries, engineers, artists, and astronauts in space exploration. Just as the space station was assembled piece by piece over more than 40 missions, the mural was created using 10 separate stretched canvases bolted together. The International Space Station patch at the bottom highlights the collaboration of the 17 countries involved. “The Moon Now,” created by La Marque High School students, depicts two astronauts on the lunar surface in Axiom spacesuits with mirrored visors. A student-created vision titled “The Moon Now” showcased two astronauts on the lunar surface wearing Axiom spacesuits, with helmet visors designed as mirrors, signifying the next generation to envision themselves contributing to the next giant leap in space exploration. The students created individual pieces depicting the Milky Way and other astronomical objects, which were collaged onto the surface of the artwork. Through partnerships like this, NASA continues to embrace STEAM—science, technology, engineering, art, and math—to empower the Artemis Generation to dare, unite, and explore. View the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video The Canadarm2 removes materials science samples from the Kibo laboratory module's airlock. NASA The Materials ISS Experiment Flight Facility mounted on the outside of the International Space Station allows researchers to test the performance and durability of materials and devices. This is done by exposing items of interest to everything that makes the space environment harsh, including radiation, highly reactive atomic oxygen, microgravity, and extreme temperatures. Currently, one suite on the platform holds MISSE-20-Commercial, an investigation conducting 12 experiments from different research teams. Among MISSE-20-Commercial is the Space Entanglement and Annealing Quantum Experiment (SEAQUE) which tests two technologies that could advance the field of quantum communications. The first technology is a novel method to transmit quantum data. This method could make way for a scalable quantum information network and provide the foundation of quantum cloud computing, a technology that holds the promise of operating millions of times faster than conventional computers. SEAQUE will also validate technology to “self-heal” its sensitive detectors against radiation damage using laser annealing, prolonging the life of these quantum tools in a space environment. Diana Garcia International Space Station Research Communications Team Johnson Space Center Keep Exploring Discover More Topics Benefits to Humanity Humans In Space International Space Station Space Station Research and Technology View the full article

NASA Rocket Engine Fireplace - 8 Hours in 4K

Basil Baldauff knew early in his tenure at NASA’s Johnson Space Center that he wanted to become a leader within the agency and make an impact on the future of space exploration. As a contract electrical design and test engineer working within Johnson’s Energy Systems Test Area, Baldauff had an opportunity to lead small teams in performing battery testing. Exposure to the test director role inspired him to pursue a more permanent leadership position, and today he is the lead facility engineer for the Battery Systems Test Facility. The facility supports hundreds of abuse, performance, and flight tests of batteries and cells for applications ranging from laptops and satellite phones used by astronauts to life-saving equipment used in spacesuits and backup power supplies. Baldauff ensures all battery testing is performed properly and safely while managing facility resources and maintaining the functionality of all test support systems. Official portrait of Basil Baldauff.NASA To date, one of his favorite projects at Johnson involved serving as test director for thermal runaway testing of the Artemis III Orion Crew Module battery. This test was an engineering evaluation to validate and certify that the battery’s design met requirements for handling a possible internal short circuit and preventing such an event from causing battery failure. “Being able to lead a team of engineers and technicians to help fulfill NASA’s mission at such an early part of my career is an achievement I take pride in,” he said. Baldauff is also a proud member of the Osage Nation. “I try to demonstrate some of the Osage core values daily in the workplace such as compassion, cooperation, honesty, and respect,” he said. He has been involved with the American Indian Science and Engineering Society since he was in high school, helping the organization support Indigenous students and professionals in STEM fields. He believes that NASA can further promote diversity by continuing to highlight and celebrate the many different groups and cultures within the agency’s workforce. Basil Baldauff attends Osage I’n-Lon-Schka, a ceremonial tribal dance that takes place each June.Image courtesy of Basil Baldauff Reflecting on his three years at Johnson, Baldauff highlighted the value of mentorship. “Finding or having a mentor early on in your career who can help you navigate unencountered situations or lend advice when needed is crucial,” he said. “It is vital to learn as much as you can from your mentor or supervisor, since they have most likely walked in your exact footsteps at some time.” Baldauff noted that challenges can arise in any job. “Staying positive and keeping an open mind when searching for solutions can go a long way,” he said. Baldauff is excited to see humanity’s return to the Moon and establishment of a long-term presence on the lunar surface. “I look forward to seeing how what I achieved in my career at NASA helped to make that future a reality.” He also encourages the Artemis Generation to never stop learning. “I hope to pass on the eagerness to always keep learning, no matter how old or where you are in your career,” he said. View the full article

6 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) The Milky Way pictured from the International Space Station in a long-duration photographCredits: NASA NASA and its commercial partners continue to drive innovation in space exploration, achieving milestones that will ultimately benefit human spaceflight and commercial low Earth orbit efforts. These recent achievements from NASA’s industry partners include completed safety milestones, successful flight tests, and major technological advancements. “Our commercial partners’ growing capabilities in low Earth orbit underscore NASA’s commitment to advance scientific discovery, pioneering space technology, and support future deep space exploration,” said Angela Hart, manager of the Commercial Low Earth Orbit Development Program at NASA’s Johnson Space Center in Houston. As NASA expands opportunities in low Earth orbit, the agency is working with seven U.S. companies to meet future commercial and government needs through the second Collaborations for Commercial Space Capabilities initiative. The first and second stages of Blue Origin’s New Glenn test vehicle pictured at the company’s orbital launch vehicle factory in Cape Canaveral, FloridaCredits: Blue Origin Blue Origin Blue Origin continues to make progress in the development of an integrated commercial space transportation capability that ensures safe, affordable, and high-frequency U.S. access to orbit for crew and other missions. Northrop Grumman’s Cygnus spacecraft pictured approaching the International Space StationCredits: NASA Northrop Grumman Northrop Grumman is evolving the company’s Cygnus spacecraft as a foundational logistics and research platform to support NASA’s next generation of low Earth orbit ventures. The company recently completed a project management review with NASA, presenting the roadmap and enhancements to commercialize the spacecraft. Northrop Grumman also continues to make progress toward the implementation of docking capability through a partnership with Starlab Space. Sierra Space’s LIFE (Large Integrated Flexible Environment) habitat following a full-scale ultimate burst pressure test at NASA’s Marshall Space Flight Center in Huntsville, Alabama.Credits: Sierra Space Sierra Space Sierra Space recently completed two full-scale ultimate burst pressure tests of its LIFE (Large Integrated Flexible Environment) habitat structure, an element of a NASA-funded commercial space station for new destinations in low Earth orbit. The company also has selected and tested materials for the habitat’s air barrier, focusing on permeability and flammability testing to meet the recommended safety standards. The inflatable habitat is designed to expand in orbit, creating a versatile living and working area for astronauts with a flexible, durable structure that allows for compact launch and significant expansion upon deployment. Sierra Space also has advanced in high velocity impact testing and micro-meteoroid and orbital debris configuration and material selection, crucial for ensuring the safety and durability of the company’s space structures, along with advancing radiator designs to optimize thermal management for long-duration missions. The SpaceX Starship spacecraft, a fully reusable transportation, ahead of a test flight at the company’s Starbase facilities in Boca Chica, Texas.Credits: SpaceX SpaceX SpaceX continues developing the company’s Starship spacecraft, a fully reusable transportation system designed for missions to low Earth orbit, the Moon, Mars, and beyond. SpaceX completed multiple flight tests, launching the spacecraft on the Super Heavy, the launch system’s booster, from the company’s Starbase facility in Boca Chica, Texas. During the tests, SpaceX demonstrated key capabilities needed for the system’s reusability, including landing burns and reentry from hypersonic velocities. SpaceX is preparing to launch newer generations of the Starship system, powered by upgraded versions of its reusable methane-oxygen staged-combustion Raptor engines, as it works to operationalize the system ahead of the first crewed lunar landing missions under the agency’s Artemis campaign. An engineer for Special Aerospace Services tests the company’s Autonomous Maneuvering UnitCredits: Special Aerospace Services Special Aerospace Services Special Aerospace Services is developing an Autonomous Maneuvering Unit that incorporates in-space servicing, propulsion, and robotic technologies. The company is evaluating customer needs and establishing the details and features for the initial flight unit. Special Aerospace Services also is working on a prototype unit at its Special Projects Research Facility in Arvada, Colorado, and has started construction of a new campus and final assembly facility in Huntsville, Alabama. The application of these technologies is intended for the safer assembly of commercial destinations, servicing, retrieval, and inspection of in-space systems. Two twin containers hosting the welding experiment developed by ThinkOrbital, validated by NASA and ESA (European Space Agency),Credits: ThinkOrbital ThinkOrbital ThinkOrbital recently demonstrated autonomous welding in space, validated by NASA and ESA (European Space Agency). The company will further test in-space welding, cutting, and X-ray inspection technologies on another mission later this year. ThinkOrbital’s third mission, scheduled for late 2025, will focus on developing commercially viable products, including a robotic arm with advanced end-effector solutions and standalone X-ray inspection capabilities. In-space welding technologies could enable building larger structures for future commercial space stations. The qualification primary structure of Vast’s Haven-1 commercial space station during final welding stages at the company’s headquarters in Long Beach, California Credits: Vast Vast Vast continues development progress on the Haven-1 commercial space station, targeted to launch in 2025. The company recently completed several technical milestones, including fabricating key components such as the primary structure pathfinder, hatch, battery module, and control moment gyroscope. Vast also completed a solar array deployment test and the station’s preliminary design review with NASA’s support. While collaborating with the agency on developing and testing the commercial station’s dome-shaped window, Vast performed rigorous pressure testing to meet safety requirements. In addition to these efforts, NASA also is collaborating with two businesses through its Small Business Innovation Research Ignite initiative, which focuses on commercially viable technology ideas aligned with the agency’s mission needs. Both companies are developing technologies for potential use on the International Space Station and future commercial space stations. A ceramic heat shield, or thermal protection system, being developed by Canopy Aerospace Credits: Canopy Aerospace Canopy Aerospace Canopy Aerospace is developing a new manufacturing system aimed at improving the production of ceramic heat shields, also known as thermal protection systems. The company recently validated the material properties of a low-density ceramic insulator using an alumina-enhanced thermal barrier formulation. Canopy Aerospace also continues development of a 3D-printed, low-density ablator designed to provide thermal protection during extreme heating. The company also worked on other 3D-printed materials, such as aluminum nitride and oxide ceramic products, which could be useful in various applications across the energy, space, aerospace, and industrial sectors, including electromagnetic thrusters for satellites. Canopy Aerospace also developed standard layups of fiber-reinforced composites and integrated cork onto composite panels. The Cargo Ferry, a reusable cargo transportation vehicle, prototype during a recent high-altitude flight test to test its recovery system and range capabilities.Credits: Outpost Technologies Outpost Technologies Outpost Technologies completed a high-altitude flight test of its Cargo Ferry, a reusable cargo transportation vehicle. The company dropped a full-scale prototype from 82,000 feet via weather balloon to test its recovery system and range capabilities. The key innovation is a robotic paraglider that guides the vehicle to a precise landing. The paraglider deployed at a record-setting altitude of 65,000 feet, marking the highest flight ever for such a system. During the test, the vehicle autonomously flew 165 miles before it was safely recovered at the landing site, demonstrating the system’s reliability. The company’s low-mass re-entry system can protect payload mass and volume for future space cargo return missions and point-to-point delivery. NASA’s low Earth orbit microgravity strategy builds on the agency’s extensive human spaceflight experience to advance future scientific and exploration goals. As the International Space Station nears the end of operations, NASA plans to transition to a new low Earth orbit model to continue leveraging microgravity benefits. Through commercial partnerships, NASA aims to maintain its leadership in microgravity research and ensure continued benefits for humanity. Learn more about NASA’s low Earth orbit microgravity strategy at: https://www.nasa.gov/leomicrogravitystrategy News Media Contacts Claire O’Shea Headquarters, Washington 202-358-1100 claire.a.o’shea@nasa.gov Anna Schneider Johnson Space Center, Houston 281-483-5111 anna.c.schneider@nasa.gov Keep Exploring Discover More Topics From NASA Low Earth Orbit Economy Commercial Destinations in Low Earth Orbit Commercial Use of the International Space Station Commercial Space View the full article

Caption: Artist’s concept of Dragonfly soaring over the dunes of Saturn’s moon Titan. NASA/Johns Hopkins APL/Steve Gribben NASA has selected SpaceX to provide launch services for the Dragonfly mission, a rotorcraft lander mission under NASA’s New Frontiers Program, designed to explore Saturn’s moon Titan. The mission will sample materials and determine surface composition in different geologic settings, advancing our search for the building blocks of life. The firm-fixed-price contract has a value of approximately $256.6 million, which includes launch services and other mission related costs. The Dragonfly mission currently has a targeted launch period from July 5, 2028, to July 25, 2028, on a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. Dragonfly centers on novel approach to planetary exploration, employing a rotorcraft-lander to travel between and sample diverse sites on Saturn’s largest moon. With contributions from partners around the globe, Dragonfly’s scientific payload will characterize the habitability of Titan’s environment, investigate the progression of prebiotic chemistry on Titan, where carbon-rich material and liquid water may have mixed for an extended period, and search for chemical indications of whether water-based or hydrocarbon-based life once existed on Saturn’s moon. NASA’s Launch Services Program at the agency’s Kennedy Space Center is responsible for managing the launch service. Managed for NASA at Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, the Dragonfly team comprises scientists, engineers, technologists, managers and more who have deep experience on missions that have explored the solar system from the Sun to Pluto and beyond, as well as experts in rotorcraft, autonomous flight, and space systems from around the globe. Dragonfly is the fourth mission in NASA’s New Frontiers Program, managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. For more information about NASA programs and missions, visit: https://www.nasa.gov -end- Julian Coltre / Tiernan Doyle Headquarters, Washington 202-358-1600 julian.n.coltre@nasa.gov / tiernan.p.doyle@nasa.gov View the full article

NASA/JPL-Caltech A 16.5-inch-long prototype of a robot designed to explore subsurface oceans of icy moons is reflected in the water’s surface during a test in a competition swimming pool in September 2024. Conducted by NASA’s Jet Propulsion Laboratory, the testing showed the feasibility of a mission concept called SWIM, short for Sensing With Independent Micro-swimmers. The project envisions a swarm of dozens of self-propelled, cellphone-size robots looking for signs of life on ocean worlds. SWIM is funded by NASA’s Innovative Advanced Concepts program under the agency’s Space Technology Mission Directorate. Learn more about the next generation of robotic concepts that could potentially plunge into the watery depths of Europa and other ocean worlds. Image credit: NASA/JPL-Caltech View the full article

The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) Forrest Melton, Ariel Deutsch, Dan Sirbu, and Chanel Idos. Their commitment to the NASA mission represents the entrepreneurial spirit, technical expertise, and collaborative disposition needed to explore this world and beyond. Earth Science Star: Forrest Melton Forrest Melton serves as Senior Research Scientist with the Atmospheric Science Branch, and leads the OpenET consortium, which develops a unique satellite-driven support system for water resources management using six satellite-driven models and publicly available data from NASA, USGS and NOAA. OpenET currently provides data for 23 states in the western U.S., delivers data at daily, monthly, seasonal and annual timescales, and has become a necessary tool for domestic and international water managers and agricultural producers (feature story). Space Science & Astrobiology Star: Ariel Deutsch Ariel Deutsch is an early career planetary scientist in the Planetary Systems Branch for the Bay Area Environmental Research Institute. She is recognized for being invited to join the Artemis II Science Team to support the Artemis II Lunar Science Objectives. Her Lunar Data Analysis Program grant was selected to improve our understanding of the distribution and abundance of volatiles cold-trapped on the Moon, which include Artemis III candidate landing sites. Space Science & Astrobiology Star: Dan Sirbu Dan Sirbu is a key member of the Exoplanet Technologies group within the Astrophysics Branch. He currently serves as the principal investigator on the Photonic Integrated Circuit High-Contrast Imaging for Space Astronomy (AstroPIC) early career initiative, serves multiple roles on the Multi-Star Wavefront Control (MSWC) project, and is involved in outreach efforts. In recent months, Dan has been the primary operator performing MSWC testing, setting several new performance records demonstrating high contrast imaging of planets around binary stars. Dan’s work also advances NASA’s and humanity’s capability of imaging exoplanets in multi-star systems, including Alpha Centauri, the nearest star system to the Sun. Space Biosciences Star: Chanel Idos Chanel Idos serves as the ARC Resource Analyst for the Human Research Program (HRP) in the Space Biosciences Division. HRP is a multifaceted initiative encompassing six Elements and Offices at JSC and three Divisions across two Directorates at ARC. Her exceptional expertise, coupled with outstanding organizational skills and clear, effective communication, have been instrumental in ensuring the seamless operation of HRP activities at ARC. Chanel’s contributions have been pivotal in achieving excellent cost performance for FY24, positioning ARC to enter FY25 in an optimal state. View the full article

Space-grown crystals could lead to targeted cancer drugs Researchers used space-grown protein crystals to determine the structure of a helix-loop-helix (HLH) peptide (one with a double helix and connecting loop) in a complex with vascular endothelial growth factor-A (VEGF). VEGF prompts the formation of new blood vessels and inhibiting it can stop tumor growth. This finding suggests that HLH peptides could be used to create drugs to target disease-related proteins like VEGF. JAXA PCG, an investigation from JAXA (Japan Aerospace Exploration Agency), grew protein crystals in microgravity and returned them to Earth for detailed analysis of their structures. Microgravity enables production of high-quality crystals, and examining their structures supports the design of new drugs and other types of research. Japan Aerospace Exploration Agency astronaut Soichi Noguchi works on the PCG experiment aboard the International Space Station.NASA Wood could make satellites more sustainable Wood exposed to space for approximately 10 months showed no change in weight and no erosion due to atomic oxygen. This finding could inform selection of the appropriate species and thickness of wood for use in building satellites. Metal satellites reentering Earth’s atmosphere can generate particles and aerosols that may harm the ozone layer. Wood becomes water and carbon dioxide on reentry, does not contribute to atmospheric pollution, and could provide a more sustainable option for future space exploration. JAXA’s Exposure of Wood to Outer Space evaluated how atomic oxygen, galactic cosmic rays, and solar energetic particles in space affect the mechanical properties of wood. Different types of wood to be tested in space as a building material for satellites. Kyoto University Analyzing glass-forming ability of magnesium silicates Researchers report detailed structural and atomic information for glassy and liquid magnesium silicates, which are important in glass science and geoscience. The results suggest that electronic structure does not play an important role in determining glass-forming ability, but atomic structure does. JAXA’s Fragility measured thermophysical properties such as density and viscosity of oxidized molten metals using the International Space Station’s Electrostatic Levitation Furnace (ELF) to gain insight into glass formation and the design of novel materials. The ELF makes it possible to observe the behavior of materials without the use of a container, providing information crucial for examining glass formation. NASA astronaut Scott Kelly works on the Electrostatic Levitation Furnace aboard the International Space Station.NASAView the full article

5 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) An artist’s concept of NASA’s Europa Clipper shows the spacecraft in silhouette against Europa’s surface, with the magnetometer boom fully deployed at top and the antennas for the radar instrument extending out from the solar arrays.NASA/JPL-Caltech Headed to Jupiter’s moon Europa, the spacecraft is operating without a hitch and will reach Mars in just three months for a gravity assist. NASA’s Europa Clipper, which launched Oct. 14 on a journey to Jupiter’s moon Europa, is already 13 million miles (20 million kilometers) from Earth. Two science instruments have deployed hardware that will remain at attention, extending out from the spacecraft, for the next decade — through the cruise to Jupiter and the entire prime mission. A SpaceX Falcon Heavy rocket launched it away from Earth’s gravity, and now the spacecraft is zooming along at 22 miles per second (35 kilometers per second) relative to the Sun. Europa Clipper is the largest spacecraft NASA has ever developed for a planetary mission. It will travel 1.8 billion miles (2.9 billion kilometers) to arrive at Jupiter in 2030 and in 2031 will begin a series of 49 flybys, using a suite of instruments to gather data that will tell scientists if the icy moon and its internal ocean have the conditions needed to harbor life. For now, the information mission teams are receiving from the spacecraft is strictly engineering data (the science will come later), telling them how the hardware is operating. Things are looking good. The team has a checklist of actions the spacecraft needs to take as it travels deeper into space. Here’s a peek: Boom Times Shortly after launch, the spacecraft deployed its massive solar arrays, which extend the length of a basketball court. Next on the list was the magnetometer’s boom, which uncoiled from a canister mounted on the spacecraft body, extending a full 28 feet (8.5 meters). To confirm that all went well with the boom deployment, the team relied on data from the magnetometer’s three sensors. Once the spacecraft is at Jupiter, these sensors will measure the magnetic field around Europa, both confirming the presence of the ocean thought to be under the moon’s icy crust and telling scientists about its depth and salinity. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video This animation shows how the boom of Europa Clipper’s magnetometer deployed — while the spacecraft was in flight — to its full length of 28 feet (8.5 meters). NASA/JPL-Caltech On the Radar After the magnetometer, the spacecraft deployed several antennas for the radar instrument. Now extending crosswise from the solar arrays, the four high-frequency antennas form what look like two long poles, each measuring 57.7 feet (17.6 meters) long. Eight rectangular very-high-frequency antennas, each 9 feet (2.76 meters) long, were also deployed — two on the two solar arrays. “It’s an exciting time on the spacecraft, getting these key deployments done,” said Europa Clipper project manager Jordan Evans of NASA’s Jet Propulsion Laboratory in Southern California. “Most of what the team is focusing on now is understanding the small, interesting things in the data that help them understand the behavior of the spacecraft on a deeper level. That’s really good to see.” Instrument Checkout The remaining seven instruments will be powered on and off through December and January so that engineers can check their health. Several instruments, including the visible imager and the gas and dust mass spectrometers, will keep their protective covers closed for the next three or so years to guard against potential damage from the Sun during Europa Clipper’s time in the inner solar system. Mars-Bound Once all the instruments and engineering subsystems have been checked out, mission teams will shift their focus to Mars. On March 1, 2025, Europa Clipper will reach Mars’ orbit and begin to loop around the Red Planet, using the planet’s gravity to gain speed. (This effect is similar to how a ball thrown at a moving train will bounce off the train in another direction at a higher speed.) Mission navigators already have completed one trajectory correction maneuver, as planned, to get the spacecraft on the precise course. At Mars, scientists plan to turn on the spacecraft’s thermal imager to capture multicolored images of Mars as a test operation. They also plan to collect data with the radar instrument so engineers can be sure it’s operating as expected. The spacecraft will perform another gravity assist in December 2026, swooping by Earth before making the remainder of the long journey to the Jupiter system. At that time, the magnetometer will measure Earth’s magnetic field, calibrating the instrument. More About Europa Clipper Europa Clipper’s three main science objectives are to determine the thickness of the moon’s icy shell and its interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission’s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet. Managed by Caltech in Pasadena, California, JPL leads the development of the Europa Clipper mission in partnership with the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, for NASA’s Science Mission Directorate in Washington. APL designed the main spacecraft body in collaboration with JPL and NASA’s Goddard Space Flight Center in Greenbelt, Maryland, NASA’s Marshall Space Flight Center in Huntsville, Alabama, and Langley Research Center in Hampton, Virginia. The Planetary Missions Program Office at Marshall executes program management of the Europa Clipper mission. NASA’s Launch Services Program, based at Kennedy, managed the launch service for the Europa Clipper spacecraft. Find more information about Europa Clipper here: https://science.nasa.gov/mission/europa-clipper 8 Things to Know About Europa Clipper Europa Clipper Teachable Moment NASA’s Europa Clipper Gets Its Giant Solar Arrays Kids Can Explore Europa With NASA’s Space Place News Media Contacts Gretchen McCartney Jet Propulsion Laboratory, Pasadena, Calif. 818-287-4115 gretchen.p.mccartney@jpl.nasa.gov Karen Fox / Molly Wasser NASA Headquarters, Washington 202-358-1600 karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov 2024-163 Share Details Last Updated Nov 25, 2024 Related TermsEuropa ClipperEuropaJet Propulsion Laboratory Explore More 5 min read NASA Ocean World Explorers Have to Swim Before They Can Fly Article 5 days ago 5 min read NASA’s Curiosity Mars Rover Takes a Last Look at Mysterious Sulfur Article 7 days ago 4 min read Precision Pointing Goes the Distance on NASA Experiment Article 2 weeks ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

4 min read NASA, JAXA XRISM Mission Looks Deeply Into ‘Hidden’ Stellar System The Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) observatory has captured the most detailed portrait yet of gases flowing within Cygnus X-3, one of the most studied sources in the X-ray sky. Cygnus X-3 is a binary that pairs a rare type of high-mass star with a compact companion — likely a black hole. Cygnus X-3 is a high-mass binary consisting of a compact object (likely a black hole) and a hot Wolf-Rayet star. This artist’s concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, emanating from the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole’s gravity captures some of the wind into an accretion disk around it, and the disk’s orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole. NASA’s Goddard Space Flight Center “The nature of the massive star is one factor that makes Cygnus X-3 so intriguing,” said Ralf Ballhausen, a postdoctoral associate at the University of Maryland, College Park, and NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “It’s a Wolf-Rayet star, a type that has evolved to the point where strong outflows called stellar winds strip gas from the star’s surface and drive it outward. The compact object sweeps up and heats some of this gas, causing it to emit X-rays.” A paper describing the findings, led by Ballhausen, will appear in a future edition of The Astrophysical Journal. “For XRISM, Cygnus X-3 is a Goldilocks target — its brightness is ‘just right’ in the energy range where XRISM is especially sensitive,” said co-author Timothy Kallman, an astrophysicist at NASA Goddard. “This unusual source has been studied by every X-ray satellite ever flown, so observing it is a kind of rite of passage for new X-ray missions.” XRISM (pronounced “crism”) is led by JAXA (Japan Aerospace Exploration Agency) in collaboration with NASA, along with contributions from ESA (European Space Agency). NASA and JAXA developed the mission’s microcalorimeter spectrometer instrument, named Resolve. Observing Cygnus X-3 for 18 hours in late March, Resolve acquired a high-resolution spectrum that allows astronomers to better understand the complex gas dynamics operating there. These include outflowing gas produced by a hot, massive star, its interaction with the compact companion, and a turbulent region that may represent a wake produced by the companion as it orbits through the outrushing gas. XRISM’s Resolve instrument has captured the most detailed X-ray spectrum yet acquired of Cygnus X-3. Peaks indicate X-rays emitted by ionized gases, and valleys form where the gases absorb X-rays; many lines are also shifted to both higher and lower energies by gas motions. Top: The full Resolve spectrum, from 2 to 8 keV (kiloelectron volts), tracks X-rays with thousands of times the energy of visible light. Some lines are labeled with the names of the elements that produced them, such as sulfur, argon, and calcium, along with Roman numerals that refer to the number of electrons these atoms have lost. Bottom: A zoom into a region of the spectrum often dominated by features produced by transitions in the innermost electron shell (K shell) of iron atoms. These features form when the atoms interact with high-energy X-rays or electrons and respond by emitting a photon at energies between 6.4 and 7 keV. These details, clearly visible for the first time with XRISM’s Resolve instrument, will help astronomers refine their understanding of this unusual system. JAXA/NASA/XRISM Collaboration In Cygnus X-3, the star and compact object are so close they complete an orbit in just 4.8 hours. The binary is thought to lie about 32,000 light-years away in the direction of the northern constellation Cygnus. While thick dust clouds in our galaxy’s central plane obscure any visible light from Cygnus X-3, the binary has been studied in radio, infrared, and gamma-ray light, as well as in X-rays. The system is immersed in the star’s streaming gas, which is illuminated and ionized by X-rays from the compact companion. The gas both emits and absorbs X-rays, and many of the spectrum’s prominent peaks and valleys incorporate both aspects. Yet a simple attempt at understanding the spectrum comes up short because some of the features appear to be in the wrong place. That’s because the rapid motion of the gas displaces these features from their normal laboratory energies due to the Doppler effect. Absorption valleys typically shift up to higher energies, indicating gas moving toward us at speeds of up to 930,000 mph (1.5 million kph). Emission peaks shift down to lower energies, indicating gas moving away from us at slower speeds. Some spectral features displayed much stronger absorption valleys than emission peaks. The reason for this imbalance, the team concludes, is that the dynamics of the stellar wind allow the moving gas to absorb a broader range of X-ray energies emitted by the companion. The detail of the XRISM spectrum, particularly at higher energies rich in features produced by ionized iron atoms, allowed the scientists to disentangle these effects. “A key to acquiring this detail was XRISM’s ability to monitor the system over the course of several orbits,” said Brian Williams, NASA’s project scientist for the mission at Goddard. “There’s much more to explore in this spectrum, and ultimately we hope it will help us determine if Cygnus X-3’s compact object is indeed a black hole.” XRISM is a collaborative mission between JAXA and NASA, with participation by ESA. NASA’s contribution includes science participation from CSA (Canadian Space Agency). Download additional images from NASA’s Scientific Visualization Studio By Francis Reddy NASA’s Goddard Space Flight Center, Greenbelt, Md. Media Contact: Claire Andreoli 301-286-1940 claire.andreoli@nasa.gov NASA’s Goddard Space Flight Center, Greenbelt, Md. Share Details Last Updated Nov 25, 2024 Related Terms Black Holes Electromagnetic Spectrum Galaxies, Stars, & Black Holes Research Goddard Space Flight Center Stars Stellar-mass Black Holes The Universe X-ray Binaries XRISM (X-Ray Imaging and Spectroscopy Mission) Facebook logo @NASAUniverse @NASAUniverse Instagram logo @NASAUniverse Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

Caption: Firefly Aerospace’s Blue Ghost Mission One lander, seen here, will carry 10 NASA science and technology instruments to the Moon’s near side when it launches from NASA’s Kennedy Space Center in Florida on a SpaceX Falcon 9 rocket, as part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign. Credit: Firefly Aerospace Media accreditation is open for the next delivery to the Moon through NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign for the benefit of humanity. A six-day launch window opens no earlier than mid-January 2025 for the first Firefly Aerospace launch to the lunar surface. The Blue Ghost flight, carrying 10 NASA science and technology instruments, will launch on a SpaceX Falcon 9 rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida. Media prelaunch and launch activities will take place at NASA Kennedy. Attendance for this launch is open to U.S. citizens and international media. International media must apply by Monday, Dec. 9, and U.S. media must apply by Thursday, Jan. 2. Media interested in participating in launch activities must apply for credentials at: https://media.ksc.nasa.gov Credentialed media will receive a confirmation email upon approval. NASA’s media accreditation policy is available online. For questions about accreditation or to request special logistical support such as space for satellite trucks, tents, or electrical connections, please send an email by Thursday, Jan. 2, to: ksc-media-accreditat@mail.nasa.gov. For other questions, please contact Kennedy’s newsroom at: 321-867-2468. Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo o Messod Bendayan a: antonia.jaramillobotero@nasa.gov o messod.c.bendayan@nasa.gov. The company named the mission Ghost Riders in the Sky. It will land near a volcanic feature called Mons Latreille within Mare Crisium, a more than 300-mile-wide basin located in the northeast quadrant of the lunar near side. The mission will carry NASA investigations and first-of-their-kind technology demonstrations to further our understanding of the Moon’s environment and help prepare for future human missions to the lunar surface, as part of the agency’s Moon to Mars exploration approach. This includes payloads testing lunar subsurface drilling, regolith sample collection, global navigation satellite system abilities, radiation tolerant computing, and lunar dust mitigation. The data captured also benefits humanity by providing insights into how space weather and other cosmic forces impact Earth. Under the CLPS model, NASA is investing in commercial delivery services to the Moon to enable industry growth and support long-term lunar exploration. As a primary customer for CLPS deliveries, NASA aims to be one of many customers on future flights. As part of its Artemis campaign, NASA is working with multiple U.S. companies to deliver science and technology to the lunar surface. These companies are eligible to bid on task orders to deliver NASA payloads to the Moon. The task order includes payload integration and operations and launching from Earth and landing on the surface of the Moon. Existing CLPS contracts are indefinite-delivery/indefinite-quantity contracts with a cumulative maximum contract value of $2.6 billion through 2028. For more information about the agency’s Commercial Lunar Payload Services initiative, see: https://www.nasa.gov/clps -end- Alise Fisher Headquarters, Washington 202-358-2546 alise.m.fisher@nasa.gov Wynn Scott / Natalia Riusech Johnson Space Center, Houston 281-483-5111 wynn.b.scott@nasa.gov / nataila.s.riusech@nasa.gov Antonia Jaramillo Kennedy Space Center, Florida 321-867-2468 antonia.jaramillobotero@nasa.gov Share Details Last Updated Nov 25, 2024 LocationNASA Headquarters Related TermsMissionsArtemisCommercial Lunar Payload Services (CLPS) View the full article

5 Min Read Hats Off to NASA’s Webb: Sombrero Galaxy Dazzles in New Image NASA’s James Webb Space Telescope recently imaged the Sombrero galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring. Credits: NASA, ESA, CSA, STScI In a new image from NASA’s James Webb Space Telescope, a galaxy named for its resemblance to a broad-brimmed Mexican hat appears more like an archery target. In Webb’s mid-infrared view of the Sombrero galaxy, also known as Messier 104 (M104), the signature, glowing core seen in visible-light images does not shine, and instead a smooth inner disk is revealed. The sharp resolution of Webb’s MIRI (Mid-Infrared Instrument) also brings into focus details of the galaxy’s outer ring, providing insights into how the dust, an essential building block for astronomical objects in the universe, is distributed. The galaxy’s outer ring, which appeared smooth like a blanket in imaging from NASA’s retired Spitzer Space Telescope, shows intricate clumps in the infrared for the first time. Image A: Sombrero Galaxy (MIRI Image) NASA’s James Webb Space Telescope recently imaged the Sombrero galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring. This image includes filters representing 7.7-micron light as blue, 11.3-micron light as green, and 12.8-micron light as red. NASA, ESA, CSA, STScI Image B: Sombrero Galaxy (Hubble and Webb Image) Image Before/After Researchers say the clumpy nature of the dust, where MIRI detects carbon-containing molecules called polycyclic aromatic hydrocarbons, can indicate the presence of young star-forming regions. However, unlike some galaxies studied with Webb, including Messier 82, where 10 times as many stars are born than the Milky Way galaxy, the Sombrero galaxy is not a particular hotbed of star formation. The rings of the Sombrero galaxy produce less than one solar mass of stars per year, in comparison to the Milky Way’s roughly two solar masses a year. Even the supermassive black hole, also known as an active galactic nucleus, at the center of the Sombrero galaxy is rather docile, even at a hefty 9-billion-solar masses. It’s classified as a low luminosity active galactic nucleus, slowly snacking on infalling material from the galaxy, while sending off a bright, relatively small, jet. Also within the Sombrero galaxy dwell some 2,000 globular clusters, collections of hundreds of thousands of old stars held together by gravity. This type of system serves as a pseudo laboratory for astronomers to study stars — thousands of stars within one system with the same age, but varying masses and other properties is an intriguing opportunity for comparison studies. In the MIRI image, galaxies of varying shapes and colors litter the background of space. The different colors of these background galaxies can tell astronomers about their properties, including how far away they are. The Sombrero galaxy is around 30 million light-years from Earth in the constellation Virgo. Video: Sombrero Galaxy Fade (Spitzer, Webb, Hubble) A Bright Future Ahead Stunning images like this, and an array of discoveries in the study of exoplanets, galaxies through time, star formation, and our own solar system, are still just the beginning. Recently, scientists from all over the world applied for observation time with Webb during its fourth year of science operations, which begins in July 2025. General Observer time with Webb is more competitive than ever. A record-breaking 2,377 proposals were submitted by the Oct. 15, 2024, deadline, requesting about 78,000 hours of observation time. This is an oversubscription rate, the ratio defining the observation hours requested versus the actual time available in one year of Webb’s operations, of around 9 to 1. The proposals cover a wide array of science topics, with distant galaxies being among the most requested observation time, followed by exoplanet atmospheres, stars and stellar populations, then exoplanet systems. The Space Telescope Science Institute manages the proposal and program selection process for NASA. The submissions will now be evaluated by a Telescope Allocation Committee, a group of hundreds of members of the worldwide astronomical community, on a dual-anonymous basis, with selections announced in March 2025. While time on Webb is limited, data from all of Webb’s programs is publicly archived, immediately after it’s taken, or after a time of exclusive access, in the Mikulski Archive for Space Telescopes (MAST) so it can be used by anyone in the world. 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 Right click any image to save it or open a larger version in a new tab/window via the browser’s popup menu. 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. Hannah Braun – hbraun@stsci.edu, Christine Pulliam – cpulliam@stsci.edu Space Telescope Science Institute, Baltimore, Md. Related Information Article: Types of Galaxies Video: Celestial Tour: Different types of galaxies Article: Sombrero Galaxy’s Halo Suggests Turbulent Past More images: Images of the Sombrero Galaxy in different types of light Video: Sonification of Sombrero Galaxy images More Webb News More Webb Images Webb Science Themes Webb Mission Page Related For Kids What is a galaxy? What is the Webb Telescope? SpacePlace for Kids En Español ¿Qué es una galaxia? 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… Galaxies Galaxies Stories Messier 104 (The Sombrero Galaxy) Hubble easily resolves some of the Sombrero galaxy’s roughly 2,000 globular clusters. Share Details Last Updated Nov 25, 2024 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms Astrophysics Galaxies Goddard Space Flight Center James Webb Space Telescope (JWST) Science & Research Spiral Galaxies The Universe View the full article

Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 2 min read Sol 4370-4371: All About the Polygons NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on Nov. 20, 2024 — sol 4369, or Martian day 4,369 of the Mars Science Laboratory mission — at 05:47:04 UTC. NASA/JPL-Caltech Earth planning date: Wednesday, Nov. 20, 2024 We planned two very full sols today! The sol 4369 drive completed successfully, and the rover was in a stable enough position that we could unstow the arm — something we don’t take for granted in the exceedingly rocky terrain of the sulfate unit! Today the team decided to investigate several rocks in our workspace that are covered in cracks, or fractures, that form polygonal patterns. We are interested to better characterize the geometry of these cracks and to see if they are associated with any compositional differences from the rock. Both pieces of information will give us clues about how they formed. Did they form when stresses pushed on the rock in just the right manner to fracture it into polygonal shapes? Or do the cracks record the rock expanding and contracting, either due to massive changes in temperatures on the Martian surface, or minerals within the rock gaining and losing water? Or perhaps it is something different? We selected two contact science targets to investigate in our attempt to answer these questions. The target named “Buttermilk” is one of the skinny raised ridges associated with these cracks. We will be placing APXS at three different places over this feature to try to characterize its chemistry. Our second contact science target, “Lee Vining,” gives us a nice 3D view into these cracks. Here, we will collect two MAHLI mosaics, one on each side of the rock that’s close to the rover, to characterize the geometry of the fractures. ChemCam will also get in on the action with a LIBS observation on a fracture fill named “Crater Crest,” as well as an observation on a dark-toned, platy rock called “Lost Arrow.” Mastcam will collect observations of several more polygonally fractured rocks further away from Curiosity in “The Dardanelles” series of mosaics. Some environmental science observations will round out the plan before our drive will take us about 25 meters further (about 82 feet) to the southwest. Written by Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory Share Details Last Updated Nov 23, 2024 Related Terms Blogs Explore More 3 min read Sols 4368-4369: The Colors of Fall – and Mars Article 2 days ago 3 min read Sols 4366–4367: One of Those Days on Mars (Sulfate-Bearing Unit to the West of Upper Gediz Vallis) Article 4 days ago 2 min read Sols 4362-4363: Plates and Polygons Article 1 week ago Keep Exploring Discover More Topics From NASA Mars Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited… All Mars Resources Explore this collection of Mars images, videos, resources, PDFs, and toolkits. Discover valuable content designed to inform, educate, and inspire,… Rover Basics Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a… Mars Exploration: Science Goals The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four… View the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Dr. Misty Davies receives the prestigious AIAA Fellowship in May 2024 for her contributions to aerospace safety and autonomous systems, recognized at a ceremony in Washington, DC.NASA In May 2024, Dr. Misty Davies joined the American Institute of Aeronautics and Astronautics (AIAA) Class of 2024 Fellows at a ceremony in Washington, DC. The AIAA website states that, “AIAA confers Fellow upon individuals in recognition of their notable and valuable contributions to the arts, sciences or technology of aeronautics and astronautics.” The first AIAA Fellows were elected in 1934; since then only 2064 people have been selected for the honor. Dr. Davies has focused her career at NASA Ames Research Center on developing tools and techniques that enable the safety assurance of increasingly autonomous systems. She currently serves as the Associate Chief for Aeronautics Systems in the Intelligent Systems Division at NASA Ames and is the Aerospace Operations and Safety Program (AOSP) Technical Advisor for Assurance and Safety. More information on AIAA Fellows is at https://www.aiaa.org/news/news/2024/02/08/aiaa-announces-class-of-2024-honorary-fellows-and-fellows Share Details Last Updated Nov 22, 2024 Related TermsGeneral Explore More 8 min read SARP East 2024 Ocean Remote Sensing Group Article 52 mins ago 10 min read SARP East 2024 Atmospheric Science Group Article 52 mins ago 10 min read SARP East 2024 Hydroecology Group Article 52 mins ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

8 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Return to 2024 SARP Closeout Faculty Advisors: Dr. Tom Bell, Woods Hole Oceanographic Institution Dr. Kelsey Bisson, NASA Headquarters Science Mission Directorate Graduate Mentor: Kelby Kramer, Massachusetts Institute of Technology Kelby Kramer, Graduate Mentor Kelby Kramer, graduate mentor for the 2024 SARP Ocean Remote Sensing group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship. Lucas DiSilvestro Shallow Water Benthic Cover Type Classification using Hyperspectral Imagery in Kaneohe Bay, Oahu, Hawaii Lucas DiSilvestro Quantifying the changing structure and extent of benthic coral communities is essential for informing restoration efforts and identifying stressed regions of coral. Accurate classification of shallow-water benthic coral communities requires high spectral and spatial resolution, currently not available on spaceborne sensors, to observe the seafloor through an optically complex seawater column. Here we create a shallow water benthic cover type map of Kaneohe Bay, Oahu, Hawaii using the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) without requiring in-situ data as inputs. We first run the AVIRIS data through a semi-analytical inversion model to derive color dissolved organic matter, chlorophyll concentration, bottom albedo, suspended sediment, and depth parameters for each pixel, which are then matched to a Hydrolight simulated water column. Pure reflectance for coral, algae, and sand are then projected through each water column to create spectral endmembers for each pixel. Multiple Endmember Spectral Mixture Analysis (MESMA) provides fractional cover of each benthic class on a per-pixel basis. We demonstrate the efficacy of using simulated water columns to create surface reflectance spectral endmembers as Hydrolight-derived in-situ endmember spectra strongly match AVIRIS surface reflectance for corresponding locations (average R = 0.96). This study highlights the capabilities of using medium-fine resolution hyperspectral imagery to identify fractional cover type of localized coral communities and lays the groundwork for future spaceborne hyperspectral monitoring of global coral communities. Atticus Cummings Quantifying Uncertainty In Kelp Canopy Remote Sensing Using the Harmonized Landsat Sentinel-2 Dataset Atticus Cummings California’s giant kelp forests serve as a major foundation for the region’s rich marine biodiversity and provide recreational and economic value to the State of California. With the rising frequency of marine heatwaves and extreme weather onset by climate change, it has become increasingly important to study these vital ecosystems. Kelp forests are highly dynamic, changing across several timescales; seasonally due to nutrient concentrations, waves, and predator populations, weekly with typical growth and decay, and hourly with the tides and currents. Previous remote sensing of kelp canopies has relied on Landsat imagery taken with a eight-day interval, limiting the ability to quantify more rapid changes. This project aims to address uncertainty in kelp canopy detection using the Harmonized Landsat and Sentinel-2 (HLS) dataset’s zero to five-day revisit period. A random forest classifier was used to identify pixels that contain kelp, on which Multiple Endmember Spectral Mixture Analysis (MESMA) was then run to quantify intrapixel kelp density. Processed multispectral satellite images taken within 3 days of one another were paired for comparison. The relationship between fluctuations in kelp canopy density with tides and currents was assessed using in situ data from an acoustic doppler current profiler (ADCP) at the Santa Barbara Long Term Ecological Research site (LTER) and a NOAA tidal buoy. Preliminary results show that current and tidal trends cannot be accurately correlated with canopy detection due to other sources of error. We found that under cloud-free conditions, canopy detection between paired images varied on average by 42%. Standardized image processing suggests that this uncertainty is not created within the image processing step, but likely arises due to exterior factors such as sensor signal noise, atmospheric conditions, and sea state. Ultimately, these errors could lead to misinterpretation of remotely sensed kelp ecosystems, highlighting the need for further research to identify and account for uncertainties in remote sensing of kelp canopies. Jasmine Sirvent Kelp Us!: A Methods Analysis for Predicting Kelp Pigment Concentrations from Hyperspectral Reflectance Jasmine Sirvent Ocean color remote sensing enables researchers to assess the quantity and physiology of life in the ocean, which is imperative to understanding ecosystem health and formulating accurate predictions. However, without proper methods to analyze hyperspectral data, correlations between spectral reflectance and physiological traits cannot be accurately derived. In this study, I explored different methods—single variable regression, partial least squares regressions (PLSR), and derivatives—in analyzing in situ Macrocystis pyrifera (giant kelp) off the coast of Santa Barbara, California in order to predict pigment concentrations from AVIRIS hyperspectral reflectance. With derivatives as a spectral diagnostic tool, there is evidence suggesting high versus low pigment concentrations could be diagnosed; however, the fluctuations were within 10 nm of resolution, thus AVIRIS would be unable to reliably detect them. Exploring a different method, I plotted in situ pigment measurements — chlorophyll a, fucoxanthin, and the ratio of fucoxanthin to chlorophyll a—against hyperspectral reflectance that was resampled to AVIRIS bands. PLSR proved to be a more successful model because of its hyperdimensional analysis capabilities in accounting for multiple wavelength bands, reaching R2 values of 0.67. Using this information, I constructed a model that predicts kelp pigments from simulated AVIRIS reflectance using a spatial time series of laboratory spectral measurements and photosynthetic pigment concentrations. These results have implications, not only for kelp, but many other photosynthetic organisms detectable by hyperspectral airborne or satellite sensors. With these findings, airborne optical data could possibly predict a plethora of other biogeochemical traits. Potentially, this research would permit scientists to acquire data analogous to in situ measurements about floating matters that cannot financially and pragmatically be accessed by anything other than a remote sensor. Isabelle Cobb Correlations Between SSHa and Chl-a Concentrations in the Northern South China Sea Isabelle Cobb Sea surface height anomalies (SSHa)–variations in sea surface height from climatological averages–occur on seasonal timescales due to coastal upwelling and El Niño-Southern Oscillation (ENSO) cycles. These anomalies are heightened when upwelling plumes bring cold, nutrient-rich water to the surface, and are particularly strong along continental shelves in the Northern South China Sea (NSCS). This linkage between SSHa and nutrient availability has interesting implications for changing chlorophyll-a (chl-a) concentrations, a prominent indicator of phytoplankton biomass that is essential to the health of marine ecosystems. Here, we evaluate the long-term (15 years) relationship between SSHa and chl-a, in both satellite remote sensing data and in situ measurements. Level 3 SSHa data from Jason 1/2/3 satellites and chl-a data from MODIS Aqua were acquired and binned to monthly resolution. We found a significant inverse correlation between SSHa and chl-a during upwelling months in both the remote sensing (Spearman’s R=-0.57) and in situ data, with higher resolution in situ data from ORAS4 (an assimilation of buoy observations from 2003-2017) showing stronger correlations (Spearman’s R=-0.75). In addition, the data reveal that the magnitude of SSH increases with time during instances of high correlation, possibly indicating a trend of increased SSH associated with reduced seasonal chl-a concentrations. Thus, this relationship may inform future work predicting nutrient availability and threats to marine ecosystems as climate change continues to affect coastal sea surface heights. Alyssa Tou Exploring Coastal Sea Surface Temperature Anomalies and their effect on Coastal Fog through analyzing Plant Phenology Alyssa Tou Marine heat waves (MHW) have been increasing in frequency, duration and intensity, giving them substantial potential to influence ecosystems. Do these MHWs sufficiently enhance coastal precipitation such that plant growth is impacted? Recently, the Northeast Pacific experienced a long, intense MHW in 2014/2015, and another short, less intense MHW in 2019/2020. Here we investigate how the intensity and duration of MHWs influence the intensity and seasonal cycle of three different land cover types (‘grass’, ‘trees’, and a combination of both ‘combined’’) to analyze plant phenology trends in Big Sur, California. We hypothesize that longer intense MHWs decrease the ocean’s evaporative capacity, decreasing fog, thus lowering plant productivity, as measured by Normalized Difference Vegetation Index (NDVI). Sea surface temperature (SST) and NDVI data were collected from the NOAA Coral Reef Watch, and NASA MODIS/Terra Vegetation Indices 16-Day L3 Global 250m products respectively. Preliminary results show no correlation (R2=0.02) between SSTa and combined NDVI values and no correlation (R2=0.01) between SST and NDVI. This suggests that years with anomalously high SST do not significantly impact plant phenology. During the intense and long 2014/2015 MHW, peak NDVI values for ‘grass’ and ‘combined’ pixels were 2.0 and 1.7 standard deviations above the climatological average, while the shorter 2019/2020 MHW saw higher peaks of 3.2 and 2.4 standard deviations. However, the ‘grass’, ‘tree’ and ‘combined’ NDVI anomalies were statistically insignificant during both MHWs, showing that although NDVI appeared to increase during the shorter and less intense MHW, these values may be attributed to other factors. The data qualitatively suggest that MHW’s don’t impact the peak NDVI date, but more data at higher temporal resolution are necessary. Further research will involve analyzing fog indices and exploring confounding variables impacting NDVI, such as plant physiology, anthropogenic disturbance, and wildfires. In addition, it’s important to understand to what extent changes in NDVI are attributed to the driving factors of MHWs or the MHWs themselves. Ultimately, mechanistically understanding the impacts MHW intensity and duration have on terrestrial ecosystems will better inform coastal community resilience. Return to 2024 SARP Closeout Share Details Last Updated Nov 22, 2024 Related TermsGeneral Explore More 10 min read SARP East 2024 Atmospheric Science Group Article 21 mins ago 10 min read SARP East 2024 Hydroecology Group Article 21 mins ago 11 min read SARP East 2024 Terrestrial Fluxes Group Article 22 mins ago View the full article

10 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Return to 2024 SARP Closeout Faculty Advisors: Dr. Guanyu Huang, Stony Brook University Graduate Mentor: Ryan Schmedding, McGill University Ryan Schmedding, Graduate Mentor Ryan Schmedding, graduate mentor for the 2024 SARP Atmospheric Science group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship. Danielle Jones Remote sensing of poor air quality in mountains: A case study in Kathmandu, Nepal Danielle Jones Urban activity produces particulate matter in the atmosphere known as aerosol particles. These aerosols can negatively affect human health and cause changes to the climate system. Measures for aerosols include surface level PM2.5 concentration and aerosol optical depth (AOD). Kathmandu, Nepal is an urban area that rests in a valley on the edge of the Himalayas and is home to over three million people. Despite the prevailing easterly winds, local aerosols are mostly concentrated in the valley from the residential burning of coal followed by industry. Exposure to PM2.5 has caused an estimated ≥8.6% of deaths annually in Nepal. We paired NASA satellite AOD and elevation data, model meteorological data, and local AirNow PM2.5 and air quality index (AQI) data to determine causes of variation in pollutant measurement during 2023, with increased emphasis on the post-monsoon season (Oct. 1 – Dec. 31). We see the seasonality of meteorological data related to PM2.5 and AQI. During periods of low temperature, low wind speed, and high pressure, PM2.5 and AQI data slightly diverge. This may indicate that temperature inversions increase surface level concentrations of aerosols but have little effect on the total air column. The individual measurements of surface pressure, surface temperature, and wind speed had no observable correlation to AOD (which was less variable than PM2.5 and AQI over the entire year). Elevation was found to have no observable effect on AOD during the period of study. Future research should focus on the relative contributions of different pollutants to the AQI to test if little atmospheric mixing causes the formation of low-altitude secondary pollutants in addition to PM2.5 leading to the observed divergence in AQI and PM2.5. Madison Holland Analyzing the Transport and Impact of June 2023 Canadian Wildfire Smoke on Surface PM2.5 Levels in Allentown, Pennsylvania Madison Holland The 2023 wildfire season in Canada was unparalleled in its severity. Over 17 million hectares burned, the largest area ever burned in a single season. The smoke from these wildfires spread thousands of kilometers, causing a large population to be exposed to air pollution. Wildfires can release a variety of air pollutants, including fine particulate matter (PM2.5). PM2.5 directly affects human health – exposure to wildfire-related PM2.5 has been associated with respiratory issues such as the exacerbation of asthma and chronic obstructive pulmonary disease. In June 2023, smoke from the Canadian wildfires drifted southward into the United States. The northeastern United States reported unhealthy levels of air quality due to the transportation of the smoke. In particular, Pennsylvania reported that Canadian wildfires caused portions of the state to have “Hazardous” air quality. Our research focused on how Allentown, PA experienced hazardous levels of air quality from this event. To analyze the concentrations of PM2.5 at the surface level, NASA’s Hazardous Air Quality Ensemble System (HAQES) and the EPA’s Air Quality System (AQS) ground-based site data were utilized. By comparing HAQES’s forecast of hazardous air quality events with recorded daily average PM2.5 with the EPA’s AQS, we were able to compare how well the ensemble system was at predicting total PM2.5 during unhealthy air quality days. NOAA’s Hybrid Single-Particle Lagrangian Integrated Trajectory model, pyrsig, and the Canadian National Fire Database were used. These datasets revealed the trajectory of aerosols from the wildfires to Allentown, Pennsylvania, identified the densest regions of the smoke plumes, and provided a map of wildfire locations in southeastern Canada. By integrating these datasets, we traced how wildfire smoke transported aerosols from the source at the ground level. Michele Iraci Trends and Transport of Tropospheric Ozone From New York City to Connecticut in the Summer of 2023 Michele Iraci Tropospheric Ozone, or O₃, is a criteria pollutant contributing to most of Connecticut and New York City’s poor air quality days. It has adverse effects on human health, particularly for high-risk individuals. Ozone is produced by nitrogen oxides and volatile organic compounds from fuel combustion reacting with sunlight. The Ozone Transport Region (OTR) is a collection of states in the Northeast and Mid-Atlantic United States that experience cross-state pollution of O₃. Connecticut has multiple days a year where O₃ values exceed the National Ambient Air Quality Standards requiring the implementation of additional monitoring and standards because it falls in the OTR. Partially due to upstream transport from New York City, Connecticut experiences increases in O₃ concentrations in the summer months. Connecticut has seen declines in poor air quality days from O₃ every year due to the regulations on ozone and its precursors. We use ground-based Lidar, Air Quality System data, and a back-trajectory model to examine a case of ozone enhancement in Connecticut caused by air pollutants from New York between June and August 2023. In this time period, Connecticut’s ozone enhancement was caused by air pollutants from New York City. As a result, New York City and Connecticut saw similar O₃ spikes and decline trends. High-temperature days increase O₃ in both places, and wind out of the southwest may transport O₃ to Connecticut. Production and transport of O₃ from New York City help contribute to Connecticut’s poor air quality days, resulting in the need for interstate agreements on pollution management. Stefan Sundin Correlations Between the Planetary Boundary Layer Height and the Lifting Condensation Level Stefan Sundin The Planetary Boundary Layer (PBL) characterizes the lowest layer in the atmosphere that is coupled with diurnal heating at the surface. The PBL grows during the day as solar heating causes pockets of air near the surface to rise and mix with cooler air above. Depending on the type of terrain and surface albedo that receives solar heating, the depth of the PBL can vary to a great extent. This makes PBL height (PBLH) a difficult variable to quantify spatially and temporally. While several methods have been used to obtain the PBLH such as wind profilers and lidar techniques, there is still a level of uncertainty associated with PBLH. One method of predicting seasonal PBLH fluctuation and potentially lessening uncertainty that will be discussed in this study is recognizing a correlation in PBLH with the lifting condensation level (LCL). Like the PBL, the LCL is used as a convective parameter when analyzing upper air data, and classifies the height in the atmosphere at which a parcel becomes saturated when lifted by a forcing mechanism, such as a frontal boundary, localized convergence, or orographic lifting. A reason to believe that PBLH and LCL are interconnected is their dependency on both the amount of surface heating and moisture that is present in the environment. These thermodynamic properties are of interest in heavily populated metropolitan areas within the Great Plains, as they are more susceptible to severe weather outbreaks and associated economic losses. Correlations between PBLH and LCL over the Minneapolis-St. Paul metropolitan statistical area during the summer months of 2019-2023 will be discussed. Angelica Kusen Coupling of Chlorophyll-a Concentrations and Aerosol Optical Depth in the Subantarctic Southern Ocean and South China Sea (2019-2021) Angelica Kusen Air-sea interactions form a complex feedback mechanism, whereby aerosols impact physical and biogeochemical processes in marine environments, which, in turn, alter aerosol properties. One key indicator of these interactions is chlorophyll-a (Chl-a), a pigment common to all phytoplankton and a widely used proxy for primary productivity in marine ecosystems. Phytoplankton require soluble nutrients and trace metals for growth, which typically come from oceanic processes such as upwelling. These nutrients can also be supplied via wet and dry deposition, where atmospheric aerosols are removed from the atmosphere and deposited into the ocean. To explore this interaction, we analyze the spatial and temporal variations of satellite-derived chl-a and AOD, their correlations, and their relationship with wind patterns in the Subantarctic Southern Ocean and the South China Sea from 2019 to 2021, two regions with contrasting environmental conditions. In the Subantarctic Southern Ocean, a positive correlation (r²= 0.26) between AOD and Chl-a was found, likely due to dust storms following Austrian wildfires. Winds deposit dust aerosols rich in nutrients, such as iron, to the iron-limited ocean, enhancing phytoplankton photosynthesis and increasing chl-a. In contrast, the South China Sea showed no notable correlation (r² = -0.02) between AOD and chl-a. Decreased emissions due to COVID-19 and stricter pollution controls likely reduced the total AOD load and shifted the composition of aerosols from anthropogenic to more natural sources. These findings highlight the complex interrelationship between oceanic biological activity and the chemical composition of the atmosphere, emphasizing that atmospheric delivery of essential nutrients, such as iron and phosphorus, promotes phytoplankton growth. Finally, NASA’s recently launched PACE mission will contribute observations of phytoplankton community composition at unprecedented scale, possibly enabling attribution of AOD levels to particular groups of phytoplankton. Chris Hautman Estimating CO₂ Emission from Rocket Plumes Using in Situ Data from Low Earth Atmosphere Chris Hautman Rocket emissions in the lower atmosphere are becoming an increasing environmental concern as space exploration and commercial satellite launches have increased exponentially in recent years. Rocket plumes are one of the few known sources of anthropogenic emissions directly into the upper atmosphere. Emissions in the lower atmosphere may also be of interest due to their impacts on human health and the environment, in particular, ground level pollutants transported over wildlife protected zones, such as the Everglades, or population centers near launch sites. While rockets are a known source of atmospheric pollution, the study of rocket exhaust is an ongoing task. Rocket exhaust can have a variety of compositions depending on the type of engine, the propellants used, including fuels, oxidizers, and monopropellants, the stoichiometry of the combustion itself also plays a role. In addition, there has been increasing research into compounds being vaporized in atmospheric reentry. These emissions, while relatively minimal compared to other methods of travel, pose an increasing threat to atmospheric stability and environmental health with the increase in human space activity. This study attempts to create a method for estimating the total amount of carbon dioxide released by the first stage of a rocket launch relative to the mass flow of RP-1, a highly refined kerosene (C₁₂H₂₆)), and liquid oxygen (LOX) propellants. Particularly, this study will focus on relating in situ CO₂ emission data from a Delta II rocket launch from Vandenberg Air Force Base on April 15, 1999, to CO₂ emissions from popular modern rockets, such as the Falcon 9 (SpaceX) and Soyuz variants (Russia). The findings indicate that the CO₂ density of any RP-1/LOX rocket is 6.9E-7 times the mass flow of the sum of all engines on the first stage. The total mass of CO₂ emitted can be further estimated by modeling the volume of the plume as cylindrical. Therefore, the total mass can be calculated as a function of mass flow and first stage main engine cutoff. Future CO₂ emissions on an annual basis are calculated based on these estimations and anticipated increases in launch frequency. Return to 2024 SARP Closeout Share Details Last Updated Nov 22, 2024 Related TermsGeneral Explore More 8 min read SARP East 2024 Ocean Remote Sensing Group Article 21 mins ago 10 min read SARP East 2024 Hydroecology Group Article 21 mins ago 11 min read SARP East 2024 Terrestrial Fluxes Group Article 22 mins ago View the full article

10 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Return to 2024 SARP Closeout Faculty Advisors: Dr. Dom Ciruzzi, College of William & Mary Graduate Mentor: Marley Majetic, Pennsylvania State University Marley Majetic, Graduate Mentor Marley Majetic, graduate mentor for the 2024 SARP Hydroecology group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship. Jordan DiPrima How are different land cover types affected by land subsidence on the U.S. Atlantic Coast? Jordan DiPrima Land subsidence is a frequently overlooked geologic hazard that is caused by natural processes and, more recently, anthropogenic stressors. The goal of this study is to observe subsidence trends and hotspots among land cover types on Virginia’s Eastern Shore and Long Island, New York. This study utilizes interferometric synthetic aperture radar, or InSAR, satellite data from Sentinel-1 to map vertical land motion from 2017 to 2023. Land cover data were sourced from Landsat 8 satellite imagery. Subsidence was mapped within the following land cover types on the Eastern Shore: urban, wetland, cropland, temperate or sub-polar grassland, temperate or sub-polar shrubland, mixed forest, and temperate or subpolar needleleaf forest. These land cover types have mean vertical velocities ranging from -0.2 mm/yr to -5.2 mm/yr. Results suggest that land subsidence is most severe in cropland areas on the Eastern Shore, with a mean vertical velocity of -5.2 mm/yr. In contrast, wetlands display the most subsidence on Long Island with a mean vertical velocity of -2.1 mm/yr. Long Island lacked distinct trends among land cover types and instead showed evidence of subsidence hotspots. These hotspots exist in the following land cover types: temperate or sub-polar grassland, barren lands, wetland, cropland, and temperate or sub-polar broadleaf deciduous forest. Overall, Eastern Shore croplands and Long Island wetlands were determined to be the most susceptible land cover types. These findings highlight regions at risk of sea level rise, flooding, and coastal erosion as a result of subsidence. With further research, we can map subsiding landscapes on a global scale to improve resource allocation and mitigation techniques. Isabelle Peterson Total Thermokarst Lake Changes on the Seward Peninsula, Alaska: 2016 to 2024 Isabelle Peterson Thermokarst landscapes have and will continue to change as the arctic landscape warms due to climate change. Permafrost underlies much of these arctic landscapes, and as it melts, thermokarst landscapes are left behind. The Seward Peninsula in Alaska has an abundance of these landscapes, and thermokarst lakes are present in the northernmost portion. Several lakes have come and gone, but with increasing climate instability and warming of the area, there is a possibility of more permafrost melting, creating more of these lakes. To capture these changes, Harmonized Landsat Sentinel-2 (HLS) imagery were used to create annual lake maps of the northern portion of the Seward Peninsula from 2016 to 2024. Much of the methodology was informed from Jones et al. (2011); however, their study used eCognition, while the present study used ArcGIS Pro. This caused some differences in results likely due to the differences in software, satellite imagery, and the proposed study area. Lake number changes were observed annually. From this annual change, several 10 to 40 ha lakes disappeared and reappeared within the study period, along with smaller lakes filling in where larger lakes once were. Thermokarst lake drainage is a process described by Jones and Arp (2015) which has devastating geomorphological impacts on the surrounding area, creating large drainage troughs which diminish surrounding permafrost in a quick time frame. To capture these events and overall changes, satellite imagery is essential. This is especially true in remote regions which are hard to reach by foot and require flight missions to be scheduled over the area for aerial photography. However, LVIS and other higher resolution aerial instruments would provide higher accuracy when identifying smaller lakes, as satellite imagery does not accurately capture lakes below 1 ha in the study area. This assertion is made due to conflicting results compared to Jones et al (2011). While the methodologies of this study have been executed manually, Qin, Zhang, and Lu (2023) have proposed the idea of using Sentinel-2 imagery to map thermokarst lakes through automatic methods. While automatization has not yet been perfected, the potential is there and can be used to analyze thermokarst areas effectively. With more satellite imagery, annual, monthly, and potentially daily changes can be captured in favorable months to monitor changing landscapes in arctic regions. Thermokarst lakes have been changing, and monitoring them can help in the process of understanding the changing climate in arctic areas, especially through the lens melting permafrost. Emmanelle Cuasay Finding Refuge in Climate Crisis: Analyzing the Differences between Refugia and Non-Refugia in the Northern Philippines Using Remote Sensing Emmanelle Cuasay Refugia are areas that are characterized by stable environmental conditions that can act as a refuge for species as Earth’s climate warms. In this study, fourteen Harmonized Landsat Sentinel-2 images from February 2014 – March 2024 of the northern Philippines region were used. The region of interest is the terrestrial biome by Lake Taal. Normalized Difference Vegetation Index (NDVI) maps were created from all fourteen images to determine the NDVI 25th highest quartiles of the long-term average NDVI images and of a dry and wet year NDVI image. These values were then used to create refugia and non-refugia maps using ArcGIS Pro. Land cover data from Sentinel-2 and a digital elevation model (DEM), using the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), were plotted in ArcGIS Pro to determine the slope and aspect of the area. Global Ecosystems Dynamics Investigation (GEDI) data were used to look at forest height of the study area, and the distribution of forest height, slope, aspect, and elevation were plotted to determine their probability densities in refugia and non-refugia areas. Results of this study show increased biomass in refugia areas. This suggests that conservation practices are crucial to aid in the preservation of biodiversity and biomass within these refugia areas. Jayce Crayne Site-Based Observations of a Saharan Dust Storm’s Impacts on Evapotranspiration in North-Central Florida Jayce Crayne Saharan dust storms serve an important role in the western Atlantic’s climate in their contribution to Earth’s radiation budget, modulating sea surface temperatures (SSTs), fertilizing ecosystems, and suppressing cloud and precipitation patterns (Yuan et al., 2020). However, Saharan dust storms are expected to become less frequent in this region as SSTs continue to rise (Yuan et al., 2020). Predicting the climate response to this change requires a keen understanding of how the presence of these storms affect evapotranspiration (ET) and its indicators. This study utilizes site-based observational data from an AmeriFlux tower near Gainesville, FL recorded during a large dust storm in late June 2020. The storm’s progression was documented using satellite imagery from Aqua and Terra and aerosol optical depth (AOD) measurements from an Aerosol Robotic Network (AERONET) station co-located with the AmeriFlux tower. Indicators of ET such as surface air temperature, vapor pressure deficit, photosynthetic photon flux density, and net radiation were analyzed. Findings were compared to modeled ET and latent energy flux reanalysis data provided by the Global Land Data Assimilation System (GLDAS). Both model simulations and on-site observations support that ET decreased during the days dust concentrations were heaviest and for a short time thereafter. Cloud cover data adopted from meteorological aerodrome reports (METARs) provided by an automated surface observing system (ASOS) located in Gainesville showed that clouds were not a major contributor in decreasing ET during the days of heaviest dust. The results of this study show a considerable decrease in ET as a result of dust aerosols. Further research is necessary to determine whether changes in ET due to Saharan dust storms are significant enough to alter climates in the western Atlantic and, if so, what the climate response will be if the frequency of storms decreases. Brandon Wilson Predicting 2025 and 2028 dNBR and dNDIV for Csarf Smith River Complex / Evaluating the Effects of 2019 California Wildfire Fund Brandon Wilson Biodiverse regions across California remain vulnerable to harmful wildfires year round. Quantifying and measuring these regions’ wildfire resilience is necessary for understanding where/how to allocate environmental resources. Several ecological wildfire studies have been conducted utilizing artificial intelligence and remote sensing to analyze and predict biodiversity damage across wildfire prone regions, including Northern Algeria and Arkansas, USA. The current case study aims to analyze biodiversity damage from the 2023 Csarf Smith River Complex Fire in Six Rivers National Forest, California and predict the difference in Normalized Burn Ratio (dNBR) and difference in Normalized Difference Vegetation Index (dNDVI) for 2025 and 2028 using remote-sensing-based random forest (RF) regression. Furthermore, to observe, holistically, a practical method California has implemented to address state-wide wildfire damage, the 2019 California Wildfire Fund (AB 1054 and AB 111) was evaluated using the synthetic control method (SCM). For this case study, remote sensing data from the United States Geological Survey (USGS) and NASA (Landsat 9 Satellite C2 L2, TerraClimate and the Land Data Assimilation System) were utilized for processing relevant spectral indexes for the RF. Data from NOAA, Energy Information Agency, International Monetary Fund and Bureau of Economic Analysis were utilized as synthetic control datasets to evaluate the effects of the 2019 California Wildfire Fund. Elevated topography in this study area is susceptible to high severity burn effects, while less elevated topography burns less. This result affected dNBR and dNDVI predictions as elevated areas seemingly did not have strong resilience to rampant burns. This demonstrates a direct correlation to potential lower transpiration rates for elevated areas, warranting further analysis. Results of low variance, post-treatment, between the treated unit and the synthetic control unit, poses concern for the positive effect of the 2019 Wildfire Fund. Carrie Hashimoto Describing changes in evapotranspiration following the 2020 Creek Fire in the southern Sierra Nevada Carrie Hashimoto Climatic warming and high tree density have caused larger and more severe wildfires to occur in western United States forests over time. Wildfires affect both the hydrology and ecology of forests via alterations to the water balance (e.g., evapotranspiration, streamflow, infiltration, and more) and could shift vegetation communities and subsequent ecosystem structure and function. This project explores ecological characteristics of a landscape that predict the extent to which the Creek Fire in the southern Sierra Nevada has affected evapotranspiration. Strides in understanding of consequential evapotranspiration changes can create pathways to address emerging forest health challenges posed by similar western fires. For analysis, various remote sensing and modeled data were collected from OpenET, the North American Land Data Assimilation System, TerraClimate, Harmonized LandSat Sentinel-2 data, and the Shuttle Radar Topography Mission. Multiple linear regression and generalized additive models were constructed. Relative change in evapotranspiration served as the response variable. Model covariates included average temperature, total precipitation in the preceding months, average soil moisture, elevation, slope, aspect, northness, latitude, pre-fire normalized difference vegetation index (NDVI), and post-fire change in normalized burn ratio (dNBR). Best subset selection with cross validation demonstrated minimization of cross-validation error with a 7-covariate model. This reduced model yields lower complexity and more interpretability while sustaining an adjusted R2 of 0.626, compared to the full model’s adjusted R2 of 0.663. A reduced generalized additive model (GAM) with interaction terms drawn from the linear model variable selection demonstrated an adjusted R2 of 0.695, indicating a better fit that comes at the cost of reduced interpretability and higher computational requirements than the linear models. The goal of this work is to disentangle environmental indicators of post-fire evapotranspiration change, such that predictive modeling of future wildfire impacts on evapotranspiration can be achieved. Return to 2024 SARP Closeout Share Details Last Updated Nov 22, 2024 Related TermsGeneral Explore More 8 min read SARP East 2024 Ocean Remote Sensing Group Article 21 mins ago 10 min read SARP East 2024 Atmospheric Science Group Article 21 mins ago 11 min read SARP East 2024 Terrestrial Fluxes Group Article 22 mins ago View the full article

11 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Return to 2024 SARP Closeout Faculty Advisors: Dr. Lisa Haber, Virginia Commonwealth University Dr. Brandon Alveshere, Virginia Commonwealth University Dr. Chris Gough, Virginia Commonwealth University Graduate Mentor: Mindy Priddy, Virginia Commonwealth University Mindy Priddy, Graduate Mentor Mindy Priddy, graduate mentor for the 2024 SARP Terrestrial Fluxes group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship. Angelina De La Torre Using NDVI as a Proxy for GPP to Predict Carbon Dioxide Fluxes Angelina De La Torre Climate change, driven primarily by greenhouse gases, poses a threat to the future of our planet. Among these gases is carbon dioxide (CO₂), which has a much longer atmospheric residence time compared to other greenhouse gases. One potential factor in reducing atmospheric CO₂ enrichment is plant productivity. Gross Primary Productivity (GPP) estimates the amount of CO₂ fixed during photosynthesis. The Normalized Difference Vegetation Index (NDVI) provides insight into the health of an ecosystem by measuring the density and greenness of vegetation. Therefore, it can be inferred that there is a relationship between NDVI and GPP, as greener plants are likely more productive. In this study, we used NDVI as a proxy for GPP and analyzed the effect NDVI had on CO₂ fluxes during California’s wet season between January and March 2023 in a restored tidal freshwater wetland. GPP and CO₂ flux data were obtained from the Dutch Slough AmeriFlux tower in Oakley, California. Landsat data were used to calculate the average NDVI. The influence of NDVI on GPP was assessed using linear regression. A second linear regression was then performed using NDVI and CO₂ flux, of which GPP is one component. We anticipate that wetlands with greater vegetation density will have lower CO₂ emissions. Because Landsat data scans in 16-day intervals, daily variation in NDVI could not be observed. This translates to a frequency discrepancy between the Landsat and AmeriFlux data, as AmeriFlux towers measure in half-hour intervals. Additionally, the wet season represented was limited by data availability, as the data before 2023 were unavailable. Despite data limitations in this study, the outlined process could be repeated in various wetland and climate classifications for further analysis of a larger sample size. This study could assist in developing strategies to increase CO₂ sequestration in an attempt to slow the effects of climate change. Samarth Jayadev Using Machine Learning to Assess Relationships between NDVI and Net Carbon Exchange During the COVID-19 Pandemic Samarth Jayadev Understanding the movement of carbon between Earth’s land surface and atmosphere is essential for ecosystem monitoring, creating climate change mitigation strategies, and assessing the carbon budget on national to global scales. Measures of greenness serve as indicators of processes such as photosynthesis that control carbon exchange and are vital in modeling of carbon fluxes. NASA’s Orbiting Carbon Observatory (OCO-2) provides high quality measurements of column-averaged CO₂ concentrations that can be used to derive net carbon exchange (NCE), a measure of CO₂ flux between terrestrial ecosystems and the atmosphere. From OCO-2, NCE data collected at the land nadir, land glint satellite position combined with in situ sampling can provide accurate measurements on a 1°x1° scale suitable for carbon flux characterization across the contiguous United States (CONUS). Normalized difference vegetation index (NDVI), which ranges from -1 to +1, measures the greenness of vegetation, serving as an indicator of plant density and health. This can help to understand ecosystem to carbon-cycle interactions and be leveraged for determining patterns with NCE. We examined the relationship between NDVI and NCE across CONUS during 2020 using Gradient Boosting Decision Trees (GBDT) which specialize in classifying and predicting non-linear relationships. This algorithm takes multiple weak learners (decision trees) and combines their predictions in an iterative ensemble method to improve prediction accuracy. Feature and permutation importance tests found that January and August (trough and peak NDVI, respectively) were the highest weighted predictor variables related to NCE. The dataset was split in a 90% training 10% test ratio across latitude/longitude grid cells to assess and verify model performance. Using the mean squared error loss function and hyperparameters with optimal estimators, tree depth, sample split, and learning rate the algorithm was able to converge the test predictions to match the deviance of the training data. The gradient boosting model can be applied to different months and years of NDVI/NCE to further explore these relationships or a multitude of research questions. Further studies should consider integrating land use and land cover change variables such as bare land and urbanization to improve predictions of NCE. Makai Ogoshi Deep-learning Derived Spaceborne Canopy Structural Metrics Predict Forest Carbon Fluxes Makai Ogoshi Terrestrial and airborne lidar data products describing canopy structure are potent predictors of forest carbon fluxes, but whether satellite data products produce similarly robust indicators of canopy structure is not known. The assessment of contemporary spaceborne lidar and other remote sensing data products as predictors of carbon fluxes is crucial to next generation instrument and data product design and large-spatial scale modeling. We investigated relationships between deciduous broadleaf forest canopy structure, derived from deep-learning models created with lidar data from GEDI and optical imagery from Sentinel-2, and forest carbon exchange. These included comparisons to in-situ continuous net ecosystem exchange (NEE), gross primary production (GPP), and net primary production (NPP). We find that the mean canopy height from the gridded spaceborne product has a strong correlation with forest NPP, similar to prior analysis with ground-based lidar (portable canopy lidar; PCL). For comparison to NPP, heights taken from the gridded spaceborne product were compared by overlapping the product with nine terrestrial forest sites from the National Ecological Observatory Network (NEON). We used standard deviation of canopy height as a measure of canopy structural complexity. Complexity derived from the gridded spaceborne product does not show the same strong correlation with NPP as found when using PCL. Mean annual GPP and NEE across five years were compared to the gridded spaceborne product at six Fluxnet2015-tower sites with continuous, gap-filled carbon flux data. When compared to in-situ flux tower data, neither mean canopy height nor structural complexity strongly correlate to annual NEE or GPP. Primarily, the finding that derived spaceborne products exhibit a strong correlation between forest canopy height and NPP will advance global-scale application of forest-carbon flux predictions. Secondarily, a variety of limitations highlight shortcomings in the current terrestrial flux data network. A small number of available study sites, both spatially and temporally, and lack of resolution in vertical complexity of canopy structure both contribute to uncertainty in assessing the relationships to NEE and GPP. Sebastian Reed Porewater Methane Concentrations Vary Significantly Across A Freshwater Tidal Wetland Sebastian Reed Methane is a potent greenhouse gas that is over 80 times more powerful than CO₂ at trapping heat and accounts for an estimated 30% of global temperature rise associated with climate change. The largest natural source of methane worldwide is wetlands. Despite the role of methane in driving climate change, the magnitude of global annual wetland methane flux remains highly uncertain. This study analyzes the effects of greenness (assessed using Normalized Difference Vegetation Index; NDVI), plant species composition, rooting depth, atmospheric methane concentration, and plant longevity on porewater methane concentration at the Kimages Rice Rivers Center tidal freshwater wetland. Samples for atmospheric and porewater concentrations were conducted in situ in June 2024. For each sampling location (n = 23) we collected whole air samples (WAS) 2m above the marsh surface and porewater samples 5cm below the marsh surface. We visually assessed species composition at each sample location, with 12 species of wetland plants present overall. We used the TRY plant database to find the rooting depth, leaf nitrogen content, and lifespan of each species. Drone multispectral data from 2023 was used to estimate NDVI values. These variables were compared to the pore water methane concentration via stepwise linear regression. Leaf N content, NDVI, plant species, and WAS sampling did not show statistically significant correlation to porewater methane concentration. Rooting depth showed a slight positive correlation with porewater methane (alpha = 0.1, p = 0.08, R^2 = 0.1). Samples with only perennial plants (as opposed to annual plants) had a higher mean value of porewater methane (p = 0.1). Analyzing porewater methane provides insight as to what wetland components affect methanogenesis and methane release, which aids in assessing which plant functional traits are most responsible for driving or mitigating climate change. Results from this study and future research in this area has the potential to more accurately assess how methane cycles through wetlands to the atmosphere. Nohemi Rodarte Understanding the vertical profile of CO₂ concentration: How carbon dioxide levels change with altitude Nohemi Rodarte Carbon dioxide (CO₂) is one of the main greenhouse gasses that contribute to global warming.While the relationship between CO₂ concentrations and land cover types, such as forests and urban areas, is well documented, there is limited knowledge of how CO₂ concentrations vary with altitude at fine spatial scales. Guided by our hypothesis that CO₂ levels vary with altitude and increase with elevation, we used airborne data collected from the B200 aircraft, which flew at different altitudes (400 to 1200 feet) above the urban area of Hopewell, Virginia, between 9:40 AM and 10:40 AM. We analyzed the CO₂ concentrations recorded by the flight to obtain the median and range for each 100 feet of altitude. Our results reveal that carbon dioxide concentrations varied significantly across the range of altitudes investigated. Within the area studied, CO₂ concentrations were found to range between 410 and 470 ppm. The distribution of these concentrations along the altitude gradient shows a bimodal pattern, with notable peaks at altitudes of 700 to 800 feet and 1100 to 1200 feet. Although CO₂ levels were present at all measured altitudes, there was a noticeable drop in the mean concentration at 800 feet,which then stabilized until reaching 1,000 feet before rising again. This pattern indicates that the concentrations of this greenhouse gas are not uniformly distributed with altitude, but rather vary significantly, showing higher concentrations at certain elevations and lower concentrations at others. The CO₂ distribution fluctuates with altitude, showing higher or lower levels at specific heights rather than a smooth gradient, indicating that altitude impacts CO₂ concentrations. While we did not identify the drivers of this change, future studies could evaluate how factors such as surface emissions, atmospheric mixing, and local conditions may contribute to vertical CO₂ profiles, since the altitudes we considered in this research are within the troposphere. Camille Shaw Linking NDVI with CO₂ and CH₄ Fluxes: Insights into Vegetation and Urban Source-Sink Dynamics in the Great Dismal Swamp Camille Shaw In recent years, carbon dioxide, methane, and other greenhouse gases have gained attention because of their contribution to the rise in Earth’s global mean temperature. Methane and carbon dioxide have various sources and sinks, but an expanding array of sources have created a need to assess ongoing change in carbon balance. This study aims to quantify the relationship between Normalized Difference Vegetation Index, or NDVI, and methane and carbon dioxide fluxes. We measured carbon dioxide and methane concentrations within the boundary layer using the PICARRO instrument, focusing on the Great Dismal Swamp, a forested wetland, and surrounding areas in the Eastern Mid-Atlantic Region. Data collection occurred at various times of day and along different flight paths in 2016, 2017, and 2024, with each year representing data from a single season, either spring or fall, for temporal analysis. We calculated methane and carbon dioxide fluxes along the flight paths using airborne eddy covariance, a method for capturing accurate flux measurements while accounting for the mixing of gases in the boundary layer caused by heat. Additionally, we calculated NDVI for this area using NASA’s Landsat 8 and 9 satellite imagery. Analysis of the afternoon flight data revealed a negative linear correlation between NDVI and carbon dioxide flux. Urban areas, characterized by low NDVI, exhibit a positive carbon dioxide flux as a consequence of emissions from vehicles, while forested areas, with high NDVI, show a negative carbon dioxide flux because of photosynthesis. In contrast, methane flux shows minimal correlation with NDVI. The lack of correlation arises because forested wetlands, with high NDVI, emit substantial amounts of methane, while urban areas, despite having low NDVI, still produce significant methane emissions from landfills and industrial activities. Future research could further investigate how seasonal and diurnal variations influence the correlations between NDVI and greenhouse gases by collecting comprehensive data across all seasons within a given year and at various times of the day. Return to 2024 SARP Closeout Share Details Last Updated Nov 22, 2024 Related TermsGeneral Explore More 8 min read SARP East 2024 Ocean Remote Sensing Group Article 21 mins ago 10 min read SARP East 2024 Atmospheric Science Group Article 21 mins ago 10 min read SARP East 2024 Hydroecology Group Article 21 mins ago View the full article

NASA has awarded Bastion Technologies Inc., of Houston, the Center Occupational Safety, Health, Medical, System Safety and Mission Assurance Contract (COSMC) at the agency’s Ames Research Center in California’s Silicon Valley. The COSMC contract is a hybrid cost-plus-fixed-fee and firm-fixed-price contract, with an indefinite-delivery/indefinite-quantity component and maximum potential value of $53 million. The contract phase-in begins Thursday, Jan. 2, 2025, followed by a one-year base period that begins Feb. 14, 2025, and options to extend performance through Aug. 13, 2030. Under this contract, the company will provide support for occupational safety, industrial hygiene, health physics, safety and health training, emergency response, safety culture, medical, wellness, fitness, and employee assistance. The contractor also will provide subject matter expertise in several areas including system safety, software safety and assurance, quality assurance, pressure system safety, procurement quality assurance, and range safety. Work will primarily be performed at NASA Ames and NASA’s Armstrong Flight Research Center in Edwards, California, as needed. For information about NASA and agency programs, visit: https://www.nasa.gov -end- Tiernan Doyle NASA Headquarters, Washington 202-358-1600 tiernan.p.doyle@nasa.gov Rachel Hoover Ames Research Center, Silicon Valley, Calif. 650-604-4789 rachel.hoover@nasa.gov View the full article

NASA Deputy Administrator Pam Melroy speaks during an agency town hall on Sept. 21, 2021 at NASA Headquarters in Washington. Credit: NASA/Aubrey Gemignani NASA Deputy Administrator Pam Melroy and Nicola Fox, associate administrator for NASA’s Science Mission Directorate, will travel to Mexico City on Sunday, Nov. 24, for a multi-day trip to build on previous engagements and advance scientific and technological collaboration between the United States and Mexico. This visit will focus on fostering partnerships in astronomy and astrophysics research, as well as highlighting opportunities for economic, educational, and science, technology, engineering, and math collaborations between the two nations. Melroy’s trip will include high-level meetings with senior Mexican government officials, including the secretariat-designate for Science, Technology, Humanities, and Innovation. Melroy and Fox also will meet with leaders from academia, industry, and scientific institutions. These discussions will emphasize expanding cooperation in space science, with particular focus on Mexico’s growing astronomy programs. This visit builds on Melroy’s trip to Mexico City earlier this year and reflects NASA’s commitment to advancing international cooperation in space and science for the benefit of all. For more information about NASA’s international partnerships, visit: https://www.nasa.gov/oiir -end- Amber Jacobson / Katherine Rohloff Headquarters, Washington 202-358-1600 amber.c.jacobson@nasa.gov / katherine.a.rohloff@nasa.gov Share Details Last Updated Nov 22, 2024 EditorJessica TaveauLocationNASA Headquarters Related TermsScience Mission DirectorateOffice of International and Interagency Relations (OIIR) View the full article

A cyclone is a low-pressure area of winds that spiral inwards. Although tropical storms most often come to mind, these spiraling storms can also form at mid- and high latitudes. Two such cyclones formed in tandem south of Iceland in November 2006.NASA/Jesse Allen The Moderate Resolution Imaging Spectroradiometer flying aboard NASA’s Terra satellite took this picture of two cyclones near Iceland on Nov. 20, 2006. Though we usually think of cyclones occurring in the tropics, these spiraling storms can also form at mid- and high latitudes. Cyclones at these latitudes are actually fairly common, and they drive much of the Earth’s weather. Image credit: NASA/Jesse Allen View the full article

NASA’s Human Landing System (HLS) will transport the next astronauts that land on the Moon, including the first woman and first person of color, beginning with Artemis III. For safety and mission success, the landers and other equipment in development for NASA’s Artemis campaign must work reliably in the harshest of environments. The Hub for Innovative Thermal Technology Maturation and Prototyping (HI-TTeMP) lab at NASA’s Marshall Space Flight Center in Huntsville, Alabama, provides engineers with thermal analysis of materials that may be a prototype or in an early developmental stage using a vacuum chamber, back left, and a conduction chamber, right. NASA/Ken Hall Engineers at NASA’s Marshall Space Flight Center in Huntsville, Alabama, are currently testing how well prototype insulation for SpaceX’s Starship HLS will insulate interior environments, including propellant storage tanks and the crew cabin. Starship HLS will land astronauts on the lunar surface during Artemis III and Artemis IV. Marshall’s Hub for Innovative Thermal Technology Maturation and Prototyping (HI-TTeMP) laboratory provides the resources and tools for an early, quick-check evaluation of insulation materials destined for Artemis deep space missions. “Marshall’s HI-TTeMP lab gives us a key testing capability to help determine how well the current materials being designed for vehicles like SpaceX’s orbital propellant storage depot and Starship HLS, will insulate the liquid oxygen and methane propellants,” said HLS chief engineer Rene Ortega. “By using this lab and the expertise provided by the thermal engineers at Marshall, we are gaining valuable feedback earlier in the design and development process that will provide additional information before qualifying hardware for deep space missions.” A peek inside the conductive test chamber at NASA Marshall’s HI-TTeMP lab where thermal engineers design, set up, execute, and analyze materials destined for deep space to better understand how they will perform in the cold near-vacuum of space. NASA/Ken Hall On the Moon, spaceflight hardware like Starship HLS will face extreme temperatures. On the Moon’s south pole during lunar night, temperatures can plummet to -370 degrees Fahrenheit (-223 degrees Celsius). Elsewhere in deep space temperatures can range from roughly 250 degrees Fahrenheit (120 degrees Celsius) in direct sunlight to just above absolute zero in the shadows. There are two primary means of managing thermal conditions: active and passive. Passive thermal controls include materials such as insulation, white paint, thermal blankets, and reflective metals. Engineers can also design operational controls, such as pointing thermally sensitive areas of a spacecraft away from direct sunlight, to help manage extreme thermal conditions. Active thermal control measures that could be used include radiators or cryogenic coolers. Engineers use two vacuum test chambers in the lab to simulate the heat transfer effects of the deep space environment and to evaluate the thermal properties of the materials. One chamber is used to understand radiant heat, which directly warms an object in its path, such as when heat from the Sun shines on it. The other test chamber evaluates conduction by isolating and measuring its heat transfer paths. NASA engineers working in the HI-TTeMP lab not only design, set up, and run tests, they also provide insight and expertise in thermal engineering to assist NASA’s industry partners, such as SpaceX and other organizations, in validating concepts and models, or suggesting changes to designs. The lab is able to rapidly test and evaluate design updates or iterations. NASA’s HLS Program, managed by NASA Marshall, is charged with safely landing astronauts on the Moon as part of Artemis. NASA has awarded contracts to SpaceX for landing services for Artemis III and IV and to Blue Origin for Artemis V. Both landing services providers plan to transfer super-cold propellant in space to send landers to the Moon with full tanks. With Artemis, NASA will explore more of the Moon than ever before, learn how to live and work away from home, and prepare for future human exploration of Mars. NASA’s SLS (Space Launch System) rocket, exploration ground systems, and Orion spacecraft, along with the HLS, next-generation spacesuits, Gateway lunar space station, and future rovers are NASA’s foundation for deep space exploration. For more on HLS, visit: https://www.nasa.gov/humans-in-space/human-landing-system News Media Contact Corinne Beckinger Marshall Space Flight Center, Huntsville, Ala. 256.544.0034 corinne.m.beckinger@nasa.gov Explore More 8 min read Preguntas frecuentes: La verdadera historia del cuidado de la salud de los astronautas en el espacio Article 1 day ago 6 min read FAQ: The Real Story About Astronaut Health Care in Space Article 1 day ago 3 min read Ready, Set, Action! Our Sun is the Star in Dazzling Simulation Article 1 day ago r View the full article

2 Min Read Why NASA Is a Great Place to Launch Your Career Students at NASA's Jet Propulsion Laboratory pose for photos around the laboratory wearing their eclipse glasses. Credits: NASA/JPL-Caltech Recently recognized as the most prestigious internship program by Vault.com, NASA has empowered countless students and early-career professionals to launch careers in science, technology, engineering, and mathematics (STEM) fields. NASA interns make real contributions to space and science missions, making it one of the best places to start your career. “NASA internships give students the chance to work on groundbreaking projects alongside experts, providing impactful opportunities for professional growth,” said Mike Kincaid, associate administrator for NASA’s Office of STEM Engagement. “Since starting my career as an intern at NASA’s Johnson Space Center in Houston, I’ve experienced firsthand how NASA creates lasting connections and open doors—not just for me, but for former interns who are now colleagues across the agency. These internships build STEM skills, confidence, and networks, preparing the next generation of innovators and leaders.” NASA interns achieve impressive feats, from discovering new exoplanets to becoming astronauts and even winning Webby Awards for their science communication efforts. These valuable contributors play a crucial role in NASA’s mission to explore the unknown for the benefit of all. Many NASA employees start their careers as interns, a testament to the program’s lasting impact. Students congratulate the 23rd astronaut class at NASA’s Johnson Space Center in Houston on March 5, 2024.NASA/Josh Valcarcel Additionally, NASA is recognized as one of America’s Best Employers for Women and one of America’s Best Employers for New Graduates by Forbes, reflecting the agency’s commitment to fostering a diverse and inclusive environment. NASA encourages people from underrepresented groups to apply, creating a diverse cohort of interns who bring a wide range of perspectives and ideas to the agency. “My internship experience has been incredible. I have felt welcomed by everyone I’ve worked with, which has been so helpful as a Navajo woman as I’ve often felt like an outsider in male-dominated STEM spaces,” said Tara Roanhorse, an intern for NASA’s Office of STEM Engagement. If you’re passionate about space, technology, and making a difference in the world, NASA’s internship program is the perfect place to begin your journey toward a fulfilling and impactful career. To learn more about NASA’s internship programs, visit: https://www.intern.nasa.gov/ Keep Exploring Discover More STEM Topics From NASA For Colleges and Universities For Students Grades 9-12 Join Artemis Learning Resources View the full article