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3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Francisco Rodriguez (aircraft mechanic) services liquid oxygen or LOX on the ER-2 during the Geological Earth Mapping Experiment (GEMx) research project. Experts like Rodriguez sustain a high standard of safety on airborne science aircraft like the ER-2 and science missions like GEMx. The ER-2 is based out of NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Steve Freeman Operating at altitudes above 99% of the Earth’s atmosphere, NASA’s ER-2 aircraft is the agency’s highest-flying airborne science platform. With its unique ability to observe from as high as 65,000 feet, the ER-2 aircraft is often a platform for Earth science that facilitates new and crucial information about our planet, especially when the plane is part of collaborative and multidisciplinary projects. “We’re deploying instruments and people everywhere from dry lakebeds in the desert to coastal oceans and from the stratosphere to marine layer clouds just above the surface,” said Kirk Knobelspiesse, an atmospheric scientist at NASA’s Goddard Space Flight Center. “We live on a changing planet, and it is through collaborative projects that we can observe and understand those changes.” One mission that recently benefitted from the ER-2’s unique capabilities is the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) project. The PACE-PAX mission uses the ER-2’s capabilities to confirm data collected from the PACE satellite, which launched in February 2024. The PACE observatory is making novel measurements of the ocean, atmosphere, and land surfaces, noted Knobelspiesse, the mission scientist for PACE-PAX. This mission is all about checking the accuracy of those new satellite measurements. Sam Habbal (quality inspector), Darick Alvarez (aircraft mechanic), and Juan Alvarez (crew chief) work on the network “canoe” on top of the ER-2 aircraft, which provides network communication with the pilot onboard. Experts like these sustain a high standard of safety while outfitting instruments onboard science aircraft like the ER-2 and science missions like the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) mission. The ER-2 is based out of NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Genaro Vavuris “The ER-2 is the ideal platform for PACE-PAX because it’s about the closest we can get to putting instruments in orbit without actually doing so,” Knobelspiesse said. The collaborative project includes a diverse team of researchers from across NASA, plus the National Oceanic and Atmospheric Administration (NOAA), the Netherlands Institute for Space Research (SRON), the University of Maryland, Baltimore County, the Naval Postgraduate School, and other institutions. Similarly, the Geological Earth Mapping eXperiment (GEMx) science mission is using the ER-2 over multiple years to collect observations of critical mineral resources across the Western United States. “Flying at this altitude means the GEMx mission can acquire wide swaths of data with every overflight,” said Kevin Reath, NASA’s associate project manager for the GEMx mission, a collaboration between the United States Geological Survey (USGS) and NASA. The ER-2 conducted over 80 flight hours in service of the Plankton, Aerosol, Cloud, ocean Ecosystem Postlaunch Airborne eXperiment (PACE-PAX) mission. The ER-2 is uniquely qualified to conduct the high-altitude scientific flights that this project required, and is based at NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Genaro Vavuris The GEMx team collects visible, shortwave infrared, and thermal infrared data using instruments installed onboard the ER-2. Combining these instruments with the aircraft’s capability to fly at high altitudes bears promising results. “The dataset being produced is the largest airborne surface mineralogy dataset captured in a single NASA campaign,” Reath said. “These data could help inform federal, tribal, state, and community leaders to make decisions that protect or develop our environment.” Learn more about the ER-2 aircraft. Learn more about the PACE-PAX mission. Learn more about the GEMx mission. Learn more about NASA’s Airborne Science Program. Share Details Last Updated Oct 24, 2024 EditorDede DiniusContactErica HeimLocationArmstrong Flight Research Center Related TermsArmstrong Flight Research CenterAirborne ScienceEarth ScienceEarth's AtmosphereER-2PACE (Plankton, Aerosol, Cloud, Ocean Ecosystem)Science Mission Directorate Explore More 2 min read Hubble Sees a Celestial Cannonball The spiral galaxy in this NASA/ESA Hubble Space Telescope image is IC 3225. It looks… Article 5 hours ago 1 min read PSI Database is Live with New Features to Improve User Experience Since its launch in 2014, the Physical Sciences Informatics (PSI) system has served as NASA’s… Article 22 hours ago 7 min read S-MODE, ASIA-AQ, and the Role of ESPO in Complex Airborne Campaigns Article 7 days ago Keep Exploring Discover More Topics From NASA Armstrong Flight Research Center Armstrong Science Projects Aircraft Flown at Armstrong Earth Science View the full article
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The next CSUG event will take place November 6 – 7 at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Throughout the CSUG, representatives from NASA’s Space Communications and Navigation program and CSP’s industry partners will share updates on commercial SATCOM capability developments and the commercial service demonstrations taking place under CSP. NASA attendees must be badged and have physical access to Goddard Space Flight Center to attend in-person. There will be limited in-person seating, so RSVPs are required. Meeting invitations and an agenda will be provided to CSP’s active CSUG roster as details are finalized. Please contact mission support lead engineer Aaron Smith, aaron.smith@nasa.gov, or CSUG team member Michele Vlach, michele.m.vlach@nasa.gov , for inquires and requests to be added to the CSUG distribution list. Funded Space Act Agreement Partners In 2022, CSP awarded six funded Space Act Agreements to members of industry to develop and demonstrate space-based relay services that can meet NASA mission needs. Inmarsat Government Inc. Download Inmarsat Government will demonstrate a variety of space-based applications enabled by their established ELERA worldwide L-band network and ELERA satellites. Kuiper Government Solutions LLC Download Kuiper will deploy over 3,000 satellites in low-Earth orbit that link to small customer terminals on one end and a global network of hundreds of ground gateways on the other. SES Government Solutions Download SES will develop a real-time, high-availability connectivity solution enabled by their established geostationary and medium-Earth orbit satellite constellations. Space Exploration Technologies Download SpaceX plans to connect their established Starlink constellation and extensive ground system to user spacecraft through optical intersatellite links for customers in low-Earth orbit. Telesat U.S. Services LLC Download Telesat plans to leverage their Telesat Lightspeed network with optical intersatellite link technology to provide seamless end-to-end connectivity for low-Earth orbit missions. Viasat Incorporated Download Viasat’s Real-Time Space Relay service, enabled by the anticipated ViaSat-3 network, is designed to offer a persistent on-demand capability for low-Earth orbit operators. Non-Reimbursable Space Act Agreement Partners CSP is also formulating non-reimbursable Space Act Agreements with members of industry to grow the domestic SATCOM market, potentially expanding future space-relay offerings for NASA missions. Kepler Communications US Inc. Kepler Communications US Inc. plans to deliver data at lightspeed with a Space Development Agency-compatible optical data relay network, connecting space and Earth communications with low latency, high throughput, and enhanced security. The Kepler Network plans to provide complete coverage of all low-Earth orbit above 400 km altitude. Explore More 5 min read October Transformer of the Month: Nipa Phojanamongkolkij Article 2 days ago 2 min read NASA Ames Stars of the Month: October 2024 Article 2 days ago 4 min read NASA Begins New Deployable Solar Array Tech Demo on Pathfinder Spacecraft Article 2 days ago View the full article
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4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA’s Stennis Space Center near Bay St. Louis, Mississippi, achieved a key milestone this week for testing a new SLS (Space Launch System) rocket stage to fly on future Artemis missions to the Moon and beyond. Over a two-week period beginning Oct. 10, crews completed a safe lift and installation of the interstage simulator component needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. “NASA Stennis is at the front end of the critical path for future space exploration,” said Barry Robinson, project manager for exploration upper stage Green Run testing on the Thad Cochran Test Stand. “Installing the interstage simulator is a significant step in our preparation to ensure the new, more powerful upper stage is ready to safely fly on future Artemis missions.” Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin The EUS unit, built by Boeing at NASA’s Michoud Assembly Facility in New Orleans, which will be the upper stage for the evolved Block 1B version of SLS and will enable NASA to launch its most ambitious deep space missions. The new stage will replace the current interim cryogenic propulsion stage on the Block 1 version of SLS, which features a single engine and is capable of lifting 27 tons of crew and cargo to lunar orbit. The new exploration upper stage will be powered by four RL10 engines, manufactured by SLS engines contractor L3Harris. It will increase payload capacity by 40%, enabling NASA to send 38 tons of cargo with a crew to the Moon or 42 tons of cargo without a crew. In the first two weeks of October 2024, crews at NASA’s Stennis Space Center completed a successful lift and installation of an interstage simulator unit on the B-2 side of the Thad Cochran test Stand. The interstage simulator is a key component for future testing of NASA’s new exploration upper stage that will fly on Artemis missions to the Moon and beyond. Before the first flight of the exploration upper stage on the Artemis IV mission, the stage will undergo a series of Green Run tests of its integrated systems at NASA Stennis. The test series will culminate with a hot fire of the stage’s four RL10 engines, just as during an actual mission. The simulator component installed on the Thad Cochran Test Stand (B-2) at NASA Stennis weighs 103 tons and measures 31 feet in diameter and 33 feet tall. It will function like the SLS interstage section to protect EUS electrical and propulsion systems during Green Run testing. The top portion of the simulator also will serve as a thrust takeout system to absorb the thrust of the EUS hot fire and transfer it back to the test stand. The four-engine EUS provides more than 97,000 pounds of thrust. Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin Teams at NASA’s Stennis Space Center complete a safe lift and install of an interstage simulator unit needed for future testing of NASA’s exploration upper stage (EUS) in the B-2 position of the Thad Cochran Test Stand. The lift and install, completed over a two-week period that began Oct. 10, marks a milestone for testing the new SLS (Space Launch System) rocket stage that will fly on future Artemis missions to the Moon and beyond. The EUS will undergo a series of Green Run tests of its integrated systems prior to its first flight. During testing, the interstage simulator component will function like the SLS interstage section that helps protect the upper stage during Artemis launches. NOTE: Right click on photo to open full image in new tab.NASA/Danny Nowlin NASA Stennis crews previously lifted the interstage simulator to measure and align it relative to the test stand. It is now outfitted with all piping, tubing, and electrical systems necessary to support future Green Run testing. Installation onto the test stand enables NASA Stennis crews to begin fabricating the mechanical and electrical systems connecting the facility to the simulator. As fabrication of the systems are completed, crews will conduct activation flows to ensure the test stand can operate to meet test requirements. Through Artemis, NASA will establish the foundation for long-term scientific exploration at the Moon; land the first woman, first person of color and first international partner astronaut on the lunar surface; and prepare for human expeditions to Mars for the benefit of all. For information about NASA’s Stennis Space Center, visit: https://www.nasa.gov/stennis Explore More 4 min read Lagniappe for October 2024 Article 3 weeks ago 4 min read NASA Stennis Completes Key Test Complex Water System Upgrade Article 4 weeks ago 7 min read Lagniappe for September 2024 Article 2 months ago Share Details Last Updated Oct 25, 2024 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related TermsStennis Space CenterStennis Test Facility and Support Infrastructure Keep Exploring Discover More Topics From NASA Stennis Multi-User Test Complex Propulsion Test Engineering NASA Stennis Front Door NASA Stennis Media Resources View the full article
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Hubble Space Telescope Home Hubble Sees a Celestial… Hubble Space Telescope Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts E-books Lithographs Fact Sheets Glossary Posters Hubble on the NASA App More Online Activities 2 min read Hubble Sees a Celestial Cannonball This NASA/ESA Hubble Space Telescope image features the spiral galaxy IC 3225. ESA/Hubble & NASA, M. Sun The spiral galaxy in this NASA/ESA Hubble Space Telescope image is IC 3225. It looks remarkably as if it was launched from a cannon, speeding through space like a comet with a tail of gas streaming from its disk behind it. The scenes that galaxies appear in from Earth’s point of view are fascinating; many seem to hang calmly in the emptiness of space as if hung from a string, while others star in much more dynamic situations! Appearances can be deceiving with objects so far from Earth — IC 3225 itself is about 100 million light-years away — but the galaxy’s location suggests some causes for this active scene, because IC 3225 is one of over 1,300 members of the Virgo galaxy cluster. The density of galaxies in the Virgo cluster creates a rich field of hot gas between them, called ‘intracluster medium’, while the cluster’s extreme mass has its galaxies careening around its center in some very fast orbits. Ramming through the thick intracluster medium, especially close to the cluster’s center, places enormous ‘ram pressure’ on the moving galaxies that strips gas out of them as they go. As a galaxy moves through space, the gas and dust that make up the intracluster medium create resistance to the galaxy’s movement, exerting pressure on the galaxy. This pressure, called ram pressure, can strip a galaxy of its star-forming gas and dust, reducing or even stopping the creation of new stars. Conversely, ram pressure can also cause other parts of the galaxy to compress, which can boost star formation. IC 3225 is not so close to the cluster core right now, but astronomers have deduced that it has undergone ram pressure stripping in the past. The galaxy looks compressed on one side, with noticeably more star formation on that leading edge (bottom-left), while the opposite end is stretched out of shape (upper-right). Being in such a crowded field, a close call with another galaxy may also have tugged on IC 3225 and created this shape. The sight of this distorted galaxy is a reminder of the incredible forces at work on astronomical scales, which can move and reshape entire galaxies! Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, MD claire.andreoli@nasa.gov Share Details Last Updated Oct 24, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Hubble Space Telescope The Universe Keep Exploring Discover More Topics From NASA Hubble Space Telescope Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe. Hubble’s Galaxies Hubble Focus: Galaxies through Space and Time Hubble Focus: Galaxies through Space and Time Hubble’s Partners in Science View the full article
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NASA’s SpaceX Crew-8 members, from left to right, Roscosmos cosmonaut Alexander Grebenkin and NASA astronauts Michael Barratt, Matthew Dominick, and Jeanette Epps, are seen inside the Dragon spacecraft shortly after having landed off the coast of Pensacola, Florida, on Oct. 25, 2024. Credit: NASA/Joel Kowsky NASA’s SpaceX Crew-8 mission successfully splashed down at 3:29 a.m. EDT Friday, off Pensacola, Florida, concluding a nearly eight-month science mission and the agency’s eighth commercial crew rotation mission to the International Space Station. After launching March 3 on a SpaceX Falcon 9 rocket from NASA’s Kennedy Space Center in Florida, NASA astronauts Matthew Dominick, Michael Barratt, and Jeanette Epps, as well as Roscosmos cosmonaut Alexander Grebenkin, spent 232 days aboard the space station. Recovery teams from NASA and SpaceX quickly secured the spacecraft and assisted the astronauts during exit. The crew now will head to NASA’s Johnson Space Center in Houston, while the Dragon spacecraft will return to SpaceX facilities at Cape Canaveral Space Force Station in Florida for inspection and refurbishment for future missions. During their mission, crew members traveled nearly 100 million miles and completed 3,760 orbits around Earth. They conducted new scientific research to advance human exploration beyond low Earth orbit and benefit human life on Earth. Research and technology demonstrations included conducting stem cell research to develop organoid models for studying degenerative diseases, exploring how fuel temperature affects material flammability, and studying how spaceflight affects immune function in astronauts. Their work aims to improve astronaut health during long-duration spaceflights, contributing to critical advancements in space medicine and benefitting humanity. Crew-8’s return follows the arrival of NASA’s SpaceX Crew-9 to the orbiting laboratory Sept. 29. These missions are part of NASA’s Commercial Crew Program, which provides reliable access to space, maximizing the use of the station for research and development and supporting future missions beyond low Earth orbit by partnering with private companies to transport astronauts to and from the space station. Learn more about NASA’s Commercial Crew program at: https://www.nasa.gov/commercialcrew -end- Josh Finch / Jimi Russell Headquarters, Washington 202-358-1100 joshua.a.finch@nasa.gov / james.j.russell@nasa.gov Leah Cheshier / Sandra Jones Johnson Space Center, Houston 281-483-5111 leah.d.cheshier@nasa.gov / sandra.p.jones@nasa.gov Steve Siceloff / Stephanie Plucinsky Kennedy Space Center, Florida 321-867-2468 steven.p.siceloff@nasa.gov / stephanie.n.plucinsky@nasa.gov Share Details Last Updated Oct 25, 2024 EditorJessica TaveauLocationNASA Headquarters Related TermsCommercial CrewHumans in SpaceInternational Space Station (ISS)ISS Research View the full article
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1 Min Read Sinister Solar System A witch appears to be screaming in space in this image from NASA’s Wide-Field Infrared Survey Explorer (WISE). Credits: NASA/WISE Our universe is full of mysterious sights. Explore some of our most frightful finds from past Halloweens. Keep Exploring Discover More Topics From NASA Solar System Exploration Europa Clipper Europa Clipper will search for signs of potential habitability on Jupiter’s icy ocean moon Europa. Europa Jupiter About the Author NASA Science Editorial Team Share Details Last Updated Oct 24, 2024 Related Terms The Solar System Explore More 3 min read Europa Trek: NASA Offers a New Guided Tour of Jupiter’s Ocean Moon Article 1 day ago 5 min read Old Data Yields New Secrets as NASA’s DAVINCI Preps for Venus Trip How NASA’s DAVINCI mission to Venus uses old data to reveal new secrets. Article 1 week ago 4 min read New Team to Assess NASA’s Mars Sample Return Architecture Proposals NASA announced Wednesday a new strategy review team will assess potential architecture adjustments for the… Article 1 week ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article
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Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 4 min read Sols 4341-4342: A Bumpy Road This image was taken by Left Navigation Camera aboard NASA’s Mars rover Curiosity on Sol 4329 — Martian day 4,329 of the Mars Science Laboratory mission — on Oct. 10, 2024, at 05:35:08 UTC. NASA/JPL-Caltech Earth planning date: Monday, Oct. 21, 2024 After Curiosity’s busy weekend, the team is ready for another day of planning. We are able to take advantage of the Earth-Mars time offset to full plan on both sols of our plan today. For this plan, I served as Mobility Rover Planner, and planned Curiosity’s drive. The first sol begins with some remote science. In this block, there is a ChemCam LIBS and Mastcam joint observation of “Ewe Lake,” to look for variation across the different layers in the rock. There is also a ChemCam RMI and a Mastcam of the “Olmstead Point” target, to see if there are chemical differences that make it darker than the surrounding rocks. Mastcam also is taking a stereo image of “Depressed Lake” (in order to see if this loose block belongs to the Stimson or the Sulfate units) and an image of the ChemCam AEGIS target the rover automatically found after the last drive. After a nap, Curiosity wakes up to do some contact science on the “Chuck Pass” target, which is a piece of bedrock with laminations and nodules. We perform DRT brushing, MAHLI, and APXS observations of this rock before stowing the arm so we can be ready to drive on the second sol. In the late afternoon, to take advantage of the lighting conditions, we have another short set of Mastcam imaging — an atmospheric sky column observation and a stereo mosaic of “Fascination Turret” from this new angle. The second sol also kicks off with some remote sensing. We follow up the contact science with ChemCam LIBS and Mastcam of Chuck Pass. ChemCam also takes an RMI looking east back to the area of the white sulfur stones below “Whitebark Pass” to get yet another viewing angle. There is also some atmospheric imaging, Navcam deck monitoring (to see how the dust is moving around on the rover’s deck) and a large dust devil survey. After the imaging, we are ready to drive. This terrain has been very tricky. While the slopes are not steep, this is a very rocky area, as you can see in the image, making finding a safe path difficult. We don’t only need to worry about driving over things that are too big or too sharp, but we also have to make sure not to scrape the wheels along the side of a rock or steer them into a rock, making them wedge and stall. It also means that we do not have good stereo data out very far because the rocks block our view. The last complication is that we have to drive backwards — otherwise, the rover hardware will block Curiosity’s view of Earth during the time we want to send her the new plan. When we drive backwards, the rover hardware will block Curiosity’s view, so we need to turn to get a clear view in our images. We also take additional frames to be sure we can find the best path for the next drive. With all this, we ended up being able to drive about 32 meters today (about 105 feet). After a short diversion to get around a steering hazard, we were able to drive a fairly straight route along the path to our next major imaging stop. After the drive, we have our normal post-drive imaging, including a twilight MARDI image. We have been lucky so far on this terrain and been able to successfully complete our recent drives. Hopefully this drive will also be successful! Written by Ashley Stroupe, Mission Operations Engineer at NASA’s Jet Propulsion Laboratory Image Download Share Details Last Updated Oct 24, 2024 Related Terms Blogs Explore More 3 min read Sols 4338-4340: Decisions, Decisions Article 2 days ago 2 min read Sols 4336-4337: Where the Streets Have No Name Article 7 days ago 2 min read Just Keep Roving Throughout the past week, Perseverance has continued marching up the Jezero crater rim. This steep… 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
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NASA has selected the University of New Hampshire in Durham to build Solar Wind Plasma Sensors for the Lagrange 1 Series project, part of the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Next Program. This cost-plus-no-fee contract is valued at approximately $24.3 million and includes the development of two sensors that will study the Sun’s constant outflow of solar wind. The data collected will support the nation’s efforts to better understand space weather around Earth and to provide warnings about impacts such as radio and GPS interruptions from solar storms. The overall period of performance for this contract will be from Thursday, Oct. 24, and continue for a total of approximately nine years, concluding 15 months after the launch of the second instrument. The work will take place at the university’s facility in Durham, New Hampshire, and at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland. Johns Hopkins is the significant subcontractor. Under this contract, the University of New Hampshire will be required to design, analyze, develop, fabricate, integrate, test, verify, and evaluate the sensors, support their launch, supply and maintain the instrument ground support equipment, and support post-launch mission operations at the NOAA Satellite Operations Facility in Suitland, Maryland. The Solar Wind Plasma Sensors will measure solar wind, a supersonic flow of hot plasma from the Sun, and provide data to NOAA’s Space Weather Prediction Center, which issues forecasts, warnings and alerts that help mitigate space weather impacts. The measurements will be used to characterize coronal mass ejections, corotating interaction regions, interplanetary shocks and high-speed flows associated with coronal holes. The measurements will also include observing the bulk ion velocity, ion temperature and density and derived dynamic pressure. NASA and NOAA oversee the development, launch, testing, and operation of all the satellites in the L1 Series project. NOAA is the program owner that provides funds and manages the program, operations, and data products and dissemination to users. NASA and commercial partners develop, build, and launch the instruments and spacecraft on behalf of NOAA. For information about NASA and agency programs, please visit: https://www.nasa.gov -end- Jeremy Eggers Goddard Space Flight Center, Greenbelt, Md. 757-824-2958 jeremy.l.eggers@nasa.gov Share Details Last Updated Oct 24, 2024 EditorRob GarnerContactJeremy EggersLocationGoddard Space Flight Center Related TermsHeliophysicsGoddard Space Flight CenterHeliophysics DivisionNOAA (National Oceanic and Atmospheric Administration) View the full article
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NASA/Ben Smegelsky Clouds curling around the full “blue” moon gives the night sky an eerie feel in this image from Aug. 19, 2024. As seen here, a blue moon is not actually blue; the third full moon in a season with four full Moons is called a “blue” moon. Another moon will be visible in the sky the morning of Oct. 25: Jupiter’s icy moon Europa, the destination of NASA’s recently launched Europa Clipper, will be easily observable with binoculars on one side of Jupiter by itself. Get more skywatching tips. Image credit: NASA/Ben Smegelsky View the full article
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Listen to Chief AI Officer Dave Salvagnini represent NASA in a Federal Executive Forum webinar on “Artificial Intelligence Strategies in Government Progress and Best Practices 2024.” I see an acceptance of AI as the digital assistant, that capability that is going to enable every member of the workforce to be more effective with their time. Dave Salvagnini NASA Chief Artificial Intelligence Officer, and Chief Data Officer Featuring Chief AI Officers and technology experts at the IRS, Office of the National Coordinator for Health Information Technology, Red Hat, Deloitte, and Pure Storage, this discussion covers current AI use cases across the private and public sectors. Artificial intelligence, particularly GenAI, is changing landscapes ranging from medicine to tax systems to aeronautics. The webinar covers AI use cases for medical devices, tax amendments, and more, including a segment on how NASA is using AI capabilities for earth sciences, climate modeling, and deep space exploration. Although NASA has a long history with AI, Salvagnini notes, GenAI is changing the way we view and use these technologies. How do we equip the workforce to democratized, accessible AI capabilities, and what policies should we create to mitigate potential risks like bias, inaccuracies, and copyright issues? The webinar participants voice similar AI priorities in the coming year: building infrastructure to use these technologies at scale, equipping the workforce with training and resources, delivering AI capabilities that increase efficiencies, and establishing governance and risk management policies. The episode ends with a discussion of the near future, with each technology leader outlining their agency’s expected output and accomplishments regarding AI. At NASA, Salvagnini expects a perspective shift toward AI in our daily work. “I see an acceptance of AI as the digital assistant, that capability that is going to enable every member of the workforce to be more effective with their time.” View the full article
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Since its launch in 2014, the Physical Sciences Informatics (PSI) system has served as NASA’s online repository for physical science data. Now, the PSI system is live with new updates to further align with NASA’s open data policy. With its first significant update in over five years, the data repository has been completely redesigned, featuring a new layout, improved structure, and enhanced search functionalities. This updated system was created with a focus on user experience, and more updates are anticipated as new features are introduced. A key new feature of the system is, the PSI Submission Portal. This tool is designed to streamline the processes of collecting, curating, and publishing new data by enabling Principal Investigators and scientific teams to upload files directly to the system with the support of a data curator. The Portal also offers a dedicated workspace for data submitters, assigns a unique digital object identifier to each dataset, and standardizes the documentation and data structure for each investigation. Both the updated PSI system and Submission Portal can be accessed at PSI.NASA.gov. View the full article
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Learn Home Educator Night at the Museum… Heliophysics Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 2 min read Educator Night at the Museum of the North: Activating Science in Fairbanks Classrooms The NASA Heliophysics Education Activation Team (NASA HEAT) set out to activate science in Fairbanks classrooms in early October at the University of Alaska’s Museum of the North annual Educators’ Night. This free Fall semester event introduces educators and school staff to a variety of resources and connections, connecting attendees with resources and university departments that will support their classroom efforts. In 2024, over 100 guests received support from exhibitors on classroom topics. The museum put several dynamic activity kits on display – Cultural Connections Northern Lights, Energetic Aurora, and Sun Discovery – and helped participants explore and engage with them as supplementary materials for their classroom units and opportunities for hands-on exploration. The museum also promoted an upcoming Spring 2025 teacher workshop focused on the aurora. The Geophysical Institute’s (GI) Education Outreach Office – another active element of the NASA HEAT team – hosted a table to display some of their co-produced resources, including the Cultural Connections Northern Lights (Kiġuyat) student guides, which blend Iñupiaq culture and aurora borealis science. After directing educators on how to locate physical and digital resources, the GI Education Outreach team encouraged their visitors to wrap the term “heliophysics” into their own vocabulary! The University of Alaska Museum of the North’s Education & Public Programs team are an impactful part of NASA HEAT, which is part of NASA’s Science Activation portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn https://www.uaf.edu/museum/education/educators/educators-night Pulled from their kits and displayed for perusing, the Cultural Connections to Northern Lights kit is ready to be explored. UAF Geophysical Education Outreach staff Kaz Storm (left) and Mariah McNamara (right) introducing educators to curriculum materials co-produced with Alaska Native communities. Share Details Last Updated Oct 24, 2024 Editor NASA Science Editorial Team Related Terms Grades 5 – 8 for Educators Grades 9-12 for Educators Grades K – 4 for Educators Heliophysics Opportunities For Educators to Get Involved Science Activation Explore More 3 min read Europa Trek: NASA Offers a New Guided Tour of Jupiter’s Ocean Moon Article 1 day ago 6 min read NASA, NOAA: Sun Reaches Maximum Phase in 11-Year Solar Cycle Article 1 week ago 3 min read Eclipse Megamovie Coding Competition Article 1 week ago Keep Exploring Discover More Topics From NASA James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Perseverance Rover This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial… Parker Solar Probe On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona… Juno NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to… View the full article
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NASA logo NASA has awarded $15.6 million in grant funding to 15 projects supporting the maintenance of open-source tools, frameworks, and libraries used by the NASA science community, for the benefit of all. The agency’s Open-Source Tools, Frameworks, and Libraries awards provide support for the sustainable development of tools freely available to everyone and critical for the goals of the agency’s Science Mission Directorate. “We received almost twice the number of proposals this year than we had in the previous call,” said Steve Crawford, program executive, Open Science implementation, Office of the Chief Science Data Officer, NASA Headquarters in Washington. “The NASA science community’s excitement for this program demonstrates the need for sustained support and maintenance of open-source software. These projects are integral to our missions, critical to our data infrastructure, underpin machine learning and data science tools, and are used by our researchers, every day, to advance science that protects our planet and broadens our understanding of the universe.” This award program is one of several cross-divisional opportunities at NASA focused on advancing open science practices. The grants are funded by NASA’s Office of the Chief Science Data Officer through the agency’s Research Opportunities for Space and Earth Science. The solicitation sought proposals through two types of awards: Foundational awards: cooperative agreements for up to five years for open-source tools, frameworks, and libraries that have a significant impact on two or more divisions of the Science Mission Directorate. Sustainment awards: grants or cooperative agreements of up to three years for open-source tools, frameworks, and libraries that have significant impact in one or more divisions of the Science Mission Directorate. 2024 awardees are: Foundation awards: NASA’s Ames Research Center, Silicon Valley, CaliforniaPrincipal investigator: Ross Beyer “Expanding and Maintaining the Ames Stereo Pipeline” Caltech, Pasadena, CaliforniaPrincipal investigator: Brigitta Sipocz “Enhancement of Infrastructure and Sustained Maintenance of Astroquery” Cornell University, Scarsdale, New YorkPrincipal investigator: Ramin Zabih “Modernize and Expand arXiv’s Essential Infrastructure” NASA’s Goddard Space Flight Center, Greenbelt, MarylandPrincipal investigator: D. Cooley “Enabling SMD Science Using the General Mission Analysis Tool” NumFOCUS, Austin, TexasPrincipal investigator: Thomas Caswell “Sustainment of Matplotlib and Cartopy” NumFOCUSPrincipal investigator: Erik Tollerud “Investing in the Astropy Project to Enable Research and Education in Astronomy” Sustainment awards: NASA’s Jet Propulsion Laboratory, Southern CaliforniaPrincipal investigator: Cedric David “Sustain NASA’s River Software for the Satellite Data Deluge,” three-year award Pennsylvania State University, University ParkPrincipal investigator: David Radice “AthenaK: A Performance Portable Simulation Infrastructure for Computational Astrophysics,” three-year award United States Geological Survey, Reston, VirginiaPrincipal investigator: Trent Hare “Planetary Updates for QGIS,” one-year award NASA JPLPrincipal investigator: Michael Starch “How To F Prime: Empowering Science Missions Through Documentation and Examples,” three-year award NASA GoddardPrincipal investigator: Albert Shih “Enhancing Consistency and Discoverability Across the SunPy Ecosystem,” three-year award Triad National Security, LLC, Los Alamos, New MexicoPrincipal investigator: Julia Kelliher “Enhancing Analysis Capabilities of Biological Data With the NASA EDGE Bioinformatics Platform,” four-year award iSciences LLC, Burlington, VermontPrincipal investigator: Daniel Baston “Sustaining the Geospatial Data Abstraction Library,” three-year award University of Maryland, College Park,Principal investigator: C Max Stevens “Sustaining the Community Firn Model,” three-year award Quansight, LLC, Austin, TexasPrincipal investigator: Dharhas Pothina “Ensuring a Fast and Secure Core for Scientific Python – Security, Accessibility and Performance of NumPy, SciPy and scikit-learn; Going Beyond NumPy With Accelerator Support,” three-year award For information about open science at NASA, visit: https://science.nasa.gov/open-science -end- Alise Fisher Headquarters, Washington 202-617-4977 alise.m.fisher@nasa.gov View the full article
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2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA logo In fiscal year 2023, NASA investments supported 66,208 jobs in the state of California, generated $18.5 billion in economic output and $1 billion in tax revenue to the state’s economy. Overall, NASA generated an estimated $9.5 billion in federal, state, and local taxes throughout the United States. NASA’s Armstrong Flight Research Center in Edwards, California is one of three NASA centers in the state that contributes to this economic achievement. The center supports critical research in sustainable flight, air mobility, and airborne science, reinforcing the region as a hub of aerospace innovation. Most notably, NASA Armstrong plays a unique role in the Quesst mission and X-59 project, aimed at reducing the sonic booms into quieter “sonic thumps,” to change regulations impeding supersonic flight over land. Additionally, maturing key airframe technologies with the X-66 aircraft in the Sustainable Flight Demonstrator project which may influence the next generation single-aisle seat class airliner. The Center also supports the research of electric air taxis and drones to operate safely in the national airspace as well as supporting science aircraft for NASA’s Earth Science Mission. NASA’s Moon to Mars campaign generated 16,129 jobs and $4.7 billion in economic output in California. Collaborations with contractors like Boeing and Lockheed Martin further extended these benefits by creating thousands of high-skilled jobs in the Antelope Valley and across the state. NASA also fosters partnerships with educational institutions across the state, investing $39.5 million in universities to cultivate the next generation of aerospace innovators. These investments bring STEM opportunities to local communities and prepare students for careers in cutting-edge industries – adding to the agency’s most valuable asset, its workforce. NASA embraces the challenges of exploring the unknown and making the impossible possible as we continue our global leadership in science, human spaceflight, aerospace innovation, and technology development, and support the U.S. economy and benefit all. Read the full Economic Impact Report for Fiscal Year 2023. -end- Nicolas Cholula / Sarah Mann NASA’s Armstrong Flight Research Center 661-714-3853 / 661-233-2758 nicolas.h.cholula@nasa.gov /sarah.mann@nasa.gov Share Details Last Updated Oct 24, 2024 EditorDede DiniusContactNicolas Cholulanicolas.h.cholula@nasa.govSarah Mannsarah.mann@nasa.govLocationArmstrong Flight Research Center Related TermsArmstrong Flight Research Center Explore More 4 min read NASA Pilots Add Perspective to Research Article 1 week ago 3 min read Sacrifice and Success: NASA Engineer Honors Family Roots Article 1 week ago 4 min read Sacrificio y Éxito: Ingeniero de la NASA honra sus orígenes familiares Article 1 week ago Keep Exploring Discover More Topics From NASA Armstrong Flight Research Center Armstrong People Armstrong Capabilities & Facilities Aircraft Flown at Armstrong View the full article
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Kennedy Space Center Director Janet Petro speaks in March 2022 during the annual State of NASA event at the Florida spaceport. NASA/Kim Shiflett America is returning to the Moon with our sights set on Mars, and NASA is leading the way. Along with our industry and international partners, we’re advancing scientific research, inspiring the next generation of explorers, and ensuring reliable and continuous access to space for our nation. NASA’s Economic Impact Report for fiscal year (FY) 2023 highlights the nation’s strong return on its investment in NASA. Our missions help unveil the secrets of the universe and our home planet while also benefitting the taxpayers, communities, and industries across the country. Here at the agency’s Kennedy Space Center in Florida, we are on track for another record-setting year of launches from our Space Coast. Recent NASA missions will tell us more about Earth’s weather and climate, explore Jupiter’s moon Europa for the ingredients of life, and enable more innovative research on the International Space Station. We’re also busy building the Artemis rockets, spacecraft, and technologies that will allow our astronauts to live and work on the Moon. While exploring the universe for the benefit of all, NASA is also supporting the U.S. economy. During FY23, an investment of less than one-half of 1% of the federal budget, the agency generated $76 billion in total economic output nationwide. In Florida alone, NASA activities in FY2023 supported 35,685 jobs in the state and $8.2 billion in economic output, resulting in an additional $286.6 million in state tax revenue. NASA Kennedy’s unique facilities, proven technical capabilities, and master plan enable nearly 250 partnerships with 100 private-sector partners. And the dedication and commitment of our workforce means that our spaceport remains the world’s leader in space science, human exploration, and technology development. As we look toward a future of more exploration and discovery, I invite you to learn more about the impacts that NASA missions may have had in your life. The agency’s technology transfer initiatives transition NASA innovations into private hands, where real impacts are made. And NASA’s STEM engagements encourage research and the study of science, technology, engineering, and math at all ages. And, of course, I hope you will learn more about the exciting work we’re doing at Earth’s premier spaceport by visiting: www.nasa.gov/kennedy -end- Images of Janet Petro are available from NASA’s image library in vertical and horizontal formats. Patti Bielling Kennedy Space Center, Florida 321-501-7575 patricia.a.bielling@nasa.gov View the full article
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5 min read NASA Science on Health, Safety to Launch on 31st SpaceX Resupply Mission New science experiments for NASA are set to launch aboard the agency’s SpaceX 31st commercial resupply services mission to the International Space Station. The six investigations aim to contribute to cutting-edge discoveries by NASA scientists and research teams. The SpaceX Dragon spacecraft will liftoff aboard the company’s Falcon 9 rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. Science experiments aboard the spacecraft include a test to study smothering fires in space, evaluating quantum communications, analyzing antibiotic-resistant bacteria, examining health issues like blood clots and inflammation in astronauts, as well as growing romaine lettuce and moss in microgravity. Developing Firefighting Techniques in Microgravity Putting out a fire in space requires a unique approach to prioritize the safety of the spacecraft environment and crew. The SoFIE-MIST (Solid Fuel Ignition and Extinction – Material Ignition and Suppression Test) is one of five investigations chosen by NASA since 2009 to develop techniques on how to contain and put out fires in microgravity. Research from the experiment could strengthen our understanding of the beginning stages of fire growth and behavior, which will assist in building and developing more resilient space establishments and creating better plans for fire suppression in space NASA astronaut Jessica Watkins services components that support the SOFIE (Solid Fuel Ignition and Extinction) fire safety experiment inside the International Space Station’s combustion integrated rack Credit: NASA Combating Antibiotic Resistance Resistance to antibiotics is as much of a concern for astronauts in space as it is for humans on Earth. Research determined that the impacts of microgravity can weaken a human’s immune system during spaceflight, which can lead to an increase of infection and illness for those living on the space station. The GEARS (Genomic Enumeration of Antibiotic Resistance in Space) investigation scans the orbiting outpost for bacteria resistant to antibiotics and these organisms are studied to learn how they thrive and adapt to microgravity. Research results could help increase the safety of astronauts on future missions as well as provide clues to improving human health on Earth. A sample media plate pictured aboard the International Space Station. The GEARS (Genomic Enumeration of Antibiotic Resistance in Space) investigation surveys the orbiting laboratory for antibiotic-resistant organisms. Genetic analysis could provide knowledge that informs measures to protect astronauts on future long-duration missions Credit: NASA Understanding Inflammation and Blood Clotting Microgravity takes a toll on the human body and studies have shown that astronauts have had cases of inflammation and abnormally regulated blood clotting. The MeF-1 (Megakaryocytes Orbiting in Outer Space and Near Earth: The MOON Study (Megakaryocyte Flying-One)) investigation will conduct research on how the conditions in microgravity can impact the creation and function of platelets and bone-marrow megakaryocytes. Megakaryocytes, and their progeny, platelets, are key effector cells bridging the inflammatory, immune, and hemostatic continuum. This experiment could help scientists learn about the concerns caused by any changes in the formation of clots, inflammation, and immune responses both on Earth and during spaceflight. A scanning electron-microscopy image of human platelets taken at the NASA Space Radiation Laboratory NASA Space Radiation Laboratory Building the Space Salad Bar The work continues to grow food in the harsh environment of space that is both nutritious and safe for humans to consume. With Plant Habitat-07, research continues on ‘Outredgeous’ romaine lettuce, first grown on the International Space Station in 2014. This experiment will sprout this red lettuce in microgravity in the space station’s Advanced Plant Habitat and study how optimal and suboptimal moisture conditions impact plant growth, nutrient content, and the plant microbiome. The knowledge gained will add to NASA’s history of growing vegetables in space and could also benefit agriculture on Earth. Pace crop production scientist Oscar Monje harvests Outredgeous romaine lettuce for preflight testing of the Plant Habitat-07 experiment inside a laboratory at the Space Systems Processing Facility at NASA’s Kennedy Space Center in Florida NASA/Ben Smegelsky Mixing Moss with Space Radiation ARTEMOSS (ANT1 Radiation Tolerance Experiment with Moss in Orbit on the Space Station) continues research that started on Earth with samples of Antarctic moss that underwent simulated solar radiation at the NASA Space Radiation Lab at Brookhaven National Lab in Upton, New York. After exposure to radiation some of the moss samples will spend time on the orbiting outpost in the microgravity environment and some will remain on the ground in the 1g environment. ARTEMOSS will study how Antarctic moss recovers from any potential damage from ionizing radiation exposure when plants remain on the ground and when plants grow in spaceflight microgravity. This study leads the way in understanding the effects of combined simulated cosmic ionizing radiation and spaceflight microgravity on live plants, providing more clues to plant performance in exploration missions to come. An example of moss plants grown for the ARTEMOSS mission Credit: NASA Enabling Communication in Space Between Quantum Computers The SEAQUE (Space Entanglement and Annealing Quantum Experiment) will experiment with technologies that, if successful, will enable communication on a quantum level using entanglement. Researchers will focus on validating in space a new technology, enabling easier and more robust communication between two quantum systems across large distances. The research from this experiment could lead to developing building blocks for communicating between equipment such as quantum computers with enhanced security. A quantum communications investigation, called SEAQUE (Space Entanglement and Annealing Quantum Experiment), is pictured as prepared for launch to the International Space Station on NASA’s SpaceX 31st commercial resupply services mission. The investigation is integrated on a MISSE-20 (Materials International Space Station Experiment) device, which is a platform for experiments on the outside of space station exposing instrumentation directly to the space environment. SEAQUE will conduct experiments in quantum entanglement while being exposed to the radiation environment of space Credit: NASA Related resources: SoFIE-MIST (Solid Fuel Ignition and Extinction – Material Ignition and Suppression Test) SoFIE (Solid Fuel Ignition and Extinction) | Glenn Research Center | NASA GEARS Space Station to Host ‘Self-Healing’ Quantum Communications Tech Demo – NASA MeF1 (Megakaryocyte Flying-One) ARTEMOSS NASA’s Biological and Physical Sciences Division pioneers scientific discovery and enables exploration by using space environments to conduct investigations not possible on Earth. Studying biological and physical phenomenon under extreme conditions allows researchers to advance the fundamental scientific knowledge required to go farther and stay longer in space, while also benefitting life on Earth. Explore More 3 min read Europa Trek: NASA Offers a New Guided Tour of Jupiter’s Ocean Moon Article 22 hours ago 2 min read NASA Reveals Prototype Telescope for Gravitational Wave Observatory Article 2 days ago 2 min read Hubble Captures a New View of Galaxy M90 Article 6 days ago View the full article
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NASA’s work, including its Moon to Mars exploration approach, is advancing science and technology for the Artemis Generation, while also driving significant economic growth across the United States, the agency announced Thursday. In its third agencywide economic impact report, NASA highlighted how its Moon to Mars activities, climate change research and technology development, and other projects generated more than $75.6 billion in economic output across all 50 states and Washington, D.C., in fiscal year 2023. “To invest in NASA is to invest in American workers, American innovation, the American economy, and American economic competitiveness,” says NASA Administrator Bill Nelson. “Our work doesn’t just expand our understanding of the universe — it fuels economic growth, inspires future generations, and improves our quality of life. As we embark on the next great chapter of exploration, we are proud to help power economic strength, job creation, scientific progress, and American leadership on Earth, in the skies, and in the stars.” Combined, NASA’s missions supported 304,803 jobs nationwide, and generated an estimated $9.5 billion in federal, state, and local taxes throughout the United States. The study found NASA’s Moon to Mars activities generated more than $23.8 billion in total economic output and supported an estimated 96,479 jobs nationwide. For investments in climate research and technology, the agency’s activities generated more than $7.9 billion in total economic output and supported an estimated 32,900 jobs in the U.S. Additional key findings of the study include: Every state in the country benefits economically through NASA activities. Forty-five states have an economic impact of more than $10 million. Of those 45 states, eight have an economic impact of $1 billion or more. The agency’s Moon to Mars initiative, which includes the Artemis missions, generated nearly $2.9 billion in tax revenue. These activities provided about 32% of NASA’s economic impact. The agency’s investments in climate change research and technology generated more than $1 billion in tax revenue. Approximately 11% of NASA’s economic impacts are attributable to its investments in climate change research and technology. NASA had more than 644 active international agreements for various scientific research and technology development activities in the 2023 fiscal year. The International Space Station, representing 15 countries and five space agencies, has a predominant role in the agency’s international partnerships. In fiscal year 2023, NASA oversaw 2,628 active domestic and international non-procurement partnership agreements, which included 629 new domestic and 109 new international agreements, active partnerships with 587 different non-federal partners across the U.S., and partnerships in 47 of 50 states. NASA Spinoffs, which are public products and processes that are developed with NASA technology, funding, or expertise, provide a benefit to American lives beyond dollars and jobs. As of result of NASA missions, our fiscal year 2023 tech transfer activities produced 1,564 new technology reports, 40 new patent applications, 69 patents issued, and established 5,277 software usage agreements. Scientific research and development, which fuels advancements in science and technology that can help improve daily life on Earth and for humanity, is the largest single-sector benefitting from NASA’s work, accounting for 19% of NASA’s total economic impact. The study was conducted by the Nathalie P. Voorhees Center for Neighborhood and Community Improvement at the University of Illinois at Chicago. To review the full report, visit: https://go.nasa.gov/3NEtUIq -end- Meira Bernstein / Melissa Howell Headquarters, Washington 202-615-1747 / 202-961-6602 meira.b.bernstein@nasa.gov / melissa.e.howell@nasa.gov Share Details Last Updated Oct 24, 2024 LocationNASA Headquarters View the full article
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3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Expedition 64 Flight Engineer Victor Glover of NASA sips on a water bag. The latest book marks our third effort to review available literature regarding the role of nutrition in astronaut health. In 2009, we reviewed the existing knowledge and history of human nutrition for spaceflight, with a key goal of identifying additional data that would be required before NASA could confidently reduce the risk of an inadequate food system or inadequate nutrition to as low as possible in support of human expeditions to the Moon or Mars. We used a nutrient-by-nutrient approach to address this effort, and we included a brief description of the space food systems during historical space programs. In 2014, we published a second volume of the book, which was not so much a second edition, but rather a view of space nutrition from a different perspective. This volume updated research that had been published in the intervening 6 years and addressed space nutrition with a more physiological systems-based approach. The current version is an expanded, updated version of that second book, providing both a systems approach overall, but also including details of nutrients and their roles within each system. As such, this book is divided into chapters based on physiological systems (e.g., bone, muscle, ocular); highlighted in each chapter are the nutrients associated with that particular system. We provide updated information on space food systems and constraints of the same, and provide dietary intake data from International Space Station (ISS) astronauts. We present data from ground-based analog studies, designed to mimic one or more conditions similar to those produced by spaceflight. Head-down tilt bed rest is a common analog of the general (and specifically musculoskeletal) disuse of spaceflight. Nutrition research from Antarctica relies on the associated confinement and isolation, in addition to the lack of sunlight exposure during the winter months. Undersea habitats help expand our understanding of nutritional changes in a confined space with a hyperbaric atmosphere. We also review spaceflight research, including data from now “historical” flights on the Space Shuttle, data from the Russian space station Mir, and earlier space programs such as Apollo and Skylab. The ISS, now more than 20 years old, has provided (and continues to provide) a wealth of nutrition findings from extended-duration spaceflights of 4 to 12 months. We review findings from this platform as well, providing a comprehensive review of what is known regarding the role of human nutrition in keeping astronauts healthy. With this latest book, we hope we have accurately captured the current state of the field of space food and nutrition, and that we have provided some guideposts for work that remains to be done to enable safe and successful human exploration beyond low-Earth orbit. Human Adaptation to Spaceflight: The Role of Food and Nutrition – 2nd Edition Download 2nd Edition PDF Human Adaptation to Spaceflight: The Role of Food and Nutrition – 1st Edition Download 1st Edition PDF Education and Outreach Share Details Last Updated Oct 23, 2024 EditorRobert E. LewisLocationJohnson Space Center Related TermsHuman Health and Performance Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article
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Dr. Nipa Phojanamongkolkij does not always do things the traditional way. As a systems engineer (SE) at Langley Research Center working closely with the Aeronautics Research Mission Directorate, Nipa pushes boundaries and draws connections where few others would think to look. When she envisioned a way to use ChatGPT to help SE teams working on the Advanced Air Mobility Mission, she presented her initial idea to her team wondering, “Is this crazy?” Her idea evolved into a successful prototype, which is now used for air traffic management in the Airspace Operations and Safety Program. She has also leveraged natural language programming and NASA’s database of lessons learned to create a bot for flagging potential risks and mitigations in real time. Nipa’s journey in becoming the digital transformer she is today involves her ability to combine engineering principles and business outcomes with creative, human-centered approaches. Nipa received an MS and PhD in industrial and systems engineering from Arizona State University after moving to the United States from Bangkok, Thailand, where she received her BS degree in electronics engineering. She joined NASA 15 years ago after honing her data analysis and process improvement skills in the business sector at Pepsi Corporation. Her previous experience molded her focus on demonstrating benefit and return on investment. In addition to a business-oriented mindset, Nipa credits much of her success at NASA to her abilities as an active listener, which helps her understand customer needs and address paint points. One cross-cutting challenge Nipa noticed within the agency’s approach to SE was the issue of silos, particularly in handling requirements and research data. Many engineers stored information in documents on individual computers or SharePoint folders, making it difficult to share data and draw connections across missions, directorates, and centers. As a systems engineer, Nipa and her team work to pull these disparate elements into a connected digital format using methodology called model-based systems engineering (MBSE). “You can think of it like a gigantic database where you have everything connected—a table of research papers, a table of requirements, and a table of concept of operations documents,” she says. However, using and leveraging this system requires specialized knowledge of the MBSE discipline and modeling language. To centralize system concept, architecture, and requirement data while democratizing access to it, Nipa conceived a way to leverage ChatGPT as an intermediary between the user and database. In fiscal year 2023, she received funding for her idea as a Digital Transformation Prototype Test, “Requirement Discovery Using Embedded Knowledge Graph with ChatGPT.” Nipa and her team developed a web-based dashboard that translates user questions into database queries and turns the database responses back into readable answers for the user. Nipa and her team curated the research used to create the database, reducing the chances of AI hallucination and misinformation. Using ChatGPT as a translator, general users benefitted from the system without needing to know how to formulate graph database queries. Requirement creation through this system was seven times faster than traditional processes and yielded results comparable to those created by subject matter experts. In some cases, the approach even resulted in more creative requirements than human-generated ones. Nipa’s prototype allowed SEs to more efficiently analyze connections between existing requirements, predict new connections, and generate new requirements, streamlining critical processes for her team. The approach could benefit SEs across NASA centers, directorates, and missions and holds exciting potential for other use cases, such as generating candidate requirements and analyzing project risk. According to NASA Digital Engineering Lead Terry Hill, “The future of engineering is understanding how to do it from a data-centric perspective. Enabling the use of new and evolving technologies like artificial intelligence, machine learning, and large language models will aid our engineers to accomplish greater things and augment our workforce.” Nipa and her team were recognized for their innovative work, receiving a Systems Engineering Technical Excellence Award (SETEA) in 2024 under the “Advancement of SE” category. Nipa’s out-of-the-box thinking has also positioned her as a trailblazer amongst her peers. “Nipa was ahead of everyone in terms of understanding what Digital Transformation is,” says Ian Levitt, Concepts Team Manager at Langley Research Center and co-lead on the Requirement Discovery Prototype Test. “She is extremely smart as well as practical, which is a rare combination. She has wonderful insights and helps me see more clearly what I am trying to do.” As a leader in the Digital Transformation community, Nipa recognizes the importance of collaboration, noting that her transformative work would not have been successful without her team. Their trust is what makes her ideas possible, along with Digital Transformation’s willingness to take chances on innovative, cutting-edge ideas. “They’re at the forefront of technology, so they’re receptive to high-risk projects,” she says. “That’s why I enjoy working with the Digital Transformation team.” In turn, Nipa is excited to continue building community and momentum around transformation initiatives. Her team’s work inspired one group at Johnson Space Center to replicate their requirement discovery approach, and she has received multiple inquiries for demos on their prototype. Seeing how her work inspires and impacts others at the agency is one way she measures success. Whether she is connecting data sources or people, Nipa continues to push toward a more unified NASA, exemplifying what it means to be a digital transformer. View the full article
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2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Hundreds of students, scientists, and other stakeholders listen in person and online as NASA leaders discuss the Artemis missions during the 2023 von Braun Space Exploration Symposium held Oct. 25–27 at the University of Alabama in Huntsville. NASA / Charles Beason Media are invited to attend the 2024 von Braun Space Exploration Symposium Monday Oct. 28 to Wednesday, Oct. 30 at the University of Alabama in Huntsville. Organized by the American Astronautical Society in collaboration with NASA’s Marshall Space Flight Center in Huntsville, the annual symposium gathers leaders from across government, industry, policy, and academia to discuss the current landscape of space exploration and chart a path forward amid the challenges that lie ahead. The theme of this year’s event is “Expanding Exploration: From Vision to Reality,” focusing on NASA’s and Marshall’s plans for the future and the broader discourse about exploration and discovery, technology, the workforce, and other elements of the space ecosystem. Media members interested should register with the astronautical society as a media representative under these guidelines for in-person or online attendance. Marshall Center Director Joseph Pelfrey will deliver opening remarks on Oct. 28, followed by panels on Artemis, artificial intelligence, and workforce development. NASA Deputy Associate Administrator Casey Swails will deliver a keynote address to close out the first day. Panels on, Oct. 29, will focus on space nuclear propulsion, science, and lunar logistics and mobility. Col. Eric Zarybnisky, Office of Space Launch director at the National Reconnaissance Office, will provide the luncheon keynote. The third and final day of the symposium Oct. 30, will include discussions on nuclear propulsion, space technology, and human exploration beyond low-Earth orbit. NASA Associate Administrator Jim Free and Wayne Hale, who retired in 2010 as the deputy associate administrator of strategic partnerships at NASA Headquarters in Washington, will lead a discussion and present awards at the closing luncheon. To arrange interviews with NASA Marshall speakers, contact Hannah Maginot, 256-932-1937, or Molly Porter, 256-424-5158. For more information on NASA’s Marshall Space Flight Center, visit: https://www.nasa.gov/marshall Hannah Maginot Marshall Space Flight Center, Huntsville, Ala. hannah.l.maginot@nasa.gov 256-932-1937 Molly Porter Marshall Space Flight Center, Huntsville, Ala. molly.a.porter@nasa.gov 256-424-5158 Share Details Last Updated Oct 23, 2024 EditorBeth RidgewayContactMolly Portermolly.a.porter@nasa.govLocationMarshall Space Flight Center Related TermsMarshall Space Flight Center Explore More 19 min read The Marshall Star for October 23, 2024 Article 1 hour ago 4 min read NASA Begins New Deployable Solar Array Tech Demo on Pathfinder Spacecraft Article 5 hours ago 5 min read NASA’s IXPE Helps Researchers Determine Shape of Black Hole Corona Article 6 days ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article
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19 Min Read The Marshall Star for October 23, 2024 Editor’s Note: Starting Nov. 4, the Office of Communications at NASA’s Marshall Space Flight Center will no longer publish the Marshall Star on nasa.gov. The last public issue will be Oct. 30. To continue reading Marshall news, visit nasa.gov/marshall. Habitation Systems Business Unit Spotlight: Living and Working in Space For centuries, humans have dreamed of the ability to live safely on the Moon and Mars. At NASA’s Marshall Space Flight Center, team members supporting habitation systems development bring that dream closer to reality by envisioning and shaping humanity’s future in deep space and on the surface of other worlds. Marshall’s Habitation Systems business unit – the center’s featured organization for October – develops the next generation of habitation systems to make living and working in space and on planetary bodies possible. These efforts are carried out through the Habitation Systems Development Office, in which the team works across programmatic and engineering organizations to support formulation activities for planetary surface habitation (Moon and Mars), transit habitats for deep space exploration, and the Gateway program. In addition, the Marshall team collaborates with commercial partners on future habitation concept development and risk reduction activities through NextSTEP Appendix A: Habitation Systems and Reimbursable Space Act Agreements. Seth BellNASA Seth Bell is currently the technical monitor for NASA’s commercial partner Sierra Space. Sierra has executed both full scale and subscale inflatable habitat burst tests at Marshall’s East Test Area. Bell has worked as a subsystem manager for the Mars Ascent Vehicle and as a system’s engineer and Engineering Directorate integrator. “I am excited to eventually see softgood inflatables in low Earth orbit,” Bell said. “Seeing the success of the many teams working in this office is exciting, especially after developing so many lasting relationships and putting so much time and energy into this work.” Yancy YoungNASA Since joining NASA in 2008, Yancy Young has served in multiple positions, including manager of several International Space Station research projects and Launch Package manager for Gateway Co-manifested Payloads. Currently, Young is the technical monitor for Boeing efforts under NASA’s NextSTEP Appendix A Broad Agency Announcement (BAA) for the development of deep space habitation concepts. “I love being a part of laying the foundation for long term deep space exploration,” Young said. Boeing’s current focus is a Design Analysis Cycle investigating the benefits and challenges of using composite materials in a pressurized Lunar Surface Habitat. Brooke ThorntonNASA In her 25-plus years at NASA, Brooke Thornton has worked on everything from ionized space radiation analysis to Earth observing satellites. Currently, Thornton is the industry engagement manager for the Habitation Systems Development Office and Strategy and Architecture Office. Thornton manages NextSTEP-2 Appendix A-Habitation Systems and Appendix R-Logistics and Mobility Systems BAA. In addition, Thornton fosters collaboration between industry and NASA for the Moon to Mars mission. “I am excited about working with industry to develop the elements and concepts of operations for humans to live on the Moon and beyond,” Thornton said. › Back to Top Team Members Enjoy Marshall Exchange BBQ Fest Joseph Pelfrey, center, director of NASA’s Marshall Space Flight Center, talks with team members during the BBQ Fest hosted by the Marshall Exchange on Oct. 21. The event was held on the walking trail behind the Wellness Center and was open to team members, their family members, and retirees. “My thanks to those who came out to this year’s BBQ – and especially to those who helped make it happen,” Pelfrey said. “I could not have asked for better weather or a better group of people to spend the afternoon with. It was great to see everyone’s families join us on site to celebrate the hard work our teams have put in this year.” (NASA/Charles Beason) Children play on an inflatable at the BBQ Fest with a space shuttle inflatable in the background. (NASA/Charles Beason) Marshall team members participate in Bingo during the BBQ hosted by the Marshall Exchange. (NASA/Charles Beason) › Back to Top Tony Clark Named Deputy Director of Marshall’s Engineering Directorate Tony Clark has been named to the Senior Executive Service position of deputy director of the Engineering Directorate at NASA’s Marshall Space Flight Center, effective immediately. In this role, Clark will be help lead the center’s largest organization, comprised of more than 2,500 civil service and contractor personnel, who design, test, evaluate, and operate flight hardware and software associated with Marshall-developed space transportation and spacecraft systems, science instruments, and payloads. Tony Clark has been named to the Senior Executive Service position of deputy director of the Engineering Directorate at NASA’s Marshall Space Flight Center.NASA Clark previously served as deputy director of the Space Systems Department at Marshall from 2021-2024 and served as acting director in 2024. In this role, Clark led the design, development, assembly, integration, testing, and delivery of flight, ground, prototype, and development products for NASA human spaceflight programs, science investigations, and exploration initiatives. He aided in the oversight of an annual budget of approximately $70 million and helped manage a diverse, highly technical workforce of approximately 660 civil service employees and contractors. Over his three decades of service to NASA, Clark has held numerous key leadership roles, bringing a wealth of technical and supervisory experience to Marshall’s broad range of engineering endeavors. He served as manager of the vehicle equipment area in Johnson Space Center’s Vehicle Systems Integration Office of the Gateway Program from 2018-2021. He was also manager of the Engineering Resource Management Office in Marshall’s Engineering Directorate from 2014-2018, tasked with leading and coordinating resources among eight engineering departments, laboratories and offices staffed by more than 2,300 civil service and contract personnel. He was acting deputy manager of the Engineering Directorate’s Spacecraft and Vehicle Systems Department from February 2014 to October 2014. Prior to that, Clark was chief of the directorate’s Electrical Integration and Fabrication Division from 2007-2014, and chief of the Electromagnetic Environmental Effects and Electrical Integration Branch from 2004-2007. He joined Marshall in September 1991 as an electromagnetic environmental effects engineer. Clark earned a bachelor’s degree in electrical engineering from Tennessee Technological University in Cookeville in 1989 and a master’s degree in electrical engineering from The Ohio State University in Columbus in 1991. Among his many professional awards and honors, Clark received the NASA Exceptional Achievement Medal in 2010 for his work on the Ares IX, the launch vehicle which informed development of NASA’s new rocket, the Space Launch System. He also received a Silver Snoopy award in 1999, reflecting outstanding service and the highest dedication to safe human spaceflight. Clark was a founding member in 2004 of the Huntsville Chapter of the Institute of Electrical and Electronic Engineers’ Electromagnetic Compatibility Society. › Back to Top I Am Artemis: Sarah Ryan A passion for puzzles, problem-solving, and propulsion led Sarah Ryan – a native of Columbus, Ohio – to her current position as Raptor engine lead for NASA’s HLS (Human Landing System) insight team at NASA’s Marshall Space Flight Center. The SpaceX Raptor rocket engine powers the company’s Starship and Super Heavy rocket. SpaceX will land astronauts on the Moon for NASA’s Artemis III and Artemis IV missions using the Starship HLS. NASA’s Artemis campaign aims to land the first woman, first person of color, and first international partner astronaut on the Moon. NASA’s Sarah Ryan is the Raptor engine lead for NASA’s HLS (Human Landing System) Program at NASA’s Marshall Space Flight Center. “With Artemis, we’re moving beyond what NASA did with Apollo and that’s really inspiring, especially to our younger workforce. We’re trying to push farther and it’s really going to drive a lot of technology development on the way there,” Ryan said. “This is a dream come true to be working on Artemis and solving problems so humanity can get back to the Moon then on to Mars.”NASA/Ken Hall “My team looks at how the components of the Raptor engine work together. Then, we evaluate the performance of the full system to make sure it will accomplish the NASA HLS and Artemis missions,” Ryan said. “I get to see lots of pieces and parts of the puzzle and then look at the system as a whole to make sure it meets NASA’s needs.” While earning a bachelor’s degree from Case Western Reserve University in Cleveland with a dual major in aerospace engineering and mechanical engineering, Ryan had an internship at Marshall, working on a payload for a science mission onboard the International Space Station. After working for a year on satellite design, Ryan returned to Marshall. She noted that the opportunity to work in Marshall’s Engine Systems branch, to be involved with pushing technology forward, and to work on Artemis, really drew her back to NASA. Ryan later earned a master’s degree in aerospace systems from the University of Alabama in Huntsville. When not occupied with rocket engine development, Ryan likes to work on quieter hobbies in her free time, including reading, board games, crocheting, and solving all manner of puzzles – crosswords, number games, word games, and more. Her interest for solving puzzles carries over into her work on the Raptor rocket engines for HLS. “My favorite tasks are the ones that most resemble a puzzle,” Ryan said. “If we’re investigating an issue and have a lot of information to assess, I love putting all the pieces together and figuring out what happened, why, and the path forward. I enjoy digging into the data and solving those puzzles.” 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. › Back to Top I Am Artemis: Casey Wolfe While precision, perseverance, and engineering are necessary skills in building a Moon rocket, Casey Wolfe knows that one of the most important aspects for the job is teamwork. “Engineering is vital, but to get this type of work done, you need to take care of the human element,” said Wolfe, the assistant branch chief of the advanced manufacturing branch in the Materials and Processes Laboratory at NASA’s Marshall Space Flight Center. Casey Wolfe is developing and producing the next generation payload adapter for NASA’s SLS (Space Launch System) super-heavy lift rocket. The adapter is made with some of the world’s most advanced composite manufacturing techniques.NASA/Sam Lott Together with her team, Wolfe is developing and producing the next generation payload adapter for NASA’s SLS (Space Launch System) super-heavy lift rocket. The adapter is made with some of the world’s most advanced composite manufacturing techniques. Wolfe’s work integrates the technical day-to-day operations and personnel management of the composites manufacturing team and additive manufacturing team, balancing production of SLS hardware with the creation of new engines using the latest manufacturing technologies. “A lot of my day to day is in managing our two teams, making connections, building relationships, and making sure people feel supported,” Wolfe said. “I conduct individual tag ups with each team member so we can be proactive about anticipating and addressing problems.” Wolfe grew up in Huntsville, a place known as the “Rocket City,” but it wasn’t until she visited a job fair while studying at Auburn University for a polymer and fiber engineering degree that she began to consider a career at Marshall. Wolfe applied for and was selected to be a NASA intern through the Pathways Program, working in the non-metallic materials branch of the Materials and Processes Laboratory. Wolfe supported a coating system for electrostatic discharge on the first uncrewed test flight of the Orion spacecraft. Launching Dec. 5, 2014, Orion traveled to an altitude of 3,600 miles, orbited Earth twice, and splashed down in the Pacific Ocean. It was during her internship that Wolfe realized how inspirational it felt to be treated like a vital part of a team. “The SLS program gave everyone permission to sign the hardware, even me – even though I was just an intern,” Wolfe said. “It was impactful to me, knowing that something I had worked on had my name on it and went to space.” Since being hired by NASA, Wolfe’s work has supported development of the Orion stage adapter diaphragms for Artemis II and Artemis III, and the payload adapters for Artemis IV and beyond. The first three Artemis flights use the SLS Block 1 rocket variant, which can send more than 27 metric tons (59,500 pounds) to the Moon in a single launch. Beginning with Artemis IV, the SLS Block 1B variant will use the new, more powerful exploration upper stage to enable more ambitious missions to deep space, with the cone-shaped payload adapter situated atop the rocket’s exploration upper stage. The new variant will be capable of launching more than 38 metric tons (84,000 pounds) to the Moon in a single launch. “While the engineering development unit of the payload adapter is undergoing large-scale testing, our team is working on the production of the qualification article, which will also be tested,” Wolfe said. “Flight components should be starting fabrication in the next six months.” When Wolfe isn’t working, she enjoys hiking, gardening, and hanging out with her dogs and large family. Recently, she signed another piece of SLS hardware headed to space: the Orion stage adapter for the second Artemis mission. With as many responsibilities as Wolfe juggles, it’s easy to lose sight of her work’s impact. “I work in the lab around the hardware all the time, and in many ways, it can become very rote,” she said. But Wolfe won’t forget what she saw one evening when she worked late: “Everybody was gone, and as I walked past the launch vehicle stage adapter, there were two security guards taking pictures of each other in front of it. It was one of those things that made me step back and reflect on what my team accomplishes every day: making history happen.” NASA is working to land the first woman, first person of color, and its first international partner astronaut on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, supporting ground systems, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single launch. › Back to Top NASA’s IXPE Helps Researchers Determine Shape of Black Hole Corona By Rick Smith New findings using data from NASA’s IXPE (Imaging X-ray Polarimetry Explorer) mission offer unprecedented insight into the shape and nature of a structure important to black holes called a corona. A corona is a shifting plasma region that is part of the flow of matter onto a black hole, about which scientists have only a theoretical understanding. The new results reveal the corona’s shape for the first time, and may aid scientists’ understanding of the corona’s role in feeding and sustaining black holes. This illustration of material swirling around a black hole highlights a particular feature, called the “corona,” which can be seen as a purple haze floating above the underlying accretion disk and extending slightly inside its inner edge. The material within the inner accretion disk is incredibly hot and would glow with a blinding blue-white light, but here has been reduced in brightness to make the corona stand out with better contrast. Its purple color is purely illustrative, standing in for the X-ray glow that would not be obvious in visible light. The warp in the disk is a realistic representation of how the black hole’s immense gravity acts like an optical lens, distorting our view of the flat disk that encircles it.NASA/Caltech-IPAC/Robert Hurt Many black holes, so named because not even light can escape their titanic gravity, are surrounded by accretion disks, debris-cluttered whirlpools of gas. Some black holes also have relativistic jets – ultra-powerful outbursts of matter hurled into space at high speed by black holes that are actively eating material in their surroundings. Less well known, perhaps, is that snacking black holes, much like Earth’s Sun and other stars, also possess a superheated corona. While the Sun’s corona, which is the star’s outermost atmosphere, burns at roughly 1.8 million degrees Fahrenheit, the temperature of a black hole corona is estimated at billions of degrees. Astrophysicists previously identified coronae among stellar-mass black holes – those formed by a star’s collapse – and supermassive black holes such as the one at the heart of the Milky Way galaxy. “Scientists have long speculated on the makeup and geometry of the corona,” said Lynne Saade, a postdoctoral researcher at NASA’s Marshall Space Flight Center and lead author of the new findings. “Is it a sphere above and below the black hole, or an atmosphere generated by the accretion disk, or perhaps plasma located at the base of the jets?” Enter IXPE, which specializes in X-ray polarization, the characteristic of light that helps map the shape and structure of even the most powerful energy sources, illuminating their inner workings even when the objects are too small, bright, or distant to see directly. Just as we can safely observe the Sun’s corona during a total solar eclipse, IXPE provides the means to clearly study the black hole’s accretion geometry, or the shape and structure of its accretion disk and related structures, including the corona. “X-ray polarization provides a new way to examine black hole accretion geometry,” Saade said. “If the accretion geometry of black holes is similar regardless of mass, we expect the same to be true of their polarization properties.” IXPE demonstrated that, among all black holes for which coronal properties could be directly measured via polarization, the corona was found to be extended in the same direction as the accretion disk – providing, for the first time, clues to the corona’s shape and clear evidence of its relationship to the accretion disk. The results rule out the possibility that the corona is shaped like a lamppost hovering over the disk. The research team studied data from IXPE’s observations of 12 black holes, among them Cygnus X-1 and Cygnus X-3, stellar-mass binary black hole systems about 7,000 and 37,000 light-years from Earth, respectively, and LMC X-1 and LMC X-3, stellar-mass black holes in the Large Magellanic Cloud more than 165,000 light-years away. IXPE also observed a number of supermassive black holes, including the one at the center of the Circinus galaxy, 13 million light-years from Earth, and those in galaxies NGC 1068 and NGC 4151, 47 million light-years away and nearly 62 million light-years away, respectively. Stellar mass black holes typically have a mass roughly 10 to 30 times that of Earth’s Sun, whereas supermassive black holes may have a mass that is millions to tens of billions of times larger. Despite these vast differences in scale, IXPE data suggests both types of black holes create accretion disks of similar geometry. That’s surprising, said Marshall astrophysicist Philip Kaaret, principal investigator for the IXPE mission, because the way the two types are fed is completely different. “Stellar-mass black holes rip mass from their companion stars, whereas supermassive black holes devour everything around them,” he said. “Yet the accretion mechanism functions much the same way.” That’s an exciting prospect, Saade said, because it suggests that studies of stellar-mass black holes – typically much closer to Earth than their much more massive cousins – can help shed new light on properties of supermassive black holes as well. The team next hopes to make additional examinations of both types. Saade anticipates there’s much more to glean from X-ray studies of these behemoths. “IXPE has provided the first opportunity in a long time for X-ray astronomy to reveal the underlying processes of accretion and unlock new findings about black holes,” she said. The complete findings are available in the latest issue of The Astrophysical Journal. Smith, an Aeyon employee, supports the Marshall Office of Communications. › Back to Top Michoud Gets a Rare Visitor The Oort Cloud comet, called C/2023 A3 Tsuchinshan-ATLAS, passes over Southeast Louisiana near New Orleans, home of NASA’s Michoud Assembly Facility on Oct. 13. The comet is making its first appearance in documented human history; it was last seen in the night sky 80,000 years ago. The Tsuchinshan-ATLAS comet made its first close pass by Earth in mid-October and will remain visible to viewers in the Northern Hemisphere just between the star Arcturus and planet Venus through early November. Eric Bordelon, a photographer for Michoud, captured the image, which was featured as NASA’s image of the day. “On Sunday evening I decided to head out to find the comet I’ve read so much about,” Bordelon said. “Struggling at first to see it, once my eyes adjusted to the darkness I could faintly see it. I pulled my camera out and set up a tripod, with a longer exposure around six seconds I was able to capture this shot with a single frame. The far off setting sun made a beautiful color gradient in the dark sky with the other stars just beginning to appear.” Read more about the comet. (NASA/Eric Bordelon) › Back to Top Hubble Captures New View of Galaxy M90 A new NASA/ESA Hubble Space Telescope image features the striking spiral galaxy Messier 90 (M90, also NGC 4569), located in the constellation Virgo. In 2019, Hubble released an image of M90 created with Wide Field and Planetary Camera 2 (WFPC2) data taken in 1994, soon after its installation. That WFPC2 image has a distinctive stair-step pattern due to the layout of its sensors. Wide Field Camera 3 (WFC3) replaced WFPC2 in 2009 and Hubble used WFC3 when it turned its aperture to Messier 90 again in 2019 and 2023. That data resulted in this stunning new image, providing a much fuller view of the galaxy’s dusty disk, its gaseous halo, and its bright core. This eye-catching image offers us a new view of the spiral galaxy Messier 90 from the NASA/ESA Hubble Space Telescope. ESA/Hubble & NASA, D. Thilker, J. Lee and the PHANGS-HST Team The inner regions of M90’s disk are sites of star formation, seen here in red H-alpha light from nebulae. M90 sits among the galaxies of the relatively nearby Virgo Cluster, and its orbit took M90 on a path near the cluster’s center about three hundred million years ago. The density of gas in the inner cluster weighed on M90 like a strong headwind, stripping enormous quantities of gas from the galaxy and creating the diffuse halo we see around it. This gas is no longer available to form new stars in M90, with the spiral galaxy eventually fading as a result. M90 is located 55 million light-years from Earth, but it’s one of the very few galaxies getting closer to us. Its orbit through the Virgo cluster has accelerated so much that M90 is in the process of escaping the cluster entirely. By happenstance, it’s moving in our direction. Astronomers have measured other galaxies in the Virgo cluster at similar speeds, but in the opposite direction. As M90 continues to move toward us over billions of years, it will also be evolving into a lenticular galaxy. › Back to Top View the full article
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NASA’s SpaceX Crew-8 Re-entry and Splashdown
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Astronaut and Artemis II pilot, Victor Glover, maneuvers the latch handle on an Orion test side hatch during performance evaluations at the Lockheed Martin Space campus in Littleton, Colorado.Photo credit: Lockheed Martin Artemis II NASA astronauts Victor Glover, Christina Koch, and Reid Wiseman, and CSA (Canadian Space Agency) astronaut Jeremy Hansen recently traveled to Lockheed Martin Space in Littleton, Colorado, where they practiced opening and closing an Orion crew module side hatch model to help demonstrate its reliability and durability during their 10-day mission around the Moon. During normal mission operations, the crew will not operate the hatches – the ground systems team at NASA’s Kennedy Space Center in Florida will assist the crew into Orion at the launch pad, then close the hatch behind them prior to liftoff. After splashdown in the Pacific Ocean, recovery teams will open the side hatch and help crew to exit. Back-up crew members Andre Douglas of NASA and Jenni Gibbons of CSA also trained on hatch operations, which help ensure the crew can safely enter and exit the spacecraft in the event of an emergency. The side hatch is normally opened using a manual gearbox system, but in an emergency, the hatch has release mechanisms containing small pyrotechnic (explosive) devices that release the latch pins on the hatch instantaneously, allowing the hatch to open quickly. Under NASA’s Artemis campaign, the agency will establish the foundation for long-term scientific exploration at the Moon, land the first woman, first person of color, and its first international partner astronaut on the lunar surface, and prepare for human expeditions to Mars for the benefit of all. View the full article
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The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) America Reyes Wang, Sepideh Khajehei, Julie Nottage, and Ryan Felton. Their commitment to the NASA mission represents the talent, camaraderie, and vision needed to explore this world and beyond. Space Biosciences Star: America Reyes Wang America Reyes Wang serves as the Space Biology Biospecimen Sharing Program (BSP) Lead in the Space Biosciences Research Branch, where she guides a team of support scientists and a logistics coordinator in planning and performing detailed, collaborative dissections to maximize the scientific return from biological investigations. Under her leadership, the BSP team has contributed over 5,000 samples to the NASA Biological Institutional Scientific Collection (NBISC), approximately half of which were collected in the last 10 months. Earth Science Star: Sepideh Khajehei Sepideh Khajehei is a NASA Earth eXchange (NEX) Data and Research Scientist in the Biospheric Science Branch, for the Bay Area Environmental Research Institute. She is recognized for her dedicated support of the NASA Administrator’s Earth Information Center, and recently for her outstanding support for an urgent request to revise climate indices just days before the October 7, 2024, opening of NASA’s Hometown Climate Dashboard at the Smithsonian Institute in Washington, D.C. Space Science & Astrobiology Star: Julie Nottage Julie Nottage continuously goes above and beyond in her role as the Space and Earth Sciences Facilities Service Manager. She keeps a multi-use interdisciplinary science building running across all aspects of operations and is the go-to person for any problem. Her can-do approach and wealth of knowledge ensures the facility’s high-quality operation that enables scientists and engineers to focus on their research and instrument work. Her quality work and extensive coordination of the Voluntary Protection Program allowed these month-long inspections to run smoothly with an improved safety outcome. Space Science & Astrobiology Star: Ryan Felton Ryan Felton, a NASA Postdoctoral Management Fellow with the Exobiology Branch, is recognized for his successful coordination of an engaging community-wide seminar series focused on Artificial Intelligence/Machine Learning (AI/ML). This seminar series featured four speakers so far over six months on a variety of exciting topics to advance AI/ML knowledge and use in the branch’s research. View the full article
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NASA Associate Administrator Jim Free welcomed the Republic of Cyprus as the latest nation to commit to the responsible use of space for humanity on Wednesday, marking 46 signatories to date. “We applaud Cyprus’ commitment to the Artemis Accords, which will enhance the country’s engagement with NASA and the international community,” said Free, who participated virtually. “By joining 45 other country signatories in this effort, Cyprus will help play a role in implementing the accords and exploration that is open, responsible, transparent, and peaceful for the benefit of all.” Nicodemos Damianou, Cyprus’ deputy minister of research, innovation, and digital policy, signed the Artemis Accords during a ceremony in Nicosia, Cyprus. James O’Brian, assistant secretary for European and Eurasian Affairs for the U.S. Department of State, also attended the event. “Today marks a significant milestone for Cyprus as we officially sign the Artemis Accords,” said Damianou. “As we embark on this exciting journey, we reaffirm our commitment to a safe and responsible space exploration, as well as our strong belief in the importance of international cooperation in ensuring space is utilized to the benefit of all humanity. Cyprus, an European Union member state, is capitalizing on its geostrategic location between three continents, and aspires to play an integral role in the international space community.” The signing with Cyprus comes on the heels of an Artemis Accords meeting in Milan earlier this month with dozens of signatory countries, including the United States. In 2020, NASA, in coordination with the U.S. Department of State and seven other initial signatory nations, established the Artemis Accords, which identified an early set of principles promoting the beneficial use of space for humanity. The Artemis Accords are grounded in the Outer Space Treaty and other agreements including the Registration Convention, the Rescue and Return Agreement, as well as best practices and norms of responsible behavior that NASA and its partners have supported, including the public release of scientific data. The commitments of the Artemis Accords and efforts by the signatories to advance implementation of these principles support the safe and sustainable exploration of space. More countries are expected to sign in the coming days and weeks ahead. Learn more about the Artemis Accords at: https://www.nasa.gov/artemis-accords -end- Kathryn Hambleton / Elizabeth Shaw Headquarters, Washington 202-358-1600 kathryn.a.hambleton@nasa.gov / elizabeth.a.shaw@nasa.gov Share Details Last Updated Oct 23, 2024 LocationNASA Headquarters Related TermsOffice of International and Interagency Relations (OIIR)artemis accords View the full article