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NASA/Kim Shiflett

The Artemis II crew (from front left to back right) – pilot Victor Glover, commander Reid Wiseman, mission specialist Jeremy Hansen of CSA (Canadian Space Agency), and mission specialist Christina Koch – walk out of the Neil A. Armstrong Operations and Checkout Building at NASA’s Kennedy Space Center in Florida on Monday, Aug. 11, 2025.

During a two-day training, the crew practiced launch day operations if the Artemis II test flight launches at night.

Join the Artemis II mission and sign up to launch your name aboard the Orion spacecraft and SLS (Space Launch System) rocket alongside the crew.

Through the Artemis program, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and to build the foundation for the first crewed missions to Mars – for the benefit of all.

Image credit: NASA/Kim Shiflett

Research Astrophysicist and Roman’s Deputy Wide Field Instrument Scientist – Goddard Space Flight Center

From a young age, Ami Choi — now a research astrophysicist at NASA — was drawn to the vast and mysterious. By the fifth grade, she had narrowed her sights to two career paths: marine biology or astrophysics. 

“I’ve always been interested in exploring big unknown realms, and things that aren’t quite tangible,” Choi said. That curiosity has served her all throughout her career.

In addition to conducting research, Ami Choi shares science with the public at various outreach events, including tours at NASA’s Goddard Space Flight Center in Greenbelt, Md. This photo captures one tour stop, outside the largest clean room at Goddard.Credit: NASA/Travis Wohlrab

As a student at University Laboratory High School in Urbana, Illinois, Choi gravitated toward astrophysics and was fascinated by things like black holes. She studied physics as an undergraduate at the University of Chicago, though she says math and physics didn’t necessarily come easily to her.

“I wasn’t very good at it initially, but I really liked the challenge so I stuck with it,” Choi said.

Early opportunities to do research played a pivotal role in guiding her career. As an undergraduate, Choi worked on everything from interacting galaxies to the stuff in between stars in our galaxy, called the interstellar medium. She learned how to code, interpret data, and do spectroscopy, which involves splitting light from cosmic objects into a rainbow of colors to learn about things like their composition.

After college, Choi read an article about physicist Janet Conrad’s neutrino work at Fermilab and was so inspired by Conrad’s enthusiasm and inclusivity that she cold-emailed her to see if there were any positions available in her group. 

On October 14, 2023, Ami took a break from a thermal vacuum shift to snap a selfie with a partial eclipse. She was visiting BAE, Inc. in Boulder, Co., where the primary instrument for NASA’s Nancy Grace Roman Space Telescope was undergoing testing. Credit: Courtesy of Ami Choi

“That one email led to a year at Fermilab working on neutrino physics,” Choi said.

She went on to earn a doctorate at the University of California, Davis, where she studied weak gravitational lensing — the subtle warping of light by gravity — and used it to explore dark matter, dark energy, and the large-scale structure of the universe.

Her postdoctoral work took Choi first to the University of Edinburgh in Scotland, where she contributed to the Kilo-Degree Survey, and later to The Ohio State University, where she became deeply involved in DES (the Dark Energy Survey) and helped lay the groundwork for the Nancy Grace Roman Space Telescope — NASA’s next flagship astrophysics mission. 

“One of my proudest moments came in 2021, when the DES released its third-year cosmology results,” Choi said. “It was a massive team effort conducted during a global pandemic, and I had helped lead as a co-convener of the weak lensing team.”

Choi regularly presents information about NASA’s Nancy Grace Roman Space Telescope to fellow scientists and the public. Here, she gives a Hyperwall talk at an AAS (American Astronomical Society) meeting.Credit: Courtesy of Ami Choi

After a one-year stint at the California Institute of Technology in Pasadena, where Choi worked on SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer)—an observatory that’s surveying stars and galaxies—she became a research astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. She also serves as the deputy Wide Field Instrument scientist for Roman. Choi operates at the intersection of engineering, calibration, and cosmology, helping translate ground-based testing into flight-ready components that will help Roman reveal large swaths of the universe in high resolution.

“I’m very excited for Roman’s commissioning phase — the first 90 days when the spacecraft will begin transmitting data from orbit,” Choi said. 

Choi, photographed here in Death Valley, finds joy in the natural world outside of work. She cycles, hikes, and tends a small vegetable garden with a friend from grad school. Credit: Insook Choi (used with permission)

She’s especially drawn to so-called systematics, which are effects that can alter the signals scientists are trying to measure. “People sometimes think of systematics as nuisances, but they’re often telling us something deeply interesting about either the physics of something like a detector or the universe itself,” Choi said. “There’s always something more going on under the surface.”

While she’s eager to learn more about things like dark energy, Choi is also looking forward to seeing all the other ways our understanding of the universe grows. “It’s more than just an end goal,” she said. “It’s about everything we learn along the way. Every challenge we overcome, every detail we uncover, is an important discovery too.”

For those who hope to follow a similar path, Choi encourages staying curious, being persistent, and taking opportunities to get involved in research. And don’t let the tricky subjects scare you away! “You don’t have to be perfect at math or physics right away,” she said. “What matters most is a deep curiosity and the tenacity to keep pushing through.”

By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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Details Last Updated Sep 09, 2025 EditorAshley BalzerLocationGoddard Space Flight Center Related Terms

• Goddard Space Flight Center
• Nancy Grace Roman Space Telescope
• People of Goddard

Research Astrophysicist and Roman’s Deputy Wide Field Instrument Scientist – Goddard Space Flight Center

From a young age, Ami Choi — now a research astrophysicist at NASA — was drawn to the vast and mysterious. By the fifth grade, she had narrowed her sights to two career paths: marine biology or astrophysics. 

“I’ve always been interested in exploring big unknown realms, and things that aren’t quite tangible,” Choi said. That curiosity has served her all throughout her career.

In addition to conducting research, Ami Choi shares science with the public at various outreach events, including tours at NASA’s Goddard Space Flight Center in Greenbelt, Md. This photo captures one tour stop, outside the largest clean room at Goddard.Credit: NASA/Travis Wohlrab

As a student at University Laboratory High School in Urbana, Illinois, Choi gravitated toward astrophysics and was fascinated by things like black holes. She studied physics as an undergraduate at the University of Chicago, though she says math and physics didn’t necessarily come easily to her.

“I wasn’t very good at it initially, but I really liked the challenge so I stuck with it,” Choi said.

Early opportunities to do research played a pivotal role in guiding her career. As an undergraduate, Choi worked on everything from interacting galaxies to the stuff in between stars in our galaxy, called the interstellar medium. She learned how to code, interpret data, and do spectroscopy, which involves splitting light from cosmic objects into a rainbow of colors to learn about things like their composition.

After college, Choi read an article about physicist Janet Conrad’s neutrino work at Fermilab and was so inspired by Conrad’s enthusiasm and inclusivity that she cold-emailed her to see if there were any positions available in her group. 

On October 14, 2023, Ami took a break from a thermal vacuum shift to snap a selfie with a partial eclipse. She was visiting BAE, Inc. in Boulder, Co., where the primary instrument for NASA’s Nancy Grace Roman Space Telescope was undergoing testing. Credit: Courtesy of Ami Choi

“That one email led to a year at Fermilab working on neutrino physics,” Choi said.

She went on to earn a doctorate at the University of California, Davis, where she studied weak gravitational lensing — the subtle warping of light by gravity — and used it to explore dark matter, dark energy, and the large-scale structure of the universe.

Her postdoctoral work took Choi first to the University of Edinburgh in Scotland, where she contributed to the Kilo-Degree Survey, and later to The Ohio State University, where she became deeply involved in DES (the Dark Energy Survey) and helped lay the groundwork for the Nancy Grace Roman Space Telescope — NASA’s next flagship astrophysics mission. 

“One of my proudest moments came in 2021, when the DES released its third-year cosmology results,” Choi said. “It was a massive team effort conducted during a global pandemic, and I had helped lead as a co-convener of the weak lensing team.”

Choi regularly presents information about NASA’s Nancy Grace Roman Space Telescope to fellow scientists and the public. Here, she gives a Hyperwall talk at an AAS (American Astronomical Society) meeting.Credit: Courtesy of Ami Choi

After a one-year stint at the California Institute of Technology in Pasadena, where Choi worked on SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer)—an observatory that’s surveying stars and galaxies—she became a research astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. She also serves as the deputy Wide Field Instrument scientist for Roman. Choi operates at the intersection of engineering, calibration, and cosmology, helping translate ground-based testing into flight-ready components that will help Roman reveal large swaths of the universe in high resolution.

“I’m very excited for Roman’s commissioning phase — the first 90 days when the spacecraft will begin transmitting data from orbit,” Choi said. 

Choi, photographed here in Death Valley, finds joy in the natural world outside of work. She cycles, hikes, and tends a small vegetable garden with a friend from grad school. Credit: Insook Choi (used with permission)

She’s especially drawn to so-called systematics, which are effects that can alter the signals scientists are trying to measure. “People sometimes think of systematics as nuisances, but they’re often telling us something deeply interesting about either the physics of something like a detector or the universe itself,” Choi said. “There’s always something more going on under the surface.”

While she’s eager to learn more about things like dark energy, Choi is also looking forward to seeing all the other ways our understanding of the universe grows. “It’s more than just an end goal,” she said. “It’s about everything we learn along the way. Every challenge we overcome, every detail we uncover, is an important discovery too.”

For those who hope to follow a similar path, Choi encourages staying curious, being persistent, and taking opportunities to get involved in research. And don’t let the tricky subjects scare you away! “You don’t have to be perfect at math or physics right away,” she said. “What matters most is a deep curiosity and the tenacity to keep pushing through.”

By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Share

Details Last Updated Sep 09, 2025 EditorAshley BalzerLocationGoddard Space Flight Center Related Terms

• Goddard Space Flight Center
• Nancy Grace Roman Space Telescope
• People of Goddard

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) This artist’s concept shows a brown dwarf — an object larger than a planet but not massive enough to kickstart fusion in its core like a star. Brown dwarfs are hot when they form and may glow like this one, but over time they get closer in temperature to gas giant planets like Jupiter. NOIRLab/NSF/AURA/R. Proctor

An unusual cosmic object is helping scientists better understand the chemistry hidden deep in Jupiter and Saturn’s atmospheres — and potentially those of exoplanets.

Why has silicon, one of the most common elements in the universe, gone largely undetected in the atmospheres of Jupiter, Saturn, and gas planets like them orbiting other stars? A new study using observations from NASA’s James Webb Space Telescope sheds light on this question by focusing on a peculiar object that astronomers discovered by chance in 2020 and called “The Accident.”

The results were published on Sept. 4 in the journal Nature.

As shown in this graphic, brown dwarfs can be far more massive than even large gas planets like Jupiter and Saturn. However, they tend to lack the mass that kickstarts nuclear fusion in the cores of stars, causing them to shine. NASA/JPL-Caltech

The Accident is a brown dwarf, a ball of gas that’s not quite a planet and not quite a star. Even among its already hard-to-classify peers, The Accident has a perplexing mix of physical features, some of which have been previously seen in only young brown dwarfs and others seen only in ancient ones. Because of those features, it slipped past typical detection methods before being discovered five years ago by a citizen scientist participating in Backyard Worlds: Planet 9. The program lets people around the globe look for new discoveries in data from NASA’s now-retired NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer), which was managed by NASA’s Jet Propulsion Laboratory in Southern California.

The brown dwarf nicknamed “The Accident” can be seen moving in the bottom left corner of this video, which shows data from NASA’s now-retired NEOWISE (Near-Earth Object Wide-Field Infrared Survey Explorer), launched in 2009 with the moniker WISE. NASA/JPL-Caltech/Dan Caselden  

The Accident is so faint and odd that researchers needed NASA’s most powerful space observatory, Webb, to study its atmosphere. Among several surprises, they found evidence of a molecule they couldn’t initially identify. It turned out to be a simple silicon molecule called silane (SiH4). Researchers have long expected — but been unable — to find silane not only in our solar system’s gas giants, but also in the thousands of atmospheres belonging to brown dwarfs and to the gas giants orbiting other stars. The Accident is the first such object where this molecule has been identified.

Scientists are fairly confident that silicon exists in Jupiter and Saturn’s atmospheres but that it is hidden. Bound to oxygen, silicon forms oxides such as quartz that can seed clouds on hot gas giants, bearing a resemblance to dust storms on Earth. On cooler gas giants like Jupiter and Saturn, these types of clouds would sink far beneath lighter layers of water vapor and ammonia clouds, until any silicon-containing molecules are deep in the atmosphere, invisible even to the spacecraft that have studied those two planets up close.

Some researchers have also posited that lighter molecules of silicon, like silane, should be found higher up in these atmospheric layers, left behind like traces of flour on a baker’s table. That such molecules haven’t appeared anywhere except in a single, peculiar brown dwarf suggests something about the chemistry occurring in these environments.

“Sometimes it’s the extreme objects that help us understand what’s happening in the average ones,” said Faherty, a researcher at the American Museum of Natural History in New York City, and lead author on the new study.

Happy accident

Located about 50 light-years from Earth, The Accident likely formed 10 billion to 12 billion years ago, making it one of the oldest brown dwarfs ever discovered. The universe is about 14 billion years old, and at the time that The Accident developed, the cosmos contained mostly hydrogen and helium, with trace amounts of other elements, including silicon. Over eons, elements like carbon, nitrogen, and oxygen forged in the cores of stars, so planets and stars that formed more recently possess more of those elements.

Webb’s observations of The Accident confirm that silane can form in brown dwarf and planetary atmospheres. The fact that silane seems to be missing in other brown dwarfs and gas giant planets suggests that when oxygen is available, it bonds with silicon at such a high rate and so easily, virtually no silicon is left over to bond with hydrogen and form silane.

So why is silane in The Accident? The study authors surmise it is because far less oxygen was present in the universe when the ancient brown dwarf formed, resulting in less oxygen in its atmosphere to gobble up all the silicon. The available silicon would have bonded with hydrogen instead, resulting in silane.

“We weren’t looking to solve a mystery about Jupiter and Saturn with these observations,” said JPL’s Peter Eisenhardt, project scientist for the WISE (Wide-field Infrared Survey Explorer) mission, which was later repurposed as NEOWISE. “A brown dwarf is a ball of gas like a star, but without an internal fusion reactor, it gets cooler and cooler, with an atmosphere like that of gas giant planets. We wanted to see why this brown dwarf is so odd, but we weren’t expecting silane. The universe continues to surprise us.”

Brown dwarfs are often easier to study than gas giant exoplanets because the light from a faraway planet is typically drowned out by the star it orbits, while brown dwarfs generally fly solo. And the lessons learned from these objects extend to all kinds of planets, including ones outside our solar system that might feature potential signs of habitability. 

“To be clear, we’re not finding life on brown dwarfs,” said Faherty. “But at a high level, by studying all of this variety and complexity in planetary atmospheres, we’re setting up the scientists who are one day going to have to do this kind of chemical analysis for rocky, potentially Earth-like planets. It might not specifically involve silicon, but they’re going to get data that is complicated and confusing and doesn’t fit their models, just like we are. They’ll have to parse all those complexities if they want to answer those big questions.”

More about WISE, Webb  

A division of Caltech, JPL managed and operated WISE for NASA’s Science Mission Directorate. The mission was selected competitively under NASA’s Explorers Program managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland. The NEOWISE mission was a project of JPL and the University of Arizona in Tucson, supported by NASA’s Planetary Defense Coordination Office.

For more information about WISE, go to:

https://www.nasa.gov/mission_pages/WISE/main/index.html

The James Webb Space Telescope is the world’s premier space science observatory, and an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

To learn more about Webb, visit:

https://science.nasa.gov/webb

News Media Contacts

Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
626-808-2469
calla.e.cofield@jpl.nasa.gov

Christine Pulliam
Space Telescope Science Institute, Baltimore, Md.
cpulliam@stsci.edi

2025-113

Share

Details Last Updated Sep 09, 2025 Related Terms

• James Webb Space Telescope (JWST)
• Brown Dwarfs
• Exoplanets
• The Search for Life

Explore More 6 min read NASA Webb Looks at Earth-Sized, Habitable-Zone Exoplanet TRAPPIST-1 e

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6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) This artist’s concept shows a brown dwarf — an object larger than a planet but not massive enough to kickstart fusion in its core like a star. Brown dwarfs are hot when they form and may glow like this one, but over time they get closer in temperature to gas giant planets like Jupiter. NOIRLab/NSF/AURA/R. Proctor

An unusual cosmic object is helping scientists better understand the chemistry hidden deep in Jupiter and Saturn’s atmospheres — and potentially those of exoplanets.

Why has silicon, one of the most common elements in the universe, gone largely undetected in the atmospheres of Jupiter, Saturn, and gas planets like them orbiting other stars? A new study using observations from NASA’s James Webb Space Telescope sheds light on this question by focusing on a peculiar object that astronomers discovered by chance in 2020 and called “The Accident.”

The results were published on Sept. 4 in the journal Nature.

As shown in this graphic, brown dwarfs can be far more massive than even large gas planets like Jupiter and Saturn. However, they tend to lack the mass that kickstarts nuclear fusion in the cores of stars, causing them to shine. NASA/JPL-Caltech

The Accident is a brown dwarf, a ball of gas that’s not quite a planet and not quite a star. Even among its already hard-to-classify peers, The Accident has a perplexing mix of physical features, some of which have been previously seen in only young brown dwarfs and others seen only in ancient ones. Because of those features, it slipped past typical detection methods before being discovered five years ago by a citizen scientist participating in Backyard Worlds: Planet 9. The program lets people around the globe look for new discoveries in data from NASA’s now-retired NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer), which was managed by NASA’s Jet Propulsion Laboratory in Southern California.

The brown dwarf nicknamed “The Accident” can be seen moving in the bottom left corner of this video, which shows data from NASA’s now-retired NEOWISE (Near-Earth Object Wide-Field Infrared Survey Explorer), launched in 2009 with the moniker WISE. NASA/JPL-Caltech/Dan Caselden  

The Accident is so faint and odd that researchers needed NASA’s most powerful space observatory, Webb, to study its atmosphere. Among several surprises, they found evidence of a molecule they couldn’t initially identify. It turned out to be a simple silicon molecule called silane (SiH4). Researchers have long expected — but been unable — to find silane not only in our solar system’s gas giants, but also in the thousands of atmospheres belonging to brown dwarfs and to the gas giants orbiting other stars. The Accident is the first such object where this molecule has been identified.

Scientists are fairly confident that silicon exists in Jupiter and Saturn’s atmospheres but that it is hidden. Bound to oxygen, silicon forms oxides such as quartz that can seed clouds on hot gas giants, bearing a resemblance to dust storms on Earth. On cooler gas giants like Jupiter and Saturn, these types of clouds would sink far beneath lighter layers of water vapor and ammonia clouds, until any silicon-containing molecules are deep in the atmosphere, invisible even to the spacecraft that have studied those two planets up close.

Some researchers have also posited that lighter molecules of silicon, like silane, should be found higher up in these atmospheric layers, left behind like traces of flour on a baker’s table. That such molecules haven’t appeared anywhere except in a single, peculiar brown dwarf suggests something about the chemistry occurring in these environments.

“Sometimes it’s the extreme objects that help us understand what’s happening in the average ones,” said Faherty, a researcher at the American Museum of Natural History in New York City, and lead author on the new study.

Happy accident

Located about 50 light-years from Earth, The Accident likely formed 10 billion to 12 billion years ago, making it one of the oldest brown dwarfs ever discovered. The universe is about 14 billion years old, and at the time that The Accident developed, the cosmos contained mostly hydrogen and helium, with trace amounts of other elements, including silicon. Over eons, elements like carbon, nitrogen, and oxygen forged in the cores of stars, so planets and stars that formed more recently possess more of those elements.

Webb’s observations of The Accident confirm that silane can form in brown dwarf and planetary atmospheres. The fact that silane seems to be missing in other brown dwarfs and gas giant planets suggests that when oxygen is available, it bonds with silicon at such a high rate and so easily, virtually no silicon is left over to bond with hydrogen and form silane.

So why is silane in The Accident? The study authors surmise it is because far less oxygen was present in the universe when the ancient brown dwarf formed, resulting in less oxygen in its atmosphere to gobble up all the silicon. The available silicon would have bonded with hydrogen instead, resulting in silane.

“We weren’t looking to solve a mystery about Jupiter and Saturn with these observations,” said JPL’s Peter Eisenhardt, project scientist for the WISE (Wide-field Infrared Survey Explorer) mission, which was later repurposed as NEOWISE. “A brown dwarf is a ball of gas like a star, but without an internal fusion reactor, it gets cooler and cooler, with an atmosphere like that of gas giant planets. We wanted to see why this brown dwarf is so odd, but we weren’t expecting silane. The universe continues to surprise us.”

Brown dwarfs are often easier to study than gas giant exoplanets because the light from a faraway planet is typically drowned out by the star it orbits, while brown dwarfs generally fly solo. And the lessons learned from these objects extend to all kinds of planets, including ones outside our solar system that might feature potential signs of habitability. 

“To be clear, we’re not finding life on brown dwarfs,” said Faherty. “But at a high level, by studying all of this variety and complexity in planetary atmospheres, we’re setting up the scientists who are one day going to have to do this kind of chemical analysis for rocky, potentially Earth-like planets. It might not specifically involve silicon, but they’re going to get data that is complicated and confusing and doesn’t fit their models, just like we are. They’ll have to parse all those complexities if they want to answer those big questions.”

More about WISE, Webb  

A division of Caltech, JPL managed and operated WISE for NASA’s Science Mission Directorate. The mission was selected competitively under NASA’s Explorers Program managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland. The NEOWISE mission was a project of JPL and the University of Arizona in Tucson, supported by NASA’s Planetary Defense Coordination Office.

For more information about WISE, go to:

https://www.nasa.gov/mission_pages/WISE/main/index.html

The James Webb Space Telescope is the world’s premier space science observatory, and an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

To learn more about Webb, visit:

https://science.nasa.gov/webb

News Media Contacts

Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
626-808-2469
calla.e.cofield@jpl.nasa.gov

Christine Pulliam
Space Telescope Science Institute, Baltimore, Md.
cpulliam@stsci.edi

2025-113

Share

Details Last Updated Sep 09, 2025 Related Terms

• James Webb Space Telescope (JWST)
• Brown Dwarfs
• Exoplanets
• The Search for Life

Explore More 6 min read NASA Webb Looks at Earth-Sized, Habitable-Zone Exoplanet TRAPPIST-1 e

Scientists are in the midst of observing the exoplanet TRAPPIST-1 e with NASA’s James Webb…

Article 1 day ago 5 min read Glittering Glimpse of Star Birth From NASA’s Webb Telescope

This is a sparkling scene of star birth captured by NASA’s James Webb Space Telescope.…

Article 5 days ago 5 min read Astronomers Map Stellar ‘Polka Dots’ Using NASA’s TESS, Kepler

Scientists have devised a new method for mapping the spottiness of distant stars by using…

Article 2 weeks ago Keep Exploring Discover Related Topics

Missions

Humans in Space

Climate Change

Solar System

Los nombres de los participantes irán en tarjetas de embarque a bordo de la misión Artemis II de la NASA en 2026.Crédito: NASA

Read this press release in English here.

La NASA invita al público a unirse al vuelo de prueba Artemis II de la agencia en el que cuatro astronautas emprenderán un viaje alrededor de la Luna y de regreso a la Tierra para poner a prueba los sistemas y el hardware necesarios para la exploración del espacio profundo. Como parte de la iniciativa de la agencia “Envía tu nombre con Artemis II”, cualquiera puede asegurar su lugar a registrándose antes del 21 de enero. 

Los nombres de los participantes en esta iniciativa viajarán en la nave espacial Orion y el cohete Sistema de Lanzamiento Espacial (SLS, por sus siglas en inglés) junto a los astronautas de la NASA Reid Wiseman, Victor Glover, Christina Koch y el astronauta de la CSA (Agencia Espacial Canadiense) Jeremy Hansen. 

“Artemis II es un vuelo de prueba clave en nuestro esfuerzo por enviar de nuevo a seres humanos a la superficie de la Luna y desarrollar futuras misiones a Marte. También es una oportunidad para inspirar a personas de todo el mundo y darles la oportunidad de acompañarnos mientras lideramos el camino en la exploración humana hacia lugares más profundos en el espacio”, dijo Lori Glaze, administradora asociada interina en la Dirección de Misiones de Desarrollo de Sistemas de Exploración en la sede central de la NASA en Washington. 

Los nombres recopilados se incluirán en una tarjeta de memoria SD que será cargada a bordo de Orion antes del lanzamiento. A cambio, los participantes pueden descargar una tarjeta de embarque con su nombre como un recuerdo coleccionable. 

Para añadir tu nombre y recibir una tarjeta de embarque en español, visita el sitio web:

https://go.nasa.gov/TuNombreArtemis

Para añadir tu nombre y recibir una tarjeta de embarque en inglés, visita el sitio web: 

https://go.nasa.gov/artemisnames

Como parte de una edad de oro de innovación y exploración, el vuelo de prueba Artemis II es el primer vuelo tripulado de la campaña Artemis de la NASA. Tendrá una duración aproximada de 10 días y despegará a más tardar en abril de 2026. Este es otro paso hacia nuevas misiones tripuladas de Estados Unidos a la superficie de la Luna que ayudarán a la agencia a prepararse para enviar a los primeros astronautas estadounidenses a Marte.

Para obtener más información acerca de esta misión, visita el sitio web (en inglés): 

https://www.nasa.gov/mission/artemis-ii/

-fin-

Rachel Kraft / María José Viñas 
Sede central, Washington 
202-358-1600
rachel.h.kraft@nasa.gov / maria-jose.vinasgarcia@nasa.gov

Share

Details Last Updated Sep 09, 2025 LocationNASA Headquarters Related Terms

• NASA en español
• Artemis
• Artemis 2
• Exploration Systems Development Mission Directorate
• Missions

Los nombres de los participantes irán en tarjetas de embarque a bordo de la misión Artemis II de la NASA en 2026.Crédito: NASA

Read this press release in English here.

La NASA invita al público a unirse al vuelo de prueba Artemis II de la agencia en el que cuatro astronautas emprenderán un viaje alrededor de la Luna y de regreso a la Tierra para poner a prueba los sistemas y el hardware necesarios para la exploración del espacio profundo. Como parte de la iniciativa de la agencia “Envía tu nombre con Artemis II”, cualquiera puede asegurar su lugar a registrándose antes del 21 de enero. 

Los nombres de los participantes en esta iniciativa viajarán en la nave espacial Orion y el cohete Sistema de Lanzamiento Espacial (SLS, por sus siglas en inglés) junto a los astronautas de la NASA Reid Wiseman, Victor Glover, Christina Koch y el astronauta de la CSA (Agencia Espacial Canadiense) Jeremy Hansen. 

“Artemis II es un vuelo de prueba clave en nuestro esfuerzo por enviar de nuevo a seres humanos a la superficie de la Luna y desarrollar futuras misiones a Marte. También es una oportunidad para inspirar a personas de todo el mundo y darles la oportunidad de acompañarnos mientras lideramos el camino en la exploración humana hacia lugares más profundos en el espacio”, dijo Lori Glaze, administradora asociada interina en la Dirección de Misiones de Desarrollo de Sistemas de Exploración en la sede central de la NASA en Washington. 

Los nombres recopilados se incluirán en una tarjeta de memoria SD que será cargada a bordo de Orion antes del lanzamiento. A cambio, los participantes pueden descargar una tarjeta de embarque con su nombre como un recuerdo coleccionable. 

Para añadir tu nombre y recibir una tarjeta de embarque en español, visita el sitio web:

https://go.nasa.gov/TuNombreArtemis

Para añadir tu nombre y recibir una tarjeta de embarque en inglés, visita el sitio web: 

https://go.nasa.gov/artemisnames

Como parte de una edad de oro de innovación y exploración, el vuelo de prueba Artemis II es el primer vuelo tripulado de la campaña Artemis de la NASA. Tendrá una duración aproximada de 10 días y despegará a más tardar en abril de 2026. Este es otro paso hacia nuevas misiones tripuladas de Estados Unidos a la superficie de la Luna que ayudarán a la agencia a prepararse para enviar a los primeros astronautas estadounidenses a Marte.

Para obtener más información acerca de esta misión, visita el sitio web (en inglés): 

https://www.nasa.gov/mission/artemis-ii/

-fin-

Rachel Kraft / María José Viñas 
Sede central, Washington 
202-358-1600
rachel.h.kraft@nasa.gov / maria-jose.vinasgarcia@nasa.gov

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Details Last Updated Sep 09, 2025 LocationNASA Headquarters Related Terms

• NASA en español
• Artemis
• Artemis 2
• Exploration Systems Development Mission Directorate
• Missions

NASA Stennis Buffer ZoneNASA / Stennis

NASA’s Stennis Space Center is widely known for rocket propulsion testing, especially to support the NASA Artemis program to send astronauts to the Moon to prepare for future human exploration of Mars.

What may not be so widely known is that the site also is a unique federal city, home to more than 50 federal, state, academic, and commercial tenants and serving as both a model of government efficiency and a powerful economic engine for its region.

“NASA Stennis is a remarkable story of vision and innovation,” Center Director John Bailey said. “That was the case 55 years ago when the NASA Stennis federal city was born, and it remains the case today as we collaborate and grow to meet the needs of a changing aerospace world.”

Apollo Years

Nearly four years after its first Saturn V stage test, NASA’s Stennis Space Center faced a crossroads to the future. Indeed, despite its frontline role in supporting NASA’s Apollo lunar effort, it was not at all certain a viable future awaited the young rocket propulsion test site.

In 1961, NASA announced plans to build a sprawling propulsion test site in south Mississippi to support Apollo missions to the Moon. The news was a significant development for the sparsely populated Gulf Coast area.  

The new site, located near Bay St. Louis, Mississippi, conducted its first hot fire of a Saturn V rocket stage in April 1966. Saturn V testing progressed steadily during the next years. In fall 1969, however, NASA announced an end to Apollo-related testing, leading to an existential crisis for the young test site.

What was to become of NASA Stennis?

An Expanded Vision

Some observers speculated the location would close or be reduced to caretaker status, with minimal staffing. Either scenario would deliver a serious blow to the families who had re-located to make way for the site and the local communities who had heavily invested in municipal projects to support the influx of workforce personnel.

Such outcomes also would run counter to assurances provided by leaders that the new test site would benefit its surrounding region and involve area residents in “something great.”

For NASA Stennis manager Jackson Balch and others, such a result was unacceptable. Anticipating the crisis, Balch had been working behind the scenes to communicate – and realize – the vision of a multiagency site supporting a range of scientific and technological tenants and missions.

A Pivotal Year

The months following the Saturn V testing announcement were filled with discussions and planning to ensure the future of NASA Stennis. The efforts began to come to fruition in 1970 with key developments:

• In early 1970, NASA Administrator Thomas Paine proposed locating a regional environmental center at NASA Stennis. U.S. Sen. John C. Stennis (Mississippi) responded with a message of the president, “urgently requesting” that a National Earth Resources and Environmental Data Program be established at the site.
• In May 1970, President Richard Nixon offered assurances that an Earth Resources Laboratory would be established at NASA Stennis and that at least two agencies are preparing to locate operations at the site.
• U.S. congressional leaders earmarked $10 million to enable the location of an Earth Resources Laboratory at NASA Stennis.
• On July 9, 1970, the U.S. Coast Guard’s National Data Buoy Project (now the National Data Buoy Center) announced it was relocating to NASA Stennis, making it the first federal city tenant. The project arrived onsite two months later on September 9.
• On Sept. 9, 1970, NASA officially announced establishment of an Earth Resources Laboratory at NASA Stennis.

Time to Grow

By the end of 1970, Balch’s vision was taking shape, but it needed time to grow. The final Saturn V test had been conducted in October – with no new campaign scheduled.

A possibility was on the horizon, however. NASA was building a reusable space shuttle vehicle. It would be powered by the most sophisticated rocket engine ever designed – and the agency needed a place to conduct developmental and flight testing expected to last for decades.

Three sites vied for the assignment. Following presentations and evaluations, NASA announced its selection on March 1, 1971. Space shuttle engine testing would be conducted at NASA Stennis, providing time for the location to grow.

A Collaborative Model

By the spring of 1973, preparations for the space shuttle test campaign were progressing and NASA Stennis was on its way to realizing the federal city vision. Sixteen agencies and universities were now located at NASA Stennis.

The resident tenants followed a shared model in which they shared in the cost of basic site services, such as medical, security, and fire protection. The shared model freed up more funding for the tenants to apply towards innovation and assigned mission work. It was a model of government collaboration and efficiency.

As the site grew, leaders then began to call for it to be granted independent status within NASA, a development not long in coming. On June 14, 1974, just more than a decade after site construction began, NASA Administrator James Fletcher announced the south Mississippi location would be renamed National Space Technology Laboratories and would enjoy equal, independent status alongside other NASA centers.

“Something Great”

For NASA Stennis leaders and supporters, independent status represented a milestone moment in their effort to ensure NASA Stennis delivered on its promise of greatness.

There still were many developments to come, including the first space shuttle main engine test and the subsequent 34-year test campaign, the arrival and growth of the U.S. Navy into the predominant resident presence onsite, the renaming of the center to NASA Stennis, and the continued growth of the federal city.

No one could have imagined it all at the time. However, even in this period of early development, one thing was clear – the future lay ahead, and NASA Stennis was on its way.

Read More About Stennis Space Center Share

Details Last Updated Sep 09, 2025 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms

• Stennis Space Center

Explore More 4 min read NASA Stennis Provides Ideal Location for Range of Site Tenants Article 15 hours ago 4 min read NASA Stennis Provides Ideal Setting for Range Operations Article 2 weeks ago 10 min read NASA’s Stennis Space Center Employees Receive NASA Honor Awards Article 4 weeks ago

NASA Stennis Buffer ZoneNASA / Stennis

NASA’s Stennis Space Center is widely known for rocket propulsion testing, especially to support the NASA Artemis program to send astronauts to the Moon to prepare for future human exploration of Mars.

What may not be so widely known is that the site also is a unique federal city, home to more than 50 federal, state, academic, and commercial tenants and serving as both a model of government efficiency and a powerful economic engine for its region.

“NASA Stennis is a remarkable story of vision and innovation,” Center Director John Bailey said. “That was the case 55 years ago when the NASA Stennis federal city was born, and it remains the case today as we collaborate and grow to meet the needs of a changing aerospace world.”

Apollo Years

Nearly four years after its first Saturn V stage test, NASA’s Stennis Space Center faced a crossroads to the future. Indeed, despite its frontline role in supporting NASA’s Apollo lunar effort, it was not at all certain a viable future awaited the young rocket propulsion test site.

In 1961, NASA announced plans to build a sprawling propulsion test site in south Mississippi to support Apollo missions to the Moon. The news was a significant development for the sparsely populated Gulf Coast area.  

The new site, located near Bay St. Louis, Mississippi, conducted its first hot fire of a Saturn V rocket stage in April 1966. Saturn V testing progressed steadily during the next years. In fall 1969, however, NASA announced an end to Apollo-related testing, leading to an existential crisis for the young test site.

What was to become of NASA Stennis?

An Expanded Vision

Some observers speculated the location would close or be reduced to caretaker status, with minimal staffing. Either scenario would deliver a serious blow to the families who had re-located to make way for the site and the local communities who had heavily invested in municipal projects to support the influx of workforce personnel.

Such outcomes also would run counter to assurances provided by leaders that the new test site would benefit its surrounding region and involve area residents in “something great.”

For NASA Stennis manager Jackson Balch and others, such a result was unacceptable. Anticipating the crisis, Balch had been working behind the scenes to communicate – and realize – the vision of a multiagency site supporting a range of scientific and technological tenants and missions.

A Pivotal Year

The months following the Saturn V testing announcement were filled with discussions and planning to ensure the future of NASA Stennis. The efforts began to come to fruition in 1970 with key developments:

• In early 1970, NASA Administrator Thomas Paine proposed locating a regional environmental center at NASA Stennis. U.S. Sen. John C. Stennis (Mississippi) responded with a message of the president, “urgently requesting” that a National Earth Resources and Environmental Data Program be established at the site.
• In May 1970, President Richard Nixon offered assurances that an Earth Resources Laboratory would be established at NASA Stennis and that at least two agencies are preparing to locate operations at the site.
• U.S. congressional leaders earmarked $10 million to enable the location of an Earth Resources Laboratory at NASA Stennis.
• On July 9, 1970, the U.S. Coast Guard’s National Data Buoy Project (now the National Data Buoy Center) announced it was relocating to NASA Stennis, making it the first federal city tenant. The project arrived onsite two months later on September 9.
• On Sept. 9, 1970, NASA officially announced establishment of an Earth Resources Laboratory at NASA Stennis.

Time to Grow

By the end of 1970, Balch’s vision was taking shape, but it needed time to grow. The final Saturn V test had been conducted in October – with no new campaign scheduled.

A possibility was on the horizon, however. NASA was building a reusable space shuttle vehicle. It would be powered by the most sophisticated rocket engine ever designed – and the agency needed a place to conduct developmental and flight testing expected to last for decades.

Three sites vied for the assignment. Following presentations and evaluations, NASA announced its selection on March 1, 1971. Space shuttle engine testing would be conducted at NASA Stennis, providing time for the location to grow.

A Collaborative Model

By the spring of 1973, preparations for the space shuttle test campaign were progressing and NASA Stennis was on its way to realizing the federal city vision. Sixteen agencies and universities were now located at NASA Stennis.

The resident tenants followed a shared model in which they shared in the cost of basic site services, such as medical, security, and fire protection. The shared model freed up more funding for the tenants to apply towards innovation and assigned mission work. It was a model of government collaboration and efficiency.

As the site grew, leaders then began to call for it to be granted independent status within NASA, a development not long in coming. On June 14, 1974, just more than a decade after site construction began, NASA Administrator James Fletcher announced the south Mississippi location would be renamed National Space Technology Laboratories and would enjoy equal, independent status alongside other NASA centers.

“Something Great”

For NASA Stennis leaders and supporters, independent status represented a milestone moment in their effort to ensure NASA Stennis delivered on its promise of greatness.

There still were many developments to come, including the first space shuttle main engine test and the subsequent 34-year test campaign, the arrival and growth of the U.S. Navy into the predominant resident presence onsite, the renaming of the center to NASA Stennis, and the continued growth of the federal city.

No one could have imagined it all at the time. However, even in this period of early development, one thing was clear – the future lay ahead, and NASA Stennis was on its way.

Read More About Stennis Space Center Share

Details Last Updated Sep 09, 2025 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms

• Stennis Space Center

Explore More 4 min read NASA Stennis Provides Ideal Location for Range of Site Tenants Article 2 hours ago 4 min read NASA Stennis Provides Ideal Setting for Range Operations Article 2 weeks ago 10 min read NASA’s Stennis Space Center Employees Receive NASA Honor Awards Article 4 weeks ago

Boarding passes will carry participants’ names on NASA’s Artemis II mission in 2026.Credit: NASA

Lee este comunicado de prensa en español aquí.

NASA is inviting the public to join the agency’s Artemis II test flight as four astronauts venture around the Moon and back to test systems and hardware needed for deep space exploration. As part of the agency’s “Send Your Name with Artemis II” effort, anyone can claim their spot by signing up before Jan. 21.
 
Participants will launch their name aboard the Orion spacecraft and SLS (Space Launch System) rocket alongside NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen.
 
“Artemis II is a key test flight in our effort to return humans to the Moon’s surface and build toward future missions to Mars, and it’s also an opportunity to inspire people across the globe and to give them an opportunity to follow along as we lead the way in human exploration deeper into space,” said Lori Glaze, acting associate administrator, Exploration Systems Development Mission Directorate at NASA Headquarters in Washington. 
 
The collected names will be put on an SD card loaded aboard Orion before launch. In return, participants can download a boarding pass with their name on it as a collectable.
 
To add your name and receive an English-language boarding pass, visit: 

https://go.nasa.gov/artemisnames
 

To add your name and receive a Spanish-language boarding pass, visit: 

https://go.nasa.gov/TuNombreArtemis

 
As part of a Golden Age of innovation and exploration, the approximately 10-day Artemis II test flight, launching no later than April 2026, is the first crewed flight under NASA’s Artemis campaign. It is another step toward new U.S.-crewed missions on the Moon’s surface that will help the agency prepare to send the first astronauts – Americans – to Mars.
 
To learn more about the mission visit:

 
https://www.nasa.gov/mission/artemis-ii/
 
-end-

 
Rachel Kraft
Headquarters, Washington
202-358-1600
rachel.h.kraft@nasa.gov

Share

Details Last Updated Sep 09, 2025 LocationNASA Headquarters Related Terms

• Artemis 2
• Artemis
• Missions

Boarding passes will carry participants’ names on NASA’s Artemis II mission in 2026.Credit: NASA

Lee este comunicado de prensa en español aquí.

NASA is inviting the public to join the agency’s Artemis II test flight as four astronauts venture around the Moon and back to test systems and hardware needed for deep space exploration. As part of the agency’s “Send Your Name with Artemis II” effort, anyone can claim their spot by signing up before Jan. 21.
 
Participants will launch their name aboard the Orion spacecraft and SLS (Space Launch System) rocket alongside NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen.
 
“Artemis II is a key test flight in our effort to return humans to the Moon’s surface and build toward future missions to Mars, and it’s also an opportunity to inspire people across the globe and to give them an opportunity to follow along as we lead the way in human exploration deeper into space,” said Lori Glaze, acting associate administrator, Exploration Systems Development Mission Directorate at NASA Headquarters in Washington. 
 
The collected names will be put on an SD card loaded aboard Orion before launch. In return, participants can download a boarding pass with their name on it as a collectable.
 
To add your name and receive an English-language boarding pass, visit: 

https://go.nasa.gov/artemisnames
 

To add your name and receive a Spanish-language boarding pass, visit: 

https://go.nasa.gov/TuNombreArtemis

 
As part of a Golden Age of innovation and exploration, the approximately 10-day Artemis II test flight, launching no later than April 2026, is the first crewed flight under NASA’s Artemis campaign. It is another step toward new U.S.-crewed missions on the Moon’s surface that will help the agency prepare to send the first astronauts – Americans – to Mars.
 
To learn more about the mission visit:

 
https://www.nasa.gov/mission/artemis-ii/
 
-end-

 
Rachel Kraft
Headquarters, Washington
202-358-1600
rachel.h.kraft@nasa.gov

Share

Details Last Updated Sep 09, 2025 LocationNASA Headquarters Related Terms

• Artemis 2
• Artemis
• Missions

Teams at NASA’s Stennis Space Center conduct a hot fire test of an Aerojet AJ26 rocket engine on the E-1 Test Stand in November 2013.NASA/Stennis

If location, location, location is the overarching mantra in real estate, it is small wonder that NASA’s Stennis Space Center is considered a national asset and prime aerospace and technology operations site.

It has long stood as a premier – and the nation’s largest – rocket propulsion test site. With unparalleled test infrastructure and expertise, NASA Stennis has helped power the nation’s human space exploration for almost 60 years. It continues to do so, testing systems and engines for NASA’s Artemis program to send astronauts to the Moon to prepare for future human exploration of Mars.

In addition, NASA Stennis is the choice location for a range of agencies, organizations, offices, and companies, all of whom readily attest to the values of the setting. Ask resident tenants to note the value of their NASA Stennis location, and one hears terms like “strategic advantages,” “ideal location,” “local expertise and experience,” “collaborative opportunities,” “hub of innovation,” and “valuable security buffer.”

For the NASA Shared Services Center, its location at the south Mississippi test site provides “substantial strategic advantages” that helps the NSSC maximize its work and provide streamlined business operations for the agency.

Likewise, NASA Stennis provides an ideal location for the North Gulf Institute operated by Mississippi State University, as it conducts frontline work in hurricane forecasting, modeling and assessment, as well as fishery and ecosystem management. The location is strengthened further by the proximity to collaborative partners like the Naval Meteorology and Oceanography Command and the National Data Buoy Center.

The same holds true for the National Centers for Environmental Information operated by the National Oceanic and Atmospheric Administration. A spokesperson said the centers’ mission success is “firmly rooted in its strategic co-location with other federal partners,” including the Naval Meteorology and Oceanography Command, the National Data Buoy Center, and the Northern Gulf Institute.

For Relativity Space, the largest NASA Stennis test complex tenant, the “unparalleled infrastructure” at NASA Stennis has been key to enabling the company’s rocket engine testing. “NASA’s Stennis Space Center plays a vital role in getting Terran R to space,” said Clay Walker, vice president of test and launch for Relativity Space. “The infrastructure here allows us to test high-performance engines in ways no other place can.”

Other companies express similar sentiments, citing the unique opportunities NASA Stennis provides, as well as the value of the local workforce. For instance, L3Harris Technologies has operated at NASA Stennis under various names since the 1960s, providing support to the Apollo, Space Shuttle, and, now, Artemis programs. In 2008, Lockheed Martin opened a start-to-finish facility for production of propulsion systems, making use of the various NASA Stennis propulsion test services and resources.

Evolution Space is capitalizing on decades of aerospace experience at NASA Stennis, as well as “world-class” site infrastructure to establish production and test capabilities for solid rocket motors onsite.

Both Mississippi and Louisiana have established technology offices onsite. As a Mississippi Enterprise for Technology statement noted, “The NASA Stennis environment enhances our ability to support emerging technologies, strengthen Mississippi’s technology ecosystem, and contribute to the economic vitality of the region,” said Davis Pace, chief executive officer for the Mississippi Enterprise for Technology.

Meanwhile, the site’s most prominent tenant – the U.S. Navy – operates various offices at NASA Stennis. The Navy’s move to the site began in the 1970s to take advantage of the security provided by the surrounding NASA Stennis acoustical buffer zone. Various Navy functions eventually located continuing operations onsite, including the Naval Meteorology and Oceanography Command, the Naval Oceanographic Office, the Naval Small Craft Instruction and Technical Training School, the Navy Office of Civilian Human Resources, and the Naval Research Laboratory.

In similar fashion, the U.S. Department of Homeland Security credits the “high-quality, secure, and resilient” NASA Stennis site for its decision to location information technology and applications operations onsite.

As the very first NASA Stennis federal city tenant, arriving onsite in September 1970, the National Data Buoy Center has borne witness to it all.

“From its inception, Sen. John Stennis (and other leaders) envisioned a place where America would push the boundaries of the unknown – from the depths of the oceans to the far reaches of space,” said Dr. William Burnett, director of the National Data Buoy Center onsite. “That vision lives on at NASA Stennis, now home to one of the world’s largest concentrations of oceanographers. At the National Data Buoy Center, we proudly carry out our mission to safeguard maritime safety by harnessing the full strength of this unique scientific and technical community.

“We are deeply rooted in the community and grateful to thrive within the collaborative spirit that defines Stennis. It’s an honor to be part of its legacy – and its future.”

Read More About Stennis Space Center Share

Details Last Updated Sep 09, 2025 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms

• Stennis Space Center

Explore More 5 min read Crossroads to the Future – NASA Stennis Grows into a Model Federal City Article 15 hours ago 4 min read NASA Stennis Provides Ideal Setting for Range Operations Article 2 weeks ago 10 min read NASA’s Stennis Space Center Employees Receive NASA Honor Awards Article 4 weeks ago

Teams at NASA’s Stennis Space Center conduct a hot fire test of an Aerojet AJ26 rocket engine on the E-1 Test Stand in November 2013.NASA/Stennis

If location, location, location is the overarching mantra in real estate, it is small wonder that NASA’s Stennis Space Center is considered a national asset and prime aerospace and technology operations site.

It has long stood as a premier – and the nation’s largest – rocket propulsion test site. With unparalleled test infrastructure and expertise, NASA Stennis has helped power the nation’s human space exploration for almost 60 years. It continues to do so, testing systems and engines for NASA’s Artemis program to send astronauts to the Moon to prepare for future human exploration of Mars.

In addition, NASA Stennis is the choice location for a range of agencies, organizations, offices, and companies, all of whom readily attest to the values of the setting. Ask resident tenants to note the value of their NASA Stennis location, and one hears terms like “strategic advantages,” “ideal location,” “local expertise and experience,” “collaborative opportunities,” “hub of innovation,” and “valuable security buffer.”

For the NASA Shared Services Center, its location at the south Mississippi test site provides “substantial strategic advantages” that helps the NSSC maximize its work and provide streamlined business operations for the agency.

Likewise, NASA Stennis provides an ideal location for the North Gulf Institute operated by Mississippi State University, as it conducts frontline work in hurricane forecasting, modeling and assessment, as well as fishery and ecosystem management. The location is strengthened further by the proximity to collaborative partners like the Naval Meteorology and Oceanography Command and the National Data Buoy Center.

The same holds true for the National Centers for Environmental Information operated by the National Oceanic and Atmospheric Administration. A spokesperson said the centers’ mission success is “firmly rooted in its strategic co-location with other federal partners,” including the Naval Meteorology and Oceanography Command, the National Data Buoy Center, and the Northern Gulf Institute.

For Relativity Space, the largest NASA Stennis test complex tenant, the “unparalleled infrastructure” at NASA Stennis has been key to enabling the company’s rocket engine testing. “NASA’s Stennis Space Center plays a vital role in getting Terran R to space,” said Clay Walker, vice president of test and launch for Relativity Space. “The infrastructure here allows us to test high-performance engines in ways no other place can.”

Other companies express similar sentiments, citing the unique opportunities NASA Stennis provides, as well as the value of the local workforce. For instance, L3Harris Technologies has operated at NASA Stennis under various names since the 1960s, providing support to the Apollo, Space Shuttle, and, now, Artemis programs. In 2008, Lockheed Martin opened a start-to-finish facility for production of propulsion systems, making use of the various NASA Stennis propulsion test services and resources.

Evolution Space is capitalizing on decades of aerospace experience at NASA Stennis, as well as “world-class” site infrastructure to establish production and test capabilities for solid rocket motors onsite.

Both Mississippi and Louisiana have established technology offices onsite. As a Mississippi Enterprise for Technology statement noted, “The NASA Stennis environment enhances our ability to support emerging technologies, strengthen Mississippi’s technology ecosystem, and contribute to the economic vitality of the region,” said Davis Pace, chief executive officer for the Mississippi Enterprise for Technology.

Meanwhile, the site’s most prominent tenant – the U.S. Navy – operates various offices at NASA Stennis. The Navy’s move to the site began in the 1970s to take advantage of the security provided by the surrounding NASA Stennis acoustical buffer zone. Various Navy functions eventually located continuing operations onsite, including the Naval Meteorology and Oceanography Command, the Naval Oceanographic Office, the Naval Small Craft Instruction and Technical Training School, the Navy Office of Civilian Human Resources, and the Naval Research Laboratory.

In similar fashion, the U.S. Department of Homeland Security credits the “high-quality, secure, and resilient” NASA Stennis site for its decision to location information technology and applications operations onsite.

As the very first NASA Stennis federal city tenant, arriving onsite in September 1970, the National Data Buoy Center has borne witness to it all.

“From its inception, Sen. John Stennis (and other leaders) envisioned a place where America would push the boundaries of the unknown – from the depths of the oceans to the far reaches of space,” said Dr. William Burnett, director of the National Data Buoy Center onsite. “That vision lives on at NASA Stennis, now home to one of the world’s largest concentrations of oceanographers. At the National Data Buoy Center, we proudly carry out our mission to safeguard maritime safety by harnessing the full strength of this unique scientific and technical community.

“We are deeply rooted in the community and grateful to thrive within the collaborative spirit that defines Stennis. It’s an honor to be part of its legacy – and its future.”

Read More About Stennis Space Center Share

Details Last Updated Sep 09, 2025 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms

• Stennis Space Center

Explore More 5 min read Crossroads to the Future – NASA Stennis Grows into a Model Federal City Article 2 hours ago 4 min read NASA Stennis Provides Ideal Setting for Range Operations Article 2 weeks ago 10 min read NASA’s Stennis Space Center Employees Receive NASA Honor Awards Article 4 weeks ago

A review of the five main methods proposed for cooling down the poles or slowing the loss of ice concludes they are all wildly impractical, wouldn't work, or both

A review of the five main methods proposed for cooling down the poles or slowing the loss of ice concludes they are all wildly impractical, wouldn't work, or both

Space changes you. It strengthens some muscles, weakens others, shifts fluids within your body, and realigns your sense of balance. NASA’s Human Research Program works to understand—and sometimes even counter—those changes so astronauts can thrive on future deep space missions.  

NASA astronaut Loral O’Hara pedals on the Cycle Ergometer Vibration Isolation System (CEVIS) inside the International Space Station’s Destiny laboratory module.NASA

Astronauts aboard the International Space Station work out roughly two hours a day to protect bone density, muscle strength and the cardiovascular system, but the longer they are in microgravity, the harder it can be for the brain and body to readapt to gravity’s pull. After months in orbit, returning astronauts often describe Earth as heavy, loud, and strangely still. Some reacclimate within days, while other astronauts take longer to fully recover.

Adjusting to Gravity  

NASA’s SpaceX Crew-7 astronaut Jasmin Moghbeli after landing in the Gulf of America on March 12, 2024, completing 197 days in space.NASA/Joel Kowsky

The crew of NASA’s SpaceX Crew-7 mission— NASA astronaut Jasmin Moghbeli, ESA (European Space Agency) astronaut Andreas Mogensen, JAXA (Japan Aerospace Exploration Agency) astronaut Satoshi Furukawa, and Roscosmos cosmonaut Konstantin Borisov—landed in March 2024 after nearly 200 days in space. One of the first tests volunteer crew members completed was walking with their eyes open and then closed.  

“With eyes closed, it was almost impossible to walk in a straight line,” Mogensen said. In space, vision is the primary way astronauts orient themselves, but back on Earth, the brain must relearn how to use inner-ear balance signals. Moghbeli joked her first attempt at the exercise looked like “a nice tap dance.”   

“I felt very wobbly for the first two days,” Moghbeli said. “My neck was very tired from holding up my head.” She added that, overall, her body readapted to gravity quickly.  

Astronauts each recover on their own timetable and may encounter different challenges. Mogensen said his coordination took time to return. Furukawa noted that he could not look down without feeling nauseated. “Day by day, I recovered and got more stable,” he said. 

NASA astronaut Loral O’Hara after landing in a remote area near the town of Zhezkazgan, Kazakhstan, on April 6, 2024.NASA/Bill Ingalls

NASA astronaut Loral O’Hara returned in April 2024 after 204 days in space. She said she felt almost completely back to normal a week after returning to Earth. O’Hara added that her prior experience as an ocean engineer gave her insight into space missions. “Having those small teams in the field working with a team somewhere else back on shore with more resources is a good analog for the space station and all the missions we’re hoping to do in the future,” she said. 

NASA astronaut Nichole Ayers, who flew her first space mission with NASA’s SpaceX Crew-10, noted that the brain quickly adapts to weightlessness by tuning out the vestibular system, which controls balance. “Then, within days of being back on Earth, it remembers again—it’s amazing how fast the body readjusts,” she said. 

Expedition 69 NASA astronaut Frank Rubio outside the Soyuz MS-23 spacecraft after landing near the town of Zhezkazgan, Kazakhstan, on Sept. 27, 2023. NASA/Bill Ingalls

When NASA astronaut Frank Rubio landed in Kazakhstan in September 2023, he had just completed a record 371-day mission—the longest single U.S. spaceflight.  

Rubio said his body adjusted to gravity right away, though his feet and lower back were sore after more than a year without weight on them. Thanks to consistent workouts, Rubio said he felt mostly recovered within a couple of weeks.  

Mentally, extending his mission from six months to a year was a challenge. “It was a mixed emotional roller coaster,” he said, but regular video calls with family kept him grounded. “It was almost overwhelming how much love and support we received.” 

Crew-8 astronauts Matt Dominick, Jeanette Epps, Michael Barratt, and cosmonaut Alexander Grebenkin splashed down in October 2024 after 235 days on station. Dominick found sitting on hard surfaces uncomfortable at first. Epps felt the heaviness of Earth immediately. “You have to move and exercise every day, regardless of how exhausted you feel,” she said.  

Barratt, veteran astronaut and board certified in internal and aerospace medicine, explained that recovery differs for each crew member, and that every return teaches NASA something new. 

Still a Challenge, Even for Space Veterans  

NASA astronaut Suni Williams is helped out of a SpaceX Dragon spacecraft aboard the SpaceX recovery ship after splashing down off the coast of Tallahassee, Florida, March 18, 2025. NASA/Keegan Barber

Veteran NASA astronauts Suni Williams and Butch Wilmore returned from a nine-month mission with Crew-9 in early 2025. Despite her extensive spaceflight experience, Williams said re-adapting to gravity can still be tough. “The weight and heaviness of things is surprising,” she said. Like others, she pushed herself to move daily to regain strength and balance.  

NASA astronaut Don Pettit arrives at Ellington Field in Houston on April 20, 2025, after returning to Earth aboard the Soyuz MS-25 spacecraft. NASA/Robert Markowitz

NASA astronaut Don Pettit, also a veteran flyer, came home in April 2025 after 220 days on the space station. At 70 years old, he is NASA’s oldest active astronaut—but experience did not make gravity gentler.  During landing, he says he was kept busy, “emptying the contents of my stomach onto the steppes of Kazakhstan.” Microgravity had eased the aches in his joints and muscles, but Earth’s pull brought them back all at once.  

Pettit said his recovery felt similar to earlier missions. “I still feel like a little kid inside,” he said. The hardest part, he explained, isn’t regaining strength in big muscle groups, but retraining the small, often-overlooked muscles unused in space. “It’s a learning process to get used to gravity again.”  

Recovery happens day by day—with help from exercise, support systems, and a little humor. No matter how long an astronaut is in space, every journey back to Earth is unique. 

The Human Research Program help scientists understand how spaceflight environments affect astronaut health and performance and informs strategies to keep crews healthy for future missions to the Moon, Mars, and beyond. The program studies astronauts before, during, and after spaceflight to learn how the human body adapts to living and working in space. It also collects data through Earth-based analog missions that can help keep astronauts safer for future space exploration.  

To learn more about how microgravity affects the human body and develop new ways to help astronauts stay healthy, for example, its scientists conduct bedrest studies – asking dozens of volunteers to spend 60 days in bed with their heads tilted down at a specific angle.  Lying in this position tricks the body into responding as it would if the body was in space which allows scientists to trial interventions to hopefully counter some of microgravity’s effects.  Such studies, through led by NASA, occur at the German Aerospace Center’s Cologne campus at a facility called :envihab – a combination of “environment” and “habitat.”  

Additional Earth-based insights come from the Crew Health and Performance Exploration Analog (CHAPEA) and the Human Exploration Research Analog (HERA) at NASA’s Johnson Space Center in Houston. Both analogs recreate the remote conditions and scenarios of deep space exploration here on Earth with volunteer crews who agree to live and work in the isolation of ground-based habitats and endure challenges like delayed communication that simulates the type of interactions that will occur during deep space journeys to and from Mars. Findings from these ground-based missions and others will help NASA refine its future interventions, strategies, and protocols for astronauts in space. 

NASA and its partners have supported humans continuously living and working in space since November 2000. After nearly 25 years of continuous human presence, the space station remains the sole space-based proving ground for training and research for deep space missions, enabling NASA’s Artemis campaign, lunar exploration, and future Mars missions. 

Explore More 7 min read A Few Things Artemis Will Teach Us About Living and Working on the Moon Article 6 years ago 3 min read Inside NASA’s New Orion Mission Evaluation Room for Artemis II  Article 2 weeks ago 12 min read 15 Ways the International Space Station Benefits Humanity Back on Earth Article 3 years ago

"The trajectory of 3I/ATLAS is within the interceptable range of the mission we designed."

Space changes you. It strengthens some muscles, weakens others, shifts fluids within your body, and realigns your sense of balance. NASA’s Human Research Program works to understand—and sometimes even counter—those changes so astronauts can thrive on future deep space missions.  

NASA astronaut Loral O’Hara pedals on the Cycle Ergometer Vibration Isolation System (CEVIS) inside the International Space Station’s Destiny laboratory module.NASA

Astronauts aboard the International Space Station work out roughly two hours a day to protect bone density, muscle strength and the cardiovascular system, but the longer they are in microgravity, the harder it can be for the brain and body to readapt to gravity’s pull. After months in orbit, returning astronauts often describe Earth as heavy, loud, and strangely still. Some reacclimate within days, while other astronauts take longer to fully recover.

Adjusting to Gravity  

NASA’s SpaceX Crew-7 astronaut Jasmin Moghbeli after landing in the Gulf of America on March 12, 2024, completing 197 days in space.NASA/Joel Kowsky

The crew of NASA’s SpaceX Crew-7 mission— NASA astronaut Jasmin Moghbeli, ESA (European Space Agency) astronaut Andreas Mogensen, JAXA (Japan Aerospace Exploration Agency) astronaut Satoshi Furukawa, and Roscosmos cosmonaut Konstantin Borisov—landed in March 2024 after nearly 200 days in space. One of the first tests volunteer crew members completed was walking with their eyes open and then closed.  

“With eyes closed, it was almost impossible to walk in a straight line,” Mogensen said. In space, vision is the primary way astronauts orient themselves, but back on Earth, the brain must relearn how to use inner-ear balance signals. Moghbeli joked her first attempt at the exercise looked like “a nice tap dance.”   

“I felt very wobbly for the first two days,” Moghbeli said. “My neck was very tired from holding up my head.” She added that, overall, her body readapted to gravity quickly.  

Astronauts each recover on their own timetable and may encounter different challenges. Mogensen said his coordination took time to return. Furukawa noted that he could not look down without feeling nauseated. “Day by day, I recovered and got more stable,” he said. 

NASA astronaut Loral O’Hara after landing in a remote area near the town of Zhezkazgan, Kazakhstan, on April 6, 2024.NASA/Bill Ingalls

NASA astronaut Loral O’Hara returned in April 2024 after 204 days in space. She said she felt almost completely back to normal a week after returning to Earth. O’Hara added that her prior experience as an ocean engineer gave her insight into space missions. “Having those small teams in the field working with a team somewhere else back on shore with more resources is a good analog for the space station and all the missions we’re hoping to do in the future,” she said. 

NASA astronaut Nichole Ayers, who flew her first space mission with NASA’s SpaceX Crew-10, noted that the brain quickly adapts to weightlessness by tuning out the vestibular system, which controls balance. “Then, within days of being back on Earth, it remembers again—it’s amazing how fast the body readjusts,” she said. 

Expedition 69 NASA astronaut Frank Rubio outside the Soyuz MS-23 spacecraft after landing near the town of Zhezkazgan, Kazakhstan, on Sept. 27, 2023. NASA/Bill Ingalls

When NASA astronaut Frank Rubio landed in Kazakhstan in September 2023, he had just completed a record 371-day mission—the longest single U.S. spaceflight.  

Rubio said his body adjusted to gravity right away, though his feet and lower back were sore after more than a year without weight on them. Thanks to consistent workouts, Rubio said he felt mostly recovered within a couple of weeks.  

Mentally, extending his mission from six months to a year was a challenge. “It was a mixed emotional roller coaster,” he said, but regular video calls with family kept him grounded. “It was almost overwhelming how much love and support we received.” 

Crew-8 astronauts Matt Dominick, Jeanette Epps, Michael Barratt, and cosmonaut Alexander Grebenkin splashed down in October 2024 after 235 days on station. Dominick found sitting on hard surfaces uncomfortable at first. Epps felt the heaviness of Earth immediately. “You have to move and exercise every day, regardless of how exhausted you feel,” she said.  

Barratt, veteran astronaut and board certified in internal and aerospace medicine, explained that recovery differs for each crew member, and that every return teaches NASA something new. 

Still a Challenge, Even for Space Veterans  

NASA astronaut Suni Williams is helped out of a SpaceX Dragon spacecraft aboard the SpaceX recovery ship after splashing down off the coast of Tallahassee, Florida, March 18, 2025. NASA/Keegan Barber

Veteran NASA astronauts Suni Williams and Butch Wilmore returned from a nine-month mission with Crew-9 in early 2025. Despite her extensive spaceflight experience, Williams said re-adapting to gravity can still be tough. “The weight and heaviness of things is surprising,” she said. Like others, she pushed herself to move daily to regain strength and balance.  

NASA astronaut Don Pettit arrives at Ellington Field in Houston on April 20, 2025, after returning to Earth aboard the Soyuz MS-25 spacecraft. NASA/Robert Markowitz

NASA astronaut Don Pettit, also a veteran flyer, came home in April 2025 after 220 days on the space station. At 70 years old, he is NASA’s oldest active astronaut—but experience did not make gravity gentler.  During landing, he says he was kept busy, “emptying the contents of my stomach onto the steppes of Kazakhstan.” Microgravity had eased the aches in his joints and muscles, but Earth’s pull brought them back all at once.  

Pettit said his recovery felt similar to earlier missions. “I still feel like a little kid inside,” he said. The hardest part, he explained, isn’t regaining strength in big muscle groups, but retraining the small, often-overlooked muscles unused in space. “It’s a learning process to get used to gravity again.”  

Recovery happens day by day—with help from exercise, support systems, and a little humor. No matter how long an astronaut is in space, every journey back to Earth is unique. 

The Human Research Program help scientists understand how spaceflight environments affect astronaut health and performance and informs strategies to keep crews healthy for future missions to the Moon, Mars, and beyond. The program studies astronauts before, during, and after spaceflight to learn how the human body adapts to living and working in space. It also collects data through Earth-based analog missions that can help keep astronauts safer for future space exploration.  

To learn more about how microgravity affects the human body and develop new ways to help astronauts stay healthy, for example, its scientists conduct bedrest studies – asking dozens of volunteers to spend 60 days in bed with their heads tilted down at a specific angle.  Lying in this position tricks the body into responding as it would if the body was in space which allows scientists to trial interventions to hopefully counter some of microgravity’s effects.  Such studies, through led by NASA, occur at the German Aerospace Center’s Cologne campus at a facility called :envihab – a combination of “environment” and “habitat.”  

Additional Earth-based insights come from the Crew Health and Performance Exploration Analog (CHAPEA) and the Human Exploration Research Analog (HERA) at NASA’s Johnson Space Center in Houston. Both analogs recreate the remote conditions and scenarios of deep space exploration here on Earth with volunteer crews who agree to live and work in the isolation of ground-based habitats and endure challenges like delayed communication that simulates the type of interactions that will occur during deep space journeys to and from Mars. Findings from these ground-based missions and others will help NASA refine its future interventions, strategies, and protocols for astronauts in space. 

NASA and its partners have supported humans continuously living and working in space since November 2000. After nearly 25 years of continuous human presence, the space station remains the sole space-based proving ground for training and research for deep space missions, enabling NASA’s Artemis campaign, lunar exploration, and future Mars missions. 

Explore More 7 min read A Few Things Artemis Will Teach Us About Living and Working on the Moon Article 6 years ago 3 min read Inside NASA’s New Orion Mission Evaluation Room for Artemis II  Article 2 weeks ago 12 min read 15 Ways the International Space Station Benefits Humanity Back on Earth Article 3 years ago

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2 min read

Perseverance Meets the Megabreccia NASA’s Mars Perseverance rover acquired this image of the “Scotiafjellet” workspace on Aug. 31, 2025, using its onboard Left Navigation Camera (Navcam). The camera is located high on the rover’s mast and aids in driving. This image was acquired on Sol 1610, or Martian day 1,610 of the Mars 2020 mission, at the local mean solar time of 14:52:20. NASA/JPL-Caltech

Written by By Henry Manelski, Ph.D. student at Purdue University

Last week, the Perseverance rover began an exciting new journey. Driving northwest of the Soroya ridge, Perseverance entered an area filled with a diverse range of boulders that the science team believes could hold clues to Mars’ early history. The terrain we are exploring is known as megabreccia: a chaotic mixture of broken rock fragments likely produced during ancient asteroid impacts. Some blocks may have originated in the gargantuan Isidis impact event, which created a 1,200-mile-wide crater (about 1,930 kilometers) just east of Jezero. Studying megabreccia could help us link Jezero’s geology to the wider region around Isidis Basin, tying local observations to Mars’ global history. 

The rover is now beginning a systematic exploration of these rocks, starting at Scotiafjellet. If they are truly megabreccia, they could contain pieces of deep crustal material, offering a rare glimpse into Mars’ interior. These rocks likely predate the deltaic and volcanic deposits we explored earlier in Jezero Crater, making them some of the oldest accessible rocks Perseverance will ever encounter. They may therefore reveal to what extent water was present on ancient Mars — a key question as we continue our search for signs of past life on the Red Planet. In short, by venturing into this jumbled terrain, Perseverance is giving us a front-row seat to the earliest chapters of Mars’ story.

 

• Want to read more posts from the Perseverance team?

  
  
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• Want to learn more about Perseverance’s science instruments?

  
  
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4 min read Curiosity Blog, Sols 4641-4648: Thinking Outside and Inside the ‘Boxwork’

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Explore This Section

• Perseverance Home
• Science
• News and Features
• Multimedia
• Mars Missions
• Mars Home

2 min read

Perseverance Meets the Megabreccia NASA’s Mars Perseverance rover acquired this image of the “Scotiafjellet” workspace on Aug. 31, 2025, using its onboard Left Navigation Camera (Navcam). The camera is located high on the rover’s mast and aids in driving. This image was acquired on Sol 1610, or Martian day 1,610 of the Mars 2020 mission, at the local mean solar time of 14:52:20. NASA/JPL-Caltech

Written by By Henry Manelski, Ph.D. student at Purdue University

Last week, the Perseverance rover began an exciting new journey. Driving northwest of the Soroya ridge, Perseverance entered an area filled with a diverse range of boulders that the science team believes could hold clues to Mars’ early history. The terrain we are exploring is known as megabreccia: a chaotic mixture of broken rock fragments likely produced during ancient asteroid impacts. Some blocks may have originated in the gargantuan Isidis impact event, which created a 1,200-mile-wide crater (about 1,930 kilometers) just east of Jezero. Studying megabreccia could help us link Jezero’s geology to the wider region around Isidis Basin, tying local observations to Mars’ global history. 

The rover is now beginning a systematic exploration of these rocks, starting at Scotiafjellet. If they are truly megabreccia, they could contain pieces of deep crustal material, offering a rare glimpse into Mars’ interior. These rocks likely predate the deltaic and volcanic deposits we explored earlier in Jezero Crater, making them some of the oldest accessible rocks Perseverance will ever encounter. They may therefore reveal to what extent water was present on ancient Mars — a key question as we continue our search for signs of past life on the Red Planet. In short, by venturing into this jumbled terrain, Perseverance is giving us a front-row seat to the earliest chapters of Mars’ story.

 

• Want to read more posts from the Perseverance team?

  
  
  Visit Mission Updates
  
  

• Want to learn more about Perseverance’s science instruments?

  
  
  Visit the Science Instruments page
  
  

Share

• 
  
  
• 
  
  
• 
  
  
• 
  
  

Details

Last Updated

Sep 08, 2025

Related Terms

• Blogs

Explore More

4 min read Curiosity Blog, Sols 4641-4648: Thinking Outside and Inside the ‘Boxwork’

Article


4 days ago

2 min read Over Soroya Ridge & Onward!

Article


2 weeks ago

3 min read Curiosity Blog, Sols 4638-4640: Imaging Extravaganza Atop a Ridge

Article


2 weeks 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…