She Speaks for the Samples: Meet Dr. Juliane Gross, Artemis Campaign Sample Curation Lead 

She Speaks for the Samples: Meet Dr. Juliane Gross, Artemis Campaign Sample Curation Lead 

Based at NASA’s Johnson Space Center in Houston, the Astromaterials Research and Exploration Science Division, or ARES, curates the most extensive collection of extraterrestrial materials on Earth, ranging from microscopic cosmic dust particles to Apollo-era Moon rocks. Soon, ARES’ team of world-leading sample scientists hopes to add something new to its collection – lunar samples from the Moon’s South Pole region. 

As the Artemis campaign sample curation lead, Dr. Juliane Gross is helping ARES and NASA prepare to collect and return those samples safely. “I’m responsible for representing the voice of the Moon rocks and advocating for their protection, preservation, and maintaining their integrity during the planning and execution of all stages of the different Artemis sample return missions,” she said. 

A woman wearing a blue long sleeved shirt stands in front of four people and fives a presentation.
Juliane Gross leads a geology lesson for Artemis II crew members as part of their field training in Iceland in 2024.
NASA

Her multifaceted role includes preparing the Johnson facility that will receive new lunar samples, developing curation strategies, and collaborating with mission teams to plan sampling operations, which encompass collection, handling, transport, and storage processes for all stages of Artemis missions. She trains program managers and engineers on the importance of sample return and teaches crew members how to identify lunar samples and collect them without contamination. She also works with the different programs and teams that oversee the vehicles used at different stages of lunar missions – collaborating with the human landing system team around tool storage and delivery to the lunar surface, the Orion Program to coordinate sample stowage for the return to Earth, and Exploration Ground Systems to plan sample recovery after splashdown.  

Once samples are returned to Earth, Gross and the ARES curation team will conduct a preliminary examination of the materials and release a sample catalog from which members of the global scientific community may request loans to carry out their respective research. 

Working across Artemis teams raised an unexpected but fun challenge for Gross – learning to communicate effectively with colleagues who have different academic and professional backgrounds. “Scientists like me speak a different language than engineers, and we all speak a different language than managers or the general public,” she said. “I have worked hard to find common vocabulary and to ‘translate’ science needs into the different types of languages that exist within the Artemis campaign. I’m trying to use our differences as strengths to enable mission success and to connect and build relationships with all these different teams through my love and passion for the Moon and rocks from the Moon.” 

That passion emerged shortly after Gross completed her Ph.D. in geology, while working on lunar samples with the Lunar and Planetary Institute. She went on to become a research scientist with the American Museum of Natural History in New York, and then a tenured professor of planetary sciences at Rutgers University in Piscataway, New Jersey.  

In 2019, NASA asked Gross to join the Apollo Next Generation Sample Analysis Program. Under the program, NASA preserved some of the 382 kilograms of lunar samples returned by Apollo missions, keeping them sealed for future generations to open and analyze. “NASA had the foresight to understand that technology would evolve and our level of sophistication for handling and examining samples would greatly increase,” Gross said.  

She and two other scientists had the incredible opportunity to open and examine two samples returned by Apollo 17. Their work served as a practice run for Artemis sample returns while building upon the fundamental insights into the shared origin and history of Earth and the Moon that scientists previously derived from other Apollo samples. For example, the team extracted gas from one sample that will provide information about the volatiles that future lunar missions may encounter around the Moon’s South Pole.  

“The Apollo Next Generation Sample Analysis Program linked the first generation of lunar explorers from Apollo with future explorers of the Moon with Artemis,” Gross said. “I’m very proud to have played such an important role in this initiative that now feeds forward to Artemis.” 

A woman wearing a white hair cap and gown
Juliane Gross examines lunar samples returned by Apollo 17 in Johnson Space Center’s Lunar Sample Laboratory Facility.
NASA

Gross’ connection with NASA began even earlier in her career. She was selected to join the agency-sponsored Antarctic Search for Meteorites team and lived in the deep ice fields of Antarctica for two months with seven other people. “We lived in tiny two-person tents without any support and recovered a total of 263 space rocks under challenging conditions,” she said. “I experienced the powerful forces of Antarctica and traveled 332 miles on skidoos. My body changed in the cold – I stuffed my face with enough butter, chocolate, and peanut M&Ms to last a lifetime and yet I lost weight.”  

This formative experience taught Gross to find and celebrate beauty, even in her toughest moments. “I drank tea made with Antarctic glacier ice that is thousands to millions of years old. I will never forget the beautiful bell-like sounds that snow crystals make when being blown across the ice, the rainbow-sparkling ice crystals on a really cold day, the vast expanses of ice sheets looking like oceans frozen in eternity, and the icy bite of the wind on any unprotected skin that made me feel so alive and reminded me how vulnerable and precious life is,” she said. “And I will never ever forget the thrill and utter joy of finding a meteorite that you know no one on this planet has ever seen before you.”  

Gross ultimately received the Antarctica Service Medal of the United States Armed Forces from the U.S. Department of Defense for her work. 

Juliane Gross returns to McMurdo Station in Antarctica after working in the deep field for two months as part of the Antarctic Search for Meteorites team.
Image courtesy of Juliane Gross

Transitioning from full-time academia to her current position at NASA has been a big adjustment for Gross, but she has learned to love the change and the growth opportunities that come with it. “Being part of this incredible moment in history when we are about to return to the Moon with Artemis, our Apollo of today, feels so special and humbling that it made the transition easier,” she said.  

The job has also increased Gross’ love and excitement for space exploration and reminds her every day why sample return missions are important. “The Moon is a museum of planetary history,” she said. “It has recorded and preserved the changes that affected the Earth-Moon system and is the best and most accessible place in the solar system to study planet-altering processes that have affected our corner of the universe.”  

Still, “The Moon is only our next frontier,” she said. “Keep looking up and never give up. Ad astra!” 

Watch below to learn about NASA’s rich history of geology training and hear how scientists and engineers are getting ready to bring back samples that will help us learn about the origins of our solar system.

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Linda E. Grimm

NASA Awards Astrophysics Postdoctoral Fellowships for 2025

NASA Awards Astrophysics Postdoctoral Fellowships for 2025

5 min read

NASA Awards Astrophysics Postdoctoral Fellowships for 2025

The highly competitive NASA Hubble Fellowship Program (NHFP) recently named 24 new fellows to its 2025 class. The NHFP fosters excellence and leadership in astrophysics by supporting exceptionally promising and innovative early-career astrophysicists. Over 650 applicants vied for the 2025 fellowships. Each fellowship provides the awardee up to three years of support at a U.S. institution.

Once selected, fellows are named to one of three sub-categories corresponding to three broad scientific questions that NASA seeks to answer about the universe:

How does the universe work? – Einstein Fellows

How did we get here? – Hubble Fellows

Are we alone? – Sagan Fellows

“The 2025 class of the NASA Hubble Fellowship Program is comprised of outstanding NASA Astrophysics researchers,” said Shawn Domagal-Goldman, acting director of the Astrophysics Division at NASA Headquarters in Washington. “This class of competitively-selected fellows will inspire future generations through the products of their research, and by sharing the results of that work with the public. Their efforts will help NASA continue its worldwide leadership in space-based astrophysics research.”

The class of 2025 NHFP Fellows are shown in this photo montage (left to right, top to bottom): The Einstein Fellows (seen in the blue hexagons) are: Shi-Fan Chen, Nicolas Garavito Camargo, Jason Hinkle, Itai Linial, Kenzie Nimmo, Massimo Pascale, Elia Pizzati, Jillian Rastinejad and Aaron Tohuvavohu. The Hubble Fellows (seen in the red hexagons) are: Aliza Beverage, Anna de Graaff, Karia Dilbert, Emily Griffith, Viraj Karambelkar, Lindsey Kwok, Abigail Lee, Aaron Pearlman, Dominick Rowan, Nicholas Rui, Nadine Soliman, Bingjie Wang. The Sagan Fellows (seen in green hexagons) are: Kyle Franson, Caprice Phillips, and Keming Zhang.
The class of 2025 NHFP Fellows are shown in this photo montage (left to right, top to bottom): The Einstein Fellows (seen in the blue hexagons) are: Shi-Fan Chen, Nicolas Garavito Camargo, Jason Hinkle, Itai Linial, Kenzie Nimmo, Massimo Pascale, Elia Pizzati, Jillian Rastinejad and Aaron Tohuvavohu. The Hubble Fellows (seen in the red hexagons) are: Aliza Beverage, Anna de Graaff, Karia Dilbert, Emily Griffith, Viraj Karambelkar, Lindsey Kwok, Abigail Lee, Aaron Pearlman, Dominick Rowan, Nicholas Rui, Nadine Soliman, Bingjie Wang. The Sagan Fellows (seen in green hexagons) are: Kyle Franson, Caprice Phillips, and Keming Zhang.
NASA, ESA, Megan Crane (Caltech/IPAC)

The list below provides the names of the 2025 awardees, their fellowship host institutions, and their proposed research topics.

The 2025 NHFP Einstein Fellows are:

  • Shi-Fan Chen, Columbia University, Galaxies, Shapes and Weak Lensing in the Effective Field Theory of Large-Scale Structure
  • Nicolas Garavito Camargo, University of Maryland, College Park, Local Group Galaxies in Disequilibrium; Building New Frameworks to Constrain the Nature of Dark Matter
  • Jason Hinkle, University of Illinois, Urbana-Champaign, Nuclear Transients in the Golden Era of Time-Domain Astronomy
  • Itai Linial, New York University, Repeating Nuclear Transients – Probes of Supermassive Black Holes and Their Environments
  • Kenzie Nimmo, Northwestern University, From Glimmering Jewels to Cosmic Ubiquity: Unraveling the Origins of FRBs
  • Massimo Pascale, University of California, Los Angeles, The Universe Seen Through Strong Gravitational Lensing
  • Elia Pizzati, Harvard University, The Missing Link: Connecting Black Hole Growth and Quasar Light Curves in the Young Universe
  • Jillian Rastinejad, University of Maryland, College Park, Illuminating the Explosive Origins of the Heavy Elements
  • Aaron Tohuvavohu, California Institute of Technology, Ultraviolet Space Telescopes for the new era of Time Domain and Multi-Messenger Astronomy

The 2025 NHFP Hubble Fellows are:

  • Aliza Beverage, Carnegie Observatories, Revealing Massive Galaxies Formation Using Chemical Abundances
  • Anna de Graaff, Harvard University, Early giants in context: How could galaxies in the first billion years grow so rapidly?
  • Karia Dibert, California Institute of Technology, Superconducting on-chip spectrometers for high-redshift astrophysics and cosmology
  • Emily Griffith, University of Colorado, Boulder, Beyond Mg and Fe: Exploring Detailed Nucleosynthetic Patterns
  • Viraj Karambelkar, Columbia University, The Anthropology of Merging Stars
  • Lindsey Kwok, Northwestern University, Determining the Astrophysical Origins of White-Dwarf Supernovae with JWST Infrared Spectroscopy
  • Abigail Lee, University of California, Berkeley, AGB Stars in the Era of NIR Astronomy: New Probes of Cosmology and Galaxy Evolution
  • Aaron Pearlman, Massachusetts Institute of Technology, Pinpointing the Origins of Fast Radio Bursts and Tracing Baryons in the Cosmic Web
  • Dominick Rowan, University of California, Berkeley, Fundamental Stellar Parameters Across the Hertzsprung-Russell Diagram
  • Nicholas Rui, Princeton University, A seismic atlas of the stellar merger sky
  • Nadine Soliman, Institute for Advanced Study, Micro Foundations, Macro Realities: Modeling the Multi-scale Physics Shaping Planets, Stars and Galaxies
  • Bingjie Wang, Princeton University, Inference at the Edge of the Universe

The 2025 NHFP Sagan Fellows are:

  • Kyle Franson, University of California, Santa Cruz, Mapping the Formation, Migration, and Thermal Evolution of Giant Planets with Direct Imaging and Astrometry
  • Caprice Phillips, University of California, Santa Cruz, Aging in the Cosmos: JWST Insights into the Evolution of Brown Dwarf Atmospheres and Clouds
  • Keming Zhang, Institute for Advanced Study, Understanding the Origin and Abundance of Free-Floating Planets via Microlensing and Machine Learning

The class of 2025 NHFP Fellows are shown in this photo montage (left to right, top to bottom): The Einstein Fellows (seen in the blue hexagons) are: Shi-Fan Chen, Nicolas Garavito Camargo, Jason Hinkle, Itai Linial, Kenzie Nimmo, Massimo Pascale, Elia Pizzati, Jillian Rastinejad and Aaron Tohuvavohu.

The Hubble Fellows (seen in the red hexagons) are: Aliza Beverage, Anna de Graaff, Karia Dilbert, Emily Griffith, Viraj Karambelkar, Lindsey Kwok, Abigail Lee, Aaron Pearlman, Dominick Rowan, Nicholas Rui, Nadine Soliman, Bingjie Wang.

The Sagan Fellows (seen in green hexagons) are: Kyle Franson, Caprice Phillips, and Keming Zhang.

For short bios and photos, please visit the link at the end of the article.

An important part of the NHFP is the annual Symposium, which allows Fellows the opportunity to present results of their research, and to meet each other and the scientific and administrative staff who manage the program. The 2024 symposium was held at the NASA Exoplanet Science Institute (NExScI) in Pasadena, California. Science topics ranged through exoplanets, gravitational waves, fast radio bursts, cosmology and more. Non-science sessions included discussions about career paths and developing mentorship skills, as well as an open mic highlighting an array of talents other than astrophysics.

The Space Telescope Science Institute in Baltimore, Maryland, administers the NHFP on behalf of NASA, in collaboration with the Chandra X-ray Center at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and the NASA Exoplanet Science Institute and the Jet Propulsion Laboratory, in Pasadena, California.

Short bios and photos of the 2025 NHFP Fellows can be found at:
https://www.stsci.edu/stsci-research/fellowships/nasa-hubble-fellowship-program/2025-nhfp-fellows

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Last Updated
Mar 31, 2025
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Andrea Gianopoulos
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Claire Andreoli
NASA’s Goddard Space Flight Center
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claire.andreoli@nasa.gov

Ray Villard
Space Telescope Science Institute
Baltimore, Maryland

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NASA Awards Launch Services Contract for SpaceX Starship

NASA Awards Launch Services Contract for SpaceX Starship

NASA logo.

NASA has awarded SpaceX of Starbase, Texas, a modification under the NASA Launch Services (NLS) II contract to add Starship to their existing Falcon 9 and Falcon Heavy launch service offerings.

The NLS II contracts provide a broad range of commercial launch services for NASA’s planetary, Earth-observing, exploration, and scientific satellites. These high-priority, low and medium risk tolerant missions have full NASA technical oversight and mission assurance, resulting in the highest probability of launch success.

The NLS II contracts are multiple award, indefinite-delivery/indefinite-quantity, with an ordering period through June 2030 and an overall period of performance through December 2032. The contracts include an on-ramp provision that provides an opportunity annually for new launch service providers to add their launch service on an NLS II contract and compete for future missions and allows existing contractors to introduce launch services not currently on their NLS II contracts.

The contracts support the goals and objectives of the agency’s Science Mission Directorate, Space Operations Mission Directorate, Explorations Systems Development Mission Directorate, and the Space Technology Mission Directorate. Under the contracts, NASA also can provide launch services to other federal government agencies.

NASA’s Launch Services Program Office at the agency’s Kennedy Space Center in Florida manages the NLS II contracts. For more information about NASA and agency programs, visit:

https://www.nasa.gov

-end-

Tiernan Doyle / Joshua Finch
Headquarters, Washington
202-358-1600 / 202-358-1100
tiernan.doyle@.nasa.gov / joshua.a.finch@nasa.gov

Patti Bielling
Kennedy Space Center, Florida
321-501-7575
patricia.a.bielling@nasa.gov

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Mar 28, 2025

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Abbey A. Donaldson

NASA Boosts Efficiency with Custom X-66 Flooring

NASA Boosts Efficiency with Custom X-66 Flooring

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A man wearing a black shirt, a mask, glasses, and a baseball cap backwards handles part of a piece of light brown plywood as he is pulling it off a machine. There is clear plastic hanging from the wall behind him. The NASA logo is also hanging on the wall behind the plastic. There is wood dust around the area of the machine.
Eric Garza, an engineering technician in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California, cuts plywood to size for temporary floorboards for the X-66 experimental demonstrator aircraft on Aug. 26, 2024.
NASA/Steve Freeman

NASA designed temporary floorboards for the MD-90 aircraft to use while it is transformed into the X-66 experimental demonstrator aircraft. These floorboards will protect the original flooring and streamline the modification process.

Supporting the agency’s Sustainable Flight Demonstrator project, a small team in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California, built temporary floorboards to save the project time and resources. Repeated removal and installation of the original flooring during the modification process was time-consuming. Using temporary panels also ensures the original floorboards are protected and remain flightworthy for when modifications are complete, and the original flooring is reinstalled.

“The task of creating the temporary floorboards for the MD-90 involves a meticulous process aimed at facilitating modifications while maintaining safety and efficiency. The need for these temporary floorboards arises from the detailed procedure required to remove and reinstall the Original Equipment Manufacturer (OEM) floorboards,” said Jason Nelson, experimental fabrication lead. He is one of two members of the fabrication team – one engineering technician and one inspector – manufacturing about 50 temporary floorboards, which range in size from 20 inches by 36 inches to 42 inches by 75 inches.

A silver drill-like machine cuts holes in light brown plywood. There are specks of wood dust around the cut.
A wood router cuts precise holes in plywood for temporary floorboards on Aug. 26, 2024, in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California. The flooring was designed for the X-66 experimental demonstrator aircraft.
NASA/Steve Freeman

Nelson continued, “Since these OEM boards will be removed and reinstalled multiple times to accommodate necessary modifications, the temporary floorboards will save the team valuable time and resources. They will also provide the same level of safety and strength as the OEM boards, ensuring that the process runs smoothly without compromising quality.”

Designing and prototyping the flooring was a meticulous process, but the temporary solution plays a crucial role in optimizing time and resources as NASA works to advance safe and efficient air travel. The agency’s Sustainable Flight Demonstrator project seeks to inform the next generation of single-aisle airliners, the most common aircraft in commercial aviation fleets around the world. NASA partnered with Boeing to develop the X-66 experimental demonstrator aircraft.

NASA Armstrong’s Experimental Fabrication Shop carries out modifications and repair work on aircraft, ranging from the creation of something as small as an aluminum bracket to modifying wing spars, fuselage ribs, control surfaces, and other tasks to support missions.

A man wearing a mask, glasses, and a baseball cap backwards watches as a silver drill-like machine cuts holes into plywood.
Eric Garza, an engineering technician in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California, observes a wood router cut holes for temporary floorboards on Aug. 26, 2024. The flooring was designed for the X-66 experimental demonstrator aircraft. 
NASA/Steve Freeman

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Dede Dinius

Visiting Mars on the Way to the Outer Solar System

Visiting Mars on the Way to the Outer Solar System

3 min read

Visiting Mars on the Way to the Outer Solar System

Written by Roger Wiens, Principal Investigator, SuperCam instrument / Co-Investigator, SHERLOC instrument at Purdue University

A color photo from the Martian surface shows pale orange, very rocky terrain in the foreground, taking up the lower two-thirds of the frame, creating a horizon line from the upper left corner of the image to the middle right side. The terrain beyond, in the distance, is blurry and takes up the rest of the frame. The rocks in the foreground range from tiny, sharp stones to large outcroppings, the latter showing some medium gray highlights among the orange rock and dust that comprise them. The largest rocks, on the left side, show numerous grooves and cracks on their faces, ranging from vertical to slightly left-skewing.
A portion of the “Sally’s Cove” outcrop where the Perseverance rover has been exploring. The radiating lines in the rock on the left of the image may indicate that it is a shatter cone, showing the effects of the shock wave from a nearby large impact. The image was taken by Mastcam-Z’s left camera on March 21, 2025 (Sol 1452, or Martian day 1,452 of the Mars 2020 mission) at the local mean solar time of 12:13:44. Mastcam-Z is a pair of cameras located high on the rover’s mast. This image was voted by the public as “Image of the week.”
NASA/JPL-Caltech/ASU

Recently Mars has had a few Earthly visitors. On March 1, NASA’s Europa Clipper flew within 550 miles (884 kilometers) of the Red Planet’s surface on its way out to Jupiter. On March 12, the European Space Agency’s Hera spacecraft flew within about 3,100 miles (5,000 kilometers) of Mars, and only 300 kilometers from its moon, Deimos. Hera is on its way to study the binary asteroid Didymos and its moon Dimorphos. Next year, in May 2026, NASA’s Psyche mission is scheduled to buzz the Red Planet on its way to the metal-rich asteroid 16 Psyche, coming within a few thousand kilometers.

Why all these visits to Mars? You might at first think that they’re using Mars as an object of opportunity for their cameras, and you would be partially right. But Mars has more to give these missions than that. The main reason for these flybys is the extra speed that Mars’ velocity around the Sun can give them. The idea that visiting a planet can speed up a spacecraft is not all that obvious, because the same gravity that attracts the spacecraft on its way towards the planet will exert a backwards force as the spacecraft leaves the planet.

The key is in the direction that it approaches and leaves the planet. If the spacecraft leaves Mars heading in the direction that Mars is traveling around the Sun, it will gain speed in that direction, slingshotting it farther into the outer solar system. A spacecraft can typically gain several percent of its speed by performing such a slingshot flyby. The closer it gets to the planet, the bigger the effect. However, no mission wants to be slowed by the upper atmosphere, so several hundred kilometers is the closest that a mission should go. And the proximity to the planet is also affected by the exact direction the spacecraft needs to go when it leaves Mars.

Clipper’s Mars flyby was a slight exception, slowing down the craft — by about 1.2 miles per second (2 kilometers per second) — to steer it toward Earth for a second gravity assist in December 2026. That will push the spacecraft the rest of the way to Jupiter, for its 2030 arrival.

While observing Mars is not the main reason for their visits, many of the visiting spacecraft take the opportunity to use their cameras either to perform calibrations or to study the Red Planet and its moons.

During Clipper’s flyby over sols 1431-1432, Mastcam-Z was directed to watch the skies for signs of the interplanetary visitor. Clipper’s relatively large solar panels could have reflected enough sunlight for it to be seen in the Mars night sky, much as we can see satellites overhead from Earth. Unfortunately, the spacecraft entered the shadow of Mars just before it came into potential view above the horizon from Perseverance’s vantage point, so the sighting did not happen. But it was worth a try.

Meanwhile, back on the ground, Perseverance is performing something of a cliff-hanger. “Sally’s Cove” is a relatively steep rock outcrop in the outer portion of Jezero crater’s rim just north of “Broom Hill.” Perseverance made an approach during March 19-23, and has been exploring some dark-colored rocks along this outcrop, leaving the spherules behind for the moment. Who knows what Perseverance will find next?

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Mar 28, 2025

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