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30 Years Ago: NASA Selects its 15th Group of Astronauts 

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

On Dec. 8, 1994, NASA announced the selection of its 15th group of astronauts. The diverse group comprised 19 candidates – 10 pilots and nine mission specialists, and included five women, two African Americans, one Asian American, and the first Peruvian-born and Indian-born astronauts. Four international astronauts, one each from Canada and Japan and two from France, joined the group later for astronaut candidate training, following which all 23 became eligible for spaceflight assignment. The two French candidates had previous spaceflight experience in cooperative missions with Russia. All members of the group completed at least one spaceflight, making significant contributions to assembly and maintenance of the space station and carrying out important science missions. Three perished in the Columbia accident. 

The Group 15 NASA and international astronaut candidates pose for a group photo – front row, Jeffrey S. Ashby, left, Dafydd “Dave” R. Williams, James F. Reilly, Scott D. Altman, Rick D. Husband, and Michael J. Bloomfield; middle row, Pamela A. Melroy, left, Michael P. Anderson, Michel Tognini, Kathryn “Kay” P. Hire, Kalpana Chawla, Carlos I. Noriega, Susan L. Still, Takao Doi, and Frederick “Rick” W. Sturckow; back row, Janet L. Kavandi, left, Edward T. Lu, Steven K. Robinson, Robert L. Curbeam, Dominic L.P. Gorie, Joe F. Edwards, Steven W. Lindsey, and Jean-Loup Chrétien.
The Group 15 NASA and international astronaut candidates pose for a group photo – front row, Jeffrey S. Ashby, left, Dafydd “Dave” R. Williams, James F. Reilly, Scott D. Altman, Rick D. Husband, and Michael J. Bloomfield; middle row, Pamela A. Melroy, left, Michael P. Anderson, Michel Tognini, Kathryn “Kay” P. Hire, Kalpana Chawla, Carlos I. Noriega, Susan L. Still, Takao Doi, and Frederick “Rick” W. Sturckow; back row, Janet L. Kavandi, left, Edward T. Lu, Steven K. Robinson, Robert L. Curbeam, Dominic L.P. Gorie, Joe F. Edwards, Steven W. Lindsey, and Jean-Loup Chrétien.
Credit: NASA

The newest class of NASA astronaut candidates included pilot candidates Scott D. Altman, Jeffrey S. Ashby, Michael J. Bloomfield, Joe F. Edwards, Dominic L.P. Gorie, Rick D. Husband, Steven W. Lindsey, Pamela A. Melroy, Susan L. Still, and Frederick “Rick” W. Sturckow, and mission specialist candidates Michael P. Anderson, Kalpana Chawla, Robert L. Curbeam, Kathryn “Kay” P. Hire, Janet L. Kavandi, Edward T. Lu, Carlos I. Noriega, James F. Reilly, and Steven K. Robinson. A January 1995 agreement among the agencies enabled Canadian Space Agency (CSA) astronaut Dafydd “Dave” R. Williams and Takao Doi of the National Space Development Agency (NASDA), now the Japan Aerospace Exploration Agency, to join the 19 NASA astronauts for training. Another agreement between NASA and the French space agency CNES enabled astronauts Jean-Loup Chrétien and Michel Tognini to also join the group. Both Chrétien and Tognini had previous spaceflight experience through joint agreements with Russia, and their experience proved helpful to NASA in the fledgling Shuttle-Mir Program. 

Group 15 astronaut candidates experience short-duration weightlessness aboard NASA’s KC-135 aircraft.
Group 15 astronaut candidates experience short-duration weightlessness aboard NASA’s KC-135 aircraft.
Credit: NASA

The 19 NASA candidates along with Williams and Doi reported to work at NASA’s Johnson Space Center in Houston on March 6, 1995, to begin their one-year training period. The two French astronauts joined them later. During the yearlong training, the candidates attended classes in applied sciences, space shuttle and space station systems, space medicine, Earth and planetary sciences, and materials sciences. They visited each of the NASA centers to learn about their functions and received instruction in flying the T-38 Talon training aircraft, high-altitude and ground egress systems, survival skills, parasail flight, and scuba. They experienced short-duration weightlessness aboard NASA’s KC-135 aircraft dubbed the Vomit Comet. After completing the astronaut candidate training, they qualified for various technical assignments within the astronaut office leading to assignments to space shuttle crews. 

The 19 NASA candidates along with Williams and Doi reported to work at NASA’s Johnson Space Center in Houston on March 6, 1995, to begin their one-year training period. The two French astronauts joined them later. During the yearlong training, the candidates attended classes in applied sciences, space shuttle and space station systems, space medicine, Earth and planetary sciences, and materials sciences. They visited each of the NASA centers to learn about their functions and received instruction in flying the T-38 Talon training aircraft, high-altitude and ground egress systems, survival skills, parasail flight, and scuba. They experienced short-duration weightlessness aboard NASA’s KC-135 aircraft dubbed the Vomit Comet. After completing the astronaut candidate training, they qualified for various technical assignments within the astronaut office leading to assignments to space shuttle crews. 

Per tradition, the previous astronaut class provided the nickname for Group 15. Originally, The Class of 1992, The Hogs, dubbed them The Snails because NASA had delayed their announcement. Then after the addition of the two French astronauts, they felt that The Flying Escargots seemed more appropriate. The Group 15 patch included an astronaut pin rising from the Earth, an orbiting space shuttle and space station, and flags of the United States, Canada, France, and Japan. 

Group 15 patch.
Group 15 patch.
Credit: NASA

Altman, a U.S. Navy pilot, hails from Illinois. He received his first spaceflight assignment as pilot of STS-90, the 16-day Neurolab mission in 1998, along with fellow Escargots Hire and Williams. He again served as pilot on STS-106, a 12-day space station resupply mission in 2000, accompanied by fellow Escargot Lu. He served as commander on his third mission, STS-109, the 11-day fourth Hubble Space Telescope (HST) servicing mission in 2002. He commanded his fourth and final mission, the 13-day final HST servicing mission, STS-125, in 2009. Altman logged a total of 51 days in space. 

Anderson, a native of upstate New York and a lieutenant colonel in the U.S. Air Force, received his first assignment as a mission specialist on STS-89, the nine-day eighth docking with Mir. Fellow Escargots Edwards and Reilly flew with Anderson, who has the distinction as the only African American astronaut to visit that space station during the mission in 1998. He next served as payload commander on the 16-day STS-107 Spacehab research mission in 2003, flying with fellow Escargots Chawla and Husband. Anderson perished in the Columbia accident. He logged nearly 25 days in space. 

Texas native and U.S. Navy captain Ashby received his first spaceflight assignment as pilot of STS-93, the five-day mission in 1999 to deploy the Chandra X-ray Observatory. Fellow Escargot Tognini served as a mission specialist on this flight. On his second mission, Ashby served as pilot of STS-100, the 12-day flight in 2001 that delivered the Canadarm2 robotic arm to the space station. Ashby commanded his third and final mission in 2002, STS-112, the 11-day space station assembly flight that delivered the S1 truss. Fellow Escargot Melroy served as pilot on this flight. During his three missions, Ashby spent nearly 28 days in space. 

Hailing from Michigan, U.S. Air Force Colonel Bloomfield received his first flight assignment as pilot of STS-86, the seventh Mir docking mission. The 11-day flight took place in 1997, with fellow Escargot Chrétien serving as a mission specialist. Bloomfield served as pilot on his second flight, STS-97, the 11-day station assembly mission in 2000 that delivered the P6 truss and the first set of U.S. solar arrays. Fellow Escargot Noriega flew as a mission specialist on this flight. Bloomfield served as commander on his third and final mission, the 11-day STS-110 assembly flight that delivered the S0 truss segment in 2002. Bloomfield logged a total of 32 days in space across his three missions. 

Chawla, the first Indian-born NASA astronaut, earned a doctorate in aerospace engineering. She received her first spaceflight assignment as a mission specialist on STS-87, the 16-day flight in 1997 that carried the fourth U.S. Microgravity Payload (USMP-4). Fellow Escargot Lindsey served as pilot on this mission, during which Chawla used the shuttle’s robotic arm to release and capture the SPARTAN-201-4 free flyer. She next served as a mission specialist on the STS-107 Spacehab research mission in 2003, along with fellow Escargots Anderson and Husband. Chawla perished in the Columbia accident. She logged nearly 32 days in space.

On his first spaceflight, Curbeam, a native of Baltimore and commander in the U.S. Navy, flew as a mission specialist on STS-85, a 12-day mission in 1997 that carried the CRISTA-SPAS-2 free flyer. Fellow Escargot Robinson accompanied Curbeam on this mission. On his next flight, he served as a mission specialist on STS-98, the 2001 station assembly flight that delivered the Destiny U.S. Lab. During that 13-day flight, Curbeam participated in three spacewalks, spending nearly 20 hours outside. On his third and final spaceflight, he served as a mission specialist on STS-116, the 13-day assembly flight in 2006 that delivered the P5 truss segment. Curbeam participated in four spacewalks to reconfigure the station’s power system, spending nearly 26 hours outside. Across his four flights, Curbeam spent more than 37 days in space, and across his seven spacewalks more than 45 hours outside.  

Edwards, a native of Virginia and U.S. Navy commander, flew his single spaceflight as pilot of STS-89, the eighth Mir docking mission in 1998. Fellow Escargots Anderson and Reilly flew with him as mission specialists on this flight. Edwards spent nine days in space. 

A native of Louisiana and U.S. Navy captain, Gorie received his first spaceflight assignment as pilot of STS-91, the 10-day ninth and final Mir docking mission in 1998, along with fellow Escargot Kavandi. In 2000, he served as pilot of STS-99, the 11-day Shuttle Radar Topography Mission (SRTM), once again with fellow Escargot Kavandi. Gorie commanded his third mission, STS-108 in 2001, the first station Utilization Flight that lasted 12 days. He also commanded his fourth and final flight, accompanied by fellow Escargot Doi, the 16-day STS-123 mission in 2008 that delivered the Japanese pressurized logistics module and the Canadian Special Purpose Dexterous Manipulator (SPDM) to the station. Over his four missions, Gorie spent more than 48 days in space. 

A native of Alabama and a captain in the U.S. Navy Reserve, Hire completed her first space mission in 1998 as a mission specialist on the 16-day STS-90 Neurolab mission, along with fellow Escargots Altman and Williams. Twelve years later, Hire flew her second and last mission, STS-130, a 14-day space station assembly mission that installed the Node 3 Tranquility module and the Cupola. During her two flights, Hire spent nearly 30 days in space. 

Hailing from Amarillo, Texas, and a colonel in the U.S. Air Force, Husband flew as the pilot of STS-96 on his first flight. The 10-day space station resupply mission took place in 1999. He served as commander on his second flight, the 16-day STS-107 Spacehab research mission in 2003, along with fellow Escargots Anderson and Chawla. Husband perished in the Columbia accident. He logged nearly 26 days in space. 

Missouri native Kavandi completed her first spaceflight as a mission specialist on STS-91, the 10-day ninth and final Mir docking mission in 1998, along with fellow Escargot Gorie. On her second flight, she served as a mission specialist on the 11-day STS-99 SRTM in 2000, once again with fellow Escargot Gorie. As a mission specialist on STS-104, her third and final spaceflight, Kavandi flew with fellow Escargots Lindsey and Reilly to install the Quest airlock on the station. On her three flights, she logged 34 days in space. Kavandi served as director of NASA’s Glenn Research Center in Cleveland from March 2016 to September 2019. 

A colonel in the U.S. Air Force, California-born Lindsey has the distinction as the only member of his class to complete five spaceflights. He served as pilot on his first spaceflight in 1997, the 16-day STS-87 USMP-4 mission, joined by fellow Escargots Chawla and Doi. He flew as pilot on his second mission in 1998, the nine-day STS-95 mission that saw astronaut John H. Glenn return to space. Fellow Escargot Robinson joined Lindsey on this mission. He commanded his third spaceflight, the 13-day STS-104 mission in 2001 that delivered the Quest airlock to the space station. Fellow Escargots Kavandi and Reilly accompanied Lindsey on this flight. He served as commander of his fourth trip into space in 2006, the 13-day STS-121 second return to flight mission after the Columbia accident that also returned the station to a 3-person crew. For his fifth and final space mission in 2011, Lindsey once again served as commander, of STS-133, the 39th and final flight of space shuttle Discovery. The fifth Utilization and Logistics Flight delivered the Permanent Multipurpose Module and the third of four EXPRESS Logistics Carriers to the space station. Lindsey’s flight on STS-133 marked the last flight by a Flying Escargot. Across his five missions, Lindsey logged nearly 63 days in space. 

Born in Massachusetts, Lu earned a doctorate in applied physics. He received his first spaceflight assignment as a mission specialist on the nine-day STS-84 flight in 1997, the sixth Mir docking mission. Fellow Escargot Noriega accompanied him on the flight. On his second trip into space, Lu served as mission specialist on STS-106, a 12-day station resupply mission in 2000. He participated in a six-hour spacewalk to complete electrical connections between two of the station’s modules. Fellow Escargot Altman flew with Lu on this mission. On his third mission, Lu served as flight engineer of Expedition 7, spending 185 days in space in 2003, the only Escargot to complete a long-duration mission. He logged 206 days in space during his three spaceflights.

 

California native Melroy, a colonel in the U.S. Air Force, received her first flight assignment as pilot of STS-92, the 13-day space station assembly flight in 2000 that delivered the Z1 truss. She served as pilot on her second mission, STS-112, the 11-day flight that brought the S1 truss to the station in 2002. Fellow Escargot Ashby commanded this mission. On her third and final mission in 2007, she served as commander of STS-120, the 15-day assembly flight that brought the Harmony Node 2 module to the station. After hatch opening, space station commander Peggy A. Whitson greeted Melroy, highlighting the first time that women commanded both spacecraft. She accumulated nearly 39 days in space during her three missions. Melroy has served as NASA’s deputy administrator since June 2021. 

Noriega has the distinction as the first Peruvian-born astronaut, and served as a lieutenant colonel in the U.S. Marine Corps. For his first spaceflight, he served as a mission specialist, along with fellow Escargot Lu, on STS-84, the nine-day sixth Mir docking mission in 1997. On his second and final mission, Noriega served as a mission specialist on STS-97, the 11-day assembly flight in 2000 that delivered the P6 truss and the first set of U.S. solar arrays to the space station. He participated in three spacewalks, spending more than 19 hours outside. Fellow Escargot Bloomfield served as pilot on this mission. Across his two flights, Noriega accumulated 20 days in space. 

Born in Idaho, Reilly earned a doctorate in geosciences. He received his first spaceflight assignment as a mission specialist on STS-89, the nine-day eighth Mir docking mission in 1998. Fellow Escargots Edwards and Anderson joined him on this mission. On his second trip to space, Reilly served as a mission specialist on STS-104, the assembly flight to install the Quest airlock on the station. Reilly participated in three spacewalks, including the first one staged from the Quest airlock, totaling 15 and a half hours. Fellow Escargots Lindsey and Kavandi accompanied Reilly on this mission. On his third and final spaceflight, Reilley flew as a mission specialist on STS-117, the 14-day flight in 2007 that delivered the S3/S4 truss segment to the station. Reilly participated in two of the mission’s spacewalks, spending more than 13 hours outside. Fellow Escargot Sturckow served as commander on this mission. Across his three spaceflights, Reilly logged more than 35 days in space and spent nearly 29 hours outside on five spacewalks. 

California native Robinson earned a doctorate in mechanical engineering. On his first spaceflight, he flew, along with fellow Escargot Curbeam, as a mission specialist on STS-85, a 12-day mission in 1997 that carried the CRISTA-SPAS-2 free flyer. On his second trip into space, he served as a mission specialist on STS-95, commanded by fellow Escargot Lindsey, the nine-day mission in 1998 that saw astronaut John H. Glenn return to space. In 2005, Robinson flew for a third time on STS-114, the 14-day return to flight mission after the Columbia accident. He participated in three spacewalks totaling 20 hours. He flew as a mission specialist on STS-130, his fourth and final spaceflight, in 2010. Fellow Escargot Hire accompanied him on the 14-day mission that brought the Tranquility Node 3 module and the Cupola to the station. Robinson logged 48 days in space across his four missions. 

Born in Georgia, and a commander in the U.S. Navy, Still received her first spaceflight assignment as pilot for STS-83, the Microgravity Sciences Laboratory (MSL) mission in 1997. She has the distinction as the first of her class to reach space. When a fuel cell problem cut the planned 16-day mission short after four days, NASA decided to refly the mission and its crew. Still returned to space as pilot of STS-94, the MSL reflight, later in 1997, and flew the full duration 16 days. She logged a total of 20 days in space. 

California native and a colonel in the U.S. Marine Corps, Sturckow received his first spaceflight assignment as pilot of STS-88, the 12-day mission in 1998 that launched the Node 1 Unity module to begin assembly of the space station. He again served as pilot on his second spaceflight, STS-105 in 2001, a 12-day station assembly, resupply, and crew rotation mission. Sturckow served as commander on his third mission, the 14-day STS-117 mission in 2007 that delivered the S3/S4 truss segment to the station. Fellow Escargot Reilly accompanied Sturckow on this mission. He once again served as commander on his fourth and final spaceflight, STS-128, the 14-day flight in 2009 that brought facilities to the station to enable a six-person permanent crew. He logged more than 51 days in space on his four missions. 

Born in La Rochelle, France, Chrétien rose to the rank of brigadier general in the French Air Force. Selected as an astronaut by CNES in 1980, Chrétien made his first spaceflight in 1982, an eight-day mission aboard the Soviet Salyut-7 space station, the first non-Soviet and non-American to reach space. Chrétien returned to space in 1988, completing a 25-day mission aboard Mir during which he participated in a six-hour spacewalk, the first non-Soviet and non-American to do so. Under a special agreement between NASA and CNES, Chrétien and Tognini joined the Group 15 astronauts for training, making them eligible for flights on the shuttle. For his third and final spaceflight, Chrétien served as a mission specialist on the 11-day STS-86 seventh Mir docking mission in 1997. Fellow Escargot Bloomfield served as pilot on this mission. Across his three flights, Chrétien logged more than 43 days in space. 

Tokyo native Doi earned a doctorate in aerospace engineering. NASDA selected him as an astronaut in 1985 and through an agreement with NASA, he joined the Group 15 astronauts for training, making him eligible for flights on the space shuttle. On his first spaceflight, he flew as a mission specialist on STS-87, accompanied by fellow Escargots Lindsey and Chawla. The 16-day mission in 1997 carried the USMP-4 suite of experiments. Doi participated in two spacewalks, spending more than 15 hours outside the shuttle. For his second and final spaceflight, Doi flew as a mission specialist on STS-123, the 16-day assembly flight in 2008 that delivered the Japanese pressurized logistics module and the SPDM to the station. Fellow Escargot Gorie served as commander on this mission. Doi logged more than 31 days in space on his two missions. 

The French space agency CNES selected Tognini, born in Vincennes, France, in 1985. He rose to the rank of brigadier general in the French Air Force. He received his first assignment as Chrétien’s backup for his 1988 mission to Mir. For his first spaceflight, Tognini spent 14 days aboard Mir in 1992. Under a special agreement between NASA and CNES, Tognini and Chrétien joined the Group 15 astronauts for training, making them eligible for flights on the shuttle. For his second spaceflight, Tognini served as a mission specialist on STS-93, the five-day mission in 1999 to deploy the Chandra X-ray Observatory. Fellow Escargot Ashby served as pilot on this mission. Tognini logged nearly 19 days in space. 

Born in Saskatoon, Saskatchewan, Williams earned a medical degree. The CSA selected him as an astronaut in 1992, and in January 1995, as part of an agreement between NASA and the CSA, he joined the Group 15 astronauts for training, making him eligible for flights on the space shuttle. His first spaceflight took place in 1998 as a mission specialist on the 16-day STS-90 Neurolab mission, under the command of fellow Escargot Altman. For his second trip into space, he served as a mission specialist on STS-118, the 13-day assembly flight in 2007 that delivered the S5 truss segment to the space station. Williams participated in three of the mission’s four spacewalks, spending nearly 18 hours outside. Across his two missions, he spent nearly 29 days in space.

Summary of spaceflights by Group 15 astronauts. Jean-Loup Chrétien completed two earlier missions, to Salyut-7 in 1982 and to Mir in 1988, while Tognini completed one earlier mission to Mir in 1992.
Summary of spaceflights by Group 15 astronauts. Jean-Loup Chrétien completed two earlier missions, to Salyut-7 in 1982 and to Mir in 1988, while Tognini completed one earlier mission to Mir in 1992.
Credit: NASA

The Group 15 NASA and international astronauts made significant contributions to spaceflight. As a group, they completed 64 flights spending 888 days, or nearly two and a half years, in space, including the three flights Chrétien and Tognini completed before their addition to the group. One Flying Escargot made a single trip into space, nine made two trips, eight made three, four made four, and one went five times. Seventeen of the 23 participated in the assembly, research, maintenance, logistics, and management of the space station. In preparation for space station operations, ten group members visited Mir, and seven visited both space stations, but only one completed a long-duration flight. Twelve contributed their talents on Spacelab or other research missions, and three performed work with the great observatories Hubble and Chandra. Eight of the 23 performed 25 spacewalks spending 161 hours, or more than six days, outside their spacecraft.  

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Dominique V. Crespo

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      NASA’s NICER (Neutron star Interior Composition Explorer) and Neil Gehrels Swift Observatory provided valuable observations of the system in high-energy light. Other telescopes contributing data included the Karl G. Jansky Very Large Array in Magdalena, New Mexico. 
      The result: scientists found the same angle of polarization across the different wavelengths.
      “That finding is compelling evidence that a single, coherent physical mechanism underpins the light we observe,” said Francesco Coti Zelati of the Institute of Space Sciences in Barcelona, Spain, co-lead author of the findings. 
      This interpretation challenges the conventional wisdom about neutron star emissions of radiation in binary systems, the researchers said. Previous models had indicated that the X-rays come from the accretion disk, but this new study shows they originate with the pulsar wind. 
      “IXPE has observed many isolated pulsars and found that the pulsar wind powers the X-rays,” said NASA Marshall astrophysicist Philip Kaaret, principal investigator for IXPE at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “These new observations show that the pulsar wind powers most of the energy output of the system.”
      Astronomers continue to study transitional millisecond pulsars, assessing how observed physical mechanisms compare with those of other pulsars and pulsar wind nebulae. Insights from these observations could help refine theoretical models describing how pulsar winds generate radiation – and bring researchers one step closer, Baglio and Coti Zelati agreed, to fully understanding the physical mechanisms at work in these extraordinary cosmic systems.
      More about IXPE
      IXPE, which continues to provide unprecedented data enabling groundbreaking discoveries about celestial objects across the universe, is a joint NASA and Italian Space Agency mission with partners and science collaborators in 12 countries. IXPE is led by NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, Inc., headquartered in Falls Church, Virginia, manages spacecraft operations together with the University of Colorado’s Laboratory for Atmospheric and Space Physics in Boulder. Learn more about IXPE’s ongoing mission here:
      https://www.nasa.gov/ixpe
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      Last Updated Jul 15, 2025 EditorBeth RidgewayContactCorinne M. Beckingercorinne.m.beckinger@nasa.govLocationMarshall Space Flight Center Related Terms
      IXPE (Imaging X-ray Polarimetry Explorer) Marshall Astrophysics Marshall Science Research & Projects Marshall Space Flight Center Explore More
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    • NASA
      One Survey by NASA’s Roman Could Unveil 100,000 Cosmic Explosions
      By NASA
      Scientists predict one of the major surveys by NASA’s upcoming Nancy Grace Roman Space Telescope may reveal around 100,000 celestial blasts, ranging from exploding stars to feeding black holes. Roman may even find evidence of some of the universe’s first stars, which are thought to completely self-destruct without leaving any remnant behind.
      This simulation showcases the dynamic universe as NASA’s Nancy Grace Roman Space Telescope could see it over the course of its five-year primary mission. The video sparkles with synthetic supernovae from observations of the OpenUniverse simulated universe taken every five days (similar to the expected cadence of Roman’s High-Latitude Time-Domain Survey, which OpenUniverse simulates in its entirety). On top of the static sky of stars in the Milky Way and other galaxies, more than a million exploding stars flare into visibility and then slowly fade away. To highlight the dynamic physics happening and for visibility at this scale, the true brightness of each transient event has been magnified by a factor of 10,000 and no background light has been added to the simulated images. The video begins with Roman’s full field of view, which represents a single pointing of Roman’s camera, and then zooms into one square.Credit: NASA’s Goddard Space Flight Center and M. Troxel Cosmic explosions offer clues to some of the biggest mysteries of the universe. One is the nature of dark energy, the mysterious pressure thought to be accelerating the universe’s expansion.
      “Whether you want to explore dark energy, dying stars, galactic powerhouses, or probably even entirely new things we’ve never seen before, this survey will be a gold mine,” said Benjamin Rose, an assistant professor at Baylor University in Waco, Texas, who led a study about the results. The paper is published in The Astrophysical Journal.
      Called the High-Latitude Time-Domain Survey, this observation program will scan the same large region of the cosmos every five days for two years. Scientists will stitch these observations together to create movies that uncover all sorts of cosmic fireworks.
      Chief among them are exploding stars. The survey is largely geared toward finding a special class of supernova called type Ia. These stellar cataclysms allow scientists to measure cosmic distances and trace the universe’s expansion because they peak at about the same intrinsic brightness. Figuring out how fast the universe has ballooned during different cosmic epochs offers clues to dark energy.
      This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s new James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth.Credit: NASA, ESA, CSA, and STScI In the new study, scientists simulated Roman’s entire High-Latitude Time-Domain Survey. The results suggest Roman could see around 27,000 type Ia supernovae—about 10 times more than all previous surveys combined.
      Beyond dramatically increasing our total sample of these supernovae, Roman will push the boundaries of how far back in time we can see them. While most of those detected so far occurred within approximately the last 8 billion years, Roman is expected to see vast numbers of them earlier in the universe’s history, including more than a thousand that exploded more than 10 billion years ago and potentially dozens from as far back as 11.5 billion years. That means Roman will almost certainly set a new record for the farthest type Ia supernova while profoundly expanding our view of the early universe and filling in a critical gap in our understanding of how the cosmos has evolved over time.
      “Filling these data gaps could also fill in gaps in our understanding of dark energy,” Rose said. “Evidence is mounting that dark energy has changed over time, and Roman will help us understand that change by exploring cosmic history in ways other telescopes can’t.”
      But type Ia supernovae will be hidden among a much bigger sample of exploding stars Roman will see once it begins science operations in 2027. The team estimates Roman will also spot about 60,000 core-collapse supernovae, which occur when a massive star runs out of fuel and collapses under its own weight.
      That’s different from type Ia supernovae, which originate from binary star systems that contain at least one white dwarf — the small, hot core remnant of a Sun-like star — siphoning material from a companion star. Core-collapse supernovae aren’t as useful for dark energy studies as type Ias are, but their signals look similar from halfway across the cosmos.
      “By seeing the way an object’s light changes over time and splitting it into spectra — individual colors with patterns that reveal information about the object that emitted the light—we can distinguish between all the different types of flashes Roman will see,” said Rebekah Hounsell, an assistant research scientist at the University of Maryland-Baltimore County working at NASA’s Goddard Space Flight Center in Greenbelt, Maryland and a co-author of the study.
      “With the dataset we’ve created, scientists can train machine-learning algorithms to distinguish between different types of objects and sift through Roman’s downpour of data to find them,” Hounsell added. “While searching for type Ia supernovae, Roman is going to collect a lot of cosmic ‘bycatch’—other phenomena that aren’t useful to some scientists, but will be invaluable to others.”
      Hidden Gems
      Thanks to Roman’s large, deep view of space, scientists say the survey should also unearth extremely rare and elusive phenomena, including even scarcer stellar explosions and disintegrating stars.
      Upon close approach to a black hole, intense gravity can shred a star in a so-called tidal disruption event. The stellar crumbs heat up as they swirl around the black hole, creating a glow astronomers can see from across vast stretches of space-time. Scientists think Roman’s survey will unveil 40 tidal disruption events, offering a chance to learn more about black hole physics.
      The team also estimates Roman will find about 90 superluminous supernovae, which can be 100 times brighter than a typical supernova. They pack a punch, but scientists aren’t completely sure why. Finding more of them will help astronomers weigh different theories.
      Even rarer and more powerful, Roman could also detect several kilonovae. These blasts occur when two neutron stars — extremely dense cores leftover from stars that exploded as supernovae — collide. To date, there has been only one definitive kilonova detection. The team estimates Roman could spot five more.
      NASA’s Roman Space Telescope will survey the same areas of the sky every few days following its launch in May 2027. Researchers will mine these data to identify kilonovae – explosions that happen when two neutron stars or a neutron star and a black hole collide and merge. When these collisions happen, a fraction of the resulting debris is ejected as jets, which move near the speed of light. The remaining debris produces hot, glowing, neutron-rich clouds that forge heavy elements, like gold and platinum. Roman’s extensive data will help astronomers better identify how often these events occur, how much energy they give off, and how near or far they are.Credit: NASA, ESA, J. Olmsted (STScI) That would help astronomers learn much more about these mysterious events, potentially including their fate. As of now, scientists are unsure whether kilonovae result in a single neutron star, a black hole, or something else entirely.
      Roman may even spot the detonations of some of the first stars that formed in the universe. These nuclear furnaces were giants, up to hundreds of times more massive than our Sun, and unsullied by heavy elements that hadn’t yet formed.
      They were so massive that scientists think they exploded differently than modern massive stars do. Instead of reaching the point where a heavy star today would collapse, intense gamma rays inside the first stars may have turned into matter-antimatter pairs (electrons and positrons). That would drain the pressure holding the stars up until they collapsed, self-destructing in explosions so powerful they’re thought to leave nothing behind.
      So far, astronomers have found about half a dozen candidates of these “pair-instability” supernovae, but none have been confirmed.
      “I think Roman will make the first confirmed detection of a pair-instability supernova,” Rose said — in fact the study suggests Roman will find more than 10. “They’re incredibly far away and very rare, so you need a telescope that can survey a lot of the sky at a deep exposure level in near-infrared light, and that’s Roman.”
      A future rendition of the simulation could include even more types of cosmic flashes, such as variable stars and active galaxies. Other telescopes may follow up on the rare phenomena and objects Roman discovers to view them in different wavelengths of light to study them in more detail.
      “Roman’s going to find a whole bunch of weird and wonderful things out in space, including some we haven’t even thought of yet,” Hounsell said. “We’re definitely expecting the unexpected.”
      For more information about the Roman Space Telescope visit www.nasa.gov/roman.
      The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
      By Ashley Balzer
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
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      Last Updated Jul 15, 2025 EditorAshley BalzerContactAshley Balzerashley.m.balzer@nasa.gov Related Terms
      Nancy Grace Roman Space Telescope Astrophysics Black Holes Dark Energy Galaxies, Stars, & Black Holes Galaxies, Stars, & Black Holes Research Goddard Space Flight Center Science & Research Stars Supernovae The Universe Explore More
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    • NASA
      Fourth NASA-Enabled Private Flight to Space Station Completes Safely
      By NASA
      The Axiom Mission 4 crew launched on June 25, 2025, aboard a SpaceX Dragon spacecraft to the International Space Station from NASA’s Kennedy Space Center in Florida. From left to right: Tibor Kapu of Hungary, ISRO (Indian Space Research Organization) astronaut Shubhanshu Shukla, former NASA astronaut Peggy Whitson, and ESA (European Space Agency) astronaut Sławosz Uznański-Wiśniewski of Poland (Credit: Axiom Space). The NASA-supported fourth private astronaut mission to the International Space Station, Axiom Mission 4, completed its flight as part of the agency’s efforts to demonstrate demand and build operational knowledge for future commercial space stations.
      The four-person crew safely returned to Earth, splashing down off the coast of California at 5:31 a.m. EDT on Tuesday, aboard a SpaceX Dragon spacecraft. Teams aboard SpaceX recovery vessels retrieved the spacecraft and astronauts. 
      Peggy Whitson, former NASA astronaut and director of human spaceflight at Axiom Space, ISRO (Indian Space Research Organization) astronaut Shubhanshu Shukla, and ESA (European Space Agency) project astronaut Sławosz Uznański-Wiśniewski of Poland, and Hungarian to Orbit (HUNOR) astronaut Tibor Kapu of Hungary, completed about two and a half weeks in space.
      The Axiom Mission 4 crew launched at 2:31 a.m. on June 25, on a Falcon 9 rocket from NASA’s Kennedy Space Center in Florida. Approximately 28 hours later, Dragon docked to the space-facing port of the space station’s Harmony module. The astronauts undocked at 7:15 a.m. on July 14, to begin the trip home.
      The crew conducted microgravity research, educational outreach, and commercial activities. The spacecraft will return to Florida for inspection and processing at SpaceX’s refurbishing facilities. Throughout their mission, the astronauts conducted about 60 science experiments, and returned science, including NASA cargo, back to Earth.
      A collaboration between NASA and ISRO allowed Axiom Mission 4 to deliver on a commitment highlighted by President Trump and Indian Prime Minister Narendra Modi to send the first ISRO astronaut to the station. The space agencies participated in five joint science investigations and two in-orbit science, technology, engineering, and mathematics demonstrations. NASA and ISRO have a long-standing relationship built on a shared vision to advance scientific knowledge and expand space collaboration.
      The private mission also carried the first astronauts from Poland and Hungary to stay aboard the space station.
      The International Space Station is a springboard for developing a low Earth orbit economy. NASA’s goal is to achieve a strong economy off the Earth where the agency can purchase services as one of many customers to meet its science and research objectives in microgravity. NASA’s commercial strategy for low Earth orbit provides the government with reliable and safe services at a lower cost, enabling the agency to focus on Artemis missions to the Moon in preparation for Mars while also continuing to use low Earth orbit as a training and proving ground for those deep space missions.
      Learn more about NASA’s commercial space strategy at:
      https://www.nasa.gov/commercial-space

      News Media Contacts:
      Claire O’Shea 
      Headquarters, Washington 
      202-358-1100 
      claire.a.o’shea@nasa.gov

      Anna Schneider 
      Johnson Space Center, Houston 
      281-483-5111 
      anna.c.schneider@nasa.gov
      Facebook logo @NASA @NASA Instagram logo @NASA Linkedin logo @NASA View the full article
    • NASA
      Melissa Harris: Shaping NASA’s Vision for a Future in Low Earth Orbit
      By NASA
      Melissa Harris’ official NASA portrait. NASA/Robert Markowitz With over 25 years of experience in human spaceflight programs, Melissa Harris has contributed to numerous programs and projects during key moments in NASA’s history. As the life cycle lead and Independent Review Team review manager for the Commercial Low Earth Orbit Development Program, she guides the agency through development initiatives leading to a new era of space exploration.  

      Harris grew up near NASA’s Johnson Space Center in Houston and spent time exploring the center and trying on astronaut helmets. She later earned her bachelor’s degree in legal studies from the University of Houston, master and subject matter expert certifications in configuration management, and ISO 9001 Lead Auditors Certification. When the opportunity arose, she jumped at the chance to join the International Space Station Program. 

      Harris (right) and her twin sister, Yvonne (left), at the Artemis I launch. Image courtesy of Melissa Harris Starting as a board specialist, Harris spent eight years supporting the space station program boards, panels, and flight reviews. Other areas of support included the International Space Station Mission Evaluation Room and the EVA Crew Systems and Robotics Division managing changes for the acquisition and building of mockups in the Neutral Buoyancy Laboratory and Space Vehicle Mockup Facility in Houston. She then took a leap to join the Constellation Program, developing and overseeing program and project office processes and procedures. Harris then transitioned to the Extravehicular Activity (EVA) Project Office where she was a member of the EVA 23 quality audit team tasked with reviewing data to determine the cause of an in-orbit failure. She also contributed to the Orion Program and Artemis campaign. After spending two years at Axiom Space, Harris returned to NASA and joined the commercial low Earth orbit team. 

      Harris said the biggest lesson she has learned during her career is that “there are always ups and downs and not everything works out, but if you just keep going and at the end of the day see that the hard work and dedication has paid off, it is always the proudest moment.”  

      Her dedication led to a nomination for the Stellar Award by the Rotary National Award for Space Achievement Foundation.

      Harris and her son, Tyler, at the Rotary National Award Banquet in 2024.Image courtesy of Melissa Harris Harris’ favorite part of her role at NASA is working “closely with brilliant minds” and being part of a dedicated and hard-working team that contributes to current space programs while also planning for future programs. Looking forward, she anticipates witnessing the vision and execution of a self-sustaining commercial market in low Earth orbit come to fruition. 

      Outside of work, Harris enjoys being with family, whether cooking on the back porch, over a campfire, or traveling both in and out of the country. She has been married for 26 years to her high school sweetheart, Steve, and has one son, Tyler. Her identical twin sister, Yvonne, also works at Johnson. 

      Harris and her twin sister Yvonne dressed as Mark and Scott Kelly for Halloween in 2024.Image courtesy of Melissa Harris Learn more about NASA’s Commercial Low Earth Orbit Development Program at: 
      www.nasa.gov/commercialspacestations
      View the full article

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