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Explore Webb Science James Webb Space Telescope (JWST) NASA Webb Looks at… Webb News Latest News Latest Images Webb’s Blog Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Webb Timeline Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Science Explainers Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Webb’s First Images Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 6 Min Read NASA Webb Looks at Earth-Sized, Habitable-Zone Exoplanet TRAPPIST-1 e This artist’s concept shows the volatile red dwarf star TRAPPIST-1 and its four most closely orbiting planets. Full image and caption shown below. Credits: Artwork: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI) Scientists are in the midst of observing the exoplanet TRAPPIST-1 e with NASA’s James Webb Space Telescope. Careful analysis of the results so far presents several potential scenarios for what the planet’s atmosphere and surface may be like, as NASA science missions lay key groundwork to answer the question, “are we alone in the universe?” “Webb’s infrared instruments are giving us more detail than we’ve ever had access to before, and the initial four observations we’ve been able to make of planet e are showing us what we will have to work with when the rest of the information comes in,” said Néstor Espinoza of the Space Telescope Science Institute in Baltimore, Maryland, a principal investigator on the research team. Two scientific papers detailing the team’s initial results are published in the Astrophysical Journal Letters. Image A: Trappist-1 e (Artist’s Concept) This artist’s concept shows the volatile red dwarf star TRAPPIST-1 and its four most closely orbiting planets, all of which have been observed by NASA’s James Webb Space Telescope. Webb has found no definitive signs of an atmosphere around any of these worlds yet. Artwork: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI) Of the seven Earth-sized worlds orbiting the red dwarf star TRAPPIST-1, planet e is of particular interest because it orbits the star at a distance where water on the surface is theoretically possible — not too hot, not too cold — but only if the planet has an atmosphere. That’s where Webb comes in. Researchers aimed the telescope’s powerful NIRSpec (Near-Infrared Spectrograph) instrument at the system as planet e transited, or passed in front of, its star. Starlight passing through the planet’s atmosphere, if there is one, will be partially absorbed, and the corresponding dips in the light spectrum that reaches Webb will tell astronomers what chemicals are found there. With each additional transit, the atmospheric contents become clearer as more data is collected. Primary atmosphere unlikely Though multiple possibilities remain open for planet e because only four transits have been analyzed so far, the researchers feel confident that the planet does not still have its primary, or original, atmosphere. TRAPPIST-1 is a very active star, with frequent flares, so it is not surprising to researchers that any hydrogen-helium atmosphere with which the planet may have formed would have been stripped off by stellar radiation. However many planets, including Earth, build up a heavier secondary atmosphere after losing their primary atmosphere. It is possible that planet e was never able to do this and does not have a secondary atmosphere. Yet researchers say there is an equal chance there is an atmosphere, and the team developed novel approaches to working with Webb’s data to determine planet e’s potential atmospheres and surface environments. World of (fewer) possibilities The researchers say it is unlikely that the atmosphere of TRAPPIST-1 e is dominated by carbon dioxide, analogous to the thick atmosphere of Venus and the thin atmosphere of Mars. However, the researchers also are careful to note that there are no direct parallels with our solar system. “TRAPPIST-1 is a very different star from our Sun, and so the planetary system around it is also very different, which challenges both our observational and theoretical assumptions,” said team member Nikole Lewis, an associate professor of astronomy at Cornell University. If there is liquid water on TRAPPIST-1 e, the researchers say it would be accompanied by a greenhouse effect, in which various gases, particularly carbon dioxide, keep the atmosphere stable and the planet warm. “A little greenhouse effect goes a long way,” said Lewis, and the measurements do not rule out adequate carbon dioxide to sustain some water on the surface. According to the team’s analysis, the water could take the form of a global ocean, or cover a smaller area of the planet where the star is at perpetual noon, surrounded by ice. This would be possible because, due to the TRAPPIST-1 planets’ sizes and close orbits to their star, it is thought that they all are tidally locked, with one side always facing the star and one side always in darkness. Image B: TRAPPIST-1 e Transmission Spectrum (NIRSpec) This graphic compares data collected by Webb’s NIRSpec (Near-Infrared Spectrograph) with computer models of exoplanet TRAPPIST-1 e with (blue) and without (orange) an atmosphere. Narrow colored bands show the most likely locations of data points for each model. Illustration: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI) Innovative new method Espinoza and co-principal investigator Natalie Allen of Johns Hopkins University are leading a team that is currently making 15 additional observations of planet e, with an innovative twist. The scientists are timing the observations so that Webb catches both planets b and e transiting the star one right after the other. After previous Webb observations of planet b, the planet orbiting closest to TRAPPIST-1, scientists are fairly confident it is a bare rock without an atmosphere. This means that signals detected during planet b’s transit can be attributed to the star only, and because planet e transits at nearly the same time, there will be less complication from the star’s variability. Scientists plan to compare the data from both planets, and any indications of chemicals that show up only in planet e’s spectrum can be attributed to its atmosphere. “We are really still in the early stages of learning what kind of amazing science we can do with Webb. It’s incredible to measure the details of starlight around Earth-sized planets 40 light-years away and learn what it might be like there, if life could be possible there,” said Ana Glidden, a post-doctoral researcher at Massachusetts Institute of Technology’s Kavli Institute for Astrophysics and Space Research, who led the research on possible atmospheres for planet e. “We’re in a new age of exploration that’s very exciting to be a part of,” she said. The four transits of TRAPPIST-1 e analyzed in the new papers published today were collected by the JWST Telescope Scientist Team’s DREAMS (Deep Reconnaissance of Exoplanet Atmospheres using Multi-instrument Spectroscopy) collaboration. The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency). To learn more about Webb, visit: https://science.nasa.gov/webb Related Information Webb Blog: Reconnaissance of Potentially Habitable Worlds with NASA’s Webb Video: How to Study Exoplanets Video: How do we learn about a planet’s Atmosphere? View more about Exoplanets More Webb News More Webb Images Webb Science Themes Webb Mission Page Related For Kids What is the Webb Telescope? SpacePlace for Kids En Español Ciencia de la NASA NASA en español Space Place para niños Related Images & Videos Trappist-1 e (Artist’s Concept) This artist’s concept shows the volatile red dwarf star TRAPPIST-1 and its four most closely orbiting planets, all of which have been observed by NASA’s James Webb Space Telescope. Webb has found no definitive signs of an atmosphere around any of these worlds yet. TRAPPIST-1 e Transmission Spectrum (NIRSpec) This graphic compares data collected by Webb’s NIRSpec (Near-Infrared Spectrograph) with computer models of exoplanet TRAPPIST-1 e with (blue) and without (orange) an atmosphere. Narrow colored bands show the most likely locations of data points for each model. Share Details Last Updated Sep 08, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Location NASA Goddard Space Flight Center Contact Media Laura Betz NASA’s Goddard Space Flight Center Greenbelt, Maryland laura.e.betz@nasa.gov Leah Ramsay Space Telescope Science Institute Baltimore, Maryland Hannah Braun Space Telescope Science Institute Baltimore, Maryland Related Terms James Webb Space Telescope (JWST) Exoplanets Related Links and Documents The science paper by N. Espinoza et al. The science paper by A. Glidden et al. JWST Telescope Science Team Keep Exploring Related Topics James Webb Space Telescope Space Telescope Exoplanets Exoplanet Stories Universe View the full article

Students prepare their robots to enter Artemis Arena during NASA’s Lunabotics competition on May 20, 2025, at the Center for Space Education near the Kennedy Space Center Visitor Complex in Florida. NASA/Isaac Watson As college students across the country embark upon the academic year, NASA is giving them something else to look forward to – the agency’s 2026 Lunabotics Challenge. Teams interested in participating can submit their applications and supporting materials through NASA’s Stem Gateway portal beginning Monday, Sept. 8. Key dates and challenge details are available in the 2026 Lunabotics Challenge Guidebook. Once all applications and supporting materials are received and evaluated, NASA will notify the selected teams to begin the challenge. Student teams participating in this year’s challenge will create robots capable of building berms out of lunar regolith – the loose, fragmental material on the Moon’s surface. Structures like these will be important during lunar missions as blast protection during lunar landings and launches, shading for cryogenic propellant tank farms, radiation shielding around nuclear power plants, and other uses critical to future Moon missions. “We are excited to continue the Lunabotics competition for universities as NASA develops new Moon to Mars technologies for the Artemis program,” said Robert Mueller, senior technologist at NASA, as well as co-founder and chief judge of the Lunabotics competition. “Excavating and moving regolith is a fundamental need to build infrastructure on the Moon and Mars and this competition creates 21st century skills in the future workforce.” An in-person qualifying event will be held May 12-17, 2026, at the University of Central Florida’s Space Institute’s Exolith Lab in Orlando. From this round, the top 10 teams will be invited to bring their robots to the final competition on May 19-21, at the Kennedy Space Center Visitor Complex’s Artemis Arena in Florida, which has an area filled with a lunar regolith simulant. The team scoring the most points will receive the Lunabotics Grand Prize and participate in an exhibition-style event at NASA Kennedy. By encouraging innovative construction techniques and assessing student designs and data the same way it does its own prototypes, NASA casts a wider net to find innovative solutions to challenges inherent in future Artemis missions, like developing future lunar excavators, in-situ resource utilization capabilities, and living on the Moon or Mars. With its multidisciplinary approach, Lunabotics also serves as a workforce pipeline, with teams gaining valuable hands-on experience in computer coding, engineering, manufacturing, fabricating, and other crucial skills, while also receiving technical expertise in space technology development. NASA’s Lunabotics Challenge, held annually since 2010, is one of several Artemis Student Challenges. The two-semester competition provides U.S. college and technical school teams an opportunity to design, build, and operate a prototype lunar robot using NASA systems engineering processes. Competitions help NASA get innovative design and operational data, reduce risks, and cultivate new ideas needed to return to the Moon under the Artemis campaign to prepare for human exploration of Mars. To learn more about Lunabotics, visit: https://www.nasa.gov/learning-resources/lunabotics-challenge/ View the full article

A child of the Space Shuttle Program, Jeni Morrison grew up walking the grounds of NASA’s Johnson Space Center in Houston with her parents and listening to family stories about human spaceflight. Now, with more than 15 years at NASA, Morrison serves as one of Johnson’s Environmental Programs managers. She ensures the center complies with laws that protect its resources by overseeing regulatory compliance for cultural and natural resources, stormwater and drinking water programs, and the National Environmental Policy Act. She also safeguards Johnson’s historic legacy as Johnson’s Cultural Resources manager. Jeni Morrison in the mall area at NASA’s Johnson Space Center in Houston, where employees often see local wildlife, including turtles, birds, deer, and the occasional alligator. “I make sure our actions comply with the National Historic Preservation act, since the center is considered a historic district with two National Historic Landmarks onsite,” Morrison said. “I make sure we respect and document Johnson’s heritage while paving the way for new efforts and mission objectives.” Morrison takes pride in finding solutions that increase efficiency while protecting resources. One example was a project with Johnson’s Geographic Information System team to create an interactive material and chemical spill plan map. The new system helps responders quickly trace spill paths above and underground to deploy resources faster, reducing cleanup costs and minimizing environmental impacts. “Every improvement we make not only saves time and resources, but strengthens our ability to support NASA’s mission,” she said. By the very nature of our work, NASA makes history all the time. That history is important for all people, both to remember the sacrifices and accomplishments of so many, but also to ensure we don’t repeat mistakes as we strive for even bolder achievements. Jeni Morrison Environmental Program Manager Jeni Morrison presents an overview of environmental compliance and center initiatives to employees at NASA’s Johnson Space Center in 2014. NASA/Lauren Harnett For Morrison, success often comes down to teamwork. She has learned to adapt her style to colleagues’ needs to strengthen collaboration. “By making the effort to accommodate others’ communication styles and learn from different perspectives, we create better, more efficient work,” she said. “Thankfully, so many people here at NASA are willing to teach and to share their experiences.” Her message to the Artemis Generation is simple: Always keep learning! “You never know when a side conversation could give you an answer to a problem you are facing down the line,” she said. “You must be willing to ask questions and learn something new to find those connections.” Jeni Morrison (second from right) with the Biobased Coolant Project Team at NASA’s Johnson Space Center in 2018. The team tested biobased metalworking coolants and identified a product that outperformed petroleum-based options, meeting flight hardware specifications while reducing waste disposal costs and labor hours. Even as a young child visiting NASA Johnson, I could feel the sense of adventure, accomplishment, and the drive to reach new heights of human capability. I realize that those experiences gave me a fascination with learning and an inherent need to find ways to do things better. jENI mORRISON Environmental Program Manager Her passion for learning and discovery connects to a family tradition at NASA. Her grandfather contributed to multiple Apollo missions, including helping solve the oxygen tank malfunction on Apollo 13. Her mother worked at the center transcribing astronaut recordings and writing proposals, and her father flew experiments aboard the space shuttle and International Space Station. Morrison’s sister and extended family also worked at Johnson. Now her son is growing up on the center grounds while attending the JSC Child Care Center. “As the fourth generation to be at Johnson, he is already talking about how he loves science and can’t wait to do his own experiments,” she said. For Morrison, carrying that family legacy forward through environmental stewardship is a privilege. “Being able to contribute to NASA’s mission through environmental compliance feels like the best of both worlds for me,” Morrison said. “It combines my love of science and NASA with my drive to find more efficient ways to operate while protecting this incredible site and everything it represents.” Explore More 4 min read Mark Cavanaugh: Integrating Safety into the Orion Spacecraft Article 1 month ago 6 min read She Speaks for the Samples: Meet Dr. Juliane Gross, Artemis Campaign Sample Curation Lead Article 5 months ago 5 min read Johnson’s Jason Foster Recognized for New Technology Reporting Record Article 3 months ago View the full article

3 Min Read NASA Seeks Industry Input on Next Phase of Commercial Space Stations The aurora australis appears over the Earth in this photograph taken from the International Space Station as it orbited 269 miles above the Indian Ocean southwest of Australia. Credits: NASA NASA is requesting feedback from American companies on the next phase of its commercial space stations strategy to ensure a seamless transition of activities in low Earth orbit from the International Space Station. The agency released a draft Phase 2 Announcement for Partnership Proposals (AFPP) Friday, asking for feedback from industry partners by 1 p.m. EDT Friday, Sept. 12. NASA will hold an informational industry briefing on Monday, Sept. 8, to provide a top-level summary of the documents and expectations. Under the direction of acting NASA Administrator Sean Duffy, the agency reassessed the commercial space stations acquisition strategy to ensure mission continuity, affordability, and national alignment, and to reduce the potential for a gap of a crew-capable platform in low Earth orbit. “NASA has led in low Earth orbit for 25 years and counting. Now, as we prepare for deorbiting the International Space Station in 2030, we’re calling on our commercial space partners to maintain this historic human presence,” Duffy said. “The American space industry is booming. Insight from these innovative companies will be invaluable as we work to chart the next phase of commercial space stations.” In Phase 2, NASA intends to support industry’s design and demonstration of commercial stations through multiple funded Space Act Agreements, selected through a full and open competition. “NASA is committed to continuing our partnership with industry to ensure a continuity in low Earth orbit,” said Angela Hart, manager, Commercial Low Earth Orbit Development Program at NASA’s Johnson Space Center in Houston. “The work done under our Phase 1 contracts and agreements have put us in a prime position to be successful for this next funded Space Act Agreement phase. By leveraging these agreements, we provide additional flexibility to our commercial partners to define the best path forward to provide NASA a safe and affordable crewed demonstration.” The Phase 2 agreements are expected to include funded milestones leading to critical design review readiness and an in-space crewed demonstration of four crew members for a minimum of 30 days. Agreements are expected to include up to a five-year period of performance. The agency’s phased approach will culminate in a follow-on Phase 3 using Federal Acquisition Regulation-based contract(s) to purchase station services through a full and open competition. This final phase will also provide formal design acceptance and certification, ensuring the commercial stations meet NASA’s safety requirements. NASA remains committed to fostering innovation and collaboration within the American space industry. The agency’s commercial strategy for low Earth orbit will provide the government with reliable and safe services at a lower cost, enabling the agency to focus on the next step in humanity’s exploration of the solar system while also continuing to use low Earth orbit as an ideal environment for training and a proving ground for Artemis missions to the Moon and Mars. Learn more about commercial space stations at: https://www.nasa.gov/commercialspacestations Keep Exploring Discover More Topics From NASA Low Earth Orbit Economy Commercial Space Stations Commercial Space News Humans In Space View the full article

A view inside the sandbox portion of the Crew Health and Performance Analog, where research volunteers participate in simulated walks on the surface of Mars. Credit: NASA Four research volunteers will soon participate in NASA’s year-long simulation of a Mars mission inside a habitat at the agency’s Johnson Space Center in Houston. This mission will provide NASA with foundational data to inform human exploration of the Moon, Mars, and beyond. Ross Elder, Ellen Ellis, Matthew Montgomery, and James Spicer enter into the 1,700-square-foot Mars Dune Alpha habitat on Sunday, Oct. 19, to begin their mission. The team will live and work like astronauts for 378 days, concluding their mission on Oct. 31, 2026. Emily Phillips and Laura Marie serve as the mission’s alternate crew members. Through a series of Earth-based missions called CHAPEA (Crew Health and Performance Exploration Analog), carried out in the 3D-printed habitat, NASA aims to evaluate certain human health and performance factors ahead of future Mars missions. The crew will undergo realistic resource limitations, equipment failures, communication delays, isolation and confinement, and other stressors, along with simulated high-tempo extravehicular activities. These scenarios allow NASA to make informed trades between risks and interventions for long-duration exploration missions. “As NASA gears up for crewed Artemis missions, CHAPEA and other ground analogs are helping to determine which capabilities could best support future crews in overcoming the human health and performance challenges of living and operating beyond Earth’s resources – all before we send humans to Mars,” said Sara Whiting, project scientist with NASA’s Human Research Program at NASA Johnson. Crew members will carry out scientific research and operational tasks, including simulated Mars walks, growing a vegetable garden, robotic operations, and more. Technologies specifically designed for Mars and deep space exploration will also be tested, including a potable water dispenser and diagnostic medical equipment. “The simulation will allow us to collect cognitive and physical performance data to give us more insight into the potential impacts of the resource restrictions and long-duration missions to Mars on crew health and performance,” said Grace Douglas, CHAPEA principal investigator. “Ultimately, this information will help NASA make informed decisions to design and plan for a successful human mission to Mars.” This mission, facilitated by NASA’s Human Research Program, is the second one-year Mars surface simulation conducted through CHAPEA. The first mission concluded on July 6, 2024. The Human Research Program pursues methods and technologies to support safe, productive human space travel. Through applied research conducted in laboratories, simulations, and aboard the International Space Station, the program investigates the effects spaceflight has on human bodies and behaviors to keep astronauts healthy and mission-ready. Primary Crew Ross Elder, Commander Ross Elder, from Williamstown, West Virginia, is a major and experimental test pilot in the United States Air Force. At the time of his selection, he served as the director of operations of the 461st Flight Test Squadron. He has piloted over 35 military aircraft and accumulated more than 1,800 flying hours, including 200 combat hours, primarily in the F-35, F-15E/EX, F-16, and A-10C. His flight test experience focuses on envelope expansion, crewed-uncrewed teaming, artificial intelligence, autonomy, mission systems, and weapons modernization. Elder earned a Bachelor of Science in astronautical engineering from the U.S. Air Force Academy in Colorado Springs, Colorado, and commissioned as an Air Force officer upon graduation. He earned a Master of Science in mechanical engineering from the University of Colorado in Colorado Springs and a master’s degree in flight test engineering from the U.S. Air Force Test Pilot School at Edwards Air Force Base in California. Ellen Ellis, Medical Officer Ellen Ellis, from North Kingstown, Rhode Island, is a colonel and an acquisitions officer in the United States Space Force. She currently serves as a senior materiel leader in the National Reconnaissance Office (NRO) Communications Systems Directorate. She is responsible for fielding commercial cloud and traditional information technology hosting solutions and building modernized data centers for the NRO. She previously served as an Intercontinental Ballistic Missile operations officer and GPS satellite engineer, and she also developed geospatial intelligence payloads and ground processing systems. She earned a Bachelor of Science in aerospace engineering at Syracuse University in New York and holds four master’s degrees, including a Master of Science in systems engineering from the Naval Postgraduate School in California, and a Master of Science in emergency and disaster management from Georgetown University in Washington. Matthew Montgomery, Science Officer Matthew Montgomery, from Los Angeles, is a hardware engineering design consultant who works with technology startup companies to develop, commercialize, and scale their products. His focus areas include LED lighting, robotics, controlled environment agriculture, and embedded control systems. Montgomery earned a Bachelor of Science and a Master of Science in electrical engineering from the University of Central Florida. He is also a founder and co-owner of Floating Lava Studios, a film production company based in Los Angeles. James Spicer, Flight Engineer James Spicer is a technical director in the aerospace and defense industry. His experience includes building radio and optical satellite communications networks; space data relay networks for human spaceflight; position, navigation, and timing research; and hands-on spacecraft design, integration, and tests. Spicer earned a Bachelor of Science and Master of Science in aeronautics and astronautics, and holds a Notation in Science Communication from Stanford University in California. He also holds commercial pilot and glider pilot licenses. Alternate Crew Emily Phillips Emily Phillips, from Waynesburg, Pennsylvania, is a captain and pilot in the United States Marine Corps. She currently serves as a forward air controller and air officer attached to an infantry battalion stationed at the Marine Corps Air Ground Combat Center in Twentynine Palms, California. Phillips earned a Bachelor of Science in computer science from the U.S. Naval Academy in Annapolis and commissioned as a Marine Corps officer upon graduation. She attended flight school, earning her Naval Aviator wings and qualifying as an F/A-18C Hornet pilot. Phillips has completed multiple deployments to Europe and Southeast Asia. Laura Marie Born in the United Kingdom, Laura Marie immigrated to the U.S. in 2016. She is a commercial airline pilot specializing in flight safety, currently operating passenger flights in Washington. Marie began her aviation career in 2019 and has amassed over 2,800 flight hours. She holds a Bachelor of Arts in philosophy and a Master of Science in aeronautics from Liberty University in Lynchburg, Virginia. In addition to her Airline Transport Pilot License, she also possesses flight instructor and advanced ground instructor licenses. Outside the flight deck, Marie dedicates her time to mentoring and supporting aspiring pilots as they navigate their careers. Explore More 4 min read NASA Glenn Tests Mini-X-Ray Technology to Advance Space Health Care Article 1 day ago 4 min read NASA’s SpaceX Crew-11 to Support Health Studies for Deep Space Travel Article 2 months ago 2 min read What Are the Dangers of Going to Space? We Asked a NASA Expert: Episode 55 Article 5 months ago Keep Exploring Discover More Topics From NASA Living in Space Artemis Human Research Program Space Station Research and Technology View the full article

NASA/Rad Sinyak Orion Mission Evaluation Room (MER) team member works during an Artemis II mission simulation on Aug. 19, 2025, from the new Orion MER inside the Mission Control Center at NASA’s Johnson Space Center in Houston. As NASA’s Orion spacecraft is carrying crew around the Moon on the Artemis II mission, a team of expert engineers in the Mission Control Center at NASA’s Johnson Space Center in Houston will be meticulously monitoring the spacecraft along its journey. They’ll be operating from a new space in the mission control complex built to host the Orion Mission Evaluation Room (MER). Through the success of Orion and the Artemis missions, NASA will return humanity to the Moon and prepare to land an American on the surface of Mars. View the full article

The Roscosmos Progress 92 cargo spacecraft approaches the International Space Station on July 5, 2025, for an automated docking to the orbital complex’s Poisk module.Credit: NASA NASA will provide live coverage of the launch and docking of a Roscosmos cargo spacecraft carrying about three tons of food, fuel, and supplies for the crew aboard the International Space Station. The unpiloted Roscosmos Progress 93 resupply spacecraft is scheduled to launch at 11:54 a.m. EDT (8:54 p.m. Baikonur time), Thursday, Sept. 11, on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan. Live coverage will begin at 11:30 a.m. on NASA+, Amazon Prime, and more. Learn how to watch NASA content through a variety of platforms, including social media. After a two-day journey to the station, the spacecraft will dock autonomously to the aft port of the station’s Zvezda module at 1:27 p.m. on Saturday, Sept. 13. NASA’s rendezvous and docking coverage will begin at 12:30 p.m. on NASA+, Amazon Prime, and more. The Progress 93 spacecraft will remain docked to the space station for approximately six months before departing for re-entry into Earth’s atmosphere to dispose of trash loaded by the crew. Ahead of the spacecraft’s arrival, the Progress 91 spacecraft will undock from the Zvezda Service Module on Tuesday, Sept. 9. NASA will not stream the undocking. The International Space Station is a convergence of science, technology, and human innovation enabling research not possible on Earth. For nearly 25 years, NASA has supported a continuous U.S. human presence aboard the orbiting laboratory, where astronauts have learned to live and work in space for extended periods of time. The space station is a springboard for developing a low Earth economy and NASA’s next great leaps in human exploration at the Moon and Mars. Learn more about the International Space Station, its research, and crew, at: https://www.nasa.gov/station -end- Jimi Russell Headquarters, Washington 202-358-1100 james.j.russell@nasa.gov Sandra Jones / Joseph Zakrzewski Johnson Space Center, Houston 281-483-5111 sandra.p.jones@nasa.gov / joseph.a.zakrzewski@nasa.gov Share Details Last Updated Sep 05, 2025 LocationNASA Headquarters Related TermsInternational Space Station (ISS)ISS ResearchJohnson Space Center View the full article

Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Universe Uncovered Hubble’s Partners in Science AI and Hubble Science Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Astronaut Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts Multimedia Images Videos Sonifications Podcasts e-Books Online Activities 3D Hubble Models Lithographs Fact Sheets Posters Hubble on the NASA App Glossary News Hubble News Social Media Media Resources More 35th Anniversary Online Activities 2 min read Hubble Spies Galaxy with Lots to See This NASA/ESA Hubble Space Telescope features the galaxy NGC 7456. ESA/Hubble & NASA, D. Thilker While it may appear as just another spiral galaxy among billions in the universe, this image from the NASA/ESA Hubble Space Telescope reveals a galaxy with plenty to study. The galaxy, NGC 7456, is located over 51 million light-years away in the constellation Grus (the Crane). This Hubble image reveals fine detail in the galaxy’s patchy spiral arms, followed by clumps of dark, obscuring dust. Blossoms of glowing pink are rich reservoirs of gas where new stars are forming, illuminating the clouds around them and causing the gas to emit this tell-tale red light. The Hubble observing program that collected this data focused on the galaxy’s stellar activity, tracking new stars, clouds of hydrogen, and star clusters to learn how the galaxy evolved through time. Hubble, with its ability to capture visible, ultraviolet, and some infrared light, is not the only observatory focused on NGC 7456. ESA’s XMM-Newton satellite imaged X-rays from the galaxy on multiple occasions, discovering many so-called ultraluminous X-ray sources. These small, compact objects emit terrifically powerful X-rays, much more than researchers would expect, given their size. Astronomers are still trying to pin down what powers these extreme objects, and NGC 7456 contributes a few more examples. The region around the galaxy’s supermassive black hole is also spectacularly bright and energetic, making NGC 7456 an active galaxy. Whether looking at its core or its outskirts, at visible light or X-rays, this galaxy has something interesting for astronomers to study! Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli (claire.andreoli@nasa.gov) NASA’s Goddard Space Flight Center, Greenbelt, MD Share Details Last Updated Sep 04, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Hubble Space Telescope Spiral Galaxies The Universe Keep Exploring Discover More Topics From Hubble Hubble Space Telescope Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe. Science Behind the Discoveries Hubble Design Hubble’s Night Sky Challenge View the full article

Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 4 min read Curiosity Blog, Sols 4641-4648: Thinking Outside and Inside the ‘Boxwork’ NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on Aug. 28, 2025 — Sol 4643, or Martian day 4,643 of the Mars Science Laboratory mission — at 20:45:52 UTC. NASA/JPL-Caltech Written by Ashley Stroupe, Mission Operations Engineer and Rover Planner at NASA’s Jet Propulsion Laboratory Earth planning week: Aug. 25, 2025. This week Curiosity has been exploring the boxwork unit, investigating both the ridges and the hollows to better characterize them and understand how they may have formed. We’ve been doing lots of remote science, contact science, and driving in each plan. In addition, we have our standard daily environmental observations to look at dust in the atmosphere. We can still see distant targets like the crater rim, but temperatures will soon begin to warm up as we start moving into a dustier part of the year. And after each drive, we also use AEGIS to do some autonomous target selection for ChemCam observations. I was the arm rover planner for the 4645-4648 plan on Friday. For Monday’s plan (sols 4641-4642), after a successful weekend drive Curiosity began on the edge of a boxwork ridge. We did a lot of imaging, including Mastcam mosaics of “El Alto,” an upturned rock near a wheel, the ridge forming the south side of the Mojo hollow, “Sauces,” our contact science target, and “Navidad,” an extension of our current workspace. We also took ChemCam LIBS of Sauces and an RMI mosaic. The rover planners did not find any bedrock large enough to brush, but did MAHLI and APXS on Sauces. Ready to drive, Curiosity drove about 15 meters (about 49 feet) around the ridge to the south and into the next hollow, named “Mojo.” In Wednesday’s plan (sols 4643-4644), Curiosity was successfully parked in the Mojo hollow. We started with a lot of imaging, including Mastcam mosaics of the ridges around the Mojo hollow, a nearby trough and the hollow floor to look for regolith movement. We also imaged a fractured float rock named “La Laguna Verde.” ChemCam planned a LIBS target on “Corani,” a thin resistant clast sticking out of the regolith, a RMI mosaic of a target on the north ridge named “Cocotoni,” and a long-distance RMI mosaic of “Babati Mons,” a mound about 100 kilometers (about 62 miles) away that we can see peeking over the rim of Gale crater! With no bedrock in the workspace, the rover planners did MAHLI and APXS observations on a regolith target named “Tarapacá.” The 12-meter drive in this plan (about 39 feet) was challenging; driving out of the hollow and up onto the ridge required the rover to overcome tilts above 20 degrees, where the rover can experience a lot of slip. Also, with the drive late in the day, it was challenging to determine where Curiosity should be looking to track her slip using Visual Odometry without getting blinded by the sun or losing features in shadows. Making sure VO works well is particularly important on drives like this when we expect a lot of slip. Friday’s plan, like most weekend plans, was more complex — particularly because this four-sol plan also covers the Labor Day holiday on Monday. Fortunately, the Wednesday drive was successful, and we reached the desired parking location on the ridge south of Mojo for imaging and contact science. The included image looks back over the rover’s shoulder, where we can see the ridge and hollow. We took a lot of imaging looking at hollows and the associated ridges. We are taking a Mastcam mosaic of “Jorginho Cove,” a target covering the ridge we are parked on and the next hollow to the south, “Pica,” a float rock that is grayish in color, and a ridge/hollow pair named “Laguna Colorada.” We also take ChemCam LIBS observations of Pica and two light-toned pieces of bedrock named “Tin Tin” and ”Olca.” ChemCam takes RMI observations of “Briones,” which is a channel on the crater rim, “La Serena,” some linear features in the crater wall, and a channel that feeds into the Peace Vallis fan. After a week of fairly simple arm targets, the rover planners had a real challenge with this workspace. The rocks were mostly too small and too rough to brush, but we did find one spot after a lot of looking. We did DRT, APXS, and MAHLI on this spot, named “San Jose,” and also did MAHLI and APXS on another rock named “Malla Qullu.” This last drive of the week is about 15 meters (about 49 feet) following along a ridge and then driving onto a nearby one. Want to read more posts from the Curiosity team? Visit Mission Updates Want to learn more about Curiosity’s science instruments? Visit the Science Instruments page NASA’s Mars rover Curiosity at the base of Mount Sharp NASA/JPL-Caltech/MSSS Share Details Last Updated Sep 04, 2025 Related Terms Blogs Explore More 2 min read Over Soroya Ridge & Onward! Article 1 week ago 3 min read Curiosity Blog, Sols 4638-4640: Imaging Extravaganza Atop a Ridge Article 1 week ago 3 min read To See the World in a Grain of Sand: Investigating Megaripples at ‘Kerrlaguna’ 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… View the full article

This competition provides a hands-on opportunity for participants to gain critical skills in engineering, computing, electronics, and more that will be required for America’s technical workforce. If you are in sixth to 12th-grade at a U.S. public, private, or charter school – including those in U.S. territories – your challenge is to team up with your schoolmates and develop a science or technology experiment idea for one of the following NASA TechRise flight vehicles: Suborbital-Spaceship with approximately 3 minutes of microgravity. High-Altitude Balloon with approximately 4 to 8 hours of flight time at 70,000 to 95,000 feet and exposure to Earth’s atmosphere, high-altitude radiation, and perspective views of our planet. Award: $1,500 each to 60 winning teams Open Date: September 4, 2025 Close Date: November 3, 2025 For more information, visit: https://www.futureengineers.org/nasatechrise View the full article

6 Min Read Upcoming Launch to Boost NASA’s Study of Sun’s Influence Across Space Soon, there will be three new ways to study the Sun’s influence across the solar system with the launch of a trio of NASA and National Oceanic and Atmospheric Administration (NOAA) spacecraft. Expected to launch no earlier than Tuesday, Sept. 23, the missions include NASA’s IMAP (Interstellar Mapping and Acceleration Probe), NASA’s Carruthers Geocorona Observatory, and NOAA’s SWFO-L1 (Space Weather Follow On-Lagrange 1) spacecraft. The three missions will launch together aboard a SpaceX Falcon 9 rocket from NASA’s Kennedy Space Center in Florida. From there, the spacecraft will travel together to their destination at the first Earth-Sun Lagrange point (L1), around one million miles from Earth toward the Sun. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system. Research and observations from the missions will help us better understand the Sun’s influence on Earth’s habitability, map our home in space, and protect satellites and voyaging astronauts and airline crews from space weather impacts. The IMAP and Carruthers missions add to NASA’s heliophysics fleet of spacecraft. Together, NASA’s heliophysics missions study a vast, interconnected system from the Sun to the space surrounding Earth and other planets to the farthest limits of the Sun’s constantly flowing streams of solar wind. The SWFO-L1 mission, funded and operated by NOAA, will be the agency’s first satellite designed specifically for and fully dedicated to continuous, operational space weather observations. Mapping our home in space: IMAP The IMAP mission will study the heliosphere, our home in space. NASA/Princeton University/Patrick McPike As a modern-day celestial cartographer, IMAP will investigate two of the most important overarching issues in heliophysics: the interaction of the solar wind at its boundary with interstellar space and the energization of charged particles from the Sun. The IMAP mission will principally study the boundary of our heliosphere — a huge bubble created by the solar wind that encapsulates our solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond. The heliosphere protects the solar system from dangerous high-energy particles called galactic cosmic rays. Mapping the heliosphere’s boundaries helps scientists understand our home in space and how it came to be habitable. “IMAP will revolutionize our understanding of the outer heliosphere,” said David McComas, IMAP mission principal investigator at Princeton University in New Jersey. “It will give us a very fine picture of what’s going on out there by making measurements that are 30 times more sensitive and at higher resolution than ever before.” The IMAP mission will also explore and chart the vast range of particles in interplanetary space. The spacecraft will provide near real-time observations of the solar wind and energetic particles, which can produce hazardous conditions not only in the space environment near Earth, but also on the ground. The mission’s data will help model and improve prediction capabilities of the impacts of space weather ranging from power-line disruptions to loss of satellites. Imaging Earth’s exosphere: Carruthers Geocorona Observatory An illustration shows the Carruthers Geocorona Observatory spacecraft. NASA/BAE Systems Space & Mission Systems The Carruthers Geocorona Observatory, a small satellite, will launch with IMAP as a rideshare. The mission was named after Dr. George Carruthers, creator of the Moon-based telescope that captured the first images of Earth’s exosphere, the outermost layer of our planet’s atmosphere. The Carruthers mission will build upon Dr. Carruthers’ legacy by charting changes in Earth’s exosphere. The mission’s vantage point at L1 offers a complete view of the exosphere not visible from the Moon’s relatively close distance to Earth. From there, it will address fundamental questions about the nature of the region, such as its shape, size, density, and how it changes over time. The exosphere plays an important role in Earth’s response to space weather, which can impact our technology, from satellites in orbit to communications signals in the upper atmosphere or power lines on the ground. During space weather storms, the exosphere mediates the energy absorption and release throughout the near-Earth space environment, influencing strength of space weather disturbances. Carruthers will help us better understand the fundamental physics of our exosphere and improve our ability to predict the impacts of the Sun’s activity. “We’ll be able to create movies of how this atmospheric layer responds when a solar storm hits, and watch it change with the seasons over time,” said Lara Waldrop, the principal investigator for the Carruthers Geocorona Observatory at the University of Illinois at Urbana-Champaign. New space weather station: SWFO-L1 SWFO-L1 will provide real-time observations of the Sun’s corona and solar wind to help forecast the resulting space weather. NOAA/BAE Systems Space & Mission Systems Distinct from NASA’s research satellites, SWFO-L1 will be an operational satellite, designed to observe solar activity and the solar wind in real time to provide critical data in NOAA’s mission to protect the nation from environmental hazards. SWFO-L1 will serve as an early-warning beacon for potentially damaging space weather events that could impact our technology on Earth. SWFO-L1 will observe the Sun’s outer atmosphere for large eruptions, called coronal mass ejections, and measure the solar wind upstream from Earth with a state-of-the-art suite of instruments and processing system. This mission is the first of a new generation of NOAA space weather observatories dedicated to 24/7 operations, working to avoid gaps in continuity. “SWFO-L1 will be an amazing deep-space mission for NOAA,” said Dimitrios Vassiliadis, SWFO program scientist at NOAA. “Thanks to its advantageous location at L1, it will continuously monitor the solar atmosphere while measuring the solar wind and its interplanetary magnetic fields well before it impacts Earth — and transmit these data in record time.” With SWFO-L1’s enhanced performance, unobstructed views, and minimal delay between observations and data return, NOAA’s Space Weather Prediction Center forecasters will give operators improved lead time required to take precautionary actions that protect vital infrastructure, economic interests, and national security on Earth and in space. By Mara Johnson-Groh NASA’s Goddard Space Flight Center, Greenbelt, Md. Share Details Last Updated Sep 04, 2025 Related Terms Carruthers Geocorona Observatory (GLIDE) Heliophysics Heliosphere IMAP (Interstellar Mapping and Acceleration Probe) NOAA (National Oceanic and Atmospheric Administration) Solar Wind Space Weather The Sun The Sun & Solar Physics Explore More 3 min read Juno Detected the Final Missing Auroral Signature from Jupiter’s Four Largest Moons Article 2 days ago 6 min read NASA, IBM’s ‘Hot’ New AI Model Unlocks Secrets of Sun Article 2 weeks ago 3 min read Sun at the Center: Teacher Ambassadors Bring Heliophysics to Classrooms Nationwide Article 2 weeks ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

Science Launching on Northrop Grumman's 23rd Cargo Resupply Mission to the Space Station

NASA and Northrop Grumman are preparing to send the company’s next cargo mission to the International Space Station, flying research to support Artemis missions to the Moon and human exploration of Mars and beyond, while improving life on Earth. SpaceX’s Falcon 9 rocket will launch Northrop Grumman’s 23rd commercial resupply services mission to the orbiting laboratory. The investigations aboard the Cygnus spacecraft aim to refine semiconductor crystals for next-generation technologies, reduce harmful microbes, improve medication production, and manage fuel pressure. NASA, Northrop Grumman, and SpaceX are targeting launch in mid-September from Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida. Read about some of the investigations traveling to the space station: Better semiconductor crystals Optical micrograph of a semiconductor composite wafer with embedded semimetal phases extracted from a space grown crystal in the SUBSA facility during Mission 1United Semiconductors LLC Researchers are continuing to fine-tune in-space production of semiconductor crystals, which are critical for modern devices like cellphones and computers. The space station’s microgravity environment could enable large-scale manufacturing of complex materials, and leveraging the orbiting platform for crystal production is expected to lead to next-generation semiconductor technologies with higher performance, chip yield, and reliability. “Semiconductor devices fabricated using crystals from a previous mission demonstrated performance gain by a factor of two and device yield enhanced by a factor of 10 compared to Earth-based counterparts,” said Partha S. Dutta, principal investigator, United Semiconductors LLC in Los Alamitos, California. Dutta highlighted that three independent parties validated microgravity’s benefits for growing semiconductor crystals and that the commercial value of microgravity-enhanced crystals could be worth more than $1 million per kilogram (2.2 pounds). Space-manufactured crystals could help meet the need for radiation-hardened, low-power, high-speed electronics and sensors for space systems. They also could provide reduced power use, increased speed, and improved safety. The technology also has ground applications, including electric vehicles, waste heat recovery, and medical tools. Learn more about the SUBSA-InSPA-SSCug experiment. Lethal light Germicidal Ultraviolet (UV) light is emitted by an optical fiber running through the center of an agar plateArizona State University Researchers are examining how microgravity affects ultraviolet (UV) light’s ability to prevent the formation of biofilms — communities of microbes that form in water systems. Investigators developed special optical fibers to deliver the UV light, which could provide targeted, long-lasting, and chemical-free disinfection in space and on Earth. “In any water-based system, bacterial biofilms can form on surfaces like pipes, valves, and sensors,” said co-investigator Paul Westerhoff, a professor at Arizona State University in Tempe. “This can cause serious problems like corrosion and equipment failure, and affect human health.” The UV light breaks up DNA in microorganisms, preventing them from reproducing and forming biofilms. Preliminary evidence suggests biofilms behave differently in microgravity, which may affect how the UV light reaches and damages bacterial DNA. “What we’ll learn about biofilms and UV light in microgravity could help us design safer water and air systems not just for space exploration, but for hospitals, homes, and industries back on Earth,” Westerhoff said. Learn more about the GULBI experiment. Sowing seeds for pharmaceuticals NASA astronaut Loral O’Hara displays the specialized sample processor used for pharmaceutical research aboard the International Space StationNASA An investigation using a specialized pharmaceutical laboratory aboard the space station examines how microgravity may alter and enhance crystal structures of drug molecules. Crystal structure can affect the production, storage, effectiveness, and administration of medications. “We are exploring drugs with applications in cardiovascular, immunologic, and neurodegenerative disease as well as cancer,” said principal investigator Ken Savin of Redwire Space Technologies in Greenville, Indiana. “We expect microgravity to yield larger, more uniform crystals.” Once the samples return to Earth, researchers at Purdue University in West Lafayette, Indiana, will examine the crystal structures. The investigators hope to use the space-made crystals as seeds to produce significant numbers of crystals on Earth. “We have demonstrated this technique with a few examples, but need to see if it works in many examples,” Savin said. “It’s like being on a treasure hunt with every experiment.” This research also helps enhance and expand commercial use of the space station for next-generation biotechnology research and in-space production of medications. Learn more about the ADSEP PIL-11 experiment. Keeping fuel cool iss0NASA astronaut Joe Acaba installs hardware for the first effort in 2017 aboard the International Space Station to test controlling pressure in cryogenic fuel tanksNASA Many spacecraft use cryogenic or extremely cold fluids as fuel for propulsion systems. These fluids are kept at hundreds of degrees below zero to remain in a liquid state, making them difficult to use in space where ambient temperatures can vary significantly. If these fluids get too warm, they turn into gas and boiloff, or slowly evaporate and escape the tank, affecting fuel efficiency and mission planning. A current practice to prevent this uses onboard fuel to cool systems before transferring fuel, but this practice is wasteful and not feasible for Artemis missions to the Moon and future exploration of Mars and beyond. A potential alternative is using special gases that do not turn into liquids at cold temperatures to act as a barrier in the tank and control the movement of the fuel. Researchers are testing this method to control fuel tank pressure in microgravity. It could save an estimated 42% of propellant mass per year, according to Mohammad Kassemi, a researcher at NASA’s National Center for Space Exploration Research and Case Western Reserve University in Cleveland. The test could provide insights that help improve the design of lightweight, efficient, long-term in-space cryogenic storage systems for future deep space exploration missions. Learn more about the ZBOT-NC experiment. Download high-resolution photos and videos of the research highlighted in this feature. Learn more about the research aboard the International Space Station at: www.nasa.gov/iss-science Keep Exploring Discover More Topics From NASA Latest News from Space Station Research Space Station Research and Technology Resources Space Station Research Results Humans In Space View the full article

NASA NASA astronauts Jonny Kim and Zena Cardman, both Expedition 73 Flight Engineers, pose for a portrait inside the International Space Station‘s Unity module during a break in weekend housecleaning and maintenance activities. Kim and Cardman are both part of NASA Astronaut Group 22 selected in June 2017 with 12 other astronauts, including two Canadian Space Agency astronauts, and affectionately nicknamed “The Turtles.” In its third decade of continuous human presence, the space station has a far-reaching impact as a microgravity lab hosting technology, demonstrations, and scientific investigations from a range of fields. The research done by astronauts on the orbiting laboratory will inform long-duration missions like Artemis and future human expeditions to Mars. Learn more about station activities by following the space station blog. View the full article

Explore Webb Webb News Latest News Latest Images Webb’s Blog Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Webb Timeline Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Science Explainers Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Webb’s First Images Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 5 Min Read Glittering Glimpse of Star Birth From NASA’s Webb Telescope Webb captured this sparkling scene of star birth in Pismis 24. Full image and caption below. Credits: Image: NASA, ESA, CSA, STScI; Image Processing: A. Pagan (STScI) This is a sparkling scene of star birth captured by NASA’s James Webb Space Telescope. What appears to be a craggy, starlit mountaintop kissed by wispy clouds is actually a cosmic dust-scape being eaten away by the blistering winds and radiation of nearby, massive, infant stars. Called Pismis 24, this young star cluster resides in the core of the nearby Lobster Nebula, approximately 5,500 light-years from Earth in the constellation Scorpius. Home to a vibrant stellar nursery and one of the closest sites of massive star birth, Pismis 24 provides rare insight into large and massive stars. Its proximity makes this region one of the best places to explore the properties of hot young stars and how they evolve. At the heart of this glittering cluster is the brilliant Pismis 24-1. It is at the center of a clump of stars above the jagged orange peaks, and the tallest spire is pointing directly toward it. Pismis 24-1 appears as a gigantic single star, and it was once thought to be the most massive known star. Scientists have since learned that it is composed of at least two stars, though they cannot be resolved in this image. At 74 and 66 solar masses, respectively, the two known stars are still among the most massive and luminous stars ever seen. Image A: Pismis 24 (NIRCam Image) Webb captured this sparkling scene of star birth in Pismis 24, a young star cluster about 5,500 light-years from Earth in the constellation Scorpius. This region is one of the best places to explore the properties of hot young stars and how they evolve. Image: NASA, ESA, CSA, STScI; Image Processing: A. Pagan (STScI) Captured in infrared light by Webb’s NIRCam (Near-Infrared Camera), this image reveals thousands of jewel-like stars of varying sizes and colors. The largest and most brilliant ones with the six-point diffraction spikes are the most massive stars in the cluster. Hundreds to thousands of smaller members of the cluster appear as white, yellow, and red, depending on their stellar type and the amount of dust enshrouding them. Webb also shows us tens of thousands of stars behind the cluster that are part of the Milky Way galaxy. Super-hot, infant stars –some almost 8 times the temperature of the Sun – blast out scorching radiation and punishing winds that are sculpting a cavity into the wall of the star-forming nebula. That nebula extends far beyond NIRCam’s field of view. Only small portions of it are visible at the bottom and top right of the image. Streamers of hot, ionized gas flow off the ridges of the nebula, and wispy veils of gas and dust, illuminated by starlight, float around its towering peaks. Dramatic spires jut from the glowing wall of gas, resisting the relentless radiation and winds. They are like fingers pointing toward the hot, young stars that have sculpted them. The fierce forces shaping and compressing these spires cause new stars to form within them. The tallest spire spans about 5.4 light-years from its tip to the bottom of the image. More than 200 of our solar systems out to Neptune’s orbit could fit into the width its tip, which is 0.14 lightyears. In this image, the color cyan indicates hot or ionized hydrogen gas being heated up by the massive young stars. Dust molecules similar to smoke here on Earth are represented in orange. Red signifies cooler, denser molecular hydrogen. The darker the red, the denser the gas. Black denotes the densest gas, which is not emitting light. The wispy white features are dust and gas that are scattering starlight. Video A: Expedition to Star Cluster Pismis 24 To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video This scientific visualization takes viewers on a journey to a glittering young star cluster called Pismis 24. NASA’s James Webb Space Telescope captured this fantastical scene in the heart of the Lobster Nebula, approximately 5,500 light-years from Earth. Video: NASA, ESA, CSA, STScI, Leah Hustak (STScI), Christian Nieves (STScI); Image Processing: Alyssa Pagan (STScI); Script Writer: Frank Summers (STScI); Narration: Frank Summers (STScI); Music: Christian Nieves (STScI); Audio: Danielle Kirshenblat (STScI); Producer: Greg Bacon (STScI); Acknowledgment: VISTA Video B: Zoom to Pismis 24 This zoom-in video shows the location of the young star cluster Pismis 24 on the sky. It begins with a ground-based photo of the constellation Scorpius by the late astrophotographer Akira Fujii. The sequence closes in on the Lobster Nebula, using views from the Digitized Sky Survey. As the video homes in on a select portion, it fades to a VISTA image in infrared light. The zoom continues in to the region around Pismis 24, where it transitions to the stunning image captured by NASA’s James Webb Space Telescope in near-infrared light. Video: NASA, ESA, CSA, STScI, Alyssa Pagan (STScI); Narration: Frank Summers (STScI); Script Writer: Frank Summers (STScI); Music: Christian Nieves (STScI); Audio: Danielle Kirshenblat (STScI); Producer: Greg Bacon (STScI); Acknowledgment: VISTA, Akira Fujii, DSS The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency). To learn more about Webb, visit: https://science.nasa.gov/webb Downloads Click any image to open a larger version. View/Download all image products at all resolutions for this article from the Space Telescope Science Institute. Media Contacts Laura Betz – laura.e.betz@nasa.gov NASA’s Goddard Space Flight Center, Greenbelt, Md. Ann Jenkins – jenkins@stsci.edu Space Telescope Science Institute, Baltimore, Md. Related Information Read more about Hubble’s view of Pismis 24 Listen to a sonification of Hubble’s view of Pismis 24 Animation Video: “How Dense Pillars Form in Molecular Clouds” Read more: Webb’s Star Formation Discoveries More Webb News More Webb Images Webb Science Themes Webb Mission Page Related For Kids What is the Webb Telescope? SpacePlace for Kids En Español Ciencia de la NASA NASA en español Space Place para niños Keep Exploring Related Topics James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Stars Stars Stories Universe Share Details Last Updated Sep 04, 2025 Related Terms James Webb Space Telescope (JWST) View the full article

Patricia White is a contracting officer at NASA’s Stennis Space Center, where she contributes to NASA’s Artemis program that will send astronauts to the Moon to prepare for future human exploration of Mars. NASA/Danny Nowlin When NASA’s Artemis II mission launches in 2026, it will inspire the world through discovery in a new Golden Age of innovation and exploration. It will be another inspiring NASA moment Patricia White can add to her growing list. White supports the Artemis program to send astronauts to the Moon to prepare for future human exploration of Mars as a contracting officer at NASA’s Stennis Space Center near Bay St. Louis, Mississippi. White takes special pride in the test operations contract she helped draft. The contract provides support to the Fred Haise Test Stand, which tests the RS-25 engines that will help power NASA’s SLS (Space Launch System) rocket on Artemis missions. “I was awestruck the first time I witnessed an engine test,” White said. “I remember how small I felt in comparison to this big and fascinating world, and I wondered what that engine would see that I would never be able to see.” Four RS-25 engines tested at NASA Stennis will help launch Artemis II with four astronauts to venture around the Moon. As the first crewed Artemis mission, it will represent another milestone for the nation’s human space exploration effort. From Interstate Signs to NASA Career White describes NASA Stennis as a hidden gem. Growing up in nearby Slidell, Louisiana, she had driven by the interstate signs pointing toward NASA Stennis her entire life. When she heard about a job opportunity at the center, she immediately applied. Initially hired as a contractor with only a high school diploma in February 2008, White found her motivation among NASA’s ranks. “I work with very inspiring people, and it only took one person to say, ‘You should go to college’ to give me the courage to go so late in life,” she said. Hard But Worth It White began college classes in her 40s and finished at 50. She balanced a marriage, full-time job, academic studies, and household responsibilities. When she started her educational journey, her children were either toddlers or newborns. They were growing up as she stayed in school for nine years while meeting life’s challenges. “It was hard, but it was so worth it,” she said. “I love my job and what I do, and even though it is crazy busy, I look forward to working at NASA every single day.” She joined NASA officially in 2013, going from contractor to civil servant. Setting an Example White’s proudest work moment came when she brought home the NASA Early Career Achievement award and medal. It served as a tangible symbol of her success she could share with her family. “It was a long road from being hired as an intern, and we all made extraordinary sacrifices,” she said. “I wanted to share it with them and set a good example for my children.” As Artemis II prepares to carry humans back to lunar orbit for the first time in over 50 years, White takes pride knowing her work helps power humanity’s return to deep space exploration. Her work is proof that sometimes the most important journeys begin right in one’s own backyard. Learn More About Careers at NASA Stennis Explore More 4 min read NASA Stennis Provides Ideal Setting for Range Operations Article 1 week ago 10 min read NASA’s Stennis Space Center Employees Receive NASA Honor Awards Article 3 weeks ago 6 min read A Defining Era: NASA Stennis and Space Shuttle Main Engine Testing Article 4 months ago View the full article

Live Video from the International Space Station (Official NASA Stream)

Live High-Definition Views from the International Space Station (Official NASA Stream)

4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Researchers Kelly Gilkey, Cy Peverill, Daniel Phan, Chase Haddix, and Ariel Tokarz test portable, handheld X-ray systems for use during future long-duration space missions at NASA’s Glenn Research Center in Cleveland on Friday, March 21, 2025. Credit: NASA/Sara Lowthian-Hanna As NASA plans future human exploration missions to the Moon, Mars, and beyond, new and unique challenges emerge — like communication delays and limited return-to-Earth options — so enhanced medical care capabilities are critical. Crews will need non-invasive imaging technology to diagnose medical conditions, like broken bones or dental injuries. Scientists at NASA’s Glenn Research Center in Cleveland are testing portable, handheld X-ray systems for use during future extended space missions. Having portable X-ray capabilities aboard spacecraft would allow astronauts to immediately assess and treat potential injuries or identify equipment issues without having to disassemble the gear. “Technological innovations like that of the mini-X-ray will help keep our astronauts healthy as we endeavor farther into space than ever before,” said acting NASA Administrator Sean Duffy. “Future missions to the Moon and Mars will be safer due to the research of our scientists at NASA Glenn.” NASA reviewed more than 200 commercial systems — analyzing size, weight, image quality, ease-of-use, cost, and safety — and selected three systems for further testing: MinXray, Remedi, and Fujifilm. “We’re working to provide evidence on why a mini-X-ray system should be included in future space exploration,” said Dr. Chase Haddix, a senior biomedical engineering research contractor working for Universities Space Research Association at NASA Glenn. “These X-rays could be used to detect both clinical and non-clinical diagnostics, meaning they can check an astronaut’s body or identify the location of a tear in an astronaut suit.” Researchers capture X-ray images of a shape memory alloy rover tire at NASA’s Glenn Research Center in Cleveland on Friday, March 21, 2025. Credit: NASA/Sara Lowthian-Hanna NASA Glenn is collaborating with other centers, including NASA’s Johnson Space Center in Houston and NASA’s Langley Research Center in Hampton, Virginia, and radiography experts at University Hospitals and Cuyahoga Community College in Cleveland. “We’re fortunate to have enthusiastic medical and radiography experts right here in our community,” said Dr. Cy Peverill, project task lead at NASA Glenn. “Their knowledge and experience are invaluable as we work to test medical technologies that could significantly improve management of astronaut health on future missions to the Moon or Mars.” Cuyahoga Community College contributed anatomical phantoms, which are lifelike models of the human body, in its radiography laboratory on the Western Campus and dental hygiene clinical facility at the Metropolitan Campus. Faculty and students consulted with NASA researchers on essential imaging principles, including patient positioning, image acquisition, and image quality. University Hospitals is partnering with NASA Glenn on a medical study with real patients to compare the performance of the X-ray systems against hospital-grade equipment, focusing on usability, image clarity, and diagnostic accuracy. “Astronauts live and work in small quarters, much smaller spaces than in a hospital,” Haddix said. “The system must be easy to use since astronauts may not be experienced in radiography. The data from these tests will guide the selection of the most suitable system for future missions.” Researchers capture X-ray images of an astronaut spacesuit at NASA’s Glenn Research Center in Cleveland on Friday, March 21, 2025. Credit: NASA/Sara Lowthian-Hanna Using portable X-rays to improve health care in inaccessible areas is not new, with systems deployed to diagnose medical issues in places such as base camps in Nepal and remote villages in South Africa. NASA researchers theorize that if these systems are successful in high elevations and extreme temperatures on Earth, perhaps they are durable enough for space missions. Glenn researchers will continue to collect data from all collaborators, including from an X-ray system sourced by SpaceX that launched in April during the Fram2 mission. The crew captured the first human X-ray images in space during their four-day mission to low Earth orbit. NASA plans to select a device near the end of 2025 and will test the chosen system aboard the International Space Station in 2026 or early 2027. The Mars Campaign Office at NASA Headquarters in Washington and the agency’s Human Research Program at NASA Johnson fund this work as both organizations focus on pursuing technologies and methods to support safe, productive human space travel. Explore More 2 min read Lydia Rodriguez Builds a Career of Service and Support at NASA Article 2 days ago 3 min read What’s Up: September 2025 Skywatching Tips from NASA Saturn’s spectacle, a Conjunction, and the Autumnal Equinox Saturn shines throughout the month, a conjunction… Article 2 days ago 2 min read Hubble Homes in on Galaxy’s Star Formation This NASA/ESA Hubble Space Telescope image features a galaxy whose asymmetric appearance may be the… Article 6 days ago View the full article

NASA/Rachel Tilling Sea ice is frozen seawater that floats in the ocean. This photo, taken from NASA’s Gulfstream V Research Aircraft on July 21, 2022, shows Arctic sea ice in the Lincoln Sea north of Greenland. This image is the NASA Science Image of the Month for September 2025. Each month, NASA’s Science Mission Directorate chooses an image to feature, offering desktop wallpaper downloads, as well as links to related topics, activities, and games. Text and image credit: NASA/Rachel Tilling View the full article

The next era of lunar exploration demands a new kind of wheel – one that can sprint across razor-sharp regolith, shrug off extremely cold nights, and keep a rover rolling day after lunar day. The Rock and Roll with NASA Challenge seeks that breakthrough. If you can imagine a lightweight, compliant wheel that stays tough at higher speeds while carrying lots of cargo, your ideas could set the pace for surface missions to follow. For this phased Challenge, Phase 1 rewards the best concepts and analyses, Phase 2 funds prototypes, and Phase 3 puts the best wheels through a live obstacle course simulating the lunar terrain. Along the way, you’ll receive feedback from NASA mobility engineers and the chance to see your hardware pushed to its limits. In Phase 3, to prove concepts, NASA is using MicroChariot, a nimble, 45 kg test rover that will test the best designs from Phase 1 & Phase 2 at the Johnson Space Center Rockyard in Houston, Texas. Whether you’re a student team, a garage inventor, or a seasoned aerospace firm, this is your opportunity to rewrite the playbook of planetary mobility and leave tread marks on the future of exploration. Follow the challenge, assemble your crew, and roll out a solution that takes humanity back to the Moon. Award: $155,000 in total prizes Open Date: Phase 1 – August 28, 2025; Phase 2 – January 2026; Phase 3 – May 2026 Close Date: Phase 1 – November 4, 2025; Phase 2 – April 2026; Phase 3 – June 2026 For more information, visit: https://www.herox.com/NASARockandRoll View the full article

Amit KshatriyaCredit: NASA Acting NASA Administrator Sean P. Duffy Wednesday named Amit Kshatriya as the new associate administrator of NASA, the agency’s top civil service role. A 20-year NASA veteran, Kshatriya was most recently the deputy in charge of the Moon to Mars Program in the Exploration Systems Development Mission Directorate (ESDMD) at NASA Headquarters in Washington. In this role, Kshatriya was responsible for program planning and implementation for crewed missions to the Moon through the Artemis campaign in preparation for humanity’s first mission to Mars. Promoting Kshatriya to NASA’s top ranks puts America’s return to the Moon through Artemis at the very core of our agency. The move exemplifies President Donald J. Trump and Duffy’s seriousness about returning Americans to the Moon and before China. “Amit has spent more than two decades as a dedicated public servant at NASA, working to advance American leadership in space. Under his leadership, the agency will chart a bold vision to return to the Moon during President Trump’s term,” said Duffy. “Amit’s knowledge, integrity, and unwavering commitment to pioneering a new era of exploration make him uniquely qualified to lead our agency as associate administrator. With Amit we’ll continue to push the boundaries of what’s possible.” Kshatriya’s promotion also signals how the Trump Administration sees the commercial space sector as an American economic engine. By putting a proven leader at the top, NASA is set to partner even more closely with America’s booming space industry, grow the space economy, and ensure the future of exploration is built in the United States. Born in Wisconsin, educated at California Institute of Technology and the University of Texas at Austin, Kshatriya is one of only about 100 people in history to serve as a mission control flight director. He brings unparalleled operational and strategic experience to NASA’s executive leadership team. -end- Bethany Stevens Headquarters, Washington 771-216-2606 bethany.c.stevens@nasa.gov View the full article

Explore This Section Overview Science Science Findings Juno’s Orbits Spacecraft People Stories Multimedia JunoCam Images Jupiter hosts the brightest and most spectacular auroras in the Solar System. Near its poles, these shimmering lights offer a glimpse into how the planet interacts with the solar wind and moons swept by Jupiter’s magnetic field. Unlike Earth’s northern lights, the largest moons of Jupiter create their own auroral signatures in the planet’s atmosphere — a phenomenon that Earth’s Moon does not produce. These moon-induced auroras, known as “satellite footprints,” reveal how each moon interacts with its local space environment. Juno capturing the marks on Jupiter of all four Galilean moons. The auroras related to each are labeled Io, Eur (for Europa), Gan (for Ganymede), and Cal (for Callisto). NASA/JPL-Caltech/SwRI/UVS team/MSSS/Gill/Jónsson/Perry/Hue/Rabia Before NASA’s Juno mission, three of Jupiter’s four largest moons, known as Galilean moons — Io, Europa, and Ganymede — were shown to produce these distinct auroral signatures. But Callisto, the most distant of the Galilean moons, remained a mystery. Despite multiple attempts using NASA’s Hubble Space Telescope, Callisto’s footprint had proven elusive, both because it is faint and because it most often lies atop the brighter main auroral oval, the region where auroras are displayed. NASA’s Juno mission, orbiting Jupiter since 2016, offers unprecedented close-up views of these polar light shows. But to image Callisto’s footprint, the main auroral oval needs to move aside while the polar region is being imaged. And to bring to bear Juno’s arsenal of instruments studying fields and particles, the spacecraft’s trajectory must carry it across the magnetic field line linking Callisto and Jupiter. These two events serendipitously occurred during Juno’s 22nd orbit of the giant planet, in September 2019, revealing Callisto’s auroral footprint and providing a sample of the particle population, electromagnetic waves, and magnetic fields associated with the interaction. Jupiter’s magnetic field extends far beyond its major moons, carving out a vast region (magnetosphere) enveloped by, and buffeted by, the solar wind streaming from our Sun. Just as solar storms on Earth push the northern lights to more southern latitudes, Jupiter’s auroras are also affected by our Sun’s activity. In September 2019, a massive, high-density solar stream buffeted Jupiter’s magnetosphere, briefly revealing — as the auroral oval moved toward Jupiter’s equator — a faint but distinct signature associated with Callisto. This discovery finally confirms that all four Galilean moons leave their mark on Jupiter’s atmosphere, and that Callisto’s footprints are sustained much like those of its siblings, completing the family portrait of the Galilean moon auroral signatures. An international team of scientists led by Jonas Rabia of the Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, in Toulouse, France, published their paper on the discovery, “In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft,” in the journal Nature Communications on Sept. 1, 2025. Share Details Last Updated Sep 02, 2025 Related Terms Auroras Callisto Juno Jupiter Jupiter Moons Keep Exploring Discover More Topics From NASA Jupiter: Exploration Jupiter Jupiter Moons Callisto View the full article

Image of Caleb Scharf _________________________________________________________________________________________ In the following interview, questions from the interviewer, Fred Van Wert, are in bold, and Caleb Scharf’s responses are in regular text. _________________________________________________________________________________________ Let’s begin with your early years. Where you were born, something about your family, what your mother and father did, your early schooling, what got you interested in the career that you’ve been pursuing, that kind of thing. Well, I was born in London, England, about a ten minute walk from the British Museum, right in the center of Old London. My parents were very interesting. My dad was American and my mother was British. They were both academics and both were art historians, in fact my dad was somewhat famous for his work in art history. My mother also did a lot of study in London. But when I was about three or four years old we moved out to a small village in England, in a county called Norfolk. It was just farms and us, so I actually grew up in a very rural part of England. Today it’s become a second home location for a lot of people but back then it was . . . well, you were excited if you saw a loaf of white bread in the village shop! So, I have a bit of an eclectic background. Like I said, my dad was American, so I have a lot of family in the U.S., mostly in Los Angeles. My father’s family had emigrated from Austria to the U.S. My grandfather was a musician and in the 1930’s he played in the Hollywood Studios, and that’s how that side of the family ended up in LA. There’s music in the family but I missed that gene! (laughs). Regarding the question of if there was something in my early childhood that got me interested in space, astronomy, and science, I feel like it may have been moving out into the countryside where suddenly you could see the sky at night. London in the late 1960’s and early ‘70’s had light pollution and other pollution everywhere. But I have memories of going out into the countryside at night, even as a little kid. I’d get excused from the dinner table and go outside to burn off some energy, and I could see these brilliant night skies, the Milky Way and all the other features, with my naked eyes. I remember spending a lot of time just gazing and thinking about that. And, although my parents wouldn’t let me watch much TV, for some reason they did let me watch Star Trek when it was a new thing. I remember being both terrified by it and hiding behind the couch, but also being fascinated. I didn’t really understand everything that was going on, but it was just so intriguing. There was this guy with pointy ears who wasn’t human. How could you not be human, right? That was a really interesting thing to me. But also seeing how this group of people, who were intelligent but weren’t sitting behind a desk all the time, could do interesting things – that stuck with me for a long time, so maybe it was a combination of pop culture and living in the countryside. Night sky with Milky Way, and a youthful scientist Star Trek’s Mr. Spock with pointy ears. It’s interesting to me how often something early on, like being able to see the beautiful night sky clearly or as with one researcher who on a Sunday drive with her family looked out the window and saw beautiful clouds. And with that interest in clouds, she decided on a career in meteorology, and then realized there were clouds on Mars, and became a planetary scientist because she wanted to study the Martian atmosphere. And it all started with being interested in something as a little kid, so there’s a commonality there. Yeah, yeah, definitely. Do you have siblings? No, I’m an only child, for which my wife always pokes fun at me. She has a sister, but I’m an only child, which, growing up in the countryside, was good and bad because you had to make an effort to go see your friends since you were more distant from each other. You didn’t have neighbors right next door. So starting in school, at some point, you had a growing interest in the stars, and that’s a science, astronomy is science. Did you find yourself in school being drawn toward, and being good in, science classes? When I was in grade school I definitely was better at things like writing and art, that kind of thing. But by the time I was sixteen or seventeen, I started to realize that science classes were really interesting, and I also began to realize I could do some of this stuff. The math was, I wouldn’t say it was easy, but it came reasonably naturally to me. In England at that time you had to pick your academic direction by the time you were sixteen, which seems crazy early looking back. So, by sixteen, I was focusing on science and by the time I was eighteen I had completed some of the more specialized science classes. I did physics. I did chemistry. I did mathematics. And then it seemed to me that the most obvious thing I wanted to do was go to college and do physics. Physics seemed like the topic to go after because it felt more fundamental. Physicists are terrible this way, right? We think that if you do physics you can do anything, which of course isn’t really true, but it was the most attractive because it was a combination of simplicity and complexity, right? With simple rules you could learn things about very complex stuff, and I think that was something that attracted me. So I went to college to do physics. I studied at the University of Durham in the north of England, which is one of the equivalents to the various Ivy League schools in the U.S. or Cambridge, Oxford, or Imperial College in England. University of Durham, England I did physics with a concentration in theoretical physics, which drove me a little crazy because it was really difficult and I saw my limits there in the very theoretical aspects of physics, realizing that this was not for me. But we had a couple of really great astronomy classes as part of the physics degree and those kind of piqued my interest. Before graduating everyone was trying to figure out what to do next and I knew I didn’t want to go work in finance or industry. In England at that time, an undergraduate degree was three years, so it was intensive, and I felt that I hadn’t had enough chance to put into action what I had learned. So I decided to go to graduate school and earn a PhD. The things that came to my mind were astronomy, cosmology, and astrophysics, so that’s what I pursued. I was really, really lucky to get into Cambridge University to do my PhD and there was a wonderful place called the Institute of Astronomy in Cambridge where Fred Hoyle, Steven Hawking, and many other luminaries of the field had worked and that was a really terrific experience. I ended up doing my PhD in cosmology, studying the large scale structure of the universe and trying to understand how we can make measurements today that inform us about the contents of the universe, things like dark matter and the history of the universe since the big bang. It was rather theoretical but it was also the beginnings of what I would call early data science. It was a lot of statistical work, a lot of analysis of catalogs of galaxies and other things like that. So that’s what I did. Cambridge University Institute of Astronomy Well, let me poke at this a little because what you’ve described is a very natural progression into your career field. The things that interested you, and were available, you were good at, and if you were going down a path that you didn’t think was right for you, you made choices, and wound up where you are, which is great. We usually ask those we interview about their path to Ames. You did your postdoc at Goddard and didn’t come to Ames until later when you were already prominent in your field. So how did you wind up coming here? Did you reach out because you wanted to come to Ames, or did Ames reach out to you because they wanted you here, Ames being the cradle of the science of astrobiology? Or was it a combination of both? I‘ve had a convoluted path! Having trained in cosmology and astrophysics, that’s what I wound up doing as a postdoc and then after, establishing a decent career. But then I switched fields almost entirely back in the early 2000’s. I made a conscious decision to switch to the kind of interesting stuff about exoplanets and astrobiology that had lingered in the background for me, but was then exploding as a field. And I established an astrobiology center at Columbia University. Then, after 22 years at Columbia, the opportunity came up to apply to the opening at Ames. It was intriguing, and I knew Ames’ reputation, I mean Ames and astrobiology, as you say, kind of go together. So it was very, very appealing, the idea of a bit of change and of coming to the place where so much of this science had begun or been scoped out in the early days, and seeing what I could do here, how I could help continue that legacy of innovation and of leading the field. Is the work that you do hindered at all by the Covid situation? Do you go into the office every day? Many people don’t anymore. I don’t run a physical lab, so while Covid was hugely impactful, it didn’t hit my work the way it did for many others. I actually work remotely, but really for family reasons. I was at Ames for seven months to get to know the place when I started in late 2022, and now I’m typically remote from New York. But I do come to Ames on a fairly regular basis. Today I’m sitting in our apartment in Manhattan. Often, I’m sitting in a falling down Victorian house up in the Catskills in New York, where it’s really quiet, and I can work to my heart’s content. I can sit in on my Teams calls and nobody knows any better! (laughs) We often ask for a comment on the value of your work to NASA and the taxpayer, but that’s probably redundant because one of the goals of astrobiology is the search for life, or evidence of life, in the Universe, and that’s the preeminent thing that people are interested in. The people underwriting our work, the taxpayers, would love an answer to that and anything that pursues the answer is going to be supported by the public at large. Has there been something important that has come from your research, some new finding or advancement in that quest, or in something else? If you’re lucky enough to stick around in science long enough, you’ll end up getting to do some things that make a genuine contribution to the field. I’ve been lucky to have worked on a number of projects in astrobiology, and also astrophysics, where we touched on new phenomena or developed new ideas that I think have been important. For instance, in astrobiology I’ve spent a number of years working with some really excellent scientists, most of whom are at NASA, developing sophisticated climate models for worlds that are not the Earth. Modeling the Earth’s climate is super difficult, but we’ve figured out how to do it well. However, modeling climate on worlds that may be configured very differently, may have a different star, may have a different day length, may be in a different orbit, may have a different configuration of land and oceans – that’s a real challenge because climate system variables are really complicated. We’ve developed ways to do this for exoplanets, for worlds where we’re just beginning to understand their configuration enough that we can plug that information into our model and derive things like how hot is this world, what kind of climate does it have, does it have seasons, what those seasons look like, what kind of cloud cover does it have, and so forth. I’ve only played a modest role in a lot of that, but I feel really happy with that work. I think it’s made a significant contribution to understanding not only the possibilities for life but also the possibilities for planets themselves. Planets are interesting objects even if there isn’t anything living there. I was also very lucky to work on a number of astrophysics projects where I think we made some significant discoveries. One I’m particularly proud of was using the Chandra X-ray Telescope, one of NASA’s Great Observatories. It lets you study very energetic phenomenon, and in one project we found evidence of a super massive black hole in the very early universe, maybe a billion or two years after the Big Bang, that was spewing material out into the surrounding cosmos and we were actually able to detect that material. It’s hot gas, the result of some complicated physics and it suggests that black holes can influence the growth and evolution of entire galaxies. I remember that work particularly because, as with all these space telescopes, you propose for the data and then you wait. Eventually, if you’re lucky, the telescope takes your data, and it gets sent to you and you’re pretty much the first person to have seen it. I remember getting this data and creating an image on my computer screen, looking at it and thinking “that’s weird”. And then printing it out, running to the printer down the hall and picking up this piece of paper, and seeing this crazy looking structure from a black hole that existed twelve and a half billion years ago, and I’m one of the first humans to hold it in my sweaty little hands and see it with my own eyes. It was a pretty thrilling moment because of the implications of that. It was at the time the most distant such object anyone had ever seen. So, there can be those “aha” moments where you’re excited and run down the hallway and tell your colleagues, “Look what I did!” Caleb during the making of a TV documentary on his work. And you don’t know what your contribution might result in until years later, maybe after you’re gone. But something that you did was important. Yeah, yeah, yeah. It’s not the first time that I’ve heard this from scientists, the appeal of being the first one to find out something or to know something, or to see something. There’s something very satisfying in that. You mentioned the Chandra X-ray telescope and I have to ask you a question: in researching your bio there was a comment of yours that I found humorous. It was that the delays in JWST occurred so we had time to develop 4K and 8K TV to properly view the images. That prompted me to look at some JWST images and I found some were labeled JWST+Hubble. Were those images somehow combined or enhanced by each other, or are they dual images? I didn’t understand in what sense they were dual. I don’t know if I’ve seen those images, but Hubble is more sensitive to visible light and blue light than JWST, which looks at the infrared, so they are looking at different parts of the electromagnetic spectrum. So, if you are looking at a beautiful nebula, you will see slightly different phenomena or slightly different things. Putting the images together gives you a much grander painting of what’s there because you’re capturing much more of the electromagnetic spectrum. The spatial resolution of both Hubble and JWST is so exquisite that you can do that and not make a mess of things. I also wondered, since the perspective from different angles would be different, how can they combine them without overlap or something? But I’m sure they can do things with computers now. I think the perspective won’t really change because of the distances involved. Oh, sure, that’s true. But when aligning those images, as any person who builds instruments will tell you, there are always subtle imperfections, and a flat surface is not always a perfectly flat surface. Even though JWST and Hubble have some of the flattest surfaces, or precisely formed surfaces, humanity has ever managed to produce, there will still be differences. So yes, making those images is actually quite an art form. But people have put quite a lot of time into getting it all perfectly lined up so that it makes sense. Thank you for that explanation. I hadn’t thought of that, but it certainly makes sense. If you weren’t a physicist, have you ever thought about another career that you would have liked to pursue? It’s a great question! I really like what I do. I feel very privileged to get to do what I do. It’s close to my dream job. I do enjoy writing a great deal, which I do in my spare time, and some part of me likes the romantic idea of being the fabulous writer who is paid so well they don’t have to care about things, they can just focus on their art. (laughs) So a bit of me feels like that would be OK. That would be a kind of nice way to be. Just get up and think great things and put them down on paper. But I’ve also long wondered what it would be like to try to make movies. I think some of that comes from my dad’s career. He was an art historian, but his specialty was the topic of photography and how that changed the way humans thought about the world. So, film and that side of things. Hollywood director, best-selling author, those sound like good career choices to me! (laughs) I liked your quote about being a writer. You said, “I’m a thinker, a writer, and sometimes both.” I don’t know if you remember that comment, but I got a kick out of it as I researched you online. Yes, I do remember that comment and it pretty much describes things. When you’re writing for your fellow scientists there are very specific ways that you construct your papers or your proposals and so on, and it’s not always clear that thinking at the same time is an advantage. (laughs) Caleb speaking about NASA science. That’s a good way to put it. Would you like to share anything about your home life, your family? Do you have a wife, partner, kids, or pets? I’m married and have two daughters who are now in their twenties, one has just graduated from college and the other is getting close to graduating, and I’m extremely proud of them both. It’s really exciting as a parent to see them beginning to find their way in the world. We don’t have any pets because everybody in the family but me is allergic! Are your daughters pursuing science? No, not science, really. I think we’ll see what they end up wanting to do. One is interested in media, in making documentaries, and using those tools for underserved and underrepresented communities in the world, which is really interesting. She’s spent a lot of time in Spain, so is very fluent in Spanish and is interested in that culture. My other daughter is interested in psychology but also in history and the way humans function as a society, which is interesting to me but is very different from my interests. They’ve clearly not followed the purely scientific pathway, but I think they’re both analytic thinkers. I recognize that so maybe it is something that runs in the family. Well, congratulations to them on where they are now; you said one has graduated and one is about to? The one who graduated is, as we speak, starting her first day working in a museum here in in New York. That’s wonderful. I can lose myself in museums. I could visit them every day. You’re obviously quite busy being a scientist and a writer and the other things that you’ve described, but when you have time, what do you like to do for fun? Sometimes I write, which may not like sound like fun to some people, but I do it also because I have books in my head that I want to write and publish. I also love being outdoors and that doesn’t mean just hiking, I just like being outside. When I’m out of a city, out in the countryside, I just like to wander around or sit there, absorbing all the plants, animals, and planetary goodness around me! I don’t know if that really counts as a hobby, but it definitely is something I enjoy a great deal. I also like a bit of gardening. I’m a strange variety of person who enjoys mowing the lawn! I find it a nice thing to do. It’s nice to do something physical where there’s an immediate outcome versus so much of science, certainly the kind of science I do, where a lot of it is sitting at a computer and you don’t necessarily see the product of your work for a while. So, physical things I enjoy. And I enjoy cycling and traveling for sure. I don’t like the process of traveling but I like it when I get there, let’s put it that way. My wife says that, too. It piqued my interest when you said you liked to mow the lawn because you can see the results of your work immediately. When I was growing up, my two siblings and I each had to choose a room in the house to clean and I chose the kitchen. It was the hardest one to keep clean because everybody’s in there all the time and there are always dirty dishes and pots and pans, but once it was clean, you could really tell. You could look in there and tell it had been cleaned. If you are vacuuming somewhere, you can’t usually tell if that’s been done or not, so I, too, like the sense of seeing what I’ve accomplished. That’s right. That’s absolutely right. And I like hedge trimming as well. I’m definitely into that, which may be the British side of me! (laughs). We like carefully pruned hedges and shrubbery, and I’ve probably become a bit obsessed with that. You don’t make figures out of your hedges, shapes and things like that, do you? No, no yet, but I am tempted. (laughs) Would you have advice for a young postdoc? Perhaps one who’s just starting out, who would like to have the kind of career and success that you are having? What advice would you give them in pursuing their dream, be it science or whatever? That’s always an interesting and quite a difficult question to answer. Some of it depends on if they find astrobiology in particular an interesting topic. I myself came to astrobiology, not right away but via a circuitous route through astrophysics, getting interested in exoplanets, then just deciding to focus on the search for life. What else is there? This is such a profound thing to do. So I would say to people, young scientists, maybe postdocs or grad students, if you have an interest in something like astrobiology, it’s really important to do two things: one is to be really skillful at a few technical areas, to specialize in useful things, but also to make sure that you look for ways to apply that specialization more broadly because that’s really what astrobiology is all about. For me it’s this playground where you can take very specialized skill sets and find new ways to apply them. Astrobiology demands that you engage with people in different fields, it really does, more than any other science that I know. So be specialized, but also be engaged with everyone around you. Scientists you might not expect to have things in common with, talk to them. Learn. See commonalities. Look for those little threads to pull on because those little threads are the interesting stuff and that might lead you to something really, really interesting, where a physicist like me can have a productive engagement with microbiologists, with very useful results. So that’s part of the advice I would say to people: don’t shut off other things, especially in astrobiology. That’s very good advice, thank you. You may have already answered this because you said you weren’t particularly musical, so you probably don’t play musical instrument, but do you have other hobbies or interests? You mentioned bicycle riding and hiking. Anything else? Art perhaps? Or literature? Or something else you’d characterize as a hobby? It’s a good question. I’m a pretty good cook, although cooking for me is primarily because I enjoy eating, so I don’t know if that really qualifies as a hobby, but it’s definitely a skill that I put into practice and it’s very different from work. I like it because there’s an end result that you see right there and you can share it with other people and that’s kind of a lovely thing. But all in all, I’m pretty boring. I spend a lot of time thinking about science and/or writing about science , so I don’t think I have hobbies in the conventional sense. Trust me, you’re not boring. I can tell just from reading your bio and having this conversation that you’re not boring. What accomplishment in your life to date are you most proud of that’s not related to your science work? Well, I think it’s probably that between my wife and myself, we’ve brought up two daughters who seem to be high functioning, decent human beings, is probably my proudest thing outside of science. If you hadn’t said that, I would have wondered why. (laughs) Who or what inspires you? That’s a very good question. I’ve been asked that question before in interviews and it’s always a struggle for me because I think I find inspiration in the most unexpected things all the time. I’ve had some of the most inspiring conversations in my life with farmers who lived down the lane from where I grew up in rural England. These people who have tended their fields for generations. They have this deep intuition about the way nature works but they were always inquisitive. As a little kid you could talk to them about all sorts of things. They were engaged with what was happening in the broader world as well as their own microcosm and I find that pretty inspiring. The ability to live a life where they’re not staring at TV screens, they’re not Tik-Tok influencers, but they’re thoughtful, observant, curious people. I always find that inspiring. I also find nature inspiring. I can sit on my back deck and just watch the birds and the bees doing their thing and I always find questions that I hadn’t thought of before. So, I think it’s a combination of, not celebrities or famous people so much, although some of them are extremely inspiring and impressive, but I’m more inspired by the day to day, and the people going about their lives quietly and carefully. That’s a very thoughtful answer and I appreciate it. One of the things we do with these conversations is invite you to provide pictures of the things you’ve talked about. Of your work of course, but also of your family perhaps or of trips you’ve taken, things that go along with the narrative because it makes the whole post more interesting. If there’s a JWST image that you find particularly appealing or interesting, one that we might we see on the wall of your office or in your house, you can include that and others when you return the edited transcript. Among the images I find most interesting are the earth from space, and the most interesting of those are where a spacecraft is on its way to do something else. Some of the earliest images were where you see the Earth and the moon in one frame and you realize how far apart they are from each other and how tiny they really are. There’s something about those images that I find quite disturbing, in a good way. Artemis Orion Completes Final Lunar Departure Maneuver, December 2022 Earthrise over moon, Apollo 8, December 1969 And there’s the famous blue dot, right? Yes. The pale blue dot. it’s a pixel and I honestly look at that and I think it’s a bit of a dud! I have to really work hard in my imagination to get there, but when you see just enough of the earth and just enough of the moon to recognize what they are and where they are, just sitting in the blackness of space, that for me is both terrifying and exhilarating. That’s kind of a special thing, the sort of picture I would have looming over me. Voyager 1’s iconic Pale Blue Dot picture, February 1990 I can just see you writing about these things and how interesting you find them. I’ll have to get one of your books and read it. Now is there a favorite quote that appeals to you because it’s clever or thought provoking or anything like that? I was thinking about this because I saw the questions and I immediately thought “Oh my gosh!”, because for me humor is incredibly important. It just is. It’s how I cope with things, but also a sense of humor is so important because it cuts through cultural differences, it cuts through differences in background, all that stuff. Oh yeah! The best I could come up with, since I’m a fan of Yogi Berra, is one that I recall because it’s so beautifully daft, where he says, “When you come to a fork in the road, take it”. (laughs) “A fork in the road” (metaphor) That’s a good one! I like that because it makes you think for a moment, to realize that he’s not really saying anything, but he’s also saying everything. To me it means “You’re going to get through it no matter what.” The most important thing is that you take that step and you will eventually find out the rest of it and everything will be OK. Is there something that you would like me to have asked you that I didn’t? No. Well, we didn’t talk much about my writing stuff. You can say something about that if you would like, sure. It’s kind of separate from science, but it is a big part of my life, and it was kind of unexpected. At a certain point maybe about ten or twelve years ago I decided to try writing for a more general audience and it’s kind of turned into this parallel career that I’ve had since then, quite unexpectedly. And it’s resulted in my writing over five hundred pieces for Scientific American over ten years and I’ve also written a bunch of books. I’m working on a new book right now, if I can put in a plug for it. It’s called “The Giant Leap” and it’s all about space exploration. That’s been an interesting turn for me, and it’s also made me realize that, much like teaching, there’s value to sitting down to write for a readership that is not specialist in any way. I try to imagine I’m writing for my mother or the guy who does my plumbing, you know? It’s incredibly useful as a scientist because it really helps you play with ideas, but it also helps you refine your own understanding because you can’t explain things simply unless you really understand them. And that’s been an interesting journey for me. Like I say, it’s been an entire parallel career, in the spare moments in between everything else, but it’s been marvelous. And as advice to younger scientists, think about that side of yourself, your capacity to share. We live in an era where it’s easier than ever to share, in many respects, for better or worse and I think scientists do have a certain obligation, especially as government scientists. We’re being paid by the taxpayer and we’re doing things for the good of the nation and for humanity. We should be more willing to share what we’re doing. People deserve to hear what we’re up to, and I think NASA does a great job at that. But as individuals, we can all help. There you go, that’s my soap box! (laughs) Thanks for the tip about your upcoming book “The Giant Leap”. And let’s not be timid about plugging your books. A brief online survey revealed these: The Copernicus Complex: Our Cosmic Significance in a Universe of Planets and Probabilities Gravity’s Engines: How Bubble-Blowing Black Holes Rule Galaxies The Zoomable Universe: An Epic Tour Through Cosmic Scale, from Almost Everything to Nearly Nothing The Ascent of Information: Books, Bits, Genes, Machines, and Life’s Unending Algorythm Extrasolar Planets and Astrobiology These all look fascinating and I hope they are doing well. Your comments describe a great ethic not only for the agency but also for individuals. I liked what you said about your writing: “anything expressed here is my fault alone”. It’s another way of saying the author is responsible. It was a little piece of humor. It’s been delightful to spend these few minutes chatting with you and I think we’re going to have a wonderful addition to our archive of scientist interviews. Sounds good. It’ll take probably two weeks, maybe three to get this on paper and then you can have whatever time you need and once you concur we will put it in a queue. It’s been a delight to chat with you today. Thank you again very much. My pleasure. Caleb standing beside a taxidermy moose head on display in Bryggen, a historic waterfront area with colorful wooden buildings in Bergen, Norway. ________________________________________________ Interview conducted by Fred Van Wert on March 28, 2024 View the full article

NASA’s Human Lander Challenge (HuLC) is an initiative supporting its Exploration Systems Development Mission Directorate’s (ESDMD’s) efforts to explore innovative solutions for a variety of known technology development areas for human landing systems (HLS). Landers are used to safely ferry astronauts to and from the lunar surface as part of the mission architecture for NASA’s Artemis campaign. Through this challenge, college students contribute to the advancement of HLS technologies, concepts, and approaches. Improvements in these technology areas have the potential to revolutionize NASA’s approach to space exploration, and contributions from the academic community are a valuable part of the journey to discovery. HuLC is open to teams comprised of full-time or part-time undergraduate and/or graduate students at an accredited U.S.-based community college, college, or university. HuLC projects allow students to incorporate their coursework into real aerospace design concepts and work together in a team environment. Interdisciplinary teams are encouraged. Award: $126,000 in total prizes Open Date: August 29, 2025 Close Date: March 4, 2026 For more information, visit: https://hulc.nianet.org/ View the full article