NASA

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 2 min read Curiosity Blog, Sols 4614-4615: Driving Along the Boxwork NASA’s Mars rover Curiosity acquired this image, looking out in the direction from where it came, with the rover’s tracks visible through the dust and sand covering the ground. Curiosity acquired this image using its Left Navigation Camera on July 28, 2025 — Sol 4612, or Martian day 4,612 of the Mars Science Laboratory mission — at 00:27:23 UTC. NASA/JPL-Caltech Written by Conor Hayes, Graduate Student at York University Earth planning date: Monday, July 28, 2025 Today was a pretty straightforward day of planning. Our drive over the weekend completed successfully, and we quickly confirmed that we are parked in a stable position. Thus, we were able to unstow the rover’s arm to poke around in our new workspace, which features a large sand-filled fracture. Aside from all of the good geology work to be done, the view from our current location is quite spectacular. We’re still in the time of year where the atmosphere at Gale is reasonably dust-free (at least, compared to later in the year), allowing us to look all the way out to and beyond the Gale crater rim. The upper slopes of Mount Sharp have also re-emerged to our east after spending months hidden behind the walls of Gediz Vallis. There’s a bit more sand and dust in this location than we’ve seen recently, so we can also see the trail left behind by the rover’s wheels as we drove to this location (see the image above). We’re still deep in our examination of the boxwork structures that we’re now driving through, so most of Curiosity’s attention in this plan is focused much closer to the rover than any of the scenic vista surrounding us. APXS, DRT, and MAHLI will all take a look at “Cañón de Palca,” some bedrock close to the large fracture in this workspace. Mastcam and ChemCam RMI will image some boxwork ridges at “Caine,” and will also collaborate on imaging of the weekend’s post-drive AEGIS target and a LIBS bedrock target “Doña Ines.” Mastcam’s solo activities include taking a look at some layering at “Paniri butte” and at MAHLI to examine a speck of dust that may have fallen on the lens. We’ll be driving away from this location along one of the boxwork ridges, which, at about 5 meters (about 16 feet) wide, is more than large enough to fit our car-sized rover. Post-drive activities are largely focused on environmental monitoring, including Navcam line-of-sight and dust-devil surveys to look at dust, and several Navcam cloud movies. As usual, ChemCam will also join the post-drive fun with an AEGIS observation. More environmental monitoring by REMS, RAD, and DAN fill out the remainder of this plan. Learn more about Curiosity’s science instruments For more Curiosity blog posts, visit MSL Mission Updates Share Details Last Updated Jul 29, 2025 Related Terms Blogs Explore More 3 min read Spheres in the Sand Article 3 hours ago 2 min read Curiosity Blog, Sols 4611-4613: Scenic Overlook Article 1 day ago 3 min read Curiosity Blog, Sols 4609–4610: Recharged and Ready To Roll Onwards Article 1 day 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

Explore This Section Perseverance Home Mission Overview Rover Components Mars Rock Samples Where is Perseverance? Ingenuity Mars Helicopter Mission Updates Science Overview Objectives Instruments Highlights Exploration Goals News and Features Multimedia Perseverance Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 3 min read Spheres in the Sand NASA’s Perseverance rover captured this image of spherule-bearing regolith at Rowsell Hill using its arm-mounted WATSON camera on July 5, 2025 — Sol 1555, or Martian day 1,555 of the Mars 2020 mission — at the local mean solar time of 12:46:29. WATSON (Wide Angle Topographic Sensor for Operations and eNgineering) is a close-range color camera that works with the rover’s SHERLOC instrument (Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals); both are located on the turret at the end of the rover’s robotic arm. NASA/JPL-Caltech Written by Andrew Shumway, Postdoctoral Researcher at the University of Washington It is not common for a rover to spot nearly perfect spheres in the soil beneath its wheels. Over two decades ago, the Opportunity rover famously discovered spherules made of hematite (nicknamed “blueberries”) near its landing site in Meridiani Planum. More recently, the Perseverance rover has similarly encountered spherules embedded in bedrock and loosely scattered throughout the region informally called “Witch Hazel Hill.” In a previous blog post, we described Perseverance’s investigations of a spherule-bearing outcrop at the “Hare Bay” abrasion patch, where the team later collected a core. With the “Bell Island” sample added to the rover’s collection, the science team next decided to take a closer look at loose spherules in the area, which appear to have eroded out of the nearby bedrock. On Sol 1555, while the United States was celebrating the Fourth of July with hotdogs and fireworks, Perseverance was hard at work studying spherule-rich regolith at the target “Rowsell Hill” using the proximity instruments on its robotic arm. SHERLOC’s Autofocus and Context Imager and WATSON camera both captured high resolution pictures of the target (shown above), while PIXL measured the elemental makeup of the spherules and surrounding grains. Despite their superficial similarity to Opportunity’s “blueberries”, the spherules at “Rowsell Hill” have a very different composition and likely origin. In Meridiani Planum, the spherules were composed of the mineral hematite and were interpreted to have formed in groundwater-saturated sediments in Mars’ distant past. By comparison, the spherules in “Rowsell Hill” have a basaltic composition and likely formed during a meteoroid impact or volcanic eruption. When a meteoroid crashes into the surface of Mars, it can melt rock and send molten droplets spraying into the air. Those droplets can then rapidly cool, solidifying into spherules that rain down on the surrounding area. Alternatively, the spherules may have formed from molten lava during a volcanic eruption. With these new data in hand, the Perseverance science team continues to search for answers about where these spherules came from. If they formed during an ancient impact, they may be able to tell us about the composition of the meteoroid and the importance of impact cratering in early Mars’s history. If they instead formed during a volcanic eruption, they could preserve clues about past volcanism in the region around Jezero crater. Either way, these spherules are a remnant of an energetic and dynamic period in Mars’ history! Learn more about Perseverance’s science instruments For more Perseverance blog posts, visit Mars 2020 Mission Updates Share Details Last Updated Jul 29, 2025 Related Terms Blogs Explore More 2 min read Curiosity Blog, Sols 4611-4613: Scenic Overlook Article 1 day ago 3 min read Curiosity Blog, Sols 4609–4610: Recharged and Ready To Roll Onwards Article 1 day ago 2 min read Feeling the Heat: Perseverance Looks for Evidence of Contact Metamorphism Article 7 days 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 artist’s concept of Blue Ghost Mission 4 shows Firefly’s Blue Ghost lunar lander and NASA payloads in the lunar South Pole Region, through NASA’s CLPS (Commercial Lunar Payload Services) initiative.Credit: Firefly Aerospace NASA has awarded Firefly Aerospace of Cedar Park, Texas, $176.7 million to deliver two rovers and three scientific instruments to the lunar surface as part of the agency’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign to explore more of the Moon than ever before. This delivery is the first time NASA will use multiple rovers and a variety of stationary instruments, in a collaborative effort with the CSA (Canadian Space Agency) and the University of Bern, to help us understand the chemical composition of the lunar South Pole region and discover the potential for using resources available in permanently shadowed regions of the Moon. “Through CLPS, NASA is embracing a new era of lunar exploration, with commercial companies leading the way,” said Joel Kearns, deputy associate administrator for exploration, Science Mission Directorate, NASA Headquarters in Washington. “These investigations will produce critical knowledge required for long-term sustainability and contribute to a deeper understanding of the lunar surface, allowing us to meet our scientific and exploration goals for the South Pole region of the Moon for the benefit of all.” Under the new CLPS task order, Firefly is tasked with delivering end-to-end payload services to the lunar surface, with a period of performance from Tuesday to March 29, 2030. The company’s lunar lander is targeted to land at the Moon’s South Pole region in 2029. This is Firefly’s fifth task order award and fourth lunar mission through CLPS. Firefly’s first delivery successfully landed on the Moon’s near side in March 2025 with 10 NASA payloads. The company’s second mission, targeting a launch in 2026, includes a lunar orbit drop-off of a satellite combined with a delivery to the lunar surface on the far side. Firefly’s third lunar mission will target landing in the Gruithuisen Domes on the near side of the Moon in 2028, delivering six experiments to study that enigmatic lunar volcanic terrain. “As NASA sends both humans and robots to further explore the Moon, CLPS deliveries to the lunar South Pole region will provide a better understanding of the exploration environment, accelerating progress toward establishing a long-term human presence on the Moon, as well as eventual human missions to Mars,” said Adam Schlesinger, manager of the CLPS initiative at NASA’s Johnson Space Center in Houston. The rovers and instruments that are part of this newly awarded flight include: MoonRanger is an autonomous microrover that will explore the lunar surface. MoonRanger will collect images and telemetry data while demonstrating autonomous capabilities for lunar polar exploration. Its onboard Neutron Spectrometer System instrument will study hydrogen-bearing volatiles and the composition of lunar regolith, or soil. Lead development organizations: NASA’s Ames Research Center in California’s Silicon Valley, and Carnegie Mellon University and Astrobotic, both in Pittsburgh. Stereo Cameras for Lunar Plume Surface Studies will use enhanced stereo imaging photogrammetry, active illumination, and ejecta impact detection sensors to capture the impact of the rocket exhaust plume on lunar regolith as the lander descends on the Moon’s surface. The high-resolution stereo images will help predict lunar regolith erosion and ejecta characteristics, as bigger, heavier spacecraft and hardware are delivered to the Moon near each other in the future. Lead development organization: NASA’s Langley Research Center in Hampton, Virginia. Laser Retroreflector Array is an array of eight retroreflectors on an aluminum support structure that enables precision laser ranging, a measurement of the distance between the orbiting or landing spacecraft to the reflector on the lander. The array is a passive optical instrument, which functions without power, and will serve as a permanent location marker on the Moon for decades to come. Lead development organization: NASA’s Goddard Space Flight Center in Greenbelt, Maryland. A CSA Rover is designed to access and explore remote South Pole areas of interest, including permanently shadowed regions, and to survive at least one lunar night. The CSA rover has stereo cameras, a neutron spectrometer, two imagers (visible to near-infrared), a radiation micro-dosimeter, and a NASA-contributed thermal imaging radiometer developed by the Applied Physics Laboratory. These instruments will advance our understanding of the physical and chemical properties of the lunar surface, the geological history of the Moon, and potential resources such as water ice. It will also improve our understanding of the environmental challenges that await future astronauts and their life support systems. Lead development organization: CSA. Laser Ionization Mass Spectrometer is a mass spectrometer that will analyze the element and isotope composition of lunar regolith. The instrument will utilize a Firefly-built robotic arm and Titanium shovel that will deploy to the lunar surface and support regolith excavation. The system will then funnel the sample into its collection unit and use a pulsed laser beam to identify differences in chemistry compared to samples studied in the past, like those collected during the Apollo program. Grain-by-grain analyses will provide a better understanding of the chemical complexity of the landing site and the surrounding area, offering insights into the evolution of the Moon. Lead development organization: University of Bern in Switzerland. Through the CLPS initiative, NASA purchases lunar landing and surface operations services from American companies. The agency uses CLPS to send scientific instruments and technology demonstrations to advance capabilities for science, exploration, or commercial development of the Moon, and to support human exploration beyond to Mars. By supporting a robust cadence of lunar deliveries, NASA will continue to enable a growing lunar economy while leveraging the entrepreneurial innovation of the commercial space industry. To learn more about CLPS and Artemis, visit: https://www.nasa.gov/clps -end- Alise Fisher Headquarters, Washington 202-358-2546 alise.m.fisher@nasa.gov Nilufar Ramji Johnson Space Center, Houston 281-483-5111 nilufar.ramji@nasa.gov Share Details Last Updated Jul 29, 2025 LocationNASA Headquarters Related TermsCommercial Lunar Payload Services (CLPS)ArtemisEarth's Moon View the full article

3 min read Adam and Hirsa Present Research on the Ring-Sheared Drop Abnormal fibrous, extracellular, proteinaceous deposits found in organs and tissues are associated with neurodegenerative diseases such as Alzheimer’s. (“Amyloid fibril formation in microgravity: Distinguishing interfacial and flow effects” NNX13AQ22G). The Ring Sheared Drop investigation studies the biophysics of protein amyloidogenesis in the absence of gravity in order to study fibril formation at fluid interfaces, in the absence of solid walls. NASA Researchers across Space Biology and Physical Sciences come together for a special presentation at the May PSI Users Group. The Ring-Sheared Drop (RSD) is a Microgravity Science Glovebox experiment that launched in July 2019 to the ISS to study shearing flow in the absence of solid walls. The major goals of this project were to adapt and use the RSD module to develop and test predictive models of non-Newtonian flow of high-concentration proteins at the interface. At the May Physical Sciences Informatics (PSI) User Group, Dr. Joe Adam, Research Scientist at Rensselaer Polytechnic Institute and University Payload Director of the RSD module, presented, “Protein Solution Hydrodynamic Studies in the Ring-Sheared Drop” detailing the history of RSD, research campaigns and data to be released in PSI. This investigation was led by Principal Investigator, Prof. Amir Hirsa of Rensselaer Polytechnic Institute. The ring-sheared drop interfacial bioprocessing of pharmaceuticals-I (RSD-IBP-I) campaign aimed to study non-Newtonian interfacial hydrodynamics of the blood transport proteins bovine serum albumin (BSA) and human serum albumin (HSA) in microgravity. Specifically, scientific aims focus on the effects of protein primary structure (BSA or HSA), protein concentration and interfacial shear rate on microgravity fluid flow, measured using velocimetry of hollow glass microsphere tracer particles within protein samples. This campaign intended to confer improved understanding of interfacial protein flows in relation to physiology, the environment, and industry relevant to both spaceflight and Earth. Results from this line of research could have applications to in situ pharmaceutical production, tissue engineering, and diseases such as Alzheimer’s, Parkinson’s, infectious prions, and type 2 diabetes. To encourage collaboration across common areas of BPS’s Physical Sciences and Biology research, PSI invited Ryan Scott, ALSDA lead Scientist, and members of the ADBR (Alz Disease & Brain Resilience) and Parkinson’s AWG subgroups to attendee this month’s meeting which fueled discussions and led to several connections. During the discussions the two relevant collaborative publications that were shared are: McMackin, P., Adam, J., Griffin, S. et al. Amyloidogenesis via interfacial shear in a containerless biochemical reactor aboard the International Space Station. npj Microgravity 8, 41 (2022). https://doi.org/10.1038/s41526-022-00227-2 Nilufar Ali paper resulting in part from a collaboration within the Parkison’s AWG subgroup Ali, N., Beheshti, A. & Hampikian, G. Space exploration and risk of Parkinson’s disease: a perspective review. npj Microgravity 11, 1 (2025). https://doi.org/10.1038/s41526-024-00457-6 Ring-Sheared Drop – Interfacial Bioprocessing of Pharmaceuticals(RSD-IBP-I) is now accessible in PSI. http://doi.org/10.60555/smat-bb74 Share Details Last Updated Jul 29, 2025 Related Terms Uncategorized Explore More 1 min read 2025 NASA Space Apps Challenge Article 22 hours ago 2 min read OSDR Chats with Begum Mathyk Article 22 hours ago 4 min read Helio Highlights: June 2025 Article 2 weeks ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

An aircraft body modeled after an air taxi with weighted test dummies inside is being prepared for a drop test by researchers at NASA’s Langley Research Center in Hampton, Virginia. The test was completed June 26, 2025, at Langley’s Landing and Impact Research Facility. The aircraft was dropped from a tall steel structure, known as a gantry, after being hoisted about 35 feet in the air by cables. NASA researchers are investigating aircraft materials that best absorb impact forces in a crash.NASA/Mark Knopp As the aviation industry works to design air taxis and other new electric aircraft, there’s a growing need to understand how the materials behave. That’s why NASA is investigating potential air taxi materials and designs to best protect passengers in the event of a crash. On June 26, 2025, at NASA’s Langley Research Center in Hampton, Virginia, researchers dropped a full-scale aircraft body modeled after an air taxi from a tall steel structure, known as a gantry. The NASA researchers behind this test and a previous one in late 2022 investigated materials that best absorb impact forces, generating data that will enable manufacturers to design safer advanced air mobility aircraft. Image Credit: NASA/Mark Knopp View the full article

NASA Astronaut Kate RubinsNASA NASA astronaut and microbiologist Kate Rubins retired Monday after 16 years with the agency. During her time with NASA, Rubins completed two long-duration missions aboard the International Space Station, logging 300 days in space and conducting four spacewalks. “I want to extend my sincere gratitude to Kate for her dedication to the advancement of human spaceflight,” said Steve Koerner, acting director of NASA’s Johnson Space Center in Houston. “She is leaving behind a legacy of excellence and inspiration, not only to our agency, but to the research and medical communities as well. Congratulations, Kate, on an extraordinary career.” Rubins’ first mission to the orbiting laboratory began in July 2016, aboard the first test flight of the new Soyuz MS spacecraft. As part of Expedition 48/49, she contributed to more than 275 scientific experiments, including molecular and cellular biology research, and she was the first person to sequence DNA in space. Her work enabled significant advances with in-flight molecular diagnostics, long-duration cell culture, and the development of molecular biology tools and processes, such as handling and transferring small amounts of liquids in microgravity. Rubins also led the integration and deployment of biomedical hardware aboard the space station, supporting crew health and scientific research in space and on Earth. She again launched in October 2020, aboard a Soyuz spacecraft from the Baikonur Cosmodrome in Kazakhstan, taking part in Expedition 63/64. Alongside her crewmates, Rubins spent hundreds of hours working on new experiments and furthering research investigations conducted during her mission, including heart research and multiple microbiology studies. She also advanced her work on DNA sequencing in space, which could allow future astronauts to diagnose illness or identify microbes growing aboard the station or during future exploration missions. “From her groundbreaking work in space to her leadership on the ground, Kate has brought passion and excellence to everything she’s done,” said Joe Acaba, chief of the Astronaut Office at NASA Johnson. “She’s been an incredible teammate and role model. We will miss her deeply, but her impact will continue to inspire.” In addition to her flight assignments, Rubins served as acting deputy director of NASA’s Human Health and Performance Directorate, where she helped guide strategy for crew health and biomedical research. More recently, she contributed to developing next-generation lunar spacesuits, helping prepare for future Artemis missions to the Moon. Before her selection as an astronaut in 2009, Rubins received a bachelor’s degree in molecular biology from the University of California, San Diego, and a doctorate in cancer biology from Stanford University Medical School’s Biochemistry Department and Microbiology and Immunology Department. After returning from her second space mission, Rubins commissioned as a major in the U.S. Army Reserve, serving as a microbiologist in the Medical Service Corps. She currently holds the role of innovation officer with the 75th U.S. Army Reserve Innovation Command’s MedBio Detachment, headquartered in Boston. A frequent keynote speaker at scientific, educational, and industry events on space biology, biomedical engineering, and human exploration, Rubins has advocated for NASA’s scientific and exploration missions. As she transitions from government service, she remains committed to advancing innovation at the intersection of biology, technology, and space. “It has been the honor of a lifetime to live and work in space,” said Rubins. “I am grateful for the extraordinary advances at NASA, and it was a privilege to serve and contribute to something so meaningful. The mission of exploration continues, and I can’t wait to watch this nation do what once seemed impossible.” Learn more about how NASA explores the unknown and innovates for the benefit of humanity at: https://www.nasa.gov/ -end- Raegan Scharfetter Johnson Space Center, Houston 281-910-4989 raegan.r.scharfetter@nasa.gov 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 2 min read Curiosity Blog, Sols 4611-4613: Scenic Overlook NASA’s Mars rover Curiosity acquired this image, sitting on top of the distinctive ridge-and-hollow terrain of the boxwork-forming unit for a panoramic view, on July 24, 2025. Curiosity used its Right Navigation Camera on Sol 4609, or Martian day 4,609 of the Mars Science Laboratory mission, at 21:29:43 UTC. NASA/JPL-Caltech Written by Lucy Lim, Planetary Scientist at NASA’s Goddard Space Flight Center Earth planning date: Friday, July 25, 2025 A 23-meter drive (about 75 feet) brought Curiosity to today’s planned “look-about” spot. The highlight of the plan will be the 360-degree Mastcam panorama that will document the ridge-and-hollow topography of the boxwork-forming unit we’ve been exploring, in addition to overlying stratigraphy in some of the nearby buttes. The right-angle ridge pattern is quite prominent in the HiRISE orbital imaging, which enabled us to plan for this stop. It has been 70 sols since the last panorama and the rover has driven quite some distance in that time! Additional detailed imaging was planned with the ChemCam remote imager (RMI) and Mastcam high-resolution M100: mosaics will cover the exposed strata underneath the ridge we’re planning to drive on (“Arequipa Airport”), two linear fractures, one parallel to the large ridge and one cross-cutting it (“Laguna de Salinas” and “Laguna Santa Rosa”), some troughs around a nearby light-toned float block (“Arubai”), and the Uyuni butte in the middle distance. The bedrock texture here was a noticeable change from the previous workspace, with a knobbly oriented texture interspersed occasionally with platier exposures. Geochemical measurements were planned with the ChemCam LIBS to complement the auto-targeted post-drive AEGIS measurement: “La Coca” on a block that appeared to show unusual colors, and “El Algodón” on a knobbly textured chunk of bedrock. APXS geochemistry was planned with dust removal on the “Yura Tuff” knobbly target and without dust removal on the “Tipnis” target. MAHLI will also provide close-up imaging on the two APXS targets. For the modern Martian environment, it’s still the cloudy season at Gale so we are planning several cloud-related activities. The Mastcam sky survey will measure abundances of atmospheric dust and water ice, whereas a special cloud altitude observation will include video of clouds and their shadows so that the altitudes and velocities of the clouds and related winds can be calculated. A separate short movie will search for dust lifting (dust devil) activity. Finally, the usual passive REMS and DAN observations will monitor the temperature, humidity, and neutron environment at Curiosity’s current location. For more Curiosity blog posts, visit MSL Mission Updates Learn more about Curiosity’s science instruments Share Details Last Updated Jul 28, 2025 Related Terms Blogs Explore More 3 min read Curiosity Blog, Sols 4609–4610: Recharged and Ready To Roll Onwards Article 4 hours ago 2 min read Feeling the Heat: Perseverance Looks for Evidence of Contact Metamorphism Article 6 days ago 3 min read Curiosity Blog, Sols 4607-4608: Deep Dip Article 6 days 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

As part of her Summer Reading Challenge, Second Lady Usha Vance will host an event for children in grades K-8 on Monday, Aug. 4, at NASA’s Johnson Space Center in Houston.Credit: White House As part of her Summer Reading Challenge, Second Lady Usha Vance will host an event for children in grades K-8 on Monday, Aug. 4, at NASA’s Johnson Space Center in Houston. Media are invited. NASA astronaut Suni Williams will join Ms. Vance to read a space-related book to children and participate in other space-related activities. Live coverage of the reading will stream about 2:45 p.m. EDT on NASA+. Learn how to watch NASA content through a variety of platforms, including social media. U.S. media interested in participating in this event must RSVP to NASA Press Secretary Bethany Stevens at: bethany.c.stevens@nasa.gov, as well as Office of the Second Lady Communications Director Nicole Reeves at: nicole.e.reeves@ovp.eop.gov. Requests must be made no later than 1 p.m. EDT on Thursday, July 31. Confirmed media will receive additional details from NASA. The agency’s media accreditation policy is online. Through her reading challenge, the Second Lady is encouraging youth to seek adventure, imagination, and discovery between the pages of a book. Students interested in participating in the challenge must read 12 books by Friday, Sept. 5. Additional details, including where to download a reading log, and how to submit it to the White House, are available online. As part of NASA’s Artemis campaign, the agency will send astronauts to the Moon to prepare for future human exploration of Mars, inspiring Golden Age explorers, and ensuring the United States continues to lead in space exploration and discovery. Learn more about NASA missions online at: https://www.nasa.gov -end- Bethany Stevens / Cheryl Warner Headquarters, Washington 202-358-1600 bethany.c.stevens@nasa.gov / cheryl.m.warner@nasa.gov Share Details Last Updated Jul 28, 2025 LocationNASA Headquarters Related TermsNASA HeadquartersJohnson Space Center View the full article

SVEC building locations including parking areas. Where to Park at the Event Center We have event spaces in multiple buildings. See below for details. At the main Event Center in building 3, at the front of the building (East side) there is a large lot with standard and accessible spaces. This is the best place to park as it affords the easiest access to the entry doors, which have an ADA accessible ramp. At the rear of the building, there is a secondary large over-flow lot. As this is on the back side of the building, you will need to walk all the way around to enter through the main entrance, or make arrangements to enter through the ADA accessible doors at the rear of the building. Inside the NASA security fence, at building N232 and the N201 Syverston Auditorium, there is very little parking available and it is first-come first-serve. We highly recommend walking or carpooling to these locations if you are attending an event in either of them Please keep in mind that if you are driving in, the driver will need a valid, RealID, drivers license. In addition, everyone in the car must have a valid form of ID; Government issued RealID, valid passport, or other form of accepted identification. Back to the SVEC Home View the full article

April 8, 2025Kenny Contreras April 10, 2025 April 10, 2025 April 10, 2025 On-Site Lodging at Ames The Exchange at Ames operates a variety of lodging options, right on center. If you’re visiting Ames for an extended period, you’ll need lodging that’s in the area, and affordable. This article will go over the lodging options that we have on-center. Who May Stay? Personnel in the following categories are considered eligible: APPEL course participants ARC college student program participants TDY visitors to NASA or other federal agencies on official orders Visiting university faculty, post-doctoral students (to NASA only) Visitors to ARC or other federal agency on-site contractors to conduct NASA or resident agency related business Active duty or reserve-on-active-duty military with orders ARC employees conducting business facilitated by overnight accommodation (e.g. ongoing experiment, major conference) ARC employees for their personal convenience NASA and military service retirees Accompanying family members of the above NRP Tenants and their guests (foreign nationals must be cleared through security prior to NRP and lodge access) Making A Reservation Please contact the front desk for all inquiries. Business Hours: Monday – Friday, 8:30am – 4:00pm Phone: (650) 604-8100 Email: info@nasalodge.com Check-In: 3:00 PM (Contactless check-in is available after business hours.) Check-Out: 11:00 AM All reservations require an email address and a cell phone number. Credit card information is required prior to check-in by calling the front desk. Cancellations or changes must be done at least 24 hours prior to check-in via email at info@nasalodge.com or calling the front desk at (650) 604-8100. If you fail to cancel your reservation, you will be charged for one night’s stay. Building 19 Premium King Room 24 Remodeled Modern Rooms Luxurious Restroom with Walk-in Shower & Towel Warmers Central A/C & Heating Spacious Closet Space Work Desk Space Mini Refrigerator with Freezer Flat Screen TV with Full DirecTV Access Including HBO, Showtime, Cinemax, Etc. In-Room Safe Complimentary Coffee & Bottled Water Iron & Ironing Board Robust Power Outlets USB-A & USB-C Dimmable Lighting Keyless RFID Entry NASA-Connect Accessible Free Parking Complimentary Breakfast Building 19- Standard Queen Room 20 Remodeled Queen Rooms A/C Window Unit Heater Unit Work Desk Space Private Bathroom Mini Refrigerator with freezer Flatscreen TV In-Room Safe Iron & Iron Board NASA-Connect Accessible Free Parking Complimentary Breakfast Buildings 583 A & B Dorms Queen & Twin Size Bed Options Work Desk Space Private Restroom Microwave Refrigerator with Freezer (Size varies) Access Communal Kitchen NASA-Connect Accessible Flatscreen TV Available in Select Rooms Back to SVEC Home View the full article

New Electronic Ames Research Center sign a the corner of Arnold Avenue. Visiting the Event Center Due to the nature of being a NASA facility, there are some special considerations that must be taken into account. Traveling To & From The Event Center is located on the publicly accessible side of the Ames campus. If you plan to arrive via ride share, please be aware that the vehicle and driver must have a valid RealID Drivers License and vehicle registration documents. All passengers will need valid ID as well. U.S. Citizens must show a valid, officially-issued RealID at the NASA Research Park gate to enter onto the NASA Research Park, where the SVEC is located. All Foreign Nationals must go through NASA badging procedures to attend meetings at the SVEC. NASA Transfer Technology and Export Control If you are having NASA speakers and Non-NASA attendees, your speakers must clear the information with the “NASA” Export Control Office. Back to SVEC Home View the full article

Generic Calendar Upcoming Events for the Public Check below for upcoming events that are open to the public being held at the Event Center SundayMondayTuesdayWednesdayThursdayFridaySaturday Back to SVEC Home View the full article

Credit: NASA NASA has selected Barrios Technology, LLC, in Houston to provide technical integration services for the agency’s human space flight programs. The Mission Technical Integration Contract is a cost-plus-award-fee and cost-plus-incentive fee contract with core and indefinite-delivery/indefinite-quantity requirements. It has a total estimated value of approximately $450 million, and a period of performance beginning Oct. 1, and ending on Sept. 30, 2027, along with four one-year option periods through 2031. Under the contract, the contractor will provide technical integration and related services for multiple human space flight programs. These services include program, business, configuration and data management, information technology, systems engineering and integration, mission integration, safety and mission assurance, and operations. For information about the agency and its programs, visit: https://www.nasa.gov -end- Tiernan Doyle Headquarters, Washington 202-358-1600 tiernan.doyle@nasa.gov Share Details Last Updated Jul 28, 2025 LocationNASA Headquarters Related TermsHumans in SpaceJohnson Space Center 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 3 min read Curiosity Blog, Sols 4609–4610: Recharged and Ready To Roll Onwards NASA’s Mars rover Curiosity acquired this image showing the boxwork hollow where it is investigating, and the boxwork ridge on the far side of the hollow, using its Left Navigation Camera. Curiosity captured the image on July 20, 2025 — Sol 4605, or Martian day 4,605 of the Mars Science Laboratory mission — at 18:51:55 UTC. NASA/JPL-Caltech Written by Catherine O’Connell-Cooper, Planetary Geologist at University of New Brunswick Earth planning date: Wednesday, July 23, 2025 For today’s planning, we were in the same workspace as the Monday plan — on purpose! We don’t often have a plan without a drive but in order to allow the battery to recover from some power-hungry SAM atmospheric measurements over the weekend and on Monday, we needed to stay put and skip our usual drive. As a result, we gained a bonus planning cycle at this interesting workspace. We are in one of the “hollows” between the resistant ridges of the “boxwork” terrain, as you can see in the image for this blog. This made for a quieter Operations day for me as the APXS planner. As Deborah noted in Monday’s blog, we have already gotten three APXS and MAHLI measurements in this workspace, so we didn’t acquire more in this plan. This morning, we focused on documenting some small light-toned, rounded, white pebbles in the workspace (you can see them in the accompanying Navcam image), which look very different from the underlying bedrock. We used our one ChemCam LIBS analysis for the plan on “Yana Qaqa.” Mastcam will image this pebble, another at “Ojos del Salado,” and a really cool-looking target with a dendritic-looking texture at “Punta de Lobos.” Further afield, Mastcam will image the adjacent boxwork ridge and hollow in our drive direction, and a series of troughs with raised edges to the right of our current workspace. ChemCam will image a long-distance RMI mosaic of “Cueva de los Vencejos y Murciélagos,” which was imaged by Mastcam on Monday, and also acquire some further images of the “Mishe Mokwa” hill. We had a bumper couple of sols of atmospheric measurements over the weekend and Monday. Now we revert back to our more normal environmental and atmospheric monitoring. These do not get as much attention sometimes as the amazing images we take of the fascinating rocks we see, but have been taking place consistently and continuously since Curiosity’s landing almost 13 years ago now. This plan includes a series of Navcam movies (suprahorizon, dust devil) and a line-of-sight observation of dust, standard REMS and DAN observations, and two Mastcam tau measurements, looking at dust in the atmosphere. Our 24-meter drive (almost 79 feet) will take us out of this hollow and back up on top of a ridge. From here, we hope to be able to spy the best driving path through the boxwork. The ridges are up to 5 meters in diameter (about 16 feet), so we are cautiously hopeful that we can just trundle along one of the ridges as we investigate this fascinating terrain. For more Curiosity blog posts, visit MSL Mission Updates Learn more about Curiosity’s science instruments Share Details Last Updated Jul 28, 2025 Related Terms Blogs Explore More 2 min read Feeling the Heat: Perseverance Looks for Evidence of Contact Metamorphism Article 6 days ago 3 min read Curiosity Blog, Sols 4607-4608: Deep Dip Article 6 days ago 3 min read Curiosity Blog, Sols 4604-4606: Taking a Deep Breath of Martian Air Article 6 days 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

Join the 2025 NASA International Space Apps Challenge: Learn, Launch, Lead On October 4–5, 2025, NASA—along with 14 international space agency partners—invites scientists, engineers, coders, designers, storytellers, and space enthusiasts of all kinds to take part in the 2025 NASA International Space Apps Challenge. This two-day global hackathon brings together diverse teams to tackle real-world problems using NASA’s open data, alongside space-based data from agencies around the world. This year’s theme, Learn, Launch, Lead, encourages participants to: Learn new skills and deepen their understanding of STEM, Launch bold ideas by transforming open data into actionable solutions, and Lead communities in pioneering innovation and discovery. Participants will collaborate to develop creative, open-source projects that address Earth and space-related challenges. Whether you’re a seasoned developer, an aspiring student, or a creative thinker, there’s a place for you in this global movement. Together, we’ll use the power of open data and global collaboration to solve some of the world’s toughest challenges—on Earth and beyond. Learn more and register now! View the full article

OSDR Chats: Dr Begum Mathyk Presents Latest Research in this OSDR-Enabled Publication Welcome to “OSDR Chats,” an interview series featuring authors of publications that were enabled by the Open Science Data Repository (OSDR). Researchers share highlights and insights into their work, emphasizing the valuable roles played by the OSDR in their research. This newest interview features Dr Begum Mathyk who discusses her paper “Spaceflight induces changes in gene expression profiles linked to insulin and estrogen“, one of 45 that were part of the Nature Press package publications. Organismal adaptations to spaceflight have been characterized at the molecular level in model organisms, including Drosophila and C. elegans. This study extends such molecular work to energy metabolism and sex hormone signaling in mice and humans. The findings of this research underscore the critical importance of in-depth hormonal studies on the effects of space travel, which are vital for enabling further human exploration of space. The study also emphasizes the need for further research focused on women’s health and the development of tailored healthcare strategies for space environments. OSDR recently spoke to Dr Mathyk to hear about the highlights of this publication and about how the OSDR and Analysis Working Groups (AWGs) enabled this publication. Link to Publication; Link to Datasets: OSD-48, OSD-98, OSD-99, OSD-100, OSD-101, OSD-102, OSD-103, OSD-104, OSD-105, OSD-168, OSD-238, OSD-239, OSD-240, OSD-241, OSD-254, OSD-530; Learn more about Analysis Working Groups (AWGs); Request to Join Analysis Working Groups (AWGs) View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) An aircraft body modeled after an air taxi with weighted test dummies inside is shown after a drop test at NASA’s Langley Research Center in Hampton, Virginia. The test was completed June 26 at Langley’s Landing and Impact Research Facility. The aircraft was dropped from a tall steel structure, known as a gantry, after being hoisted about 35 feet in the air by cables. NASA researchers are investigating aircraft materials that best absorb impact forces in a crash.NASA/Mark Knopp As the aviation industry works to develop new air taxis and other electric aircraft made from innovative, lightweight materials, there’s a growing need to understand how those materials behave under impact. That’s why NASA is investigating potential air taxi materials and designs that could best protect passengers in the event of a crash. On June 26 at NASA’s Langley Research Center in Hampton, Virginia, researchers dropped a full-scale aircraft body modeled after an air taxi from a tall steel structure, known as a gantry. The NASA researchers behind this test and a previous one in late 2022 investigated materials that best absorb impact forces, generating data that will enable manufacturers to design safer advanced air mobility aircraft. “By showcasing elements of a crash alongside how added energy-absorbing technology could help make the aircraft more robust, these tests will help the development of safety regulations for advanced air mobility aircraft, leading to safer designs,” said Justin Littell, test lead, based at Langley. An aircraft body modeled after an air taxi with weighted test dummies inside is hoisted about 35 feet in the air by cables at NASA’s Langley Research Center in Hampton, Virginia. The aircraft was dropped from a tall steel structure, known as a gantry, on June 26 at Langley’s Landing and Impact Research Facility. NASA researchers are investigating aircraft materials that best absorb impact forces in a crash.NASA/Mark Knopp During the June test, the aircraft was hoisted about 35 feet into the air and then released. It swung forward before crashing to the ground. The impact conditions were like the prior test in 2022, but with the addition of a 10-degree yaw, or twist, to the aircraft’s path. The yaw replicated a certification condition required by Federal Aviation Administration regulations for these kinds of aircraft. After the drop, researchers began to evaluate how the structure and batteries withstood the impact. As expected, the material failures closely matched predictions from computer simulations, which were updated using data from the 2022 tests. An aircraft body modeled after an air taxi with weighted test dummies inside is being prepared for a drop test by researchers at NASA’s Langley Research Center in Hampton, Virginia. The test was completed June 26 at Langley’s Landing and Impact Research Facility. The aircraft was dropped from a tall steel structure, known as a gantry, after being hoisted about 35 feet in the air by cables. NASA researchers are investigating aircraft materials that best absorb impact forces in a crash.NASA/Mark Knopp An aircraft body modeled after an air taxi with weighted test dummies inside is being prepared for a drop test by researchers at NASA’s Langley Research Center in Hampton, Virginia. The test was completed June 26 at Langley’s Landing and Impact Research Facility. The aircraft was dropped from a tall steel structure, known as a gantry, after being hoisted about 35 feet in the air by cables. NASA researchers are investigating aircraft materials that best absorb impact forces in a crash. The aircraft included energy absorbing subfloors, similar to crumple zones in cars, which appeared to crush as intended to help protect the seats inside. The battery experiment involved adding mass to simulate underfloor battery components of air taxis to collect acceleration levels. Once analyzed, the team will share the data and insights with the public to enhance further research and development in this area. Lessons learned from these tests will help the advanced air mobility industry evaluate the crashworthiness of aircraft designs before flying over communities. The work is managed by the Revolutionary Vertical Lift Technology project under NASA’s Advanced Air Vehicles Program in support of NASA’s Advanced Air Mobility mission, which seeks to deliver data to guide the industry’s development of electric air taxis and drones. Share Details Last Updated Jul 28, 2025 EditorDede DiniusContactTeresa Whitingteresa.whiting@nasa.govLocationArmstrong Flight Research Center Related TermsArmstrong Flight Research CenterAdvanced Air MobilityAdvanced Air Vehicles ProgramAeronauticsAmes Research CenterDrones & YouGlenn Research CenterLangley Research CenterRevolutionary Vertical Lift Technology Explore More 3 min read NASA Rehearses How to Measure X-59’s Noise Levels Article 3 days ago 4 min read NASA Scientist Finds Predicted Companion Star to Betelgeuse Article 5 days ago 4 min read NASA Tests 5G-Based Aviation Network to Boost Air Taxi Connectivity Article 5 days ago Keep Exploring Discover More Topics From NASA Armstrong Flight Research Center Humans in Space Climate Change Solar System View the full article

NASA's SpaceX Crew-11 Launch

NASA's SpaceX Crew-11 Mission to the International Space Station (Official NASA Trailer)

The NASA/ESA Hubble Space Telescope image features the spiral galaxy NGC 3285B, a member of the Hydra I cluster of galaxies.ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz) The swirling spiral galaxy in this NASA/ESA Hubble Space Telescope image is NGC 3285B, which resides 137 million light-years away in the constellation Hydra (the Water Snake). Hydra has the largest area of the 88 constellations that cover the entire sky in a celestial patchwork. It’s also the longest constellation, stretching 100 degrees across the sky. It would take nearly 200 full moons, placed side by side, to reach from one side of the constellation to the other. NGC 3285B is a member of the Hydra I cluster, one of the largest galaxy clusters in the nearby universe. Galaxy clusters are collections of hundreds to thousands of galaxies bound to one another by gravity. The Hydra I cluster is anchored by two giant elliptical galaxies at its center. Each of these galaxies is about 150,000 light-years across, making them about 50% larger than our home galaxy, the Milky Way. NGC 3285B sits on the outskirts of its home cluster, far from the massive galaxies at the center. This galaxy drew Hubble’s attention because it hosted a Type Ia supernova in 2023. Type Ia supernovae happen when a type of condensed stellar core called a white dwarf detonates, igniting a sudden burst of nuclear fusion that briefly shines about 5 billion times brighter than the Sun. The supernova, named SN 2023xqm, is visible here as a blueish dot on the left edge of the galaxy’s disk. Hubble observed NGC 3285B as part of an observing program that targeted 100 Type Ia supernovae. By viewing each of these supernovae in ultraviolet, optical, and near-infrared light, researchers aim to disentangle the effects of distance and dust, both of which can make a supernova appear redder than it actually is. This program will help refine cosmic distance measurements that rely on observations of Type Ia supernovae. Text credit: ESA/Hubble View the full article

NISAR Launch

For Melissa John, protecting the environment is her way of contributing to space exploration while preserving the Earth we call home. As the sustainability program lead at NASA’s White Sands Test Facility in Las Cruces, New Mexico, John manages efforts to reduce waste, prevent pollution, and promote eco-conscious practices. Over the past 13 years, she has helped shape a workplace culture that values innovation and environmental responsibility. Official portrait of Melissa John. NASA/Brandon Teeples This is how I make a difference — by protecting the land, the community, and hopefully inspiring others to do the same. Melissa John Sustainability Program Lead Through awareness campaigns and outreach events, John empowers employees to be mindful of their environmental impact. Whether she is fostering grassroots connections, leading hands-on events, or recognizing colleagues who prioritize climate-aware actions, John remains dedicated to making a lasting, positive impact on the planet. John credits her Diné heritage and cultural values for fueling her passion to protect and preserve Earth for future generations. John began her NASA career at White Sands as a document specialist, reviewing schedules and environmental reports. She later transitioned into technical editing and gradually got involved in green initiatives, volunteering her time before eventually stepping into her current leadership role. Now, she coordinates a sitewide working group dedicated to reducing the facility’s environmental impact and inspires others to think critically about everyday actions and their ripple effects. Melissa John in the propulsion test area near the main water tank at NASA’s White Sands Test Facility in Las Cruces, New Mexico.NASA/Brandon Teeples John did not always know how she would make her mark. “Growing up, I remember a teacher asking how we could make a difference in the world,” she said. “I never forgot that question.” During the years she spent working in accounting and in the mining industry, she kept returning to that question. It was not until she joined NASA that she found her answer: “This — this is how I make my difference in the world.” The work also helped John grow in ways she did not expect. “I was painfully shy as a kid and terrified of speaking in front of a crowd,” she said. “But when I took on this role, I knew I had to find my voice. I still have timid moments, but the pride I feel in this work helps me push through. I’ve been through a lot, but I’m still here learning, growing, and showing up for the team I now call family.” John credits her strong support system for that transformation. “I am in awe of the women I’ve worked with,” she said. “I hope I can inspire others as they have inspired me.” From left to right: Mary Canavan, Melissa John, Amanda Skarsgard, and Pam Egan at the annual Plant Fair Share at White Sands Test Facility. Whether on Earth or beyond it, John believes that thoughtful action today leads to a brighter tomorrow. She is committed to leaving the world a better place for the next generation. Her legacy is simple: “Clean air, clean water, and clean land — that’s what I want to pass on.” Explore More 5 min read NASA Challenge Wraps, Student Teams Complete Space Suit Challenges Article 6 days ago 3 min read Catherine Staggs: Advancing Artemis Through Contracting Expertise Article 1 week ago 6 min read NASA Program Builds Bridge From Military to Civilian Careers for Johnson Team Members Article 2 weeks ago View the full article

NASA/Jonny Kim NASA and its partners have supported humans continuously living and working in space since November 2000. A truly global endeavor, the International Space Station has been visited by more than 280 people from 23 countries and a variety of international and commercial spacecraft. The unique microgravity laboratory has hosted more than 4,000 experiments from more than 5,000 researchers in more than 110 countries. The space station also is facilitating the growth of a commercial market in low Earth orbit for research, technology development, and crew and cargo transportation. NASA created a dedicated logo to symbolize this historic achievement. The logo is visible in the cupola of the space station in this July 17, 2025, image. The central astronaut figure is representative of all those who have lived and worked aboard the station during the 25 years of continuous human presence. In the dark sky of space surrounding the astronaut are 15 stars, which symbolize the 15 partner nations that support the orbiting laboratory. There is a visual representation of the space station toward the edge of the design, where humans have had a continuous presence for the past 25 years. The Earth represents the planet which the station orbits and that science conducted aboard the orbiting laboratory is for the benefit of all. Integrated into the border of the design is the number “25” to further represent the 25 years of human presence aboard the space station. After 25 years of continuous human presence, the space station remains a training and proving ground for deep space missions, enabling NASA to focus on Artemis missions to the Moon and Mars. For more information about the International Space Station, please visit https://www.nasa.gov/international-space-station/. Text credit: Kara Slaughter Image credit: NASA/Jonny Kim View the full article

A SpaceX Falcon 9 rocket, with the company’s Dragon spacecraft, stands in a vertical position at Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida on Tuesday, March 19, 2024.SpaceX Media accreditation is open for the next launch to deliver NASA science investigations, supplies, and equipment to the International Space Station. This launch is the 33rd SpaceX commercial resupply services mission to the orbital laboratory for NASA and will liftoff on the company’s Falcon 9 rocket. NASA and SpaceX are targeting no earlier than Thursday, Aug. 21, to launch the SpaceX Dragon spacecraft from Space Launch Complex-40 at Cape Canaveral Space Force Station in Florida. Credentialing to cover prelaunch and launch activities is open to U.S. media. The application deadline for U.S. citizens is 11:59 p.m. EDT, Sunday, Aug. 3. All accreditation requests must be submitted online at: https://media.ksc.nasa.gov Credentialed media will receive a confirmation email upon approval. NASA’s media accreditation policy is available online. For questions about accreditation, or to request special logistical support, email: ksc-media-accreditat@mail.nasa.gov. For other questions, please contact NASA’s Kennedy Space Center newsroom at: 321-867-2468. Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitor entrevistas en español, comuníquese con Antonia Jaramillo o Messod Bendayan a: antonia.jaramillobotero@nasa.gov o messod.c.bendayan@nasa.gov. Each resupply mission to the station delivers scientific investigations in the areas of biology and biotechnology, Earth and space science, physical sciences, and technology development and demonstrations. Cargo resupply from U.S. companies ensures a national capability to deliver scientific research to the space station, significantly increasing NASA’s ability to conduct new investigations aboard humanity’s laboratory in space. In addition to food, supplies, and equipment for the crew, Dragon will deliver several new experiments, including bone-forming stem cells for studying bone loss prevention and materials to 3D print medical implants that could advance treatments for nerve damage on Earth. Dragon also delivers bioprinted liver tissue to study blood vessel development in microgravity and supplies to 3D print metal cubes in space. For almost 25 years, humans have continuously lived and worked aboard the International Space Station, advancing scientific knowledge and demonstrating new technologies that enable us to prepare for human exploration of the Moon as we prepare for Mars. Learn more about NASA’s commercial resupply missions at: https://www.nasa.gov/station -end- Claire O’Shea Headquarters, Washington 202-358-1100 claire.a.o’shea@nasa.gov Stephanie Plucinsky / Steven Siceloff / Danielle Sempsrott Kennedy Space Center, Fla. 321-876-2468 stephanie.n.plucinsky@nasa.gov / steven.p.siceloff@nasa.gov / danielle.c.sempsrott@nasa.gov Sandra Jones Johnson Space Center, Houston 281-483-5111 sandra.p.jones@nasa.gov Share Details Last Updated Jul 25, 2025 LocationNASA Headquarters Related TermsInternational Space Station (ISS)Commercial Resupply View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA test pilot Nils Larson walks around an F-15B research aircraft for a rehearsal flight supporting the agency’s Quesst mission at NASA’s Armstrong Flight Research Center in Edwards, California. The flight was part of a full-scale dress rehearsal for Phase 2 of the mission, which will eventually measure quiet sonic thumps generated by the X-59. The flight series helped NASA teams refine procedures and practice data collection ahead of future X-59 flights.NASA/Christopher LC Clark In a stretch of California’s Mojave Desert, NASA conducted a full-scale “dress rehearsal” to prepare how it will measure the noise generated by the X-59 quiet supersonic research aircraft. The team behind the successful test flight series operates under NASA’s Commercial Supersonic Technology project. Beginning June 3 and concluding this week, researchers conducted a dry run for Phase 2 of NASA’s Quesst mission, when it will capture audio of the sonic thumps the X-59 will produce, rather than loud sonic booms associated with supersonic flight. “The dress rehearsal was critical for us,” said Larry Cliatt, sub-project manager for the Quesst acoustic validation phase, who is based at NASA’s Armstrong Flight Research Center in Edwards, California. “It gave us the opportunity to run through every aspect of our operation, from flight planning to data collection. In between those activities, we practiced aircraft operations, setting up the Ground Recording Systems, meteorological data collecting, and refining control room procedures. We were able to fine-tune our timelines, improve communication across teams, and ensure that when we perform these test with the X-59 aircraft, everything will run smoothly.” A NASA TG-14 glider aircraft is prepared for flight at NASA’s Armstrong Flight Research Center in Edwards, California, in support of the agency’s Quesst mission. The aircraft is equipped with onboard microphones to capture sonic boom noise generated during rehearsal flights, helping researchers measure the acoustic signature of supersonic aircraft closer to the ground.NASA/Jim Ross During the tests, at NASA Armstrong, an F-15B aircraft served as a stand-in for the X-59, flying faster than the speed of sound and making multiple passes over the Mojave sands. While it flew, researchers captured acoustic data using a linear array of ground recording systems spaced across miles of open desert, recorded weather readings, and measured the shock waves it generated. For a supersonic aircraft like the F-15B, shock waves typically result in loud sonic booms, but the X-59 is designed to diffuse them in a way that will dramatically limit noise. NASA’s Quesst mission aims to enable quiet supersonic flight over land using data from the X-59. The experimental aircraft will begin making its first flights this year – the first phase of Quesst. A NASA intern sets up ground recording system (GRS) units in California’s Mojave Desert during a Phase 2 rehearsal of the agency’s Quesst mission. The GRS units were placed across miles of desert terrain to capture the acoustic signature of supersonic aircraft during rehearsal flights and in preparation for the start of the actual tests.NASA/Christopher LC Clark But even before it takes to the air, the mission began its preparations for Phase 2 with the dry run, which focused on practicing under realistic test conditions and identifying issues before the official campaign begins, not collecting data from the F-15B. Through Quesst’s development of the X-59, NASA will deliver design tools and technology for quiet supersonic airliners that will achieve the high speeds desired by commercial operators without disturbing people on the ground. NASA will also validate design tools through ground and flight testing, providing aircraft manufacturers the ability to explore new quiet supersonic concepts and have confidence that their resulting designs will meet requirements for quiet flight. Most importantly, Quesst will gather data to understand community response to sounds generated during flight – key knowledge for a quiet supersonic future. Share Details Last Updated Jul 24, 2025 EditorDede DiniusContactNicolas Cholulanicolas.h.cholula@nasa.govLocationArmstrong Flight Research Center Related TermsArmstrong Flight Research CenterAdvanced Air Vehicles ProgramAeronautics Research Mission DirectorateAmes Research CenterCommercial Supersonic TechnologyGlenn Research CenterLangley Research CenterLow Boom Flight DemonstratorQuesst (X-59)Supersonic Flight Explore More 4 min read NASA Scientist Finds Predicted Companion Star to Betelgeuse Article 2 days ago 4 min read NASA Tests 5G-Based Aviation Network to Boost Air Taxi Connectivity Article 2 days ago 3 min read NASA Tests Mixed Reality Pilot Simulation in Vertical Motion Simulator Article 2 days ago Keep Exploring Discover More Topics From NASA Armstrong Flight Research Center Humans in Space Climate Change Solar System View the full article