NASA

NASA Astronaut Don Pettit Turns the Camera on Science

4 Min Read Science Meets Art: NASA Astronaut Don Pettit Turns the Camera on Science NASA astronaut Don Pettit is scheduled to return home in mid-April after a seven-month mission aboard the International Space Station as part of Expedition 72. Throughout his stay, Pettit contributed to research that benefits humanity and future space missions. Pettit also shared what he calls “science of opportunity” to demonstrate how experimenting with our surroundings can help gain a better understanding of how things work. This understanding is perhaps enhanced when art, science, and microgravity come together. Electrostatic Displays NASA astronaut Don Pettit demonstrates electrostatic forces using charged water droplets and a knitting needle made of Teflon. This series of overlapping frames displays the unique attraction-repulsion properties of Teflon and charged droplets, similar to how charged particles from the Sun behave when they come in contact with Earth’s magnetic field. Highly energetic particles from space that collide with atoms and molecules in the atmosphere create the aurora borealis. Specialized Equipment for Superb Science NASA astronaut Don Pettit snaps an image of the hands of NASA astronauts Nick Hague, left, and Suni Williams inside the Life Science Glovebox, a facility at the International Space Station that separates the science from the scientists, thus protecting both from contamination. The freezers on the International Space Station are as crucial as its experiment modules, preserving samples for further analysis on Earth. The Minus Eighty-Degree Laboratory Freezer for International Space Station stores samples at ultra-cold temperatures. NASA astronaut Don Pettit used it to freeze thin ice wafers, which he photographed with a polarizing filter to reveal unique crystal structures. New Tech Roll-Out NASA astronaut Don Pettit films a time-lapse sequence of Canadarm2 retrieving Materials International Space Station Experiment (MISSE-20-Commercial) samples at the International Space Station. This investigation exposed various experiments to the harsh space environment, such as vacuum, radiation, and extreme temperatures. Findings could help in many areas, from designing more durable materials to advancing quantum communications. A surge in International Space Station research supports NASA’s exploration efforts at the Moon and beyond, requiring more energy to operate the orbiting laboratory. NASA astronaut Don Pettit photographs new and old solar arrays side by side. The technology used by the International Space Station Roll-Out Solar Arrays (IROSA) on the right was first tested aboard the station in 2017. By 2023, six IROSAs were deployed aboard station, providing a 20-30% increase in power for research and operations. Roll-Out Solar Arrays were also used on NASA’s DART asteroid mission and now are slated for the Gateway lunar outpost, a vital component of Artemis. Squire for Spacewalks I am the nameless boy who stays in the confines of the tent helping the Knights suit up for battle. I remain in the airlock, preparing these knights for a walk outside. Don Pettit "Space Squire" posted to X NASA astronaut Don Pettit helped his colleagues suit up for two spacewalks in January. The first spacewalk involved patching the Neutron Star Interior Composition Explorer (NICER), a telescope that measures X-rays from neutron stars and other cosmic objects. Sunlight interference affected data collection, and the patches reduced this issue. On the second spacewalk, astronauts collected samples from the exterior of the International Space Station for ISS External Microorganisms. This investigation examines whether the orbiting laboratory releases microbes, how many, and how far these may travel. Findings could inform the design of future spacecraft, including spacesuits, to limit biocontamination during future space missions. Photography with a Spin NASA astronaut Don Pettit photographs “cosmic colors at sunrise.” From 250 miles above, the International Space Station’s orbital path covers most of Earth’s population, offering valuable data and a great opportunity for shooting breathtaking photography. NASA astronaut Don Pettit leveraged his stay aboard the International Space Station to photograph our planet with an artistic twist. NASA astronaut Don Pettit wrote on social media about his snapshot of the Mediterranean Sea from the International Space Station, “Sun glint off the Mediterranean Sea (infrared and converted to black and white). When the Sun reflects off the ocean, watery details unseen with normal lighting appear. Small centimeter differences in ocean height become visible, revealing hidden currents.” NASA astronaut Don Pettit’s photography could contribute to the study of transient luminous events, colorful electrical discharges that occur above thunderstorms. His imagery can be paired with data from the Atmosphere-Space Interactions Monitor (ASIM) and Thor-Davis, a high-speed thunderstorm camera. The combined efforts of crew photography and instruments aboard the International Space Station help scientists better understand thunderstorms and their impacts on Earth’s upper atmosphere. More of Pettit’s photography can be found on his X profile, @astro_Pettit. Share Details Last Updated Apr 17, 2025 Related TermsISS ResearchDonald R. PettitExpedition 72Humans in SpaceInternational Space Station (ISS) Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

NASA Astronaut Don Pettit Soyuz MS-26 Space Station Farewells and Hatch Closing

NASA Astronaut Don Pettit Soyuz MS-26 Re-entry and Landing

NASA Astronaut Don Pettit Soyuz MS-26 Undocking

Shahab ChaudhryCredit: NASA Shahab Chaudhry, chief of the Power and Propulsion Element (PPE) Project Office at NASA’s Glenn Research Center in Cleveland, has received a 2025 NASA Program and Project Management Excellence Award. He is one of just three recipients agencywide. The award recognizes individuals and teams who exemplify excellence in program and project management and the role it plays in helping NASA achieve its strategic goals. Chaudhry was honored for his leadership as the Power and Propulsion Element Project chief, working with industry partners to develop innovative solutions to address complex programmatic and technical challenges. The powerhouse for the Gateway space station, the Power and Propulsion Element will provide the lunar outpost with vital communication capabilities, power to keep its computer systems running, and propulsion to stay in its orbit around the Moon. Return to Newsletter Explore More 1 min read NASA Glenn and Cleveland Cavaliers Score With STEM Article 13 mins ago 3 min read Going Home: NASA Retires S-3B Viking to POW/MIA Museum Article 1 day ago 4 min read NASA Propellant Tech Could Fuel Long-Duration Missions Article 3 weeks ago View the full article

NASA’s Glenn Research Center supported Northeast Ohio STEM (NEOSTEM)’s annual Score with STEM event in collaboration with the Cleveland Cavaliers at Tower City Center in Cleveland on March 16.Credit: NASA/Jef Janis NASA’s Glenn Research Center supported Northeast Ohio STEM (NEOSTEM)’s annual Score with STEM event in collaboration with the Cleveland Cavaliers on March 16 at Tower City Center in Cleveland. More than 1,500 students, their families, and others gathered at Tower City’s Skylight Park for the event. NASA Glenn’s presence included virtual reality and augmented reality experiences, a wind tunnel demonstration, and information on NASA Glenn’s STEM opportunities, internships, and career paths. Eva the astronaut mascot also made appearances throughout the event, taking photos and interacting with participants. NASA Glenn Research Center’s Kyle Monaghan, left, and Michael Borghi, center left, simulate a test in a portable wind tunnel while showcasing the capabilities and importance of NASA Glenn’s wind tunnels during the Cleveland Cavalier’s Score with STEM event in downtown Cleveland.Credit: NASA/Jef Janis Back to Newsletter Explore More 1 min read Recognizing Employee Excellence Article 8 mins ago 2 min read NASA Glenn Accepts Aviation Award for “NEAT” Facility Article 1 month ago 1 min read NASA Glenn Experts Join Law College to Talk Human Spaceflight Article 1 month ago View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Piloted by NASA’s Tim Williams, the ER-2 science aircraft ascends for one of the final science flights for the GSFC Lidar Observation and Validation Experiment (GLOVE) on Feb. 1, 2025. As a collaboration between engineers, scientists, and aircraft professionals, GLOVE aims to improve satellite data products for Earth Science applications. NASA/Steve Freeman In February, NASA’s ER-2 science aircraft flew instruments designed to improve satellite data products and Earth science observations. From data collection to processing, satellite systems continue to advance, and NASA is exploring how instruments analyzing clouds can improve data measurement methods. Researchers participating in the Goddard Space Flight Center Lidar Observation and Validation Experiment (GLOVE) used the ER-2 – based at NASA’s Armstrong Flight Research Center in Edwards, California – to validate satellite data about cloud and airborne particles in the Earth’s atmosphere. Scientists are using GLOVE instruments installed onboard the aircraft to measure and validate data about clouds generated by satellite sensors already orbiting in space around Earth. “The GLOVE data will allow us to test new artificial intelligence algorithms in data processing,” said John Yorks, principal investigator for GLOVE and research physical scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “These algorithms aim to improve the cloud and aerosol detection in data produced by the satellites.” Jennifer Moore, a researcher from NASA’s Goddard Space Flight Center, checks the cabling on the Roscoe instrument at NASA’s Armstrong Flight Research Center in Edwards, California, for the GSFC Lidar Observation and Validation Experiment (GLOVE) on Feb. 1, 2025. The Roscoe instrument will be uploaded onto NASA’s ER-2 science aircraft.NASA/Steve Freeman The validation provided by GLOVE is crucial because it ensures the accuracy and reliability of satellite data. “The instruments on the plane provide a higher resolution measurement ‘truth’ to ensure the data is a true representation of the atmospheric scene being sampled,” Yorks said. The ER-2 flew over various parts of Oregon, Arizona, Utah, and Nevada, as well as over the Pacific Ocean off the coast of California. These regions reflected various types of atmospheres, including cirrus clouds, marine stratocumulus, rain and snow, and areas with multiple types of clouds. “The goal is to improve satellite data products for Earth science applications,” Yorks said. “These measurements allow scientists and decision-makers to confidently use this satellite information for applications like weather forecasting and hazard monitoring.” Researcher Jackson Begolka from the University of Iowa examines instrument connectors onboard the ER-2 aircraft at NASA’s Armstrong Flight Research Center in Edwards, California, on Feb. 1, 2025. The GLOVE instrument will validate data from satellites orbiting the Earth.NASA/Steve Freeman The four instruments installed on the ER-2 were the Cloud Physics Lidar, the Roscoe Lidar, the enhanced Moderate Resolution Imaging Spectroradiometer Airborne Simulator, and the Cloud Radar System. These instruments validate data produced by sensors on NASA’s Ice, Cloud, and Land Elevation Satellite 2 (ICESat-2) and the Earth Cloud, Aerosol and Radiation Explorer (EarthCARE), a joint venture between the ESA (European Space Agency) and JAXA (Japan Aerospace Exploration Agency). “Additionally, the EarthCARE satellite is flying the first ever Doppler radar for measurements of air motions within clouds,” Yorks said. While the ER-2 is operated by pilots and aircrew from NASA Armstrong, these instruments are supported by scientists from NASA Goddard, NASA’s Ames Research Center in California’s Silicon Valley, and the Naval Research Laboratory office in Monterey, California, as well as by students from the University of Iowa in Iowa City and the University of Maryland College Park. Share Details Last Updated Apr 16, 2025 EditorDede DiniusContactErica HeimLocationArmstrong Flight Research Center Related TermsArmstrong Flight Research CenterAirborne ScienceEarth ScienceEarth Science Technology OfficeEarth's AtmosphereER-2Goddard Space Flight Center Explore More 4 min read Hubble Provides New View of Galactic Favorite As part of ESA/Hubble’s 35th anniversary celebrations, the European Space Agency (ESA) is sharing a new… Article 9 hours ago 4 min read NASA Aims to Fly First Quantum Sensor for Gravity Measurements Researchers from NASA’s Jet Propulsion Laboratory in Southern California, private companies, and academic institutions are… Article 1 day ago 5 min read Can Solar Wind Make Water on Moon? NASA Experiment Shows Maybe Scientists have hypothesized since the 1960s that the Sun is a source of ingredients that… Article 1 day ago Keep Exploring Discover More Topics From NASA Armstrong Flight Research Center Humans in Space Climate Change Solar System View the full article

NASA and SpaceX are targeting no earlier than 4:15 a.m. EDT on Monday, April 21, for the next launch to deliver scientific investigations, supplies, and equipment to the International Space Station. Filled with about 6,700 pounds of supplies, the SpaceX Dragon spacecraft, on the company’s Falcon 9 rocket, will lift off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. This launch is the 32nd SpaceX commercial resupply services mission to the orbital laboratory for the agency, and the 12th SpaceX launch under the Commercial Resupply Services-2 (CRS) contract. The first 20 launches were under the original resupply services contract. NASA’s live launch coverage will begin at 3:55 a.m. on NASA+. Learn how to watch NASA content through a variety of platforms. NASA’s SpaceX 32nd commercial resupply mission will launch on the company’s Dragon spacecraft on the SpaceX Falcon 9 rocket to deliver research and supplies to the International Space StationNASA NASA’s SpaceX 32nd commercial resupply mission will launch from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. Arrival & Departure The SpaceX Dragon spacecraft will arrive at the space station and dock autonomously to the zenith port of the station’s Harmony module at approximately 8:20 a.m. Tuesday, April 22. Live coverage NASA’s coverage of the rendezvous and docking will begin at 6:45 a.m on NASA+. NASA astronaut Jonny Kim, Expedition 73 commander and JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi will monitor the arrival of the spacecraft, which will stay docked to the orbiting laboratory for about one month before splashing down and returning critical science and hardware to teams on Earth. Astronauts Jonny Kim of NASA and Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) will monitor the arrival of the SpaceX Dragon cargo spacecraft from the International Space Station.NASA Research Highlights Robotic Spacecraft Guidance Smartphone Video Guidance Sensor-2 (SVGS-2) uses the space station’s Astrobee robots to demonstrate using a NASA developed, vision-based sensor to control a formation flight of small satellites.NASA Smartphone Video Guidance Sensor-2 (SVGS-2) uses the space station’s Astrobee robots to demonstrate using a NASA developed, vision-based sensor to control a formation flight of small satellites. Based on a previous in-space demonstration of the technology, this investigation is designed to refine the maneuvers of multiple robots and integrate the information with spacecraft systems. Potential benefits of this technology include improved accuracy and reliability of systems for guidance, navigation, and control that could be applied to docking crewed spacecraft in orbit and remotely operating multiple robots on the lunar or Martian surface. Protection From Particles The Aerosol Monitors investigation tests three different air quality monitors to determine which is best suited to protect crew health and ensure mission success. NASA During spaceflight, especially long-duration missions, concentrations of airborne particles must be kept within ranges safe for crew health and hardware performance. The Aerosol Monitors investigation tests three different air quality monitors to determine which is best suited to protect crew health and ensure mission success. The investigation also tests a device for distinguishing between smoke and dust. Aboard the orbital outpost, the presence of dust can cause false smoke alarms that require crew member response. Reducing false alarms could save valuable crew time while continuing to protect astronaut safety. Next-Generation Pharmaceutical Nanostructures The newest Industrial Crystallization Cassette (ADSEP-ICC) investigation adds capabilities to an existing protein crystallization facility. NASA The newest Industrial Crystallization Cassette (ADSEP-ICC) investigation adds capabilities to an existing protein crystallization facility. The cassette can process more sample types, including tiny gold particles used in devices that detect cancer and other diseases or in targeted drug delivery systems. Microgravity makes it possible to produce larger and more uniform gold particles, which improves their use in research and real-life applications of technologies related to human health. Better Materials, Better Drugs The DNA Nano Therapeutics-Mission 2 produces a special type of molecule formed by DNA-inspired, customizable building blocks known as Janus base nanomaterials.NASA The DNA Nano Therapeutics-Mission 2 produces a special type of molecule formed by DNA-inspired, customizable building blocks known as Janus base nanomaterials. It also evaluates how well the materials reduce joint inflammation and whether they can help regenerate cartilage lost due to arthritis. These materials are less toxic, more stable, and more compatible with living tissues than current drug delivery technologies. Environmental influences such as gravity can affect the quality of these materials and delivery systems. In microgravity, they are larger and have greater uniformity and structural integrity. This investigation could help identify the best formulations and methods for cost-effective in-space production. These nanomaterials also could be used to create novel systems targeting therapy delivery that improves patient outcomes with fewer side effects. Helping Plants Grow The Rhodium USAFA NIGHT payload examines how tomato plants respond to microgravity and whether a carbon dioxide replacement can reduce how much space-grown plants depend on photosynthesis.NASA The Rhodium USAFA NIGHT payload examines how tomato plants respond to microgravity and whether a carbon dioxide replacement can reduce how much space-grown plants depend on photosynthesis. Because photosynthesis needs light, which requires spacecraft power to generate, alternatives would reduce energy use. The investigation also examines whether using supplements increases plant growth on the space station, which has been observed in preflight testing on Earth. In future plant production facilities aboard spacecraft or on celestial bodies, supplements could come from available organic materials such as waste. Understanding how plants adapt to microgravity could help grow food during long-duration space missions or harsh environments on Earth. Atomic Clocks in Space An ESA (European Space Agency) investigation, Atomic Clock Ensemble in Space (ACES), examines fundamental physics concepts such as Einstein’s theory of relativity using two next-generation atomic clocks operated in microgravity.NASA An ESA (European Space Agency) investigation, Atomic Clock Ensemble in Space (ACES), examines fundamental physics concepts such as Einstein’s theory of relativity using two next-generation atomic clocks operated in microgravity. Results have applications to scientific measurement studies, the search for dark matter, and fundamental physics research that relies on highly accurate atomic clocks in space. The experiment also tests a technology for synchronizing clocks worldwide using global navigation satellite networks. Cargo Highlights NASA’s SpaceX 32nd commercial resupply mission will carry about 6,700 pounds of cargo to the International Space Station.NASA Hardware Launch: Catalytic Reactor – The catalytic reactor replacement unit oxidizes volatile organics from the wastewater so they can be removed by the gas separator and ion exchange bed replacement units as part of the station’s water recycling system. This unit failed in orbit and is being returned for analysis and refurbishment. This unit is being launched as an in-orbit spare. Food Reach Tool Assembly – An L-shaped, hand-held tool that allows crew members to reach packages in the back of the food warmer without having to insert their hands. This tool is launching to replace a unit in orbit. Reducer Cylinder Assembly – A cylinder tank that provides 15 minutes of oxygen to a crew member in case of an emergency. Launching two units as in-orbit spares. Thermal Expansion Device – A device used to allow for thermal expansion of water within the Hydrogen Dome while it is being removed and replaced. Launching to maintain minimum in-orbit spares. Return: Urine Processor Assembly Pressure Control and Pump Assembly – This multi-tube purge pump enables the removal of non-condensable gas and water vapor from the distillation assembly within the greater urine processing assembly subsystem. This unit is returning to the ground for repair and refurbishment in support of the legacy environmental control and life support system fleet. Assembly Contingency Transmitter Receiver Assembly – A part of the S-Band Radio Frequency Group, this assembly is a pressurized enclosure that contains electronics for this upper-level assembly. The Radio Frequency Group is used for command, control, and transmission communication for the space station. It was retrieved by NASA astronauts Suni Williams and Butch Wilmore during US EVA 92 and will return for repair. High Gain Antenna Feed Assembly – Part of the S-Band Radio Frequency Group, this system features a two-axis, gimballed assembly with a pedestal and a large horn antenna. It was retrieved by NASA astronauts Suni Williams and Butch Wilmore during U.S. spacewalk 92 and will return for repair. Low Gain Antenna Sub-Assembly – Part of the S-Band Radio Frequency Group, this sub-assembly consists of a helix antenna that provides a wide field of signal transmission capability. It was retrieved by NASA astronauts Suni Williams and Butch Wilmore during U.S. spacewalk 92 and will return for repair. Planar Reflector Assembly – With an aluminum base and reflective element, visiting spacecraft reflect a laser to compute relative range, velocity, and attitude to the space station. This broken unit was retrieved and replaced by NASA astronaut Suni Williams during U.S. spacewalk 91 and will return for repair. Multifiltration Bed – Supporting the water processor assembly, this spare unit will continue the International Space Station program’s effort to replace a degraded fleet of units in-orbit that improve water quality through a single bed. This unit will return for refurbishment and re-flight. Watch and Engage Live coverage of the launch from NASA Kennedy will air at 3:55 a.m. on NASA+.. For additional information on the mission, visit: https://www.nasa.gov/mission/nasas-spacex-crs-32/ View the full article

NASA/Ben Smegelsky A scrub jay perches on a branch near the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on June 22, 2020. Kennedy shares space with the Merritt Island National Wildlife Refuge, which is home to more than 65 amphibian and reptile, 25 mammal, 117 fish, and 330 bird species. At the time this photo was taken, the NASA “meatball” logo – in the background here – on the Vehicle Assembly Building was being repainted. This iconic building is where the Artemis launch vehicles are stacked and processed in preparation for future missions to the Moon. Image credit: NASA/Ben Smegelsky View the full article

6 Min Read NASA’s Chandra Releases New 3D Models of Cosmic Objects New three-dimensional (3D) models of objects in space have been released by NASA’s Chandra X-ray Observatory. These 3D models allow people to explore — and print — examples of stars in the early and end stages of their lives. They also provide scientists with new avenues to investigate scientific questions and find insights about the objects they represent. These 3D models are based on state-of-the-art theoretical models, computational algorithms, and observations from space-based telescopes like Chandra that give us accurate pictures of these cosmic objects and how they evolve over time. However, looking at images and animations is not the only way to experience this data. The four new 3D printable models of Cassiopeia A (Cas A), G292.0+1.8 (G292), Cygnus Loop supernova remnants, and the star known as BP Tau let us experience the celestial objects in the form of physical structures that will allow anyone to hold replicas of these stars and their surroundings and examine them from all angles. Cassiopeia A (Cas A) Using NASA’s James Webb Space Telescope, astronomers uncovered a mysterious feature within the remnant, nicknamed the “Green Monster,” alongside a puzzling network of ejecta filaments forming a web of oxygen-rich material. When combined with X-rays from Chandra, the data helped astronomers shed light on the origin of the Green Monster and revealed new insights into the explosion that created Cas A about 340 years ago, from Earth’s perspective. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video 3D Model of Cassiopeia A "Green Monster" INAF-Osservatorio Astronomico di Palermo/Salvatore Orlando To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video 3D Model of Cassiopeia AINAF-Osservatorio Astronomico di Palermo/Salvatore Orlando BP Tau X-ray: NASA/CXC/SAO; Optical: PanSTARRS; Image Processing: NASA/CXC/SAO/N. Wolk This 3D model shows a star less than 10 million years old that is surrounded by a disk of material. This class of objects is known as T Tauri stars, named after a young star in the Taurus star-forming region. The model describes the effects of multiple flares, or outbursts that are detected in X-rays by Chandra from one T Tauri star known as BP Tau. These flares interact with the disk of material and lead to the formation of an extended outer atmosphere composed by hot loops, connecting the disk to the developing star. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video 3D Model of BP TauINAF-Osservatorio Astronomico di Palermo/Salvatore Orlando Cygnus Loop X-ray: NASA/SAO/CXC; Optical: John Stone (Astrobin); Image Processing: NASA/SAO/CXC/L. Frattre, N. Wolk The Cygnus Loop (also known as the Veil Nebula) is a supernova remnant, the remains of the explosive death of a massive star. This 3D model is the result of a simulation describing the interaction of a blast wave from the explosion with an isolated cloud of the interstellar medium (that is, dust and gas in between the stars). Chandra sees the blast wave and other material that has been heated to millions of degrees. The Cygnus Loop is a highly extended, but faint, structure on the sky: At three degrees across, it has the diameter of six full moons. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video 3D Model of Cygnus LoopINAF-Osservatorio Astronomico di Palermo/Salvatore Orlando G292.0+1.8 X-ray: NASA/CXC/SAO; Optical:NSF/NASA/DSS; Image Processing This is a rare type of supernova remnant observed to contain large amounts of oxygen. The X-ray image of G292.0+1.8 from Chandra shows a rapidly expanding, intricately structured field left behind by the shattered star. By creating a 3D model of the system, astronomers have been able to examine the asymmetrical shape of the remnant that can be explained by a “reverse” shock wave moving back toward the original explosion. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video 3D Model of G292.0+1.8INAF-Osservatorio Astronomico di Palermo/Salvatore Orlando The 3D models here are the subject of several scholarly papers by Salvatore Orlando of INAF in Palermo, Italy, and colleagues published in The Astrophysical Journal, Astronomy & Astrophysics, and Monthly Notices of the Royal Astronomical Society. Much of this work is also publicly available work on SketchFab. NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts. Read more from NASA’s Chandra X-ray Observatory. Learn more about the Chandra X-ray Observatory and its mission here: https://www.nasa.gov/chandra https://chandra.si.edu Visual Description This release features visualizations of three supernova remnants and one star. Each is rendered as a composite image, and as a digital 3-dimensional model, presented in separate short video clips. The composite images are two dimensional and static, but the digital models rotate, showcasing their three-dimensionality. The first featured supernova is Cassiopeia A. In the X-ray, optical, and infrared composite image, the debris from an exploded star resembles a round purple gas cloud, marbled with streaks of golden light. In the rotating, 3D model, the purple gas cloud is depicted as a flat disk, like a record or CD. Bursting out the front and back of the disk is an orange and white shape similar to a ball of coral, or a head of cauliflower lined with stubby tendrils. Most of the ball, and the majority of the tendrils, appear on one side of the disk. On the opposite side, the shape resembles dollops of thick whipped cream. Next in the release is a star known as BP Tau. BP Tau is a developing star, less than 10 million years old, and prone to outbursts or flares. These flares interact with a disk of material that surrounds the young star, forming hot loops of extended atmosphere. In the composite image, BP Tau resembles a distant, glowing white dot surrounded by a band of pink light. The rotating, 3D model is far more dynamic and intriguing! Here, the disk of material resembles a large blue puck with round, ringed, concave surfaces. At the heart of the puck is a small, glowing red orb: the developing star. Shooting out of the orb are long, thin, green strands: the flares. Also emerging from the orb are orange and pink petal-shaped blobs: the loops of extended atmosphere. Together, the orb, strands, and petals resemble an exotic flowering orchid. The third celestial object in this release is the supernova remnant called Cygnus Loop. In the composite image, the remnant resembles a wispy cloud in oranges, blues, purples, and whites, shaped like a backwards letter C. The 3D model examines this cloud of interstellar material interacting with the superheated, supernova blast wave. In the 3D model, the Cygnus Loop resembles a bowl with a thick base, and a wedge cut from the side like a slice of pie. The sides of the bowl are rendered in swirled blues and greens. However, inside the thick base, revealed by the wedge-shaped cut, are streaks of red and orange. Surrounding the shape are roughly parallel thin red strands, which extend beyond the top and bottom of the digital model. The final supernova featured in this release is G292.0+1.8. The composite image depicts the remnant as a bright and intricate ball of red, blue, and white X-ray gas and debris set against a backdrop of gleaming stars. In the 3D model, the remnant is rendered in translucent icy blue and shades of orange. Here, the rotating shape is revealed to be somewhat like a bulbous arrowhead, or perhaps an iceberg on its side. News Media Contact Megan Watzke Chandra X-ray Center Cambridge, Mass. 617-496-7998 mwatzke@cfa.harvard.edu Lane Figueroa Marshall Space Flight Center, Huntsville, Alabama 256-544-0034 lane.e.figueroa@nasa.gov About the AuthorLee Mohon Share Details Last Updated Apr 16, 2025 Related TermsChandra X-Ray ObservatoryAstrophysicsGeneralMarshall AstrophysicsMarshall Space Flight CenterSupernova RemnantsThe Universe Explore More 4 min read Hubble Provides New View of Galactic Favorite As part of ESA/Hubble’s 35th anniversary celebrations, the European Space Agency (ESA) is sharing a new… Article 5 hours ago 3 min read NASA Sees Progress on Blue Origin’s Orbital Reef Design Development Article 6 hours ago 1 min read Why Do We Grow Plants in Space? Article 1 day ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

Planetary Defenders (NASA+ Original)

2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) The SpaceX Falcon 9 rocket carrying the Dragon spacecraft lifts off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida on Thursday, Nov. 9, 2023, on the company’s 29th commercial resupply services mission for the agency to the International Space Station.SpaceX NASA invites the public to participate in virtual activities ahead of the launch of SpaceX’s 32nd commercial resupply services mission for the agency. NASA and SpaceX are targeting launch at 4:15 a.m. EDT Monday, April 21, from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. In addition to food, supplies, and equipment for the crew, the SpaceX Dragon spacecraft will deliver several new experiments, including a demonstration of refined maneuvers for free-floating robots. Dragon also carries an enhanced air quality monitoring system that could protect crew members on exploration missions to the Moon and Mars, and two atomic clocks to examine fundamental physics concepts, such as relativity, and test worldwide synchronization of precision timepieces. The public can register to be virtual launch guests and receive curated mission resources, interactive opportunities, timely launch updates, and a mission-specific collectible stamp for their virtual guest passports delivered straight to their inbox after liftoff. A new way to collect and share passport stamps has arrived! Receive one for your virtual guest passport and another that is sized perfectly for sharing. Don’t have a passport yet? Print one here and start collecting! Learn more about NASA research and activities on the International Space Station at: https://www.nasa.gov/station. Share Details Last Updated Apr 16, 2025 EditorJason Costa Related TermsKennedy Space CenterCommercial ResupplyGet InvolvedInternational Space Station (ISS)ISS ResearchSpaceX Commercial ResupplyVirtual Guest Program Explore More 4 min read Atomic Clock and Plant DNA Research Launching Aboard NASA’s SpaceX CRS-32 Mission NASA’s SpaceX 32nd commercial resupply services mission, scheduled to lift off from the agency’s Kennedy… Article 1 day ago 1 min read Why Do We Grow Plants in Space? Article 1 day ago 4 min read GLOBE Mission Earth Supports Career Technical Education The NASA Science Activation program’s GLOBE Mission EARTH (GME) project is forging powerful connections between… Article 5 days ago Keep Exploring Discover Related Topics NASA’s SpaceX Crew-10 The 11th flight of the Dragon spacecraft with people as part of NASA's Commercial Crew Program launched March 14, 2025,… International Space Station (ISS) (A) The Ocean and Climate Change Our ocean is changing. With 70 percent of the planet covered in water, the seas are important drivers of the… Our Solar System Overview Our planetary system is located in an outer spiral arm of the Milky Way galaxy. We call it the… 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 Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 4 Min Read Hubble Provides New View of Galactic Favorite NASA/ESA Hubble Space Telescope image of the Sombrero Galaxy, also called Messier 104. Credits: ESA/Hubble & NASA, K. Noll As part of ESA/Hubble’s 35th anniversary celebrations, the European Space Agency (ESA) is sharing a new image series revisiting stunning, previously released Hubble targets with the addition of the latest Hubble data and new processing techniques. ESA/Hubble published a new image of NGC 346 as the first installment in the series. Now, they are revisiting a fan-favorite galaxy with new image processing techniques. The new image reveals finer detail in the galaxy’s disk, as well as more background stars and galaxies. Over the past two decades, Hubble has released several images of the Sombrero Galaxy, including this well-known Hubble image from October 2003. In November 2024, the NASA/ESA/CSA James Webb Space Telescope also provided an entirely new perspective on this striking galaxy. Located around 30 million light-years away in the constellation Virgo, the Sombrero Galaxy is instantly recognizable. Viewed nearly edge on, the galaxy’s softly luminous bulge and sharply outlined disk resemble the rounded crown and broad brim of the Mexican hat from which the galaxy gets its name. NASA/ESA Hubble Space Telescope image of the Sombrero Galaxy, also called Messier 104. ESA/Hubble & NASA, K. Noll Though packed with stars, the Sombrero Galaxy is surprisingly not a hotbed of star formation. Less than one solar mass of gas is converted into stars within the knotted, dusty disk of the galaxy each year. Even the galaxy’s central supermassive black hole, which at nine billion solar masses is more than 2,000 times more massive than the Milky Way’s central black hole, is fairly calm. The galaxy is too faint to spot with the unaided eye, but it is readily viewable with a modest amateur telescope. Seen from Earth, the galaxy spans a distance equivalent to roughly one-third the diameter of the full Moon. The galaxy’s size on the sky is too large to fit within Hubble’s narrow field of view, so this image is actually a mosaic of several images stitched together. One of the things that makes this galaxy especially notable is its viewing angle, which is inclined just six degrees off of the galaxy’s equator. From this vantage point, intricate clumps and strands of dust stand out against the brilliant white galactic nucleus and bulge, creating an effect not unlike Saturn and its rings — but on an epic galactic scale. At the same time, this extreme angle makes it difficult to discern the structure of the Sombrero Galaxy. It’s not clear whether it’s a spiral galaxy, like our own Milky Way, or an elliptical galaxy. Curiously, the galaxy’s disk seems like a fairly typical disk for a spiral galaxy, and its spheroidal bulge and halo seem fairly typical for an elliptical galaxy — but the combination of the two components resembles neither a spiral nor an elliptical galaxy. Researchers used Hubble to investigate the Sombrero Galaxy, measuring the metals (what astronomers call elements heavier than helium) in stars in the galaxy’s expansive halo. This type of measurement can help astronomers better understand a galaxy’s history, potentially revealing whether it merged with other galaxies in the past. In the case of the Sombrero Galaxy, extremely metal-rich stars in the halo point to a possible merger with a massive galaxy several billion years ago. An ancient galactic clash, hinted at by Hubble’s sensitive measurements, could explain the Sombrero Galaxy’s distinctive appearance. The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA. Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Explore Hubble Sombrero Galaxy Images and Science Sombrero Galaxy Learn more about and download the image above. Hubble’s Messier Catalog: M104 (Sombrero Galaxy) Hubble easily resolves some of the Sombrero Galaxy’s roughly 2,000 globular clusters. Beyond the Brim, Sombrero Galaxy’s Halo Suggests Turbulent Past Surprising new data from NASA’s Hubble Space Telescope suggests the smooth, settled “brim” of the Sombrero galaxy’s disk may be concealing a turbulent past. Heritage Project Celebrates Five Years of Harvesting the Best Images from Hubble Space Telescope The Hubble Heritage Project released more than 65 images of dazzling celestial objects, including planets, dying stars, regions of star formation, clusters of stars, individual galaxies, and even clusters of galaxies. Share Details Last Updated Apr 16, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Contact Media Claire Andreoli NASA’s Goddard Space Flight Center Greenbelt, Maryland claire.andreoli@nasa.gov Bethany Downer ESA/Hubble bethany.downer@esahubble.org Garching, Germany Related Terms Hubble Space Telescope Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center The Universe Related Links and Documents Hubble’s 35th Anniversary celebrations ESA/Hubble’s 35th Anniversary celebrations Release on ESA’s website 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. Galaxy Details and Mergers Hubble’s Galaxies Hubble’s 35th Anniversary View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) A digital rendering of the baseline configuration for Blue Origin’s free-flying commercial space station, Orbital Reef, which continues to be developed as part of a Space Act Agreement with NASA.Blue Origin A NASA-supported commercial space station, Blue Origin’s Orbital Reef, recently completed a human-in-the-loop testing milestone as the agency works toward developing commercial space stations in low Earth orbit. The human-in-the-loop test scenarios utilized individual participants or small groups to perform day-in-the-life walkthroughs in life-sized mockups of major station components. Participants provided feedback while simulating microgravity operations, including cargo transfer, trash transfer, stowage, and worksite assessments. “Human-in-the-loop and iterative testing are essential to inform key decisions and mitigate risks to crew health and safety,” said Angela Hart, program manager for NASA’s Commercial Low Earth Orbit Development Program at the agency’s Johnson Space Center in Houston. “NASA’s insight into our partner’s testing milestones enables the agency to gain insight into partner progress and share expertise, ultimately improving industry and NASA’s mission success.” Test subjects in the mockup for Blue Origin’s free-flying commercial space station, Orbital Reef, during the human-in-the-loop test.Blue Origin The milestone is part of a NASA Space Act Agreement originally awarded to Blue Origin in 2021 and focused on the design progress for multiple worksites, floors, and translation paths within the station. This ensures a commercial station can support human life, which is critical to advancing scientific research in a microgravity environment and maintaining a continuous human presence in low Earth orbit. The test evaluated various aspects of Orbital Reef’s environment to provide information needed for the space station’s design. Assessment areas included the private crew quarters, dining area, lavatory, research laboratory, and berthing and docking hatches. To facilitate the test, Blue Origin built stand-alone mockups of each floor in the internally developed habitable module. These mockups will be iteratively updated as the fidelity of components and subsystems matures, enabling future human-in-the-loop testing. The research team’s observations will be used to provide design recommendations for worksite volumes, layouts, restraint and mobility aid layouts, usability and workload, and positioning of interfaces and equipment. NASA supports the design and development of multiple commercial space stations, including Orbital Reef, through funded and unfunded agreements. The current design and development phase will soon be followed by the procurement of services from one or more companies, where NASA aims to be one of many customers for low Earth orbit stations. NASA is committed to maintaining a continuous human presence in low Earth orbit as the agency transitions from the International Space Station to commercial space stations. For nearly 25 years, NASA has supported a continuous presence in low Earth orbit aboard the space station and will continue to build on the agency’s extensive human spaceflight experience to advance future scientific and exploration goals. For more information about commercial space stations, visit: www.nasa.gov/commercialspacestations A test subject in the mockup for Blue Origin’s free-flying commercial space station, Orbital Reef, during the human-in-the-loop test.Blue Origin Keep Exploring Discover More Topics Low Earth Orbit Economy Commercial Space Commercial Crew Program Humans In Space View the full article

This S-3 supported vital flight research by donating parts to its sister plane, another S3-B Viking that was retired in 2021.Credit: NASA/Jordan Cochran After supporting the center’s research missions for more than a decade, NASA’s S-3B Viking aircraft is moving on from NASA’s Glenn Research Center in Cleveland to begin a new and honorable assignment. The aircraft is heading to the National POW/MIA Memorial and Museum in Jacksonville, Florida, where it will be on display, honoring all Prisoners of War (POW), those Missing in Action (MIA), and the families who seek the return of their loved ones. The museum gives visitors a place of solace to reflect, learn, and hear stories about America’s POW and MIA service members through exhibits and events. A team of volunteers, many of whom are veterans, converged to disassemble an S-3B Viking at NASA’s Glenn Research Center in Cleveland so it could be transported by truck to the National Pow/MIA Memorial and Museum in Jacksonville, Florida. Credit: NASA/Lillianne Hammel “We are honored to be part of it,” said JD Demers, chief of Aircraft Operations at NASA Glenn. “Moving the S-3 is a win-win for everybody. The museum gets an aircraft in beautiful shape, and our S-3 gets to continue living a meaningful life.” Originally designed by Lockheed Martin as an anti-submarine warfare aircraft, NASA’s S-3B Viking will travel south to its new museum home, which is located at the former Naval Air Station Cecil Field where S-3B Vikings once flew. It will be displayed with a plaque recognizing the 54 service members who perished during S-3 flight missions. NASA’s JD Demers poses with National POW/MIA Memorial and Museum’s Ed Turner in front of NASA’s S-3B Viking aircraft. Credit: NASA/Jordan Cochran “It’s really fortunate for us that this S-3 has such a well-kept, beautiful airframe that we can use as part of this plaza,” said Ed Turner, executive director of the National POW/MIA Memorial and Museum. “Cecil Field was the East Coast home for the S-3B Vikings, so we are proud to have it for display here as one of Cecil’s legacy aircraft.” Behind the scenes, this S-3 supported vital NASA flight research by donating parts to its sister plane, another S3-B Viking that was retired in 2021. Through the donation of its parts, the S-3 contributed to communications research in advanced air mobility and monitoring of algal bloom growth in Lake Erie. “Having this aircraft added an extra 10 years of life to its sister plane,” Demers said. “Those 10 years were vital for research. This plane allowed us to keep flying that aircraft after the Navy retired the S-3B Vikings in 2009. We wouldn’t have been able to find parts.” NASA prepares its S-3B Viking for its journey to the National POW/MIA Memorial and Museum in Jacksonville, Florida.Credit: NASA/Sara Lowthian-Hanna The U.S. Navy flew S-3 Vikings primarily out of three locations: North Island Naval Air Station, Naval Air Station Cecil Field, and Naval Air Station Jacksonville. There were S-3B Vikings in all locations except Jacksonville, until now. “There are three bases in three locations that used to fly S-3s, and now each area has an S-3 as part of its display,” Demers said. “It belongs there. It’s going back to its original home.” Explore More 3 min read NASA Supports Wildland Fire Technology Demonstration Article 2 weeks ago 4 min read NASA Makes Progress on Advanced Drone Safety Management System Article 2 weeks ago 5 min read NASA History News and Notes–Spring 2025 Article 2 weeks ago 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 Sols 4511-4512: Low energy after a big weekend? This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4510 (2025-04-14 03:43:40 UTC). NASA/JPL-Caltech Written by Lauren Edgar, Planetary Geologist at USGS Astrogeology Science Center Earth planning date: Monday, April 14, 2025 We all know the feeling: it’s Monday morning after a big weekend and you’re coming into the week wishing you’d had a little more time to rest and recharge. Well, Curiosity probably feels the same way today. Curiosity accomplished a lot over the weekend, including full contact science, a MAHLI stereo imaging test, testing the collection of ChemCam passive spectral data at the same time as data transmission with one of the orbiters, and some APXS and MAHLI calibration target activities, plus a long 57 m drive. It was great to see all of those activities in the plan and to see some great drive progress. But that means we’re a bit tight on power for today’s plan! I was on shift as Long Term Planner today, and the team had to think carefully about science priorities to fit within our power limit for today’s plan, and how that will prepare us for the rest of the week. The team still managed to squeeze a lot of activities into today’s 2-sol plan. First, Curiosity will acquire Mastcam mosaics to investigate local stratigraphic relationships and diagenetic features. Then we’ll acquire some imaging to document the sandy troughs between bedrock blocks to monitor active surface processes. We’ll also take a Navcam mosaic to assess atmospheric dust. The science block includes a ChemCam LIBS observation on the bedrock target “Santa Margarita” and a long distance RMI mosaic of “Ghost Mountain” to look for possible boxwork structures. Then Curiosity will use the DRT, APXS and MAHLI to investigate the finely-laminated bedrock in our workspace at a target named “The Grotto.” We’ll also collect APXS and MAHLI data on a large nodule in the workspace named “Torrey Pines” (meanwhile the Torrey Pines here on Earth was shaking in today’s southern California earthquakes! All is well but it gave some of our team members an extra jolt of adrenaline right before the SOWG meeting). The second sol is focused on continuing our drive to the south and taking post-drive imaging to prepare for Wednesday’s plan. Phew! Good job Curiosity, you made it through Monday. Explore More 3 min read Sols 4509-4510: A weekend of long drives Article 38 mins ago 2 min read Sols 4507-4508: “Just Keep Driving” Article 4 days ago 3 min read Sols 4505-4506: Up, up and onto the Devil’s Gate Article 1 week ago Keep Exploring Discover More Topics From NASA Mars Resources Explore this page for a curated collection of Mars resources. 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… The Mars Report The Mars Report newsletter from NASA is your source for everything on or about the Red Planet. We bring you… 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 Sols 4509-4510: A weekend of long drives This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4507 (2025-04-11 03:54:35 UTC). Written by Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory Earth planning date: Friday, April 11, 2025 Curiosity is continuing to book it to the potential boxwork structures. The rover drove over 50 meters on Wednesday, and we plan to drive more than 50 meters again in today’s plan thanks to an unusually good viewshed that allows us to see far ahead. We’ve been able to see glimpses of the boxwork structures in the distance for a few weeks now, and I am really excited about being able to plan long drives that get us closer and closer. What will we find when we reach them? Power was on everyone’s mind as we put the plan together today. The science team had lots of amazing ideas about observations to collect from our current location, but we had to carefully plan and prioritize them to make sure we didn’t use too much power and leave the rover battery lower than we’d like for Monday’s plan. Winter on Mars certainly keeps us on our toes! We ended up putting together what I think is a pretty good set of activities for the weekend. MAHLI, APXS, and ChemCam will all work together to observe a flat rock in front of us named “Iron Mountain.” MAHLI will also do an experiment with this rock, testing different combinations of camera positions to see which produces the best data to help us generate 3D models of the rock’s surface. I know rocks don’t have feelings, but if they did, I hope Iron Mountain can use this time to feel a bit like a movie star on the red carpet, getting photographed from all angles. Mastcam will also be photographing the surroundings, working with ChemCam’s RMI imager to take images the ridge containing boxwork structures named “Ghost Mountain,” and taking some solo shots of targets in the foreground named “Redondo Flat,” “Silverwood Sanctuary,” and the oft photographed Gould Mesa. Navcam, REMS, and DAN round out the science plan with some environmental observations. We’ll be getting one more science and engineering hybrid observation when we collect ChemCam passive spectral data of the instrument’s calibration target in parallel with one of our communication passes. This observation is part of a series of tests we’re doing to run rover activities in parallel with these passes, and if successful, will allow us to be more even more power efficient in the future. We’re also celebrating a soliday this weekend, which means we only have a two-sol plan instead of our usual three as the Mars and Earth time zones re-align for the next few weeks. I’m looking forward to seeing where Curiosity drives next week. Explore More 2 min read Sols 4511-4512: Low energy after a big weekend? Article 16 mins ago 2 min read Sols 4507-4508: “Just Keep Driving” Article 4 days ago 3 min read Sols 4505-4506: Up, up and onto the Devil’s Gate Article 1 week ago Keep Exploring Discover More Topics From NASA Mars Resources Explore this page for a curated collection of Mars resources. 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… The Mars Report The Mars Report newsletter from NASA is your source for everything on or about the Red Planet. We bring you… View the full article

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Researchers from NASA’s Jet Propulsion Laboratory in Southern California, private companies, and academic institutions are developing the first space-based quantum sensor for measuring gravity. Supported by NASA’s Earth Science Technology Office (ESTO), this mission will mark a first for quantum sensing and will pave the way for groundbreaking observations of everything from petroleum reserves to global supplies of fresh water. A map of Earth’s gravity. Red indicates areas of the world that exert greater gravitational pull, while blue indicates areas that exert less. A science-grade quantum gravity gradiometer could one day make maps like this with unprecedented accuracy. Image Credit: NASA Earth’s gravitational field is dynamic, changing each day as geologic processes redistribute mass across our planet’s surface. The greater the mass, the greater the gravity. You wouldn’t notice these subtle changes in gravity as you go about your day, but with sensitive tools called gravity gradiometers, scientists can map the nuances of Earth’s gravitational field and correlate them to subterranean features like aquifers and mineral deposits. These gravity maps are essential for navigation, resource management, and national security. “We could determine the mass of the Himalayas using atoms,” said Jason Hyon, chief technologist for Earth Science at JPL and director of JPL’s Quantum Space Innovation Center. Hyon and colleagues laid out the concepts behind their Quantum Gravity Gradiometer Pathfinder (QGGPf) instrument in a recent paper in EPJ Quantum Technology. Gravity gradiometers track how fast an object in one location falls compared to an object falling just a short distance away. The difference in acceleration between these two free-falling objects, also known as test masses, corresponds to differences in gravitational strength. Test masses fall faster where gravity is stronger. QGGPf will use two clouds of ultra-cold rubidium atoms as test masses. Cooled to a temperature near absolute zero, the particles in these clouds behave like waves. The quantum gravity gradiometer will measure the difference in acceleration between these matter waves to locate gravitational anomalies. Using clouds of ultra-cold atoms as test masses is ideal for ensuring that space-based gravity measurements remain accurate over long periods of time, explained Sheng-wey Chiow, an experimental physicist at JPL. “With atoms, I can guarantee that every measurement will be the same. We are less sensitive to environmental effects.” Using atoms as test masses also makes it possible to measure gravity with a compact instrument aboard a single spacecraft. QGGPf will be around 0.3 cubic yards (0.25 cubic meters) in volume and weigh only about 275 pounds (125 kilograms), smaller and lighter than traditional space-based gravity instruments. Quantum sensors also have the potential for increased sensitivity. By some estimates, a science-grade quantum gravity gradiometer instrument could be as much as ten times more sensitive at measuring gravity than classical sensors. The main purpose of this technology validation mission, scheduled to launch near the end of the decade, will be to test a collection of novel technologies for manipulating interactions between light and matter at the atomic scale. “No one has tried to fly one of these instruments yet,” said Ben Stray, a postdoctoral researcher at JPL. “We need to fly it so that we can figure out how well it will operate, and that will allow us to not only advance the quantum gravity gradiometer, but also quantum technology in general.” This technology development project involves significant collaborations between NASA and small businesses. The team at JPL is working with AOSense and Infleqtion to advance the sensor head technology, while NASA’s Goddard Space Flight Center in Greenbelt, Maryland is working with Vector Atomic to advance the laser optical system. Ultimately, the innovations achieved during this pathfinder mission could enhance our ability to study Earth, and our ability to understand distant planets and the role gravity plays in shaping the cosmos. “The QGGPf instrument will lead to planetary science applications and fundamental physics applications,” said Hyon. To learn more about ESTO visit: https://esto.nasa.gov Share Details Last Updated Apr 15, 2025 Editor NASA Science Editorial Team Contact Gage Taylor gage.taylor@nasa.gov Location NASA Goddard Space Flight Center Related Terms Science-enabling Technology Earth Science Technology Office Technology Highlights Explore More 5 min read Atomic Layer Processing Coating Techniques Enable Missions to See Further into the Ultraviolet Article 4 weeks ago 4 min read Novel Metasurface Optical Element Could Shed New Light on Atmospheric Aerosols Article 1 month ago 5 min read Ultra-low-noise Infrared Detectors for Exoplanet Imaging Article 2 months ago View the full article

This article is for students grades 5-8. Aerodynamics is the way objects move through air. The rules of aerodynamics explain how an airplane is able to fly. Anything that moves through air is affected by aerodynamics, from a rocket blasting off, to a kite flying. Since they are surrounded by air, even cars are affected by aerodynamics. What Are the Four Forces of Flight? The four forces of flight are lift, weight, thrust and drag. These forces make an object move up and down, and faster or slower. The amount of each force compared to its opposing force determines how an object moves through the air. What Is Weight? Gravity is a force that pulls everything down to Earth. Weight is the amount of gravity multiplied by the mass of an object. Weight is also the downward force that an aircraft must overcome to fly. A kite has less mass and therefore less weight to overcome than a jumbo jet, but they both need the same thing in order to fly — lift. What Is Lift? Lift is the push that lets something move up. It is the force that is the opposite of weight. Everything that flies must have lift. For an aircraft to move upward, it must have more lift than weight. A hot air balloon has lift because the hot air inside is lighter than the air around it. Hot air rises and carries the balloon with it. A helicopter’s lift comes from the rotor blades. Their motion through the air moves the helicopter upward. Lift for an airplane comes from its wings. How Do an Airplane’s Wings Provide Lift? The shape of an airplane’s wings is what makes it possible for the airplane to fly. Airplanes’ wings are curved on top and flatter on the bottom. That shape makes air flow over the top faster than under the bottom. As a result, less air pressure is on top of the wing. This lower pressure makes the wing, and the airplane it’s attached to, move up. Using curves to affect air pressure is a trick used on many aircraft. Helicopter rotor blades use this curved shape. Lift for kites also comes from a curved shape. Even sailboats use this curved shape. A boat’s sail is like a wing. That’s what makes the sailboat move. What Is Drag? Drag is a force that pulls back on something trying to move. Drag provides resistance, making it hard to move. For example, it is more difficult to walk or run through water than through air. Water causes more drag than air. The shape of an object also affects the amount of drag. Round surfaces usually have less drag than flat ones. Narrow surfaces usually have less drag than wide ones. The more air that hits a surface, the more the drag the air produces. What Is Thrust? Thrust is the force that is the opposite of drag. It is the push that moves something forward. For an aircraft to keep moving forward, it must have more thrust than drag. A small airplane might get its thrust from a propeller. A larger airplane might get its thrust from jet engines. A glider does not have thrust. It can only fly until the drag causes it to slow down and land. Why Does NASA Study Aerodynamics? Aerodynamics is an important part of NASA’s work. The first A in NASA stands for aeronautics, which is the science of flight. NASA works to make airplanes and other aircraft better. Studying aerodynamics is an important part of that work. Aerodynamics is important to other NASA missions. Probes landing on Mars have to travel through the Red Planet’s thin atmosphere. Having to travel through an atmosphere means aerodynamics is important on other planets too. More About Aerodynamics Dynamics of Flight Read What Is Aerodynamics (Grades K-4) Explore More For Students Grades 5-8 View the full article

3 Min Read What Is Aerodynamics? (Grades K-4) This article is for students grades K-4. What Are the Four Forces of Flight? Aerodynamics is the way air moves around things. The rules of aerodynamics explain how an airplane is able to fly. Anything that moves through air reacts to aerodynamics. A rocket blasting off the launch pad and a kite in the sky react to aerodynamics. Aerodynamics even acts on cars, since air flows around cars. The four forces of flight are lift, weight, thrust and drag. These forces make an object move up and down, and faster or slower. How much of each force there is changes how the object moves through the air. What Is Weight? Everything on Earth has weight. This force comes from gravity pulling down on objects. To fly, an aircraft needs something to push it in the opposite direction from gravity. The weight of an object controls how strong the push has to be. A kite needs a lot less upward push than a jumbo jet does. What Is Lift? Lift is the push that lets something move up. It is the force that is the opposite of weight. Everything that flies must have lift. For an aircraft to move upward, it must have more lift than weight. A hot air balloon has lift because the hot air inside is lighter than the air around it. Hot air rises and carries the balloon with it. A helicopter’s lift comes from the rotor blades at the top of the helicopter. Their motion through the air moves the helicopter upward. Lift for an airplane comes from its wings. How Do an Airplane’s Wings Provide Lift? The shape of an airplane’s wings is what makes it able to fly. Airplanes’ wings are curved on top and flatter on the bottom. That shape makes air flow over the top faster than under the bottom. So, less air pressure is on top of the wing. This condition makes the wing, and the airplane it’s attached to, move up. Using curves to change air pressure is a trick used on many aircraft. Helicopter rotor blades use this trick. Lift for kites also comes from a curved shape. Even sailboats use this concept. A boat’s sail is like a wing. That’s what makes the sailboat move. What Is Drag? Drag is a force that tries to slow something down. It makes it hard for an object to move. It is harder to walk or run through water than through air. That is because water causes more drag than air. The shape of an object also changes the amount of drag. Most round surfaces have less drag than flat ones. Narrow surfaces usually have less drag than wide ones. The more air that hits a surface, the more drag it makes. What Is Thrust? Thrust is the force that is the opposite of drag. Thrust is the push that moves something forward. For an aircraft to keep moving forward, it must have more thrust than drag. A small airplane might get its thrust from a propeller. A larger airplane might get its thrust from jet engines. A glider does not have thrust. It can only fly until the drag causes it to slow down and land. Read What Is Aerodynamics? (Grades 5-8) Explore More For Students Grades K-4 View the full article

NASA/Johns Hopkins APL/Princeton/Ed Whitman NASA’s IMAP (Interstellar Mapping and Acceleration Probe) is loaded into the X-ray and Cryogenic Facility (XRCF) thermal vacuum chamber at NASA’s Marshall Space Flight Center in Huntsville, Alabama, in this photo from March 20, 2025. There, the spacecraft will undergo testing such as dramatic temperature changes to simulate the harsh environment of space. The IMAP mission is a modern-day celestial cartographer that will map the solar system by studying the heliosphere, a giant bubble created by the Sun’s solar wind that surrounds our solar system and protects it from harmful interstellar radiation. The IMAP mission will launch on a SpaceX Falcon 9 rocket from NASA’s Kennedy Space Center in Florida, no earlier than September 2025. Image credit: NASA/Johns Hopkins APL/Princeton/Ed Whitman View the full article

A SpaceX Falcon 9 rocket carrying the company’s Dragon spacecraft is launched on NASA’s SpaceX Crew-10 mission to the International Space Station.NASA/Aubrey Gemignani Digital content creators are invited to register to attend the launch of NASA’s SpaceX Crew-11 mission to carry astronauts to the International Space Station for a science expedition as part of NASA’s Commercial Crew Program. This will be the 15th time a SpaceX Dragon spacecraft launched by a Falcon 9 rocket takes crews to the orbital laboratory. Launch of the Crew-11 mission is targeted for no earlier than July 2025 on a SpaceX Falcon 9 rocket from Florida. The launch will carry NASA astronauts Commander Zena Cardman and Pilot Mike Fincke, and mission specialists JAXA (Japan Aerospace Exploration Agency) astronaut Kimiya Yui and Roscosmos cosmonaut Oleg Platonov. If your passion is to communicate and engage the world online, then this is the event for you! Seize the opportunity to see and share the #Crew11 mission launch. A maximum of 50 social media users will be selected to attend this two-day event and will be given exclusive access to NASA’s Kennedy Space Center in Florida. NASA Social participants will have the opportunity to: View a crewed launch of the SpaceX Falcon 9 rocket and Dragon spacecraft Tour NASA facilities at the agency’s Kennedy Space Center in Florida Meet and interact with Crew-11 subject-matter experts Meet fellow space enthusiasts who are active on social media NASA Social registration for the Crew-11 launch opens on Tuesday, April 15, and the deadline to apply is at 10 a.m. EDT on Monday, April 28. All social applications will be considered on a case-by-case basis. APPLY NOW Do I need to have a social media account to register? Yes. This event is designed for people who: Actively use multiple social networking platforms and tools to disseminate information to a unique audience. Regularly produce new content that features multimedia elements. Have the potential to reach a large number of people using digital platforms, or reach a unique audience, separate and distinctive from traditional news media and/or NASA audiences. Must have an established history of posting content on social media platforms. Have previous postings that are highly visible, respected and widely recognized. Users on all social networks are encouraged to use the hashtag #NASASocial and #Crew11. Updates and information about the event will be shared on X via @NASASocial and @NASAKennedy, and via posts to Facebook and Instagram. How do I register? Registration for this event opens on Tuesday, April 15, and the deadline to apply is at 10 a.m. EDT on Monday, April 28. Registration is for one person only (you) and is non-transferable. Each individual wishing to attend must register separately. Each application will be considered on a case-by-case basis. Can I register if I am not a U.S. citizen? Yes, this event is open for all to apply, ages 18 years and older. When will I know if I am selected? After registrations have been received and processed, an email with confirmation information and additional instructions will be sent to those selected. We expect to send the acceptance notifications by May 30. What are NASA Social credentials? All social applications will be considered on a case-by-case basis. Those chosen must prove through the registration process they meet specific engagement criteria. If you do not make the registration list for this NASA Social, you still can attend the launch offsite and participate in the conversation online. Find out about ways to experience a launch here. What are the registration requirements? Registration indicates your intent to travel to NASA’s Kennedy Space Center in Florida and attend the two-day event in person. You are responsible for your own expenses for travel, accommodations, food, and other amenities. You must be able to attend all days of NASA Social activities in order to view the launch Some events and participants scheduled to appear at the event are subject to change without notice. NASA is not responsible for loss or damage incurred as a result of attending. NASA, moreover, is not responsible for loss or damage incurred if the event is cancelled with limited or no notice. Please plan accordingly. NASA Kennedy is a government facility. Those who are selected will need to complete an additional registration step to receive clearance to enter the secure areas. IMPORTANT: To be admitted, you will need to provide two forms of unexpired government-issued identification; one must be a photo ID and match the name provided on the registration. Those without proper identification cannot be admitted. For a complete list of acceptable forms of ID, please visit: NASA Credentialing Identification Requirements. All registrants must be at least 18 years old. What if the launch date changes? Many different factors can cause a scheduled launch date to change multiple times. If the launch date changes, NASA may adjust the date of the NASA Social accordingly to coincide with the new target launch date. NASA will notify registrants of any changes by email. If the launch is postponed, attendees may be invited to attend a later launch date but that is not guaranteed. NASA Social attendees are responsible for any additional costs they incur related to any launch delay. We strongly encourage participants to make travel arrangements that are refundable and/or flexible. What if I cannot come to the Kennedy Space Center? If you cannot come to the Kennedy Space Center and attend all days in person, you should not register for the NASA Social. You can follow the conversation online using #NASASocial. You can also become a virtual guest for NASA launches and milestone events. This free program gives access to curated resources, schedule changes, and mission specific information delivered straight to your inbox. Join us today! You can watch the launch on NASA+. NASA will provide regular launch and mission updates on X at @NASA, @NASAKennedy, and @Commercial_Crew, as well as on NASA’s Commercial Crew Program blog. If you cannot make this NASA Social, don’t worry; NASA is planning many other Socials in the near future at various locations! Apply Now View the full article

NASA’s SpaceX 32nd commercial resupply services mission, scheduled to lift off from the agency’s Kennedy Space Center in April, is heading to the International Space Station with experiments that include research on whether plant DNA responses in space correlate to human aging and disease, and measuring the precise effects of gravity on time. Discover more details about the two experiments’ potential impacts on space exploration and how they can enhance life on Earth: “Second Guessing” Time in Space As outlined in Einstein’s general theory of relativity, how we experience the passage of time is influenced by gravity. However, there is strong evidence to believe this theory may not be complete and that there are unknown forces at play. These new physics effects may manifest themselves in small deviations from Einstein’s prediction. The ACES (Atomic Clock Ensemble in Space) investigation is an ESA (European Space Agency) mission that aims to help answer fundamental physics questions. By comparing a highly precise atomic clock in space with numerous ground atomic clocks around the world, ACES could take global time synchronization and clock comparison experiments to new heights. Sponsored by NASA, United States scientists are participating in the mission in various ways, including contributing ground station reference clocks. Scheduled to collect data for 30 months, this vast network of precise clocks is expected to provide fresh insights into the exact relationship between gravity and time, set new limits for unknown forces, and improve global time synchronization. In addition to investigating the laws of physics, ACES will enable new terrestrial applications such as relativistic geodesy, which involves measuring Earth’s shape and gravitational field with extreme precision. These advancements are critical to space navigation, satellite operations, and GPS systems. For example, without understanding the time fluctuations between Earth and medium Earth orbit, GPS would be progressively less accurate. A robotic arm will attach ACES to the Columbus Laboratory module aboard the International Space Station. Image courtesy of ESA Probing Plants for Properties to Protect DNA The APEX-12 (Advanced Plant EXperiment-12) investigation will test the hypothesis that induction of telomerase activity in space protects plant DNA molecules from damage elicited by cellular stress evoked by the combined spaceflight stressors experienced by seedlings grown aboard the space station. It is expected that results will lead to a better understanding of differences between human and plant telomere behavior in space. Data on telomerase activity in plants could be leveraged not only to develop therapies for age-related diseases in space and on Earth, but also for ensuring food crops are more resilient to spaceflight stress. Telomeres and telomerase influence cell division and cell death, two processes crucial to understanding aging in humans. Telomeres are the protective end caps of chromosomes. Each time a cell divides, the telomeres shorten slightly, essentially acting as a biological clock for cell aging. Conversely, telomerase is an enzyme that adds nucleotide sequences to the ends of telomeres, lengthening them and counteracting their shortening. In humans, telomere shortening is linked to various age-related conditions, such as cardiovascular diseases and certain cancers. In astronauts, studies have shown that spaceflight leads to changes in telomere length, with a notable lengthening observed. This phenomenon carries potential implications for astronaut health outcomes. By contrast, plant telomere length did not change during spaceflight, despite a dramatic increase in telomerase activity. A microscopic image of plant telomeres taken under a fluorescent microscope. The chromosomes are highlighted in blue. The telomeres are highlighted in yellow. Image courtesy of Texas A&M University How this benefits space exploration: Experiments aboard NASA’s SpaceX CRS-32 mission is twofold. One, they have the potential to significantly enhance precision timekeeping, which is necessary to improve space navigation and communication. Two, they can provide insights into how plants adapt to protect DNA molecules from cellular stress caused by environmental factors experienced in spaceflight, in an effort to sustain plant life in space. How this benefits humanity: The experiments conducted on NASA’s SpaceX CRS-32 mission offer a range of potential benefits to humanity. First, improving precision timekeeping for more accurate GPS technology. Second, capturing data about how telomerase activity correlates to cellular stress in plants, which could lead to assays which better correlate telomerase activity and cellular stress and provide fundamental research to contribute to potential therapies for humans. Learn more about the investigations: ACES (Atomic Clock Ensemble in Space) Atomic Clock Ensemble in Space (ACES) is a European Space Agency (ESA) mission that aims to help answer fundamental physics questions. APEX-12 (Advanced Plant EXperiment-12) Advanced Plant EXperiment-12 (APEX-12) will test the hypothesis that induction of telomerase, a protein complex, activity in space protects plant DNA molecules from damage elicited by cellular stress evoked by the combined spaceflight stressors experienced by seedlings grown aboard the space station. About BPS NASA’s Biological and Physical Sciences Division pioneers scientific discovery and enables exploration by using space environments to conduct investigations not possible on Earth. Studying biological and physical phenomenon under extreme conditions allows researchers to advance the fundamental scientific knowledge required to go farther and stay longer in space, while also benefitting life on Earth. View the full article