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By NASA
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s C-130, now under new ownership, sits ready for its final departure from NASA’s Wallops Flight Facility in Virginia, on Friday, April 18, 2025. NASA/Garon Clark NASA’s C-130 Hercules, fondly known as the Herc, went wheels up at 9:45 a.m., Friday, April 18, as it departed from its decade-long home at NASA’s Wallops Flight Facility in Virginia, for the final time. The aircraft is embarking on a new adventure to serve and protect in the state of California where it is now under the ownership of the California Department of Forestry and Fire Protection (CAL FIRE).
The transition of the C-130 to CAL FIRE is part of a long-running, NASA-wide aircraft enterprise-management activity to consolidate the aircraft fleet and achieve greater operational efficiencies while reducing the agency’s infrastructure footprint.
The C-130 Hercules takes off for the final time from NASA’s Wallops Flight Facility in Virginia.NASA/Garon Clark “Our C-130 and the team behind it has served with great distinction over the past decade,” said David L. Pierce, Wallops Flight Facility director. “While our time with this amazing airframe has come to a close, I’m happy to see it continue serving the nation in this new capacity with CAL FIRE.”
The research and cargo aircraft, built in 1986, was acquired by NASA in 2015. Over the past decade, the C-130 supported the agency’s airborne scientific research, provided logistics support and movement of agency cargo, and supported technology demonstration missions. The aircraft logged approximately 1,820 flight hours in support of missions across the world during its time with the agency.
Additional aircraft housed at NASA Wallops will be relocated to NASA’s Langley Research Center in Hampton, Virginia, in the coming months.
For more information on NASA’s Wallops Flight Facility, visit: www.nasa.gov/wallops.
By Olivia Littleton
NASA’s Wallops Flight Facility, Wallops Island, Va.
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Last Updated Apr 18, 2025 EditorOlivia F. LittletonLocationWallops Flight Facility Related Terms
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By NASA
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/
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By NASA
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.
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Last Updated Apr 16, 2025 EditorJason Costa Related Terms
Kennedy Space Center Commercial Resupply Get Involved International Space Station (ISS) ISS Research SpaceX Commercial Resupply Virtual Guest Program Explore More
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By NASA
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.
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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
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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
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