NASA Astronaut Jessica Meir's Exercise Routine | International Space Station

NASA Astronaut Jessica Meir's Exercise Routine | International Space Station

Expedition 74 Flight Engineer and NASA Astronaut Jessica Meir: "Apologies for the background noise, life on International Space Station is loud! Without daily exercise on the ISS, we would lose significant muscle mass and bone density, since we don’t have the daily loading on our bodies that Earth’s gravitational environment provides.

We have the ARED 🏋️‍♀️ (Advanced Resistive Exercise Device), an engineering marvel that can be configured into a large number of weight lifting exercises, a cycle ergometer 🚲 (think a stationary bike with no handlebars and no seat—not needed in space!), and a treadmill. 🏃‍♀️

I started exercise right away, and it was so cool. Complete muscle memory! Really feels like I never left. Here’s a peek into our daily exercise routine!"

NASA Astronaut/Dr. Jessica Meir's Biography:
https://www.nasa.gov/people/jessica-u-meir/

Follow Expedition 74:
https://blogs.nasa.gov/spacestation/

Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: Andrey Fedyaev, Sergei Mikaev

European Space Agency Flight Engineer: Sophie Adenot

NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Credit: NASA's Johnson Space Center/Jessica Meir

Duration: 2 minute, 45 seconds
Release Date: March 6, 2026

#NASA #Space #ISS #Planets #Earth #Astronauts #JessicaMeir #AstronautExercise #AstronautHealth #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #UnitedStates #STEM #Education #HD #Video

Polar-ring Galaxy NGC 660 in Pisces: Wide-field view | Mayall Telescope

Polar-ring Galaxy NGC 660 in Pisces: Wide-field view | Mayall Telescope

This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. It shows NGC 660 and its surroundings. NGC 660 is a striking example of a polar ring galaxy.

Distance from Earth: ~40 million light-years

In the distant background are thousands of other galaxies. Nearly every small blue or yellow smudge is a very distant galaxy. A number of these, like NGC 660, show evidence of collisions or mergers. The image was generated with observations in the B (blue), V (green), I (orange) and Hydrogen-Alpha (red) filters. In this image, North is up, East is to the left.

Learn more about the Mayall Telescope: 
https://noirlab.edu/science/programs/kpno/telescopes/nicholas-mayall-4m-telescope

Credit:T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)
Release Date: June 30, 2020

#NASA #Astronomy #Space #Science #Galaxies #NGC660 #PolarRingGalaxies #InteractingGalaxies #PiscesConstellation #Cosmos #Universe #MayallTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

Polar-ring Galaxy NGC 660 in Pisces | Subaru Telescope

Polar-ring Galaxy NGC 660 in Pisces | Subaru Telescope

NGC 660 is a polar ring galaxy located in the constellation Pisces. It features a large, extended ring structure surrounding the central spiral galaxy at a near-perpendicular angle. NGC 660 spans about 40,000 light years across. The ring emits blue light from active star-forming regions within it. The dark lanes in the ring and the galactic disk intersect, highlighting its complicated structure. This ring structure is thought to have been formed through the gravitational interaction of the central galaxy with another galaxy.

Distance from Earth: ~40 million light-years

Learn more about Japan's Subaru Telescope: 
https://subarutelescope.org/en/

Image Credit: National Astronomical Observatory of Japan (NAOJ)/Masayuki Tanaka

Release Date: Oct. 16, 2024

#NASA #Astronomy #Space #Science #Galaxies #NGC660 #PolarRingGalaxies #InteractingGalaxies #PiscesConstellation #Cosmos #Universe #SubaruTelescope #すばる望遠鏡 #NAOJ #国立天文台 #HyperSuprimeCam #HSC #Japan #日本 #MaunaKea #Hawaii #UnitedStates #STEM #Education

Polar-ring Galaxy NGC 660 in Pisces | Gemini North Telescope

Polar-ring Galaxy NGC 660 in Pisces | Gemini North Telescope

This Gemini North telescope image captures the “bloody” aftermath of one galaxy piercing the heart of another. All the action appears in a single frame with the stunning polar-ring galaxy NGC 660 as the focus of attention. NGC 660 spans around 40,000 light years across and lies about 40 million light years distant in the direction of the constellation of Pisces. It has an unusually high gas content and resolves into hundreds of objects, a considerable fraction are blue and red supergiant stars. 

The ring’s youngest detected stars formed only about seven million years ago, indicating a long and ongoing process of formation. As NGC 660’s ring is not truly polar, but inclined ~45˚ from the plane of the disk, it most likely formed by a previous interaction with a gas-rich galaxy about a billion years ago. That event would have stripped the interloper of its gas, directed it into NGC 660’s core, and triggered a furious burst of star formation. When the resulting short-lived, massive stars exploded shortly thereafter as supernovae, they would have generated shock waves that triggered more star formation, and so on, even to this day. 

This image of the ring galaxy NGC 660, obtained with the Gemini Multi-Object Spectrograph on the Fredrick C. Gillett Gemini North telescope was obtained in August 2012. The image is made from three images taken through g, r, i, and hydrogen alpha filters and assigned the colors of blue, green, orange and red respectively in this color composite image. The field of view is 9.3x5.6 arcminutes and it is oriented 8 degrees clockwise from north at right and east up. The total exposure (integration) time was 1,620 seconds for all filters. 

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/

Credits: International Gemini Observatory/AURA

Color composite produced by Travis Rector, University of Alaska Anchorage
Release Date: Oct. 17, 2012

#NASA #Astronomy #Space #Science #Galaxies #NGC660 #PolarRingGalaxies #PiscesConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GeMS #AdaptiveOptics #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

US & European Astronauts Discuss Life in Space | International Space Station

US & European Astronauts Discuss Life in Space | International Space Station

Aboard the International Space Station, Expedition 74 flight engineers Jessica Meir of NASA and Sophie Adenot of European Space Agency (ESA) discussed life and work aboard the orbital outpost during an in-flight interview March 5, 2026 with spaceflightnow.com. 

Meir and Adenot are in the midst of a long-duration mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration flights as part of NASA’s Moon and Mars exploration approach, including lunar missions through NASA’s Artemis program. 

NASA Astronaut/Dr. Jessica Meir's Biography:
https://www.nasa.gov/people/jessica-u-meir/

Astronaut Sophie Adenot's Biography:
https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Astronauts/Sophie_Adenot

Follow Expedition 74:
https://blogs.nasa.gov/spacestation/

Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: Andrey Fedyaev, Sergei Mikaev

European Space Agency Flight Engineer: Sophie Adenot

NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Video Credit: NASA's Johnson Space Center
Duration: 20 minutes
Release Date: March 5, 2026

#NASA #Space #ISS #Planets #Earth #Astronauts #JessicaMeir #UnitedStates #SophieAdenot #France #ESA #Europe #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #STEM #Education #HD #Video

Planet Jupiter's 'Red Spots' (near-infrared view) | Gemini North Telescope

Planet Jupiter's 'Red Spots' (near-infrared view) | Gemini North Telescope

Gemini North adaptive optics image of Jupiter and its two red spots (appearing white because this is a near-infrared image; in visible light they appear reddish). In this color composite image, white indicates cloud features at relatively high altitudes; blue indicates lower cloud structures; and red represents still deeper cloud features. The two red spots appear more white than red, because their tops hover high above the surrounding clouds. Also prominent is the polar stratospheric haze that makes Jupiter bright near the pole (unlike the other orange/red features in this image, the polar haze is high in Jupiter's atmosphere). Other tiny white spots are regions of high clouds, like towering thunderheads. In visible light, Jupiter looks orangish, but in the near-infrared the blue color is due to strong absorption features. The blue mid-level clouds are also closest to what one would see in a visual light image.

The Great Red Spot is a massive storm on Jupiter, known for its persistent high-pressure region and anticyclonic characteristics. It has been observed for over 150 years and is the largest storm in the Solar System with winds reaching up to 432 km/h (268 mph). The exact origin of its red color is still a mystery, but it is believed to be an area of upwelling in the atmosphere. The storm has been continuously observed since 1878 with its current state being influenced by its unique dynamics and the planet's atmospheric conditions. 

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/

Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Date: July 20, 2006

#NASA #Astronomy #Space #Science #SolarSystem #Planets #Jupiter #InfraredAstronomy #NearInfrared #Atmosphere #Meteorology #Weather #RedSpots #GreatRedSpot #Storms #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GeMS #AdaptiveOptics #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

A Space Oddity: Hanny’s Voorwerp around Galaxy IC 2497 in Leo Minor | Hubble

A Space Oddity: Hanny’s Voorwerp around Galaxy IC 2497 in Leo Minor | Hubble

In this image by the NASA/European Space Agency Hubble Space Telescope, an unusual, ghostly green blob of gas appears to float near a normal-looking spiral galaxy. The bizarre object, named Hanny’s Voorwerp (Hanny’s Object in Dutch), is the only visible part of a streamer of gas stretching 300,000 light-years around the galaxy, called IC 2497. The greenish Voorwerp is visible because a searchlight beam of light from the galaxy’s core has illuminated it. This beam came from a quasar, a bright, energetic object that is powered by a black hole. The quasar may have turned off in the last 200,000 years.

Distance from Earth: ~650 million light years

This Hubble view uncovers a pocket of star clusters, the yellowish-orange area at the tip of Hanny’s Voorwerp. The star clusters are confined to an area that is a few thousand light-years wide. The youngest stars are a couple of million years old. The Voorwerp is the size of the Milky Way, and its bright green color is from glowing oxygen.

The image was made by combining data from the Advanced Camera for Surveys (ACS) and the Wide Field Camera 3 (WFC3) onboard Hubble with data from the WIYN telescope at Kitt Peak, Arizona, USA. The ACS exposures were taken April 12, 2010; the WFC3 data, April 4, 2010.

Credit: NASA, ESA, William Keel (University of Alabama, Tuscaloosa), and the Galaxy Zoo team
Release Date: Jan. 10, 2011

#NASA #ESA #Astronomy #Space #Science #Stars #StarClusters #Galaxies #IC2497 #Quasars #BlackHoles #SpiralGalaxy #Nebulae #HannysVoorwerp #EmissionNebulae #IntergalacticGas #IntergalacticGasCloud #LeoMinorConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

Lunar Eclipse & Aurora Borealis: Wide Views from Alaska

Lunar Eclipse & Aurora Borealis: Wide Views from Alaska

Astrophotographer Ayumi Yaegashi Bakken: ". . . more photos from the total lunar eclipse with the aurora near Coldfoot-Wiseman, Alaska. The sky was totally clear, and the aurora band showed up much earlier than the lunar eclipse. One incredible moment that occurred after 20-30 minutes from total eclipse was when the bright green band moved over the blood Moon. My cameras and my hands were cold enough to get frozen almost, but I will never forget this night."

Lunar eclipses occur at the full Moon phase. When Earth is positioned precisely between the Moon and Sun, Earth’s shadow falls upon the surface of the Moon, dimming it and sometimes turning the lunar surface a striking red over the course of a few hours. Each lunar eclipse is visible from half of Earth.

Learn more: https://science.nasa.gov/moon/eclipses/

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

Alaska is a non-contiguous U.S. state on the northwest extremity of North America. Part of the Western United States region, it is one of the two non-contiguous U.S. states, alongside Hawaii. Alaska is considered to be the northernmost, westernmost, and easternmost state in the United States. It borders the Canadian territory of the Yukon and the province of British Columbia to the east. It shares a western maritime border in the Bering Strait with Russia. The Chukchi and Beaufort Seas of the Arctic Ocean lie to the north, and the Pacific Ocean lies to the south.

Image Credit: Ayumi Yaegashi Bakken

Location: Coldfoot, Alaska, USA

Ayumi 's website: https://ayumibakken.com
Date: March 3, 2026

#NASA #Astronomy #Space #Science #Stars #Sun #Planets #Earth #BloodMoon #LunarEclipse #SpaceWeather #Aurora #AuroraBorealis #NorthernLights #Magnetosphere #SolarWind #SolarSystem #Astrophotography #AyumiYaegashiBakken #Astrophotographers #Coldfoot #Alaska #UnitedStates #STEM #Education

NASA Artemis II Moon Mission: "For All Humanity" | Latest Updates

NASA Artemis II Moon Mission: "For All Humanity" | Latest Updates

"Four astronauts. One historic journey. Moonbound: For All Humanity follows the paths of the Artemis II crew as they prepare to journey around the Moon and back home. This is where the next chapter of human exploration begins."

Launch is expected by April 2026.

Updates: With NASA’s Artemis II Space Launch System (SLS) rocket and Orion spacecraft in the Vehicle Assembly Building at the agency’s Kennedy Space Center in Florida, technicians have accessed the launch vehicle stage adapter to inspect components that prevented helium from flowing to the upper stage after a Feb. 21 wet dress rehearsal.

Engineers determined a seal in the quick disconnect, through which helium flows from the ground systems to the rocket, was obstructing the pathway. The team removed the quick disconnect, reassembled the system, and began validating the repairs to the upper stage by running a reduced flow rate of helium through the mechanism to ensure the issue was resolved. Engineers are assessing what allowed the seal to become dislodged to prevent the issue from recurring.

While the upper stage repair has been underway, technicians also have been working to refresh other systems on the rocket. They are activating a new set of flight termination system batteries ahead of end-to-end retesting of the system and also are replacing the flight batteries on the upper stage, core stage, and solid rocket boosters, and charging the Orion launch abort system batteries. Work to replace a seal on the core stage liquid oxygen line feed system began March 2. Once complete, teams will reassemble the oxygen tail service mast umbilical plate and perform various integrity tests to ensure the seal interface is tight.

Work on the rocket and spacecraft will continue in the coming weeks as NASA prepares for rolling the rocket out to the launch pad again later this month ahead of a potential launch in April.

NASA Artemis II Mission page updates:
https://www.nasa.gov/mission/artemis-ii/

Artemis Program blog: 

https://blogs.nasa.gov/artemis/

Video Credit: National Aeronautics and Space Administration (NASA)

Duration: 1 minute
Release Date: March 6, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrewedMissions #Astronauts #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKenendy #Florida #UnitedStates #CSA #Canada #STEM #Education #HD #Video

China's Landspace: BF20 Engine Tests for Reusable Heavy Lift Commercial Rockets

China's Landspace: BF20 Engine Tests for Reusable Heavy Lift Commercial Rockets

🔥These high-thrust, long-duration engine tests by China commercial launch services provider Landspace lay the foundation for building a high-efficiency, reusable heavy-lift launch vehicle system. The full-flow staged combustion cycle (FFSC) BF20 220-ton-class methalox engine completed its first full-system test firing in May 2025. Since then it has undergone over 100 full-system ignition tests. This marks another milestone on their way to catch up with SpaceX's capabilities.

At the beginning of the Year of the Horse, LandSpace has fully resumed its R&D, production, and testing activities. Recently, the company successfully completed long-duration full-system hot-fire tests of its independently developed blue flame (BF) 20 LOX–methane FFSC engine demonstrating continued progress in the development of high-thrust, high-performance liquid rocket engines.

The BF engine is designed using the advanced FFSC cycle, combined with a highly integrated architecture and high chamber pressure design. It features two preburners: a fuel-rich preburner driving the fuel pump and an oxygen-rich preburner driving the oxidizer pump. The two gas streams are then routed into the main combustion chamber, where they burn completely to ensure optimal performance.

Compared with conventional engine cycles, the FFSC cycle offers higher propellant utilization efficiency, greater thrust-to-weight ratio, and longer service life. However, it also introduces significant engineering challenges, including high system coupling, structural complexity, multiple vibration sources, elevated internal pressures, and intense thermal loads.

Development of the BF engine has progressed rapidly. Since its first full-system hot-fire test in May 2025, it has accomplished more than 100 full-system ignition tests. The successful completion of this latest long-duration test demonstrates steady progress in key technology development and confirms LandSpace’s capability to carry out the complete development cycle of FFSC engines, supported by an agile testing and iteration approach.

These advances further improve the engine’s technical maturity and lay a solid foundation for future development. The BF engine will serve as a critical propulsion building block for the next generation of large to heavy-lift launch vehicles, supporting the development of high-efficiency and reusable heavy-lift propulsion systems.

Beijing-based LandSpace is a leading Chinese private space company. With its Zhuque-2 rocket, LandSpace became the world's first company to launch a methane-liquid oxygen rocket to Earth orbit in July 2023, ahead of U.S. rivals, including Elon Musk's SpaceX and Jeff Bezos' Blue Origin.

Credit: Landspace

Time: 29 seconds
Date: March 6, 2025

#NASA #Space #Satellites #Earth #LEO #China #中国 #LandSpace #蓝箭 #RocketEngineTests #RocketEngines #BF20 #蓝焱20 #FFSC #ReusableRockets #LaunchVehicles #MethaneLiquidOxygen #Methalox #CommercialSpace #CommercialSpaceflight #STEM #Education #HD #Video

Lunar Eclipse: March 3, 2026: View from Utah

Lunar Eclipse: March 3, 2026: View from Utah

Astrophotographer Alan Tough: "The Total Lunar Eclipse of March 3 wasn't visible from the UK, so I took advantage of a 'free' telescope (iTelescope T11) in Utah to capture a set of data for later processing. The Moon only just fitted into the FOV!"

Lunar eclipses occur at the full Moon phase. When Earth is positioned precisely between the Moon and Sun, Earth’s shadow falls upon the surface of the Moon, dimming it and sometimes turning the lunar surface a striking red over the course of a few hours. Each lunar eclipse is visible from half of Earth.

Learn more: https://science.nasa.gov/moon/eclipses/

Utah is a landlocked state in the Mountain West subregion of the Western United States. It is one of the Four Corners states, sharing a border with Arizona, Colorado, and New Mexico. It also borders Wyoming to the northeast, Idaho to the north, and Nevada to the west.

Image Credit: Alan Tough
Image Date: March 3, 2026
Release Date: March 6, 2026

#NASA #Space #Astronomy #Science #Sun #SolarSystem #Moon #Earth #LunarEclipse #Umbra #Penumbra #Utah #UnitedStates #Astrophotography #AlanTough #Astrophotographers #Americas #STEM #Education

Mars Images: Feb. 26-March 6, 2026 | NASA's Curiosity & Perseverance Rovers

Mars Images: Feb. 26-March 6, 2026 | NASA's Curiosity & Perseverance Rovers

MSL - sol 4821

MSL - sol 4821

MSL - sol 4821

Mars 2020 - sol 1790

Mars 2020 - sol 1790

MSL - sol 4826

MSL - sol 4820

Mars 2020 - sol 1792

Become a monthly Friends of NASA supporter on our website: 

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Friends of NASA (FoN) is an independent non-governmental organization (NGO) dedicated to building international support for peaceful space exploration, commerce, scientific discovery, and STEM education. 

We depend on public donations.

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Celebrating 13+ Years on Mars (2012-2025)

Mission Name: Mars Science Laboratory (MSL)

Rover Name: Curiosity

Main Job: To determine if Mars was ever habitable to microbial life. 

Launch: Nov. 6, 2011

Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 5+ Years on Mars

Mission Name: Mars 2020

Rover Name: Perseverance

Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.

Launch: July 30, 2020    

Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS

Processing: Kevin M. Gill

Image Release Dates: Feb. 26-March 6, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Paraselenic Circle and 22° Moon Halo: View from Yukon | Earth Science

Paraselenic Circle and 22° Moon Halo: View from Yukon | Earth Science

Astrophotographer Joel Weatherly: "Last night . . . we were treated to an exceptional display of atmospheric optics, complete with paraselenae, a full paraselenic circle, and a 22° Halo around the Moon."

When sunlight or moonlight reflects or refracts from ice crystals in the atmosphere, an optical phenomenon collectively known as ‘halo’ is produced. When there are plenty of nearly vertical hexagonal ice crystals in the sky, the surfaces of the ice crystals will reflect moonlight like mirrors. A paraselenic circle will be produced if moonlight is reflected.

Yukon is a territory of Canada, bordering British Columbia to the south, the Northwest Territories to the east, the Beaufort Sea to the north, and the U.S. state of Alaska to the west. It is Canada's westernmost and smallest territory by land area.

Image Credit: Joel Weatherly
Location: Yukon territory, Canada

Joel 's website: https://jweatherly.ca
Date: Feb. 28, 2026

#NASA #Science #SolarSystem #Planets #Earth #EarthScience #Atmosphere #Halos #Moon #ParaselenicCircles #Moonlight #IceCrystals #AtmosphericOptics #Yukon #Canada #Astrophotography #JoelWeatherly #Astrophotographer #CitizenScience #UnitedStates #STEM #Education

Planet Venus: 3D Surface Model Views | NASA Magellan Mission (1990-1994)

Planet Venus: 3D Surface Model Views | NASA Magellan Mission (1990-1994)

    A portion of western Eistla Regio is shown in this three dimensional, computer-generated view of the surface of Venus. This NASA Magellan image was released on April 22, 1992.

A portion of the eastern edge of Alpha Regio is displayed in this three-dimensional perspective view of the surface of Venus from NASA Magellan spacecraft.

Maat Mons is displayed in this three-dimensional perspective view of the surface of Venus taken by NASA Magellan. The viewpoint is located north of Maat Mons.

A portion of western Eistla Regio is displayed in this three-dimensional perspective view from NASA's Magellan spacecraft of the surface of Venus.

Maat Mons is displayed in this computer generated three-dimensional perspective of the surface of Venus. This NASA's Magellan image was released on April 22, 1992.

A portion of western Eistla Regio is shown in this three dimensional, computer-generated view of the surface of Venus. This NASA Magellan image was released on April 22, 1992.

A portion of western Eistla Regio is displayed in this three-dimensional perspective view of the surface of Venus. The viewpoint is located 1,310 kilometers (812 miles) southwest of Gula Mons at an elevation of 0.78 kilometer (0.48 mile). The view is to the northeast with Gula Mons appearing on the horizon. Gula Mons, a 3 kilometer (1.86 mile) high volcano, is located at approximately 22 degrees north latitude, 359 degrees east longitude. The impact crater Cunitz, named for the astronomer and mathematician Maria Cunitz, is visible in the center of the image. The crater is 48.5 kilometers (30 miles) in diameter and is 215 kilometers (133 miles) from the viewer's position.

Gula Mons is displayed in this computer-simulated view from NASA Magellan spacecraft of the surface of Venus.

NASA Magellan spacecraft synthetic aperture radar data has been combined with radar altimetry to develop a three-dimensional map of the Venusian surface. Rays cast in a computer intersect the surface to create a three-dimensional perspective view. Simulated color and a digital elevation map developed by the U.S. Geological Survey, are used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft.

NASA's Magellan spacecraft was deployed from the cargo bay of Space Shuttle Atlantis on May 5, 1989, and entered orbit of Venus on August 10, 1990. Over its mission, it took detailed measurements of the surface of the planet using its Radar System (RDRS) instrument. Magellan's mission ended on October 13, 1994.

Learn more about NASA's Magellan Mission:
https://science.nasa.gov/mission/magellan/
https://www.jpl.nasa.gov/missions/magellan/

Credit: NASA/JPL/Caltech
Released Dates: 1991-1996

#NASA #Space #Astronomy #Science #Planets #Venus #Geology #Volcanism #Volcanoes #MagellanMission #MagellanSpacecraft #SAR #SolarSystem #SpaceExploration #PlanetaryScience #ComputerScience #3DModels #USGS #JPL #Caltech #UnitedStates #STEM #Education

European Astronaut Sophie Adenot: Training | International Space Station

European Astronaut Sophie Adenot: Training | International Space Station

European Space Agency (ESA) astronaut Sophie Adenot began her training at the European Astronaut Center (EAC) in Cologne, Germany, where she studied spacecraft systems and crew operations—learning to think and act as an astronaut. Alongside this, she conditioned her body for spaceflight and prepared for the physical and operational demands of her mission.

Her preparation includes continuous medical training and support, neutral buoyancy training for spacewalks and immersive virtual reality sessions at ESA’s XR Lab.

This video features interviews with Bimba Hoyer, Flight Surgeon at ESA; Hervé Stevenin, Head of EVA & Parabolic Flight Training Unit and Head of the Neutral Buoyancy Facility; and Lionel Ferra, Software and Artificial Intelligence Team Leader at ESA.

Astronaut Sophie Adenot's Biography:
https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Astronauts/Sophie_Adenot

Follow Expedition 74:
https://blogs.nasa.gov/spacestation/

Expedition 74 Crew

Station Commander: Sergey-Kud Sverchkov (Russia)

Roscosmos (Russia) Flight Engineer: Sergei Mikaev

NASA Flight Engineer: Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Credit: European Space Agency (ESA)
Duration: 5 minutes, 42 seconds
Release Date: March 5, 2026

#NASA #Space #ISS #Astronauts #SophieAdenot #AstronautTraining #France #Europe #ESA #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #Expedition75 #STEM #Education #HD #Video

Exploring Planet Venus' Alpha Regio Region | NASA's DAVINCI Mission

Exploring Planet Venus' Alpha Regio Region | NASA's DAVINCI Mission

Scheduled to launch in the early 2030s, NASA's DAVINCI mission will explore Venus with a spacecraft and a descent probe. DAVINCI’s probe will be the first in the 21st century to brave Venus’ atmosphere as it descends from above the planet’s clouds down to its surface. The DAVINCI spacecraft will study Venus’ clouds and highlands during two flybys. It also will release a spherical probe, about 3 feet wide, that will plunge through the planet’s thick atmosphere and corrosive clouds, taking measurements and capturing high-resolution images of the Venusian surface as it descends below the clouds.

Alpha Regio is a region of Venus extending for about 1500 kilometers centered at 22°S, 5°E. The surface of the region is what is known as tessera, meaning a terrain that has been highly deformed and where the deformation strikes in multiple directions and is closely spaced. 

Like all tessera regions, it sits above the surrounding terrain at an elevation of 1 to 2 kilometers, and is heavily deformed by what appears to be contractional folding. Like most tessera units, the surrounding volcanic plains appear to have flowed around Alpha's margins and thus are younger than Alpha. An infrared map prepared by the Venus Express orbiter shows that the rocks on the Alpha Regio plateau are lighter in color and look old compared to the majority of the planet. On Earth, such light-colored rocks are usually granite and form continents.

Learn more about NASA's DAVINCI Mission
https://ssed.gsfc.nasa.gov/davinci/mission

Video credit: NASA’s Goddard Space Flight Center
James Tralie (ADNET Systems, Inc.): Producer, Editor
James Garvin (NASA, Chief Scientist Goddard): Scientist, 
Animators: Walt Feimer (eMITS), Jenny McElligott, Jonathan North (eMITS), Adriana Manrique Gutierrez (eMITS), Michael Lentz (eMITS), Krystofer Kim (eMITS)
Duration: 1 minute, 13 seconds
Release Date: March 5, 2026

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