Friday, March 28, 2025

Soyuz MS-27 Crew Members: USA & Russia | International Space Station

Soyuz MS-27 Crew Members: USA & Russia | International Space Station

Soyuz MS-27 crew members (from left) NASA astronaut Jonny Kim and Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritskiy pose for a portrait at the Gagarin Cosmonaut Training Center in Russia.
NASA astronaut and Soyuz MS-27 Flight Engineer Jonny Kim poses for a portrait in his Sokol launch and entry suit at the Gagarin Cosmonaut Training Center in Star City, Russia.
NASA astronaut and Soyuz MS-27 Flight Engineer Jonny Kim poses for a portrait in his Sokol launch and entry suit at the Gagarin Cosmonaut Training Center in Star City, Russia.
Roscosmos cosmonaut and Soyuz MS-27 Commander Sergey Ryzhikov of Russia poses for a portrait in his Sokol launch and entry suit at the Gagarin Cosmonaut Training Center in Star City, Russia.
Roscosmos cosmonaut and Soyuz MS-27 Commander Sergey Ryzhikov of Russia poses for a portrait in his Sokol launch and entry suit at the Gagarin Cosmonaut Training Center in Star City, Russia.
Roscosmos cosmonaut and Soyuz MS-27 Commander Sergey Ryzhikov of Russia poses for a portrait in his Sokol launch and entry suit at the Gagarin Cosmonaut Training Center in Star City, Russia.
Roscosmos cosmonaut and Soyuz MS-27 Commander Sergey Ryzhikov of Russia poses for a portrait in his Sokol launch and entry suit at the Gagarin Cosmonaut Training Center in Star City, Russia.
The Soyuz MS-27 mission patch representing the three crew members with Jonny Kim of NASA and Roscosmos cosmonauts Srgey Ryzhikov and Alexey Zubritskiy of Russia launching to the International Space Station aboard the Soyuz spacecraft from the Baikonur Cosmodrome in Kazakhstan.

During his first mission to the International Space Station, NASA astronaut Jonny Kim will serve as a flight engineer and member of the upcoming Expedition 72/73 crew. Kim will launch on the Russian Roscosmos Soyuz MS-27 spacecraft no earlier than April 8, 2025, accompanied by Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky of Russia. The trio will spend approximately eight months at the space station.

While aboard the orbiting laboratory, Kim will conduct scientific investigations and technology demonstrations to help prepare the crew for future space missions and provide benefits to people on Earth.

NASA selected Kim as an astronaut in 2017. After completing the initial astronaut candidate training, Kim supported mission and crew operations in various roles, including the Expedition 65 lead operations officer, T-38 operations liaison, and space station capcom chief engineer.

A native of Los Angeles, Kim is a United States Navy lieutenant commander and dual designated naval aviator and flight surgeon. Kim also served as an enlisted Navy SEAL. He holds a bachelor’s degree in Mathematics from the University of San Diego and a medical degree from Harvard Medical School in Boston, and completed his internship with the Harvard Affiliated Emergency Medicine Residency at Massachusetts General Hospital and Brigham and Women’s Hospital.

NASA Astronaut Jonny Kim's Biography:

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. The ISS has been the most politically complex space exploration program ever undertaken.


Image Credit: Gagarin Research & Test Cosmonaut Center (GCTC)
Release Date: March 28, 2025


#NASA #Space #ISS #Science #SoyuzMS27Spacecraft #Astronaut #JonnyKim #FlightEngineer #Pilot #NavalAviator #FlightSurgeon #KoreanAmerican #AsianAmerican #UnitedStates #Cosmonauts  #SrgeyRyzhikov #AlexeyZubritskiy #Russia #Россия #Roscosmos #Роскосмос #Expedition73 #SpaceLaboratory #HumanSpaceflight #InternationalCooperation #STEM #Education

Expedition 72: New Crew Members at Work & More | International Space Station

Expedition 72: New Crew Members at Work & More | International Space Station

NASA astronaut and Expedition 72 Flight Engineer Nichole Ayers inserts a cryogenic storage unit, called a dewar, containing blood samples collected from a crew member into a science freezer for preservation and later analysis. The Minus Eighty-Degree Laboratory Freezer for International Space Station, or MELFI, is a research freezer that maintains experiment samples at ultra-cold temperatures in microgravity.
NASA astronaut Nichole Ayers: "More science! After completing a blood draw (we are our own phlebotomists up here), we spun the tubes in a centrifuge and then put them in the MELFI (Minus Eighty Degree Laboratory Freezer) for later return to the ground. 
This study is looking at bone structure pre- and post-mission, as well as bone markers in the blood to help build a digital twin model that can aid in predictions of future bone evolution."
NASA astronaut and Expedition 72 Flight Engineer Nichole Ayers works inside the International Space Station's Kibo laboratory module loading software onto an Astrobee robotic free-flyer. The software is part of a technology investigation demonstrating an adaptor for docking and close approach sensing to connect both active and passive objects in space. Results may enable applications, such as satellite servicing, orbital refueling, spacecraft repair and upgrade, and in-orbit manufacturing.
Japan Aerospace Exploration Agency (JAXA) astronaut and Expedition 72 Flight Engineer Takuya Onishi is pictured inside the cargo-packed vestibule in between the International Space Station and the SpaceX Dragon crew spacecraft. Onishi was continuing to unpack cargo stowed inside Dragon that had docked to the orbital outpost the day before with him and fellow SpaceX Crew-9 members Anne McClain and Nichole Ayers of NASA, and Kirill Peskov of Roscosmos aboard.
NASA astronaut and Expedition 72 Flight Engineer Anne McClain works on hardware maintenance tasks inside the International Space Station's Kibo laboratory module. Behind McClain is Kibo's airlock where experiment hardware, such as external exposure investigations and CubeSats are staged before being placed outside the orbiting lab into the vacuum of space.
The Russian Soyuz MS-26 spacecraft that launched NASA astronaut Don Pettit and Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner to the International Space Station is pictured docked to the Rassvet module. The orbiting lab was soaring 260 miles above Turkmenistan near the Caspian Sea.
The Russian Soyuz MS-26 spacecraft that launched NASA astronaut Don Pettit and Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner to the International Space Station is pictured docked to the Rassvet module. The orbiting lab was soaring 260 miles above Turkmenistan near the Caspian Sea.
City lights dot the Canadian landscape underneath an atmospheric glow and an aurora borealis in this photograph taken from the International Space Station 262 miles above North America at approximately 12:15 a.m. local time on March 5, 2025.

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Roscosmos cosmonaut Alexey Ovchinin (Russia)
Roscosmos (Russia) Flight Engineers: Ivan Vagner, Kirill Peskov
NASA Flight Engineers: Don Pettit, 
Anne McClain, Nichole Ayers 
JAXA Flight Engineer: Takuya Onishi

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science

For more information about STEM on Station:
https://www.nasa.gov/stemonstation


Image Credit: NASA's Johnson Space Center (JSC)
Image Dates: March 5-24, 2025


#NASA #Space #ISS #Science #Earth #Aurora #Astronauts #Japan #日本 #JAXA #Cosmonauts #SoyuzCrewSpacecraft #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #MicrogravityResearch #InternationalCooperation #Expedition72 #UnitedStates #Canada #STEM #Education

Planet Mars Images: March 25-27, 2025 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: March 25-27, 2025 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1456
Mars 2020 - sol 1456
MSL - sol 4491
Mars 2020 - sol 1456
Mars 2020 - sol 1457
MSL - sol 4491
MSL - sol 4491
Mars 2020 - sol 1456

Celebrating 12+ Years on Mars (2012-2024)
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 4+ 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: March 25-27, 2025

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

NASA's Space to Ground: Transitional Period | Week of March 28, 2025

NASA's Space to Ground: Transitional Period | Week of March 28, 2025

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. On Friday, March 28, 2025, at 6:55 a.m. EDT, the S.S. Richard “Dick” Scobee Northrop Grumman Cygnus spacecraft was released from the Canadarm2 robotic arm. It earlier detached Cygnus from the Earth-facing port of the International Space Station’s Unity module. At the time of release, the station was flying about 260 miles over the Pacific Ocean. 

The Cygnus spacecraft successfully departed the space station more than seven and a half months after arriving at the microgravity laboratory to deliver about 8,200 pounds of supplies, scientific investigations, commercial products, hardware, and other cargo for NASA. 

Following a deorbit engine firing on Sunday, March 30, Cygnus will begin a planned destructive re-entry, in which the spacecraftfilled with trash packed by the station crewwill safely burn up in Earth’s atmosphere. 

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Roscosmos cosmonaut Alexey Ovchinin (Russia)
Roscosmos (Russia) Flight Engineers: Ivan Vagner, Kirill Peskov
NASA Flight Engineers: Don Pettit, 
Anne McClain, Nichole Ayers 
JAXA Flight Engineer: Takuya Onishi

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science

For more information about STEM on Station:
https://www.nasa.gov/stemonstation


Video Credit: NASA's Johnson Space Center (JSC)
Duration: 5 minutes
Release Date: March 28, 2025


#NASA #Space #ISS #Science #CygnusCargoSpacecraft #Canadarm2 #Canada #Astronauts #Japan #日本 #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #MicrogravityResearch #InternationalCooperation #Expedition72 #UnitedStates #STEM #Education #HD #Video

Thursday, March 27, 2025

NASA Artemis II Moon Rocket Integration Update | Kennedy Space Center

NASA Artemis II Moon Rocket Integration Update | Kennedy Space Center








Teams with NASA’s Exploration Ground Systems (EGS) and primary contractor Amentum, integrate the Space Launch System (SLS) Moon rocket with the solid rocket boosters onto mobile launcher 1 inside High Bay 3 of the Vehicle Assembly Building at NASA’s Kennedy Space Center on Sunday, March 23, 2025. 

The twin solid boosters, five segments on each side, will help support the remaining rocket components and the Orion spacecraft during final assembly of the Artemis II Moon rocket and provide more than 75 percent of the total SLS thrust during liftoff from NASA Kennedy’s Launch Pad 39B.

The Artemis II test flight will be sending NASA astronauts Victor Glover, Christina Koch, and Reid Wiseman, as well as Canadian Space Agency (CSA) astronaut Jeremy Hansen, on a ten-day journey around the Moon and back.

Artemis II will launch no earlier than April 2026.

Check the NASA Artemis II Mission page for updates:

Learn more about NASA's Space Launch System (SLS) rocket: nasa.gov/sls

Follow updates on the Artemis blog: 

Image Credit: NASA's Kennedy Space Center (KSC)/Frank Michaux
Release Date: March 22, 2025

#NASA #ESA #Space #Moon #ArtemisProgram #ArtemisII #CrewedMission #Astronauts #NASASLS #SpaceLaunchSystem #SRB #DeepSpace #MoonToMars #Science #SpaceEngineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NorthropGrumman #KSC #Florida #UnitedStates #Europe #STEM #Education

Close-up | Jetting into Space: Protostars HOPS 150 & 153 in Orion | Hubble

Close-up | Jetting into Space: Protostars HOPS 150 & 153 in Orion | Hubble


This NASA/European Space Agency Hubble Space Telescope picture peers into the dusty recesses of the nearest massive star-forming region to Earth, the Orion Nebula. Just 1,300 light-years away, the Orion Nebula is visible to the naked eye below the three stars that form the ‘belt’ in the constellation Orion. The nebula is home to hundreds of newborn stars, including the subject of this imagethe protostars HOPS 150 and HOPS 153.

These protostars get their names from the Herschel Orion Protostar Survey. It was carried out with the European Space Agency’s Herschel Space Observatory. The object that can be seen in the upper-right corner of this image is HOPS 150. It is a binary system, two young protostars orbiting each other. Each has a small, dusty disc of material surrounding it that it is feeding from. The dark line that cuts across the bright glow of these protostars is a cloud of gas and dust, over 2,000 times wider than the distance between Earth and the Sun, falling in on the pair of protostars. Based on the amount of infrared versus other wavelengths of light HOPS 150 is emitting, the protostars are mid-way down the path to becoming mature stars.

Extending across the left side of the image is a narrow, colorful outflow called a jet. This jet comes from the nearby protostar HOPS 153, out of frame. HOPS 153 is a significantly younger stellar object than its neighbor, still deeply embedded in its birth nebula and enshrouded by a cloud of cold, dense gas. While Hubble cannot penetrate this gas to see the protostar, the jet HOPS 153 has emitted is brightly visible as it plows into the surrounding gas and dust of the Orion Nebula.

The transition from tightly swaddled protostar to fully fledged star will dramatically affect HOPS 153’s surroundings. As gas falls onto the protostar, its jets spew material and energy into interstellar space, carving out bubbles and heating the gas. By stirring up and warming nearby gas, HOPS 153 may regulate the formation of new stars in its neighborhood and even slow its own growth.

Image Description: An area in the Orion nebula filled with dark, puffy clouds. On the left side a large area of clouds, crossed by a dark bar, is lit up in red and whitish colors by a protostar within. At the other side a large jet of material ejected by the protostar appears, made of thin, wispy, blue and pink clouds. A couple of foreground stars shine brightly in front of the nebula.


Credit: ESA/Hubble & NASA, T. Megeath
Duration: 30 seconds
Release Date: Jan. 13, 2025


#NASA #ESA #Astronomy #Space #Science #Hubble #Nebulae #Nebula #Protostars #HOPS150 #HOPS153 #StellarJet #Orion #Constellation #MilkyWayGalaxy #Cosmos #Universe #HST #HubbleSpaceTelescope #STScI #GSFC #UnitedStates #HerschelSpaceObservatory #Europe #STEM #Education #HD #Video

Finding Clues in Ancient Dead Star's Ruins | NASA's Chandra X-ray Observatory

Finding Clues in Ancient Dead Star's Ruins NASA's Chandra X-ray Observatory

People often think about archaeology happening deep in jungles or inside ancient pyramids. However, a team of astronomers has shown that they can use stars and the remains they leave behind to conduct a special kind of archaeology in space.

Mining data from NASA’s Chandra X-ray Observatory, the team of astronomers studied the relics that one star left behind after it exploded. This “supernova archaeology” result uncovers important clues about a star that self-destructed—probably more than a million years ago.

Today, the system called GRO J1655-40 contains a black hole with nearly seven times the mass of the Sun and a star with about half as much mass. However, this was not always the case.

Originally GRO J1655-40 had two shining stars. The more massive of the two stars, however, burned through all of its nuclear fuel and then exploded in what astronomers call a supernova. The debris from the destroyed star then rained onto the companion star in orbit around it.

With its outer layers expelled, including some striking its neighbor, the rest of the exploded star collapsed onto itself and formed the black hole that exists today. Over time, the black hole and companion star moved closer. When the separation became small enough, the black hole, with its strong gravitational pull, began pulling matter from its companion, wrenching back some of the material its exploded parent star originally deposited.

While most of this material sank into the black hole, a small amount of it fell into a disk that orbits around the black hole. Through the effects of powerful magnetic fields and friction in the disk, material is being sent out into interstellar space in the form of powerful winds.

This is where the X-ray archaeological hunt enters the story. Astronomers used Chandra to observe the GRO J1655-40 system in 2005 when it was particularly bright in X-rays. Chandra detected signatures of individual elements found in the black hole’s winds by getting detailed spectra—giving X-ray brightness at different wavelengths—embedded in the X-ray light.

The team of astronomers digging through the Chandra data were able to reconstruct key physical characteristics of the star that exploded from the clues imprinted in the X-ray light by comparing the spectra with computer models of stars that explode as supernovae. They discovered that the long-gone star destroyed in the supernova was about 25 times the mass of the Sun. It was also much richer in elements heavier than helium in comparison with the Sun.

Look for more supernova archaeology stories with Chandra in the future!


Video Credit: NASA's Chandra X-ray Observatory
Duration: 3 minutes, 25 seconds
Release Date: March 27, 2025

#NASA #Space #Astronomy #Science #Stars #Star #Supernova #GROJ165540 #GROJ165540System #Scorpius #Constellation #Universe #NASAChandra #ChandraObservatory #XrayAstronomy #MSFC #SpaceTelescope #JPL #UnitedStates #STEM #Education #HD #Video

Planet Earth: Arctic Sea Ice Maximum 2025 | NASA Goddard

Planet Earth: Arctic Sea Ice Maximum 2025 | NASA Goddard

Winter sea ice cover in the Arctic was the lowest it has ever been at its annual peak on March 22, 2025, according to NASA and the National Snow and Ice Data Center (NSIDC) at the University of Colorado, Boulder. At 5.53 million square miles (14.33 million square kilometers), the maximum extent fell below the prior low of 5.56 million square miles (14.41 million square kilometers) in 2017.

Learn more about Climate Change at NASA: 
https://science.nasa.gov/climate-change/

NASA's Goddard Institute for Space Studies (GISS)


Credit: NASA's Goddard Space Flight Center/Scientific Visualization Studio
Charles Connell (NASA Intern): Lead Producer
Grace Weikert (eMITS): Producer
James Riordon (NASA/GSFC): Lead Writer
Walt Meier (NASA/GSFC): Lead Scientist
Audrey Payne (NASA/GSFC GISS): Scientist
Trent L. Schindler (URSA): Visualizer
Mark SubbaRao (NASA/GSFC): Visualizer
Katie Jepson (eMITS): Project Support
Jefferson Beck (eMITS): Videographer
Sofie Bates (eMITS): Social Media Support
Aaron E. Lepsch (ADNET): Technical Support
Duration: 2 hours, 25 minutes
Release Date: March 27, 2025

#NASA #Space #Satellites #Science #Planet #Earth #Arctic #ArcticOcean #Antarctica #SouthernOcean #SeaIce #Winter2025 #MeltingIce #Environment #ClimateChange #GlobalWarming #GlobalHeating #Atmosphere #EarthObservation #RemoteSensing #GSFC #UnitedStates #History #STEM #Education #HD #Video

Close-up: Two Galaxies and an Einstein Ring | Webb Telescope

Close-up: Two Galaxies and an Einstein Ring | Webb Telescope

This new NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope picture features a rare cosmic phenomenon called an Einstein ring. What at first appears to be a single, strangely shaped galaxy is actually two galaxies that are separated by a large distance. The closer foreground galaxy sits at the center of the image, while the more distant background galaxy appears to be wrapped around the closer galaxy, forming a ring. 

Einstein rings occur when light from a very distant object is bent (or ‘lensed’) about a massive intermediate (or ‘lensing’) object. This is possible because spacetime, the fabric of the Universe itself, is bent by mass, and therefore light travelling through space and time is bent as well. This effect is much too subtle to be observed on a local level, but it sometimes becomes clearly observable when dealing with curvatures of light on enormous, astronomical scales, such as when the light from one galaxy is bent around another galaxy or galaxy cluster.

When the lensed object and the lensing object line up just so, the result is the distinctive Einstein ring shape. It appears as a full circle (as seen here) or a partial circle of light around the lensing object, depending on the precision of the alignment. Objects like these are the ideal laboratory in which to research galaxies too faint and distant to otherwise see.

The lensing galaxy at the center of this Einstein ring is an elliptical galaxy, as can be seen from the galaxy’s bright core and smooth, featureless body. This galaxy belongs to a galaxy cluster named SMACSJ0028.2-7537. The lensed galaxy wrapped around the elliptical galaxy is a spiral galaxy. Even though its image has been warped as its light travelled around the galaxy in its path, individual star clusters and gas structures are clearly visible.

The Webb data used in this image were taken as part of the Strong Lensing and Cluster Evolution (SLICE) survey (program 5594), which is led by Guillaume Mahler at University of Liège in Belgium, and consists of a team of international astronomers. This survey aims to trace 8 billion years of galaxy cluster evolution by targeting 182 galaxy clusters with Webb’s Near-InfraRed Camera instrument. This image also incorporates data from two of the NASA/European Space Agency Hubble Space Telescope’s instruments, the Wide Field Camera 3 and the Advanced Camera for Surveys.

Image Description: In the center is an elliptical galaxy, seen as an oval-shaped glow around a small bright core. Around this is wrapped a broad band of light, appearing like a spiral galaxy stretched and warped into a ring, with bright blue lines drawn through it where the spiral arms have been stretched into circles. A few distant objects are visible around the ring on a black background.


Credit: ESA/Webb, NASA & CSA, G. Mahler
Acknowledgement: M. A. McDonald
Duration: 30 seconds
Release Date: March 27, 2025

#NASA #ESA #Astronomy #Space #Science #JWST #JamesWebb #WebbTelescope #Galaxies #Galaxy #EinsteinRing #GravitationalLensing #GalaxyClusters #Hydrus #Constellation #Universe #UnfoldTheUniverse #InfraredAstronomy #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Two Galaxies and an Einstein Ring: Gravitational Lensing in Action | Webb Telescope

Two Galaxies and an Einstein Ring: Gravitational Lensing in Action | Webb Telescope


This new NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope picture features a rare cosmic phenomenon called an Einstein ring. What at first appears to be a single, strangely shaped galaxy is actually two galaxies that are separated by a large distance. The closer foreground galaxy sits at the center of the image, while the more distant background galaxy appears to be wrapped around the closer galaxy, forming a ring. 

Einstein rings occur when light from a very distant object is bent (or ‘lensed’) about a massive intermediate (or ‘lensing’) object. This is possible because spacetime, the fabric of the Universe itself, is bent by mass, and therefore light travelling through space and time is bent as well. This effect is much too subtle to be observed on a local level, but it sometimes becomes clearly observable when dealing with curvatures of light on enormous, astronomical scales, such as when the light from one galaxy is bent around another galaxy or galaxy cluster.

When the lensed object and the lensing object line up just so, the result is the distinctive Einstein ring shape. It appears as a full circle (as seen here) or a partial circle of light around the lensing object, depending on the precision of the alignment. Objects like these are the ideal laboratory in which to research galaxies too faint and distant to otherwise see.

The lensing galaxy at the center of this Einstein ring is an elliptical galaxy, as can be seen from the galaxy’s bright core and smooth, featureless body. This galaxy belongs to a galaxy cluster named SMACSJ0028.2-7537. The lensed galaxy wrapped around the elliptical galaxy is a spiral galaxy. Even though its image has been warped as its light travelled around the galaxy in its path, individual star clusters and gas structures are clearly visible.

The Webb data used in this image were taken as part of the Strong Lensing and Cluster Evolution (SLICE) survey (program 5594), which is led by Guillaume Mahler at University of Liège in Belgium, and consists of a team of international astronomers. This survey aims to trace 8 billion years of galaxy cluster evolution by targeting 182 galaxy clusters with Webb’s Near-InfraRed Camera instrument. This image also incorporates data from two of the NASA/European Space Agency Hubble Space Telescope’s instruments, the Wide Field Camera 3 and the Advanced Camera for Surveys.

Image Description: In the center is an elliptical galaxy, seen as an oval-shaped glow around a small bright core. Around this is wrapped a broad band of light, appearing like a spiral galaxy stretched and warped into a ring, with bright blue lines drawn through it where the spiral arms have been stretched into circles. A few distant objects are visible around the ring on a black background.


Credit: ESA/Webb, NASA & CSA, G. Mahler
Acknowledgement: M. A. McDonald
Release Date: March 27, 2025

#NASA #ESA #Astronomy #Space #Science #JWST #JamesWebb #WebbTelescope #Galaxies #Galaxy #EinsteinRing #GravitationalLensing #GalaxyClusters #Hydrus #Constellation #Universe #UnfoldTheUniverse #InfraredAstronomy #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Espacio A Tierra | Cambio de turno: 21 de marzo 2025

NASA Espacio A Tierra | Cambio de turno: 21 de marzo 2025


Espacio a Tierra, la versión en español de las cápsulas Space to Ground de la NASA, te informa semanalmente de lo que está sucediendo en la Estación Espacial Internacional.

Aprende más sobre la ciencia a bordo de la estación espacial: https://www.nasa.gov/international-space-station/space-station-research-and-technology/ciencia-en-la-estacion/

Ciencia de la NASA: https://ciencia.nasa.gov

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: 
https://www.nasa.gov/suscribete

Producción: NASA
Duration: 4 minutes, 25 seconds
Release Date: March 26, 2025


#NASA #Space #ISS #Science #Earth #NASAenespañol #español #Astronauts #AnneMcClain #NicholeAyers #TakuyaOnishi #Japan #日本 #Cosmonaut #KirillPeskov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition72 #UnitedStates #STEM #Education #HD #Video

Wednesday, March 26, 2025

Aurora Borealis over Finland | Geomagnetic Storm in Progress

Aurora Borealis over Finland | Geomagnetic Storm in Progress






Sebastian Sainio: "I did not expect this! I was out photographing some pretty normal green auroras in the local area on the night of the 26th of March 2025 when all off the sudden the sky burst into flames and this beautiful corona can bee seen here behind a radio tower."

Image details: Canon EOS R6 + Irix 15mm f/2.4 Firefly

Aurora Colors According to Altitude
Above 150 miles: red, oxygen
Up to 150 miles: green, oxygen
Above 60 miles: purple or violet, nitrogen
Up to 60 miles: blue, nitrogen

The Colors of the Aurora (National Park Service)
https://www.nps.gov/articles/-articles-aps-v8-i1-c9.htm

Image Credit: Sebastian Sainio 
Location: Veikars, Finland
Release Date: March 26, 2025

#NASA #Space #Astronomy #Science #Earth #Planet #Atmosphere #Aurora #AuroraBorealis #NorthernLights #MagneticField #Magnetosphere #SolarWind #Sun #Heliophysics #Veikars #Finland #ArcticCircle #Photography #SebastianSainio #Astrophotography #STEM #Education

Accelerating Progress Toward Sustainable Flight | NASA Aeronautics

Accelerating Progress Toward Sustainable Flight | NASA Aeronautics

NASA Aeronautics is engaging with industry, academia, and other agencies through the Sustainable Flight National Partnership, accelerating U.S. progress toward up to 30% less fuel use in future airliner designs leading to significant economic benefits.

Learn more about NASA Aeronautics:
https://www.nasa.gov/aeronautics/


Video Credit: National Aeronautics and Space Administration (NASA)
Duration: 52 seconds
Release Date: March 26, 2025

#NASA #NASAAeronautics #Earth #Aerospace #Flight #Aviation #Aircraft #Boeing #BoeingAircraft #Airliners #FuelEconomy #SustainableAviation #Engineering #CivilianResearch #AeronauticalResearch #FlightTests #NeilArmstrong #AFRC #EdwardsAFB #NASAAmes #California #UnitedStates #STEM #Education #HD #Video

Prototype Immersive Technologies Lab Supporting NASA Artemis Moon Missions

Prototype Immersive Technologies Lab Supporting NASA Artemis Moon Missions

"What’s Behind This Door?" takes you behind the doors of various facilities located at NASA's Johnson Space Center in Houston being used to return humanity to the Moon, through the Artemis campaign. The series features interviews with NASA experts and provides a rare insight into all the preparation as teams get ready for lunar missions. This episode takes place in Building 16 at NASA Johnson in the Prototype Immersive Technologies (PIT) Lab. It provides a space for concept operations development, evaluation and testing. It features simulation software engineer Billy Young. He demonstrates how virtual reality provides an immersive experience to train NASA astronauts for Artemis missions where they will experience challenging lighting conditions caused by permanently shadowed regions.


Video Credit: NASA's Johnson Space Center (JSC)
Duration: 4 minute, 32 seconds
Release Date: March 24, 2025

#NASA #Space #Astronomy #Science #Earth #Moon #ArtemisProgram #SpaceSimulation #VirtualReality #Laboratory #PrototypeImmersive TechnologiesLab #PITLab #NASAJohnson #JSC #Houston #Texas #UnitedStates #HumanSpaceflight #SpaceTechnology #Engineering #STEM #Education #HD #Video

Geology Training for Lunar Exploration | Preparing for NASA Artemis Missions

Geology Training for Lunar Exploration Preparing for NASA Artemis Missions

From the volcanic fields of Arizona to the lunar-like landscape of Iceland, NASA scientists are actively preparing astronauts and mission support teams for conducting science on the Moon.

Learn about NASA’s rich history of geology training and hear how scientists and engineers are getting ready to bring back samples that will help us learn about the origins of our solar system.

0:00 Introduction

0:56 Apollo to Artemis

2:36 Training

4:33 Testing

7:57 Preparing for Samples

9:30 The Future


Credit: NASA
Producers: Rachel Barry, Nicole Rose
Duration: 11 minutes
Release Date: March 26, 2025

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How NASA’s Perseverance Rover is Helping Prepare Astronauts for Mars | JPL

How NASA’s Perseverance Rover is Helping Prepare Astronauts for Mars | JPL

NASA’s Perseverance Mars rover, with a circle indicating the location of the calibration target for the rover’s SHERLOC instrument. At right is a close-up of the calibration target. Along the bottom row are five swatches of spacesuit materials that scientists are studying as they degrade.

This graphic shows an illustration of a prototype astronaut suit, left, along with suit samples included aboard NASA’s Perseverance rover. They are the first spacesuit materials ever sent to Mars.

NASA’s Perseverance rover landed on Mars in 2021 to search for signs of ancient microbial life and to help scientists understand the planet’s climate and geography. However, another key objective is to pave the way for human exploration of Mars, and as part of that effort, the rover carries a set of five spacesuit material samples. Now, after those samples have endured four years of exposure on Mars’ dusty, radiation-soaked surface, scientists are beginning the next phase of studying them.

The end goal is to predict accurately the usable lifetime of a Mars spacesuit. What the agency learns about how the materials perform on Mars will inform the design of future spacesuits for the first astronauts on the Red Planet.

“This is one of the forward-looking aspects of the rover’s mission—not just thinking about its current science, but also about what comes next,” said planetary scientist Marc Fries of NASA’s Johnson Space Center in Houston, who helped provide the spacesuit materials. “We’re preparing for people to eventually go and explore Mars.”

The swatches, each three-quarters of an inch square (20 millimeters square), are part of a calibration target used to test the settings of SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals), an instrument on the end of Perseverance’s arm.

The samples include a piece of polycarbonate helmet visor; Vectran, a cut-resistant material used for the palms of astronaut gloves; two kinds of Teflon that has dust-repelling nonstick properties; and a commonly used spacesuit material called Ortho-Fabric. This last fabric features multiple layers, including Nomex, a flame-resistant material found in firefighter outfits; Gore-Tex, which is waterproof but breathable; and Kevlar, a strong material used in bulletproof vests that makes spacesuits more rip-resistant.

Martian Wear and Tear

Mars is far from hospitable. It has freezing temperatures, fine dust that can stick to solar panels and spacesuits (causing wear and tear on the latter), and a surface rife with perchlorates, a kind of corrosive salt that can be toxic to humans.

There is also lots of solar radiation. Unlike Earth, which has a magnetic field that deflects much of the Sun’s radiation, Mars lost its magnetic field billions of years ago, followed by much of its atmosphere. Its surface has little protection from the Sun’s ultraviolet light (which is why researchers have looked into how rock formations and caves could provide astronauts some shielding).

“Mars is a really harsh, tough place,” said SHERLOC science team member Joby Razzell Hollis of the Natural History Museum in London. “Don’t underestimate that—the radiation in particular is pretty nasty.”

Razzell Hollis was a postdoctoral fellow at NASA’s Jet Propulsion Laboratory in Southern California from 2018 to 2021, where he helped prepare SHERLOC for arrival on Mars and took part in science operations once the rover landed. A materials scientist, Razzell Hollis has previously studied the chemical effects of sunlight on a new kind of solar panel made from plastic, as well as on plastic pollution floating in the Earth’s oceans.

He likened those effects to how white plastic lawn chairs become yellow and brittle after years in sunlight. Roughly the same thing happens on Mars, but the weathering likely happens faster because of the high exposure to ultraviolet light there.

The key to developing safer spacesuit materials will be understanding how quickly they would wear down on the Martian surface. About 50% of the changes SHERLOC witnessed in the samples happened within Perseverance’s first 200 days on Mars, with the Vectran appearing to change first.

Another nuance will be figuring out how much solar radiation different parts of a spacesuit will have to withstand. For example, an astronaut’s shoulders will be more exposed—and likely encounter more radiation—than his or her palms.

Next Steps

The SHERLOC team is working on a science paper detailing initial data on how the samples have fared on Mars. Meanwhile, scientists at NASA Johnson are eager to simulate that weathering in special chambers that mimic the carbon dioxide atmosphere, air pressure, and ultraviolet light on the Martian surface. They could then compare the results generated on Earth while putting the materials to the test with those seen in the SHERLOC data. For example, the researchers could stretch the materials until they break to check if they become more brittle over time.

“The fabric materials are designed to be tough but flexible, so they protect astronauts but can bend freely,” Fries said. “We want to know the extent to which the fabrics lose their strength and flexibility over time. As the fabrics weaken, they can fray and tear, allowing a spacesuit to leak both heat and air.”

More About Perseverance

A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover is characterizing the planet’s geology and past climate, to help pave the way for human exploration of the Red Planet, and is the first mission to collect and cache Martian rock and regolith.

NASA’s Mars Sample Return Program, in cooperation with European Space Agency (ESA), is designed to send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.

The Mars 2020 Perseverance mission is part of NASA’s Mars Exploration Program (MEP) portfolio and the agency’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

Celebrating 4+ 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

Credit: NASA/JPL-Caltech/MSSS
Release Date: March 26, 2025

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