NASA's SpaceX Crew-11 Members | International Space Station
Capture Dates: Sept. 25, 2024 & Dec. 4, 2024
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NASA's SpaceX Crew-11 Members | International Space Station
The Lyra Constellation
Capture location: San Pasquale, Viggianello, Basilicate, Italy
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Meet NASA Astronaut & Flight Engineer Jonny Kim | International Space Station
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 astronaut Jonny Kim is a member of the Artemis Team, a select group of astronauts charged with focusing on the development and training efforts for early Artemis missions. Through the Artemis program, NASA and a coalition of international partners will return to the Moon to learn how to live on other worlds for the benefit of all. We will use the Moon and its resources as a technology testbed to go even farther and to learn how to establish and sustain a human presence far beyond 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.
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Soyuz MS-27 Crew Members: USA & Russia | International Space Station
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.
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.
#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
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
Planet Mars Images: March 25-27, 2025 | NASA's Curiosity & Perseverance Rovers
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 spacecraft—filled with trash packed by the station crew—will safely burn up in Earth’s atmosphere.
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 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.
Close-up | Jetting into Space: Protostars HOPS 150 & 153 in Orion | Hubble
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.
#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
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!
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.
Close-up: Two Galaxies and an Einstein Ring | Webb Telescope
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.
Two Galaxies and an Einstein Ring: Gravitational Lensing in Action | Webb Telescope
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.
NASA Espacio A Tierra | Cambio de turno: 21 de marzo 2025
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
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Aurora Borealis over Finland | Geomagnetic Storm in Progress
Image details: Canon EOS R6 + Irix 15mm f/2.4 Firefly
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.