Sunday, February 02, 2025

Nuclear Electric Propulsion Technology: Making Mars Missions Faster | NASA

Nuclear Electric Propulsion Technology: Making Mars Missions Faster | NASA

An artist’s rendering that shows the different components of a fully assembled nuclear electric propulsion system.

Modular Assembled Radiators for Nuclear Electric Propulsion Vehicles, or MARVL, aims to take a critical element of nuclear electric propulsion, its heat dissipation system, and divide it into smaller components that can be assembled robotically and autonomously in space. This is an artist’s rendering of what the fully assembled system might look like.

There are technologies that could help transport a crew on a round-trip journey in a relatively quick two years. One option NASA is exploring is nuclear electric propulsion. It employs a nuclear reactor to generate electricity that ionizes, or positively charges, and electrically accelerates gaseous propellants to provide thrust to a spacecraft.

Researchers at NASA’s Langley Research Center in Hampton, Virginia, are working on a system that could help bring nuclear electric propulsion one significant, technology-defining step closer to reality.

MARVL aims to take a critical element of nuclear electric propulsion, its heat dissipation system, and divide it into smaller components that can be assembled robotically and autonomously in space.

“By doing that, we eliminate trying to fit the whole system into one rocket fairing,” said Amanda Stark, a heat transfer engineer at NASA Langley and the principal investigator for MARVL. “In turn, that allows us to loosen up the design a little bit and really optimize it.”

Opening up the design is key, because as Stark mentioned, previous ideas called for fitting the entire nuclear electric radiator system under a rocket fairing, or nose cone that covers and protects a payload. Fully deployed, the heat dissipating radiator array would be roughly the size of a football field. You can imagine the challenge engineers would face in getting such a massive system folded up neatly inside the tip of a rocket.

The MARVL technology opens a world of possibilities. Rather than fitting the entire system into an existing rocket, this would allow researchers the flexibility to send pieces of the system to space in whatever way would make the most sense, and then having it all assembled off planet.

Once in space, robots could connect the nuclear electric propulsion system’s radiator panels where a liquid metal coolant, such as a sodium-potassium alloy, would flow.

While this is still an engineering challenge, it is exactly the kind of engineering challenge in-space-assembly experts at NASA's Langley Research Center in Hampton, Virginia have been working on for decades. The MARVL technology could mark a significant first milestone. Rather than being an add-on to an existing technology, the in-space assembly component will benefit and influence the design of the spacecraft it would support.

“Existing vehicles have not previously considered in-space assembly during the design process, so we have the opportunity here to say, ‘We’re going to build this vehicle in space. How do we do it? And what does the vehicle look like if we do that?’ I think it’s going to expand what we think of when it comes to nuclear propulsion,” said Julia Cline, a mentor for the project in NASA Langley’s Research Directorate, who led the center’s participation in the Nuclear Electric Propulsion tech maturation plan development as a precursor to MARVL. This tech maturation plan was run out of the agency’s Space Nuclear Propulsion project at NASA's Marshall Space Flight Center in Huntsville, Alabama.

NASA’s Space Technology Mission Directorate awarded the MARVL project through the Early Career Initiative, giving the team two years to advance the concept. Stark and her teammates are working with an external partner, Boyd Lancaster, Inc., to develop the thermal management system. The team also includes radiator design engineers from NASA’s Glenn Research Center in Cleveland and fluid engineers from NASA’s Kennedy Space Center in Florida. After two years, the team hopes to move the MARVL design to a small-scale ground demonstration.

The idea of robotically building a nuclear propulsion system in space is sparking imaginations.

“One of our mentors remarked, ‘This is why I wanted to work at NASA, for projects like this,’” said Stark, “which is awesome because I am so happy to be involved with it, and I feel the same way.”

Additional support for MARVL comes from the agency’s Space Nuclear Propulsion project. The project’s ongoing effort is maturing technologies for operations around the Moon and near-Earth exploration, deep space science missions, and human exploration using nuclear electric propulsion and nuclear thermal propulsion.

Learn more:

ECI Modular Assembled Radiators for NEP VehicLes (MARVL), an Overview
https://tfaws.nasa.gov/wp-content/uploads/TFAWS2024-ID-22.pdf

Ideas for Infusing In-Space Servicing, Assembly, and Manufacturing Concepts into Nuclear Electric Propulsion Architectures


Image Credit: NASA/Tim Marvel
Article Credit: NASA Langley Research Center
Release Date: Jan. 10, 2025

#NASA #Space #Astronomy #Science #Planets #Mars #Earth #HumanSpaceflight #MarsMissions #Spacecraft #SpacecraftPropulsion #MARVLTechnology #NuclearElectricPropulsion #SpaceTechnology #Engineering #DeepSpace #SolarSystem #SpaceExploration #Art #Illustrations #NASALangley #NASAGlenn #MSFC #KSC #UnitedStates #STEM #Education

Saying Goodbye to Comet C/2024 G3 ATLA

Saying Goodbye to Comet C/2024 G3 ATLAS

What is happening to Comet G3 ATLAS? After passing near the Sun in mid-January 2025, the head of the comet has become dimmer and dimmer. By late January, Comet C/2024 G3 (ATLAS) had become a headless wonder—although it continued to show impressive tails after sunset in the skies of Earth's Southern Hemisphere. A key reason is likely that the comet's nucleus of ice and rock, at the head's center, has fragmented. Comet G3 ATLAS passed well inside the orbit of planet Mercury when at its solar closest, a distance that where heat destroys many comets. Some of comet G3 ATLAS' scattering remains will continue to orbit the Sun . . .

C/2024 G3 ATLAS is a non-periodic comet. It reached perihelion (closest approach to the Sun) on January 13, 2025, at a distance of 0.09 AU (13 million km) from the Sun. It is potentially the brightest comet of 2025, with an apparent magnitude reaching −3.8 on the day of its perihelion.

Comet C/2024 G3 was found by the automated Asteroid Terrestrial-impact Last Alert System (ATLAS) on April 5, 2024, in images obtained with a 0.5-m reflector telescope located in Río Hurtado, Chile. ATLAS is funded by NASA's Planetary Defense Office. ATLAS was developed and is operated by the University of Hawaii's Institute for Astronomy.

Astrophotographer Ian Inverarity: "Refining my comet shooting technique after the dramas of last time. I used a Nikon D810A with a Sigma Art 135mm lens at f/2, ISO200, 27 x 30 second shots during and beyond astro twilight. The camera was on a ZWO AM5, I used the ZWO ASIAIR Mini to polar align, then get my framing where I was happy with it, and ran the autofocus routine with a ZWO EAF connected to the lens. Once that was done, I ran unguided in continuous exposure mode with a wired shutter release that locks on, while I shot landscape astro comet shots with the other camera. For processing I used APP, I didn't do any comet alignment. I removed much of the astro twilight colour from the sky and with more subs the satellites are almost gone. The artifact on the bottom right is from the ground getting in the frame! Final processing in Photoshop."


Image Credit: Ian Inverarity
Capture Location: Western Australia
Image Date: Feb. 1, 2025


#NASA #Space #Astronomy #Science #Planet #Earth #Comets #Comet #CometC2024G3ATLAS #C2024G3 #OortCloud #SolarSystem #Astrophotography #Astrophotographer #IanInverarity #Australia #WesternAustralia #PlanetaryDefense #JPL #UnitedStates #STEM #Education

Planet Mars Images: Jan. 30-Feb. 1, 2025 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: Jan. 30-Feb. 1, 2025 | NASA's Curiosity & Perseverance Rovers

MSL - sol 4439
MSL - sol 4437
Mars 2020 - sol 1404
Mars 2020 - sol 1403
Mars 2020 - sol 1404
Mars 2020 - sol 1405
Mars 2020 - sol 1404
MSL - sol 4439

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Celebrating 3+ 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

Celebrating 3+ 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 Date: Jan. 30-Feb. 1,2025

#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

Planet Mars: Shapes & Spots on a Polar Sand Dune | NASA MRO

Planet Mars: Shapes & Spots on a Polar Sand Dune | NASA MRO



This HiRISE image shows numerous dark shapes and bright spots on a sand dune in the Northern polar regions of Mars. The bright spots are carbon dioxide frost. On Mars, the main atmospheric component is carbon dioxide. This circulates seasonally between the atmosphere and the polar regions. One of the reasons that permit this process is the fact that temperatures on Mars are much colder than on Earth. This allows carbon dioxide frost to condense on the surface in winter.

When spring comes however, the surface heats up and the carbon dioxide frost eventually sublimates (turns directly from the solid to the vapor state), and forms jets of carbon dioxide mixed with dust, leading to the formation of the dark features we see in the image.

Such processes occur seasonally on Mars, and therefore are continuously being monitored by the HiRISE scientists to assess the differences from one year to the next.

This enhanced color images is 1 km across.

HiRISE, or the High Resolution Imaging Science Experiment, is a powerful camera that takes pictures covering vast areas of Martian terrain while being able to see features as small as a kitchen table.

Mars Reconnaissance Orbiter (MRO) is a spacecraft designed to study the geology and climate of Mars, to provide reconnaissance of future landing sites, and to relay data from surface missions back to Earth. It was launched on August 12, 2005, and reached Mars on March 10, 2006. 

The University of Arizona, in Tucson, operates HiRISE. It was built by BAE Systems in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

For more information on MRO, visit:

Video Credit: NASA/JPL-Caltech/University of Arizona
Narrator: Tre Gibbs
Caption Credit: M. Ramy El-Maarry
Duration: 55 seconds    
Capture Date: Dec. 1, 2013
Release Date: Jan. 22, 2014


#NASA #Space #Astronomy #Science #Mars #Planet #RedPlanet #Geology #Landscape #Terrain #Geoscience #SouthPole #SandDunes #CarbonDioxideIce #MRO #MarsOrbiter #MarsSpacecraft #HiRISECamera #JPL #Caltech #BallAerospace #MSSS #UnitedStates #STEM #Education #HD #Video

Chinese Scientists Discover "Space Chorus" Far from Planet Earth

Chinese Scientists Discover "Space Chorus" Far from Planet Earth

An international research team led by Chinese scientists from Beihang University has discovered chorus waves more than 160,000 km away from Earth—a space phenomena previously believed to occur only near Earth's dipole magnetic field regions, according to a study paper recently published in the scientific journal Nature.

The scientists observed chorus waves with frequencies below 100 Hz. When they converted the chorus waves into audio output, they obtained a piece of "space chorus" that human can hear. The scientists described the sound like "the chirping of birds".

"The space chorus is a kind of low-frequency electromagnetic waves found in space, with frequencies ranging from 100 Hz to several thousand Hz. Its frequency spectrum resembles the chorus of bird vocalizations we usually hear on Earth, and that's why we call it chorus," said Cao Jinbin, dean of the School of Space and Environment, Beihang University.

The Earth's magnetic field extends into space. When charged particles in the cosmos pass the magnetic field, they can excite chorus waves, or the electromagnetic waves with frequency characteristic similar to birdsongs in the morning.

As one of the most intense electromagnetic fluctuations in space, chorus waves have been at the forefront of space physics research. It was widely believed that they only occur near Earth's dipole magnetic field regions.

"Over the past seven decades, it was widely accepted that the wave exists only in near-Earth space, in the Earth's dipole magnetic field regions near the geosynchronous orbit. No one had ever considered the possibility that the wave could exist at a greater distance," said Liu Chengming, associate professor of the School of Space and Environment.

The team, which consists of researchers from China, the United States and Sweden, has analyzed vast amounts of data collected by the Magnetospheric Multiscale Mission, a solar-terrestrial probe mission.

Chorus waves play a crucial role in understanding fundamental questions in space and have wide practical implications. They are key to the acceleration of high-energy electrons in Earth's radiation belts and the generation of pulsating auroras in the polar regions. They can also influence space weather changes, endangering the stable operation of spacecraft and the health of astronauts.

These findings provide essential theoretical support for the precise modeling and forecasting of space weather, according to the study.


Video Credit: CCTV
Duration: 1 minute, 23 seconds
Release Date: Feb. 1, 2025

#NASA #Space #Astronomy #Science #Sun #SolarSystem #SolarWind #SpaceWeather #BeihangUniversity #北京航空航天大学 #ElectromagneticWaves #SpaceChorus #Heliophysics #Planet #Earth #Magnetosphere #China #中国 #Satellites #Universe #SpaceTechnology #SpaceExploration #InternationalCooperation #STEM #Education #Animation #Sonification #HD #Video

Saturday, February 01, 2025

Planet Mars: Shapes & Spots on a Polar Sand Dune | NASA MRO

Planet Mars: Shapes & Spots on a Polar Sand Dune | NASA MRO


This HiRISE image shows numerous dark shapes and bright spots on a sand dune in the Northern polar regions of Mars. The bright spots are carbon dioxide frost. On Mars, the main atmospheric component is carbon dioxide. This circulates seasonally between the atmosphere and the polar regions. One of the reasons that permit this process is the fact that temperatures on Mars are much colder than on Earth. This allows carbon dioxide frost to condense on the surface in winter.

When spring comes however, the surface heats up and the carbon dioxide frost eventually sublimates (turns directly from the solid to the vapor state), and forms jets of carbon dioxide mixed with dust, leading to the formation of the dark features we see in the image.

Such processes occur seasonally on Mars, and therefore are continuously being monitored by the HiRISE scientists to assess the differences from one year to the next.

This enhanced color images is 1 km across.

HiRISE, or the High Resolution Imaging Science Experiment, is a powerful camera that takes pictures covering vast areas of Martian terrain while being able to see features as small as a kitchen table.

Mars Reconnaissance Orbiter (MRO) is a spacecraft designed to study the geology and climate of Mars, to provide reconnaissance of future landing sites, and to relay data from surface missions back to Earth. It was launched on August 12, 2005, and reached Mars on March 10, 2006. 

The University of Arizona, in Tucson, operates HiRISE. It was built by BAE Systems in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

For more information on MRO, visit:

Image Credit: NASA/JPL-Caltech/University of Arizona
Caption Credit: M. Ramy El-Maarry  
Capture Date: Dec. 1, 2013
Release Date: Jan. 22, 2014


#NASA #Space #Astronomy #Science #Mars #Planet #RedPlanet #Geology #Landscape #Terrain #Geoscience #SouthPole #SandDunes #CarbonDioxideIce #MRO #MarsOrbiter #MarsSpacecraft #HiRISECamera #JPL #Caltech #BallAerospace #MSSS #UnitedStates #STEM #Education

February 2025 Skywatching Tips from NASA | JPL

February 2025 Skywatching Tips from NASA | JPL

Here are examples of skywatching highlights for the northern hemisphere in February 2025:

Venus blazes at its brightest in the early evening, despite  being only a slim crescent through the telescope eyepiece. Mars and Jupiter to rule the night sky after Venus sets, amid the menagerie of bright winter stars in Orion, Taurus, and Gemini. And enhance your astronomy IQ by knowing the difference between a conjunction and an appulse. 

0:00 Intro

0:13 Moon & planets

0:41 Appulses

1:39 Venus at maximum

2:51 February Moon phases

Appulse is the least apparent distance between one celestial object and another, as seen from a third body during a given period. Appulse is seen in the apparent motion typical of two planets together in the sky, or of the Moon to a star or planet while the Moon orbits Earth, as seen from Earth. An appulse is an apparent phenomenon caused by perspective only; the two objects involved are not near in physical space.

An appulse is related to a conjunction, but the definitions differ in detail. While an appulse occurs when the apparent separation between two bodies is at its minimum, a conjunction occurs at the moment when the two bodies have the same right ascension or ecliptic longitude. In general, the precise time of an appulse will be different from that of a conjunction. [Wikipedia]


Video Credit: NASA's Jet Propulsion Laboratory
Narration: Preston Dyches
Duration: 3 minutes
Release Date: Jan. 31, 2025

#NASA #Astronomy #Space #Science #Skywatching #Earth #Moon #Planets #Venus #Mars #Jupiter #Saturn #Appulses #SolarSystem #Stars #Constellations #MilkyWayGalaxy #JPL #California #Skywatching #UnitedStates #Canada #Mexico #NorthernHemisphere #STEM #Education #HD #Video

Aurora Borealis over Minnesota

Aurora Borealis over Minnesota

Photographer Thomas Spence: "The aurora are giving us a nice little display tonight with some pillars and reds. It's a cold night in Superior National Forest near Tofte, Minnesota. 8 degrees and windy but clear and beautiful."

Superior National Forest
https://www.fs.usda.gov/superior/

The aurora borealis, also known as the northern lights, occurs in an upper layer of Earth’s atmosphere called the ionosphere, but they typically originate with activity on the Sun. Occasionally, during explosions called coronal mass ejections, the Sun releases charged particles that speed across the solar system. 

Auroras are produced when the Earth's magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (thermosphere/exosphere) due to Earth's magnetic field, where their energy is lost. The resulting ionization and excitation of atmospheric constituents emits light of varying color and complexity. [Wikipedia]

Solid Colored Aurora
Green is common at the upper latitudes, while red is rare. On the other hand, aurora viewed from lower latitudes tend to be red.

Element Emission Colors
Oxygen: The big player in the aurora is oxygen. Oxygen is responsible for the vivid green (wavelength of 557.7 nm) and also for a deep brownish-red (wavelength of 630.0 nm). Pure green and greenish-yellow aurorae result from the excitation of oxygen.

Nitrogen: Nitrogen emits blue (multiple wavelengths) and red light.

Other Gases: Other gases in the atmosphere become excited and emit light, although the wavelengths may be outside of the range of human vision or else too faint to see. Hydrogen and helium, for example, emit blue and purple. Although our eyes cannot see all of these colors, photographic film and digital cameras often record a broader range of hues.

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)

Image Credit: Thomas Spence
Location: Tofte, Minnesota, United States
Thomas' website: 


#NASA #Space #Astronomy #Sun #SolarSystem #SolarWind #CME #Planet #Earth #Aurora #AuroraBorealis #Magnetosphere #Atmosphere #Science #Physics #Photography #Photographer #ThomasSpence #CitizenScience #SuperiorNationalForest #Tofte #Minnesota #UnitedStates #STEM #Education

Earth 'Eclipses' Moon | Blue Ghost Moon Mission View | Firefly Aerospace

Earth 'Eclipses' Moon Blue Ghost Moon Mission View | Firefly Aerospace


Firefly Aerospace: "I spy with my little lander, a Moon in the distance. Check out Blue Ghost's amazing view of Earth eclipsing the Moon as the lander travels on orbit. Our GhostRiders can't wait to share more postcard worthy moments as we continue on our roadtrip."

The Blue Ghost lander is currently on its 45-day journey to the Moon. Blue Ghost is seeking to land in Mare Crisium to deliver ten NASA science instruments and technology demonstrations to the Moon. They will perform numerous science and technology demonstrations, including lunar subsurface drilling, sample collection, and X-ray imaging of Earth’s magnetic field to advance research for future human missions on the Moon and provide insights into how space weather impacts the planet. Mare Crisium is a lunar mare located in the Moon's Crisium basin, just northeast of Mare Tranquillitatis. It was formed by the flooding of basaltic lava that filled an ancient asteroid impact.

Learn more: https://fireflyspace.com/missions/blue-ghost-mission-1/


Video Credit: Firefly Aerospace
Duration: 14 seconds
Release Date: Jan. 31, 2025


#NASA #Space #Astronomy #Science #Planet #Earth #ArtemisProgram #Moon #LunarLanders #FireflyAerospace #BlueGhostLunarLander #BlueGhostMission1 #BGM1 #UnitedStates #Robotics #Engineering #SpaceTechnology #SolarSystem #SpaceExploration #STEM #Education #HD #Video

Friday, January 31, 2025

The Lambda Centauri Nebula in Centaurus

The Lambda Centauri Nebula in Centaurus


IC 2944, also known as the Lambda Centauri Nebula or the λ Centauri Nebula, is an open cluster with an associated emission nebula found in the constellation Centaurus, near the star λ Centauri. 

Distance: 6,500 light years

Astrophotgrapher Ian Inverarity: ". . . a 2 panel mosaic shot over 6 nights (some half ruined by clouds!). Takahashi FSQ106N telescope on a Warp Astron WD-20 EQ mount, PHD2 guiding, controlled by NINA, processing with APP and PS. Mostly hot and windy nights! Over 33 hours of data."


Image Credit: Ian Inverarity
Release Date: Jan. 31, 2025


#NASA #Astronomy #Space #Science #Stars #Nebula #Nebula #EmissionNebula #IC2944 #StellarNursery #LambdaCentauri #RunningChickenNebula #Centaurus #Constellation #Cosmos #Universe #Astrophotography #Astrophotographer #IanInverarity #CitizenScience #Australia #STEM #Education

Williams & Wilmore on Spacewalk: EVA 274 | International Space Station

Williams & Wilmore on Spacewalk: EVA 274 | International Space Station

NASA astronaut and Expedition 72 Commander Suni Williams works outside the International Space Station during a five-hour and 26-minute spacewalk to remove and stow a radio frequency group antenna assembly. The orbital outpost was soaring 260 miles above Kazakhstan at the time of this photograph.
NASA astronaut and Expedition 72 Commander Suni Williams works outside the International Space Station during a five-hour and 26-minute spacewalk to remove and stow a radio frequency group antenna assembly. In the left foreground, is the latching end effector of the Canadarm2 robotic arm. The orbital outpost was soaring 258 miles above the Pacific Ocean near the coast of Mexico at the time of this photograph.
NASA astronaut and Expedition 72 Commander Suni Williams seemingly hangs upside down while attached to the Canadarm2 robotic arm's latching end effector during a five-hour and 26 minute spacewalk to remove and stow a radio frequency group antenna assembly. The orbital outpost was soaring 260 miles above Russia near the Sea of Azov at the time of this photograph.
NASA astronaut and Expedition 72 Commander Suni Williams is attached to the Canadarm2 robotic arm's latching end effector while being maneuvered to her worksite 264 miles above the South Pacific Ocean. Williams removed and stowed a radio frequency group antenna assembly during the five-hour and 26-minute spacewalk outside the International Space Station.
NASA astronaut and Expedition 72 Commander Suni Williams works outside the International Space Station during a five-hour and 26-minute spacewalk to remove and stow a radio frequency group antenna assembly. In the left foreground, is the latching end effector of the Canadarm2 robotic arm. The orbital outpost was soaring 267 miles above New Zealand at the time of this photograph.
Two spacewalkers, Expedition 72 Flight Engineer Butch Wilmore (upper left) and Expedition 72 Commander Suni Williams (lower right), both NASA astronauts, work outside the International Space Station during a five-hour and 26-minute spacewalk to remove radio communciations hardware and swab for microorganisms.

NASA astronauts Suni Williams and Butch Wilmore concluded their spacewalk at 1:09 p.m. Eastern Standard Time (EST) Jan. 30, 2025. It was the ninth spacewalk for Williams and the fifth for Wilmore, and it was the 274th spacewalk in support of space station assembly, maintenance, and upgrades. Williams surpassed former NASA astronaut Peggy Whitson’s record for total spacewalking time by a female astronaut. Williams now has 62 hours, 6 minutes of total spacewalk time, fourth on NASA’s all-time list.

Williams and Wilmore completed their primary objectives, including removing a radio frequency group antenna assembly from the station’s truss and collecting samples of surface material for analysis from the Destiny laboratory and the Quest airlock.

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia) Flight Engineers: Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA Flight Engineers: Butch Wilmore, Don Pettit, Nick Hague

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.


Image Credit: NASA's Johnson Space Center (JSC)
Capture Date: Jan. 31, 2025

#NASA #Space #Science #ISS #Earth #Spacewalk #EVA #EVA274 #Astronauts #SuniWilliams #ButchWilmore #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education

Shenzhou-19 Crew Commander Reflects on Mission Progress | China Space Station

Shenzhou-19 Crew Commander Reflects on Mission Progress | China Space Station

Chinese astronaut and commander of the Shenzhou-19 space mission, Cai Xuzhe, shared his experience of returning to the Tiangong Space Station while delivering a mid-mission progress review.

China launched the Shenzhou-19 crewed spacecraft on October 30 last year, sending three astronauts, Cai Xuzhe, Song Lingdong, and Wang Haoze, to the orbiting space station for a six-month mission.

Cai first joined the journey into space as a crew member of the Shenzhou-14 mission in 2022. He was honored with the title "Heroic Astronaut" for his service and accomplishments during that mission.

As the crew complete the first half of their space mission on Thursday, Cai said it has been heartwarming to return to the space home.

"After two years, I returned to the Chinese space station. It felt like returning to a familiar home, comforting and deeply heartwarming. In the past three months, we have executed the in-orbit rotation with the Shenzhou-18 astronauts, and carried out the scheduled maintenance, daily operations, and health management protocols of the space station platform as planned. In addition, we have completed two EVAs, and carried out multiple drills such as full-system stress emergency response simulations and medical rescue operations training. These exercises have significantly sharpened our ability to handle contingencies, enabling safer and more efficient mission execution," Cai said.

"During the in-orbit period, with the support of ground personnel, we completed medical cytology experiments represented by advanced research on human brain organoids, and launched a new round of material extravehicular exposure experiments. Our crew also routinely replaced related components to ensure the seamless progress of the experiments," Cai said.

"At present, the various space science experiments undertaken by our crew are progressing steadily. According to the plan, we will focus on space science research and technology experiments in the fields of space life sciences, basic physics of microgravity, space material science, aerospace medicine, and next-generation aerospace technologies. Both crew and ground teams will ensure close coordination and meticulous mission execution to guarantee the complete success of our endeavors," Cai said.

Shenzhou-19 Crew:
Commander Cai Xuzhe (蔡旭哲)
Mission Specialist Wang Haoze (王浩泽)
Mission Specialist Song Lingdong (宋令东)


Video Credit: CCTV
Duration: 2 minutes
Release Date: Jan. 30, 2025

#NASA #Space #Science #Earth #China #中国 #Shenzhou19 #神舟十九号 #Taikonauts #Astronauts #CaiXuzhe #CrewCommander #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #MicrogravityResearch #CMSA #中国载人航天工程办公室 #LongDurationMissions #HumanSpaceflight #STEM #Education #HD #Video

"Happy Anniversary!" Crawler-Transporters Reach 60 Years | NASA Kennedy

"Happy Anniversary!" Crawler-Transporters Reach 60 Years | NASA Kennedy

The crawler-transporters achieved first movement in 1965 and for the past six decades, they have moved rockets from the Vehicle Assembly Building to the launch pad. From Apollo to space shuttle to Artemis, these behemoth vehicles hold an important part in human spaceflight history.

The mobile launcher serves as the primary interface between the ground launch systems, SLS rocket, and Orion spacecraft that will launch the SLS Block 1B rocket, with its enhanced upper stage, to the Moon, allowing the agency to send astronauts and heavier cargo into lunar orbit than its predecessor, SLS Block 1. 

"With Artemis, NASA will land the first woman, first person of color, and its first international partner astronaut on the lunar surface and establish long-term exploration for scientific discovery and to prepare for human missions to Mars."


Credit: NASA
Duration: 2 minutes
Release Date: Jan. 31, 2025


#NASA #Space #Moon #ArtemisProgram #ArtemisII #MobileLauncher2 #CrawlerTransporter #OrionSpacecraft #SLS #Rocket #DeepSpace #Astronauts #HumanSpaceflight #Mars #MoonToMars #Engineering #SpaceTechnology #SpaceExploration #SolarSystem #KSC #NASAKennedy #Florida #UnitedStates #STEM #Education #HD #Video

NASA's Space to Ground: "A Historic Spacewalk" | Week of Jan. 31, 2025

NASA's Space to Ground: "A Historic Spacewalk" | Week of Jan. 31, 2025

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. NASA astronauts Suni Williams and Butch Wilmore concluded their spacewalk at 1:09 p.m. EST Jan. 30, 2025. It was the ninth spacewalk for Williams and the fifth for Wilmore, and it was the 274th spacewalk in support of space station assembly, maintenance, and upgrades. Williams surpassed former NASA astronaut Peggy Whitson’s record for total spacewalking time by a female astronaut. Williams now has 62 hours, 6 minutes of total spacewalk time, fourth on NASA’s all-time list.

Williams and Wilmore completed their primary objectives, including removing a radio frequency group antenna assembly from the station’s truss and collecting samples of surface material for analysis from the Destiny laboratory and the Quest airlock.

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
Science, Technology, Engineering, Math (STEM)

Video Credit: NASA's Johnson Space Center (JSC)
Duration: 3 minutes
Release Date: Jan. 31, 2025

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Thursday, January 30, 2025

NASA Artemis II Moon Mission Solid Rocket Booster Stacking | NASA Kennedy

NASA Artemis II Moon Mission Solid Rocket Booster Stacking | NASA Kennedy

Engineers and technicians with NASA’s Exploration Ground Systems (EGS) team lifted the left center segment, bearing NASA’s historic “worm” logo, of the Space Launch System (SLS) solid rocket boosters (SRBs) for the Artemis II Moon Mission into High Bay 3 of the Vehicle Assembly Building at NASA's Kennedy Space Center in Florida.

This is the seventh of ten motor segments stacked on the Mobile Launcher 1 by the EGS team.

These boosters will help support the remaining rocket components and the Orion spacecraft during final assembly of the Artemis II Moon rocket. They will provide more than 75 percent of the total Space Launch System (SLS) thrust during liftoff from NASA Kennedy’s Launch Pad 39B.

The Artemis II test flight will be NASA’s first mission with crew under the Artemis campaign. It will launch no earlier than April 2026. NASA's Orion spacecraft will carry NASA astronauts Victor Glover, Christina Koch, and Reid Wiseman, as well as Canadian Space Agency (CSA) astronaut Jeremy Hansen, on a 10-day journey around the Moon and back for the Artemis II test flight.

For more information about SLS, visit: 

Check the NASA Artemis II Mission page for updates:

Video Credit: NASA/Frank Michaux
Duration: 54 seconds
Capture Date: Jan. 29, 2025
Release Date: Jan. 30, 2025

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Planet Mars Images: January 30, 2025 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: January 30, 2025 | NASA's Curiosity & Perseverance Rovers

MSL - sol 4437
MSL - sol 4437
MSL - sol 4437
Mars 2020 - sol 1400
Mars 2020 - sol 1402
MSL - sol 4437
Mars 2020 - sol 1402


Celebrating 3+ 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

Celebrating 3+ 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 Date: Jan. 30, 2025

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