Saturday, February 22, 2025

NASA Expert Answers Your Questions About Asteroid 2024 YR4

NASA Expert Answers Your Questions About Asteroid 2024 YR4

You have heard about asteroid 2024 YR4 and we have heard your questions—so let us talk about it. What are the chances it will hit Earth? Why do those odds keep changing? And should you be worried? (Spoiler alert: No). Get the facts from a NASA expert and learn how we track asteroids, update predictions, and keep an eye on the skies. 

Asteroid 2024 YR4 FAQ: https://science.nasa.gov/solar-system/asteroids/2024-yr4/

Stay tuned for the latest updates: https://blogs.nasa.gov/planetarydefense/ 

Coming April 2025, NASA’s Planetary Defenders documentary will showcase the international collaboration and dedicated team of astronomers and scientists working tirelessly to track and monitor near-Earth asteroids, aiming to protect our planet from potential impacts: https://science.nasa.gov/science-research/planetary-science/planetary-defense/planetary-defenders/


Credit: NASA
Producers: Scott Bednar, Jessie Wilde, Pedro Cota
Duration: 2 minutes, 30 seconds
Release Date: Feb. 21, 2025


#NASA #Space #Earth #Planet #PlanetaryDefense #Asteroids #Asteroidasteroid2024YR4 #AsteroidBelt #Comets #NEO #NEA #SolarSystem #Science #SpaceTechnology #DARTMission #JHUAPL #JPL #Caltech #UnitedStates #STEM #Education #HD #Video

China's Tianwen-2 Probe to Collect Samples from Asteroid 2016HO3

China's Tianwen-2 Probe to Collect Samples from Asteroid 2016HO3

China's soon-to-be-launched Tianwen-2 probe will explore the asteroid 2016 HO3 in an effort to better understand the formation and evolution of the solar system, said an expert of the National Astronomical Observatories of Chinese Academy of Sciences.

The Tianwen-2 probe, scheduled for launch in the first half of 2025, will collect samples from near-Earth asteroid 2016 HO3 and explore comet 311P, the China National Space Administration announced on Thursday, February 20, 2025.

Asteroid 2016 HO3 orbits stably near Earth and is known as Earth's quasi-satellite. It is the first quasi-satellite of Earth discovered. The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) in Hawaii, USA, first captured the trace of 2016 HO3 in 2016.

However, it is neither a natural satellite of Earth nor a typical near-Earth asteroid. Instead, it is an asteroid that orbits the Sun with nearly identical orbital parameters to Earth, causing it to move in near-synchrony with our planet and "wander" around Earth.

It contains ancient materials from the early solar system, making it a "living fossil" useful for studying how the solar system formed and evolved.

A number of scientists speculate that this celestial body, with a diameter of about 40 to 100 meters, is likely a remnant of an ancient impact event.

"When the Tianwen-2 probe comes close to it, it will take photos to analyze its morphological features on the surface, rotation characteristics, and other basic physical properties. We will also analyze collected spectral data to examine some of its material components, to find out what is the similarity between its material composition and that of the Moon and Earth? This is a key focus of our exploration this time," said Yan Wei, a senior engineer at the National Astronomical Observatories of Chinese Academy of Sciences.


Video Credit: CCTV
Duration: 1 minute
Release Date: Feb. 22, 2025

#NASA #CNSA #Astronomy #Space #Science #Asteroids #AsteroidKamooalewa #Asteroid2016HO3 #AsteroidSampleReturn #Comets #Comet311P #Comet311PPANSTARRS #CometFlyby #China #中国 #Tianwen2 #Tianwen2Spacecraft #SolarSystem #SpaceExploration #Russia #Россия #InternationalCooperation #STEM #Education #HD #Video

China's Tianwen-2 Probe to Explore Comet 311P

China's Tianwen-2 Probe to Explore Comet 311P

China's soon-to-be-launched Tianwen-2 probe will explore the Comet 311P in an effort to better understand the composition, structure, and evolution of small space objects, said an expert of the National Astronomical Observatories of Chinese Academy of Sciences. 

The Tianwen-2 probe, scheduled for launch in the first half of 2025, will collect samples from near-Earth asteroid 2016 HO3 and explore Comet 311P, the China National Space Administration (CNSA) announced on Thursday, February 20, 2025.

Comet 311P orbits in the main asteroid belt between Mars and Jupiter where most asteroids reside, containing over 90 percent of the asteroids in the solar system. It displays features of both comets and asteroids. It has become the seventh main-belt comet confirmed by human beings, and it is also the most peculiar one so far.

"The main-belt comet is another type of asteroid. It should be noted that it is not a true comet, but it may share some characteristics with comets, which is why it is called a main-belt comet or active asteroid. It may emit substances, including gas and particles, when it is close to the sun, which has been observed and is another research hotspot," said Yan Wei, a senior engineer at the National Astronomical Observatories of the Chinese Academy of Sciences.

According to the conventional theory, comets typically originate from the outer edges of the solar system and are rich in ice. As they approach the sun, the heat causes the ice to vaporize, forming their characteristic tails. However, Comet 311P, located in the asteroid belt—far closer to the sun than typical comets—faces intense solar radiation, making it unlikely to retain volatile substances like water ice. This comet challenges astronomers' traditional understanding.

The Tianwen-2 probe is set to visit Comet 311P, the "rebel" of the asteroid belt, to uncover the mysteries that defy current knowledge.

Comet 311P/PanSTARRS also known as P/2013 P5 (PanSTARRS) is an active asteroid (object with asteroid-like orbit but with comet-like visual characteristics) discovered by Bryce T. Bolin using the Pan-STARRS telescope on August 27, 2013. Observations made by the Hubble Space Telescope revealed that it had six comet-like tails. The tails are suspected to be streams of material ejected by the asteroid as a result of a rubble pile asteroid spinning fast enough to remove material from it. This is similar to 331P/Gibbs, which was found to be a quickly-spinning rubble pile as well.


Video Credit: CCTV
Duration: 1 minute
Release Date: Feb. 21, 2025


#NASA #CNSA #Astronomy #Space #Science #Asteroids #AsteroidKamooalewa #Asteroid2016HO3 #AsteroidSampleReturn #Comets #Comet311P #Comet311PPANSTARRS #CometFlyby #China #中国 #Tianwen2 #Tianwen2Spacecraft #SolarSystem #SpaceExploration #Russia #Россия #InternationalCooperation #STEM #Education #HD #Video

Protecting the Horseshoe Crab: A "Far Out" Mini Episode | NASA Kennedy

Protecting the Horseshoe Crab: A "Far Out" Mini Episode  | NASA Kennedy

Kennedy Space Center is known for launching rockets into our cosmos, but it is also home to an expansive wildlife refuge and national seashore where more than 1,200 plant and wildlife species reside. Its 144,000 acres are teaming with creatures you might expect, such as alligators, snakes and eagles, and those you may not know as well like the endangered scrub-jay, tortoise and horseshoe crab.

In this mini-episode of "Far Out," viewers will meet people on the environmental team that are responsible for ensuring the wildlife remains protected and thriving at the space center.

Watch the full episode on NASA+: 
https://go.nasa.gov/4axnF3M


Video Credit: NASA's Kennedy Space Center (KSC)
Duration: 3 minutes
Release Date: Feb. 21, 2025

#NASA #Space #KennedySpaceCenter #KSC #NASAKennedy #Environment #Nature #Wildlife #WildlifeRefuge #HorseshoeCrab #HorseshoeCrabs #Spaceport #MerrittIsland #Florida #UnitedStates #STEM #Education #HD #Video

Friday, February 21, 2025

Stars, Galaxies & Earth Airglow | International Space Station

Stars, Galaxies & Earth Airglow | International Space Station






Expedition 72 flight engineer and NASA astronaut Don Pettit has captured spectacular views of a "starry night from an orbital palette". In this series of images, you can see the Earth's vibrant airglow, the Milky Way, and two neighboring galaxiesthe Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC) visible in the Earth's southern hemisphere.

Over 160,000 light-years away, the Large Magellanic Cloud is a dwarf galaxy that looms large in the southern nighttime sky at twenty times the apparent diameter of the full Moon.

The Small Magellanic Cloud is an irregular dwarf galaxy nearly 200,000 light-years way that orbits our own Milky Way spiral galaxy.

Airglow occurs when atoms and molecules in the upper atmosphere, excited by sunlight, emit light to shed their excess energy. Or, it can happen when atoms and molecules that have been ionized by sunlight collide with and capture a free electron. In both cases, they eject a particle of light—called a photon—in order to relax again. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is energized by ordinary, day-to-day solar radiation.

Unlike auroras, which are episodic and fleeting, airglow constantly shines throughout Earth’s atmosphere, and the result is a tenuous bubble of light that closely encases our entire planet. (Auroras, on the other hand, are usually constrained to Earth’s poles.) Just a tenth as bright as all the stars in the night sky, airglow is far more subdued than auroras, too dim to observe easily except in orbit or on the ground with clear, dark skies and a sensitive camera. However, it is a marker nevertheless of the dynamic region where Earth meets space . . .

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)/D.Pettit
Release Dates: Jan. 29-Feb. 15, 2025

#NASA #Space #Science #ISS #Earth #Aurora #Airglow #Stars #Galaxies #LMC #SMC #Astronauts #DonPettit #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education

What is NASA's First Polar Research Ice Mining Experiment for The Moon?

What is NASA's First Polar Research Ice Mining Experiment for The Moon?

Before Artemis astronauts land on the Moon, robots will scout the surface for resources and collect information. Landers and rovers will come equipped with handy tools, including drills and chemical analyzers, to examine what lies below the lunar surface. 

Launching no earlier than Feb. 26 aboard the Intuitive Machines second Moon mission, NASA’s Polar Resources Ice Mining Experiment 1 (PRIME-1) will demonstrate drilling into the lunar surface where it lands, bring regolith to the Moon’s surface, and use a mass spectrometer to look for the presence of volatiles.

This technology demonstration will help us better understand the Moon and its subsurface resources, paving the way for sustainable human exploration under the agency’s Artemis campaign for the benefit of all.

Learn more about the Polar Resources Ice Mining Experiment 1 (PRIME-1) at: 


Video Credit: NASA Space Tech
Duration: 2 minutes, 24 seconds
Release Date: Feb. 21, 2025

#NASA #Space #Astronomy #Science #Moon #ArtemisProgram #Prime1 #PolarIceMining #IntuitiveMachines #IM2 #IM2Mission #IM2Spacecraft #AthenaLunarLander #CommercialSpace #CLPS #Robotics #SpaceTechnology #MSFC #GSFC #Texas #UnitedStates #STEM #Education #Animation #HD #Video

NASA’s SpaceX Crew-10: Launch Preparations | International Space Station

NASA’s SpaceX Crew-10: Launch Preparations | International Space Station

The crew of NASA’s SpaceX Crew-10 mission poses for a photo during a crew equipment interface test (CEIT) inside SpaceX’s new Dragon processing facility at the agency’s Kennedy Space Center in Florida on Monday, Feb. 17, 2025. From left, Roscosmos cosmonaut Kirill Peskov of Russia, mission specialist; NASA astronauts Nichole Ayers, pilot and Anne McClain, commander; and Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, mission specialist, participated in the CEIT. It plays an important role in familiarizing crew members with the interior of the Dragon spacecraft ahead of their four-month mission to International Space Station.

Official crew portrait of NASA's SpaceX Crew-10 members: (from left) Mission Specialist Kirill Peskov of Roscosmos (Russia); Pilot Nicole Ayers and Commander Anne McClain, both NASA astronauts; and Mission Specialist Takuya Onishi from the Japan Aerospace Exploration Agency (JAXA)

The SpaceX Crew-10 Mission Emblem

Four crew members are preparing to launch for a long-duration stay aboard the International Space Station. NASA astronauts Commander Anne McClain and Pilot Nichole Ayers, Japan Aerospace Exploration Agency (JAXA) astronaut Mission Specialist Takuya Onishi, and Roscosmos cosmonaut Mission Specialist Kirill Peskov of Russia will join astronauts and cosmonauts at the orbiting laboratory by launching no earlier than March 12, 2025, from the Kennedy Space Center in Florida.

The flight is the 10th crew rotation with SpaceX to the station as part of NASA’s Commercial Crew Program (CCP). While aboard, the international crew will conduct scientific investigations and technology demonstrations to help prepare humans for future missions and benefit people on Earth.

Astronaut Nichole Ayers NASA Biography:

Japan Aerospace Exploration Agency (JAXA) astronaut Mission Specialist Takuya Onishi Biography:

NASA’s SpaceX Crew-10 mission will be the first spaceflight for Roscosmos cosmonaut Mission Specialist Kirill Peskov of Russia. Before his selection as a cosmonaut in 2018, he earned a degree in engineering from the Ulyanovsk Civil Aviation School and was a co-pilot on the Boeing 757 and 767 aircraft for airlines Nordwind and Ikar. Assigned as a test-cosmonaut in 2020, he has additional experience in skydiving, zero-gravity training, scuba diving, and wilderness survival.

Learn more about NASA's SpaceX Crew-10:

NASA's Commercial Crew Program:

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 Credits: Space Exploration Technologies Corporation (SpaceX)/NASA
Release Dates: Nov. 27, 2024-Feb. 21, 2025


#NASA #Space #ISS #Science #SpaceXCrew10 #SpaceX #CrewDragonSpacecraft #Falcon9Rocket #Astronauts #AnneMcClain #Crew10MissionCommander #NicholeAyers #TakuyaOnishi #Japan #日本 #Cosmonaut #KirillPeskov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #CCP #Expedition73 #JSC #NASAKennedy #KSC #Florida #UnitedStates #STEM #Education

Explore the NGC 3640 Galaxy Group | European Southern Observatory

Explore the NGC 3640 Galaxy Group | European Southern Observatory


This video takes you to NGC 3640, an elliptical galaxy located 88 million years away in the constellation of Leo (the lion). A galaxy’s past shapes its present, and for NGC 3640 that does not just refer to its unusual deformity, but also the clusters of stars within. Analysis of these clusters, containing a portion of the galaxy’s first-born stars, reveals a violent history of swallowing other galaxies. Fortunately for the smaller galaxy below, NGC 3641 shows no signs of deformity, suggesting NGC 3640 is just far enough away to spare its little companion the same fate.

The Very Large Survey Telescope (VST) has captured here an entire zoo of galaxies, filling the empty void of space. At the center of this varied and colorful collection, is elliptical galaxy NGC 3640, situated just above its smaller galactic neighbor NGC 3641. Astronomers are especially interested in the way these two interact with each other, studying their joint history through their populations of ancient clusters of stars.

Distance: 88 million light-years

Throughout their extremely long lifetime, galaxies change. As they soar through space, they may steal gas and stars from other galaxies, or even engulf and merge with them. After these events, galaxies can become distorted, as exemplified by the misshaped NGC 3640 and the diffuse light around it. The galaxy is then left with ‘scars’ that hint at a violent past. Astronomers can use these to know its past and present history.

To trace the history behind this galaxy and its smaller companion, a team of astronomers at the Italian National Institute for Astrophysics used the VST to analyze their globular clusters, spherical and compact aggregations of stars bound by gravity. These usually contain examples of the first stars created within a galaxy and can therefore act as fossil markers, revealing the galaxy’s history, even after merging events.

The results confirm that NGC 3640 has engulfed other galaxies before, an ominous sign for the smaller galaxy now in its path, NGC 3641. Yet, this small galactic underdog shows a distinct lack of distortions in its shape or the globular clusters within. This suggests that their interaction, while fast, is not happening close enough for NGC 3640 to pose a threat. NGC 3641 might be safe . . . for now.

Learn more about the Very Large Survey Telescope (VST):
https://www.eso.org/public/teles-instr/paranal-observatory/surveytelescopes/vst/


Credits: European Southern Observatory (ESO) / INAF / M. Mirabile et al. / R. Ragusa et al.
Script: A. Izquierdo Lopez
Editing: M. Martins
Duration: 1 minute
Release Date: Feb. 21, 2025

#NASA #FoN #ESO #Space #Astronomy #Science #Galaxies #GalacticGroup #NGC3640 #EllipticalGalaxy #Stars #StarClusters #NGC3641 #Cosmos #Universe #VST #ParanalObservatory #AtacamaDesert #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

China Tianwen-2 Sample Return Asteroid & Comet Rendezvous Mission Preview

China Tianwen-2 Sample Return Asteroid & Comet Rendezvous Mission Preview


The Tianwen-2 spacecraft for China's first asteroid sample return and comet rendezvous mission arrived at the launch site of the Xichang Satellite Launch Center in Sichuan province, southwest China on February 20, 2025, the China National Space Administration (CNSA) has announced. Scheduled for launch in the first half of 2025, it will collect samples from a near-Earth asteroid.

Tianwen-2 carries a suite of scientific instruments to analyze its targets. Multispectral and infrared spectrometers will study surface composition, while high-resolution cameras will map geological features. A radar sounder will probe subsurface structures, and a magnetometer will search for residual magnetic fields. Dust and gas analyzers will examine comet activity, and charged particle detectors will investigate solar wind interactions. The Space Research Institute of the Russian Academy of Sciences is understood to have contributed to the particle detectors. 

The Tianwen Deep Space Series

The Tianwen-2 mission is part of China’s expanding deep space plans. It follows the Tianwen-1 Mars orbiter and landing mission launched in 2020. The Zhurong rover successfully landed on the Red Planet in 2021. Tianwen-3 will be a Mars sample return mission and will launch around late 2028 or 2030. 

Tianwen-2 will first target near-Earth asteroid Kamoʻoalewa (2016 HO3), considered a quasi-satellite of Earth due to its co-orbital dynamics. It aims to collect samples from the roughly 40 to 100-meter-diameter asteroid and deliver them to Earth around 2027. Kamoʻoalewa is possibly a chunk of the moon blasted into space following an impact event, according to researchers.

The main spacecraft will then head for main-belt comet 311P/PANSTARRS. It has asteroid-like orbital characteristics but also features comet-like activity.

The two mission phases aim to provide insight into the composition and evolution of near-Earth objects and understand distribution of water and organic molecules and the history of the early solar system.

“The launch site facilities are in good condition, and the pre-launch test preparations are being carried out in an orderly manner as planned,” the CNSA statement read.

Sampling Kamoʻoalewa

Tianwen-2 will use two sampling techniques to collect material from the asteroid. These will be the touch-and-go (TAG) approach used by both NASA’s OSIRIS-REx and JAXA’s Hayabusa2, and an anchor-and-attach system featuring drills at the tips of landing legs. 

Early proposals for the mission, then named Zheng He for the Chinese admiral and explorer born in the 14th Century, indicated the spacecraft would aim to collect between 200 and 1,000 grams of samples.

Analysis of the samples aims to reveal the nature and origin of the asteroid, analyze its mineral content and provide comparisons with other asteroids. 

While China has conducted two successful sample return missions from the Moon’s near and far sides with Chang’e-5 and last year’s Chang’e-6 mission, the velocity of the reentry module will be greater, adding new challenges. The China Aerospace Science and Technology Corporation (CASC) conducted high-altitude parachute deployment tests for the mission in 2023. In contrast to the lunar sampling missions, Kamoʻoalewa will have negligible gravity, requiring unique approaches to settling on the body and obtaining samples.

China’s first excursion to an asteroid was a flyby of 4179 Toutatis in 2012, when the Chang’e-2 lunar orbiter made the pass as an extended mission objective. 

Comet rendezvous

Delivering samples to Earth will not be the end of the mission. The spacecraft will release a return module which will reenter the atmosphere, but also use the approach to the planet for a gravitational slingshot maneuver. This will send the main spacecraft on its way to the main-belt comet 311P/PANSTARRS with arrival scheduled for around 2034.

The comet is seen as an ideal target for studying transitional objects between asteroids and comets. It orbits between 1.94 and 2.44 astronomical units from the Sun and the spacecraft is expected to rendezvous with the body in the mid-2030s. The Tianwen-2 spacecraft will conduct remote sensing of the comet to characterize its orbit, shape, and rotation, examine its surface composition and volatile elements, and investigate dust emissions and activity mechanisms to understand cometary behavior in the main belt.

Tianwen-4 will launch around 2030. It will include a solar-powered Jupiter orbiter that will observe the system and then enter orbit around the moon Callisto. A smaller, radioisotope-powered spacecraft to make a flyby of Uranus.

Chinese researchers last year called for a focus on asteroid sample return missions, citing untapped potential for groundbreaking discoveries and technological innovation


Video Credit: China National Space Administration (CNSA)/CCTV
Article Credit: Andrew Jones/SpaceNews
Duration: 39 seconds
Release Date: Feb. 20, 2025

#NASA #CNSA #Astronomy #Space #Science #Asteroids #AsteroidKamooalewa #Asteroid2016HO3 #AsteroidSampleReturn #Comets #Comet311PPANSTARRS #CometFlyby #China #中国 #Tianwen2 #Tianwen2Spacecraft #SolarSystem #SpaceExploration #Russia #Россия #InternationalCooperation #STEM #Education #HD #Video

NASA's Space to Ground: Pushing Boundaries | Week of Feb. 21, 2025

NASA's Space to Ground: Pushing Boundaries | Week of Feb. 21, 2025

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. NASA’s SpaceX Crew-9 members, including NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore, as well as Roscosmos cosmonaut Aleksandr Gorbunov of Russia joined each other on Wednesday, February 19, 2025, for a refresher session and practiced on a computer the procedures for reentering the Earth’s atmosphere aboard the SpaceX Dragon crew spacecraft. The quartet is planned to undock from the space station about a week after NASA’s SpaceX Crew-10 mission arrives carrying NASA astronauts Anne McClain, Nichole Ayers, Roscosmos cosmonaut Kirill Peskov of Russia, and Japan Aerospace Exploration Agency (JAXA) Takuya Onishi. Crew-10’s four crew members are targeted to launch no earlier than March 12, 2025, from the Kennedy Space Center in Florida.

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.


Credit: NASA's Johnson Space Center (JSC)
Duration: 3 minutes
Release Date: Feb. 21, 2025


#NASA #Space #Science #ISS #Earth #SpaceXCrew9 #Astronauts #SuniWilliams #ButchWilmore #NickHague #DonPettit #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #MicrogravityResearch #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education #HD #Video

Thursday, February 20, 2025

Expedition 72 Crew Photos: February 2025 | International Space Station

Expedition 72 Crew Photos: February 2025 | International Space Station

NASA's SpaceX Crew-9 members pose together for a portrait inside the vestibule between the International Space Station and the SpaceX Dragon crew spacecraft. Clockwise from left, are NASA astronauts Butch Wimore, Nick Hague, and Suni Williams, and Roscosmos cosmonaut Aleksandr Gorbunov of Russia.
NASA's SpaceX Crew-9 members pose together for a portrait inside the SpaceX Dragon crew spacecraft docked to the International Space Station. From left, are NASA astronaut Suni Williams, Roscosmos cosmonaut Aleksandr Gorbunov of Russia, and NASA astronauts Nick Hague and Butch Wimore.

NASA's SpaceX Crew-9 members pose together for a portrait inside the International Space Station's Unity module. From left, are NASA astronaut Suni Williams, Roscosmos cosmonaut Aleksandr Gorbunov of Russia, and NASA astronauts Nick Hague and Butch Wimore.

NASA's SpaceX Crew-9 members pose together for a portrait inside the International Space Station's Unity module. Clockwise from left, are NASA astronauts Butch Wimore and Suni Williams, Roscosmos cosmonaut Aleksandr Gorbunov of Russia, and NASA astronaut Nick Hague.
NASA astronaut and Expedition 72 Commander Suni Williams measures her mass using a specialized device inside the International Space Station's Zvezda service module. The mass measurement device applies a known force to an attached astronaut and measures the resulting acceleration to acquire the crew member's mass. The result is based on a form of Newton's Second Law of Motion.
NASA astronaut and Expedition 72 Commander Suni Williams displays production packs containing geneticallly engineered yeast and edible media for incubation to activate yeast growth. The BioNutrients investigation explores using the engineered yeast to produce on-demand nutrients and avoid vitamin deficiencies for crews on long-term missions. The samples are later frozen then returned to Earth to analyze their ability promote crew health and improve the preservation of probiotics.
NASA astronaut and Expedition 72 Flight Engineer Nick Hague works in a portable glovebag and cleans pumps, replaces components, and installs bio-ink syringes inside the BioFabrication Facility being tested for its capability to print biological, or organ-like, tissues in space and learn how to eventually fabricate human organs off the Earth.
NASA astronaut and Expedition 72 Flight Engineer Nick Hague measures his mass using a specialized device inside the International Space Station's Zvezda service module. The mass measurement device applies a known force to an attached astronaut and measures the resulting acceleration to acquire the crew member's mass. The result is based on a form of Newton's Second Law of Motion.

NASA’s SpaceX Crew-9 members, including NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore, as well as Roscosmos cosmonaut Aleksandr Gorbunov of Russia joined each other on Wednesday, February 19, 2025, for a refresher session and practiced on a computer the procedures for reentering the Earth’s atmosphere aboard the SpaceX Dragon crew spacecraft. The quartet is planned to undock from the space station about a week after NASA’s SpaceX Crew-10 mission arrives carrying NASA astronauts Anne McClain, Nichole Ayers, Roscosmos cosmonaut Kirill Peskov of Russia, and Japan Aerospace Exploration Agency (JAXA) Takuya Onishi. Crew-10’s four crew members are targeted to launch no earlier than March 12, 2025, from the Kennedy Space Center in Florida.

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)
Image Dates: Feb. 11-19, 2025


#NASA #Space #Science #ISS #Earth #SpaceXCrew9 #Astronauts #SuniWilliams #ButchWilmore #NickHague #DonPettit #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #MicrogravityResearch #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education

Close-up: Galaxy UGC 5460 in Ursa Major | Hubble

Close-up: Galaxy UGC 5460 in Ursa Major | Hubble

The sparkling spiral galaxy gracing this NASA/European Space Agency Hubble Space Telescope picture is UGC 5460. It sits about 60 million light-years away in the constellation Ursa Major. This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms and bright blue star clusters. Also captured in the upper left-hand corner of this image is a far closer object: a star just 577 light-years away in our own galaxy.

UGC 5460 has hosted two recent supernovae named SN 2011ht and SN 2015as. It is because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programs that aim to study kinds of supernovae. 

SN 2015as was what is known as a core-collapse supernova: a cataclysmic explosion that happens when the core of a star far more massive than the Sun runs out of fuel and collapses under its own gravity, initiating a rebound of material outside the core. Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a supernova collides with the gas that surrounds the exploded star.

SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae. Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location, and the explosion’s identity may be revealed at last.

Image Description: A spiral galaxy seen close to face-on. The center of its disc is a bright, pale yellowish oval shape. Spiral arms extend from either side of the oval through the disc on irregular paths. They are marked throughout by bright bluish-white patches of stars. Distant background galaxies appear as small orangish blobs around the spiral galaxy. In the top-left corner a nearby star shines brightly, spikes radiating from it.


Credit: ESA/Hubble & NASA, W. Jacobson-Galán, A. Filippenko, J. Mauerhan
Duration: 30 seconds
Release Date: Feb. 17, 2025

#NASA #Astronomy #Hubble #Space #Science #Galaxies #Galaxy #UGC5460 #SpiralGalaxy #Supernovae #SN2011ht #SN2015as #LuminousBlueVariable #LBV #UrsaMajor #Constellation #Astrophysics #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #ESA #Europe #STEM #Education #HD #Video

A New Star Forms a Fiery Hourglass: Protostar L1527 | James Webb Space Telescope

New Star Forms a Fiery Hourglass: Protostar L1527 | James Webb Space Telescope

The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope has revealed the once-hidden features of the protostar within the dark cloud L1527 with its Near Infrared Camera (NIRCam), providing insight into the formation of a new star. These blazing clouds within the Taurus star-forming region are only visible in infrared light, making it an ideal target for Webb.

The protostar itself is hidden from view within the ‘neck’ of this hourglass shape. An edge-on protoplanetary disc is seen as a dark line across the middle of the neck. Light from the protostar leaks above and below this disc, illuminating cavities within the surrounding gas and dust.

The region’s most prevalent features, the blue and orange clouds, outline cavities created as material shoots away from the protostar and collides with the surrounding matter. The colors themselves are due to layers of dust between Webb and the clouds. The blue areas are where the dust is thinnest. The thicker the layer of dust, the less blue light is able to escape, creating pockets of orange.

Webb also reveals filaments of molecular hydrogen that have been shocked as the protostar ejects material away from it. Shocks and turbulence inhibit the formation of new stars that would otherwise form throughout the cloud. As a result, the protostar dominates the space, taking much of the material for itself.

Despite the chaos that L1527 is causing, it is only about 100,000 years old—a relatively young body. Given its age and its brightness in far-infrared light, L1527 is considered a class 0 protostar, the earliest stage of star formation. Protostars like these, which are still cocooned in a dark cloud of dust and gas, have a long way to go before they become fully-fledged stars. L1527 does not generate its own energy through the nuclear fusion of hydrogen yet, an essential characteristic of stars. Its shape, while mostly spherical, is also unstable, taking the form of a small, hot, and puffy clump of gas somewhere between 20% and 40% of the mass of our Sun.

As a protostar continues to gather mass, its core gradually compresses and gets closer to stable nuclear fusion. The scene shown in this image reveals that L1527 is doing just that. The surrounding molecular cloud is made up of dense dust and gas that are being drawn towards the center, where the protostar resides. As the material falls in, it spirals around the center. This creates a dense disc of material, known as an accretion disc, which feeds material onto the protostar. As it gains more mass and compresses further, the temperature of its core will rise, eventually reaching the threshold for nuclear fusion to begin.

The disc, seen in the image as a dark band in front of the bright center, is about the size of our Solar System. Given the density, it is not unusual for much of this material to clump together—the beginnings of planets. Ultimately, this view of L1527 provides a window onto what our Sun and Solar System looked like in their infancy.

Webb is the largest, most powerful telescope ever launched into space. Under an international collaboration agreement, the European Space Agency (ESA) provided the telescope’s launch service, using the Ariane 5 launch vehicle. Working with partners, ESA was responsible for the development and qualification of Ariane 5 adaptations for the Webb mission and for the procurement of the launch service by Arianespace. ESA also provided the workhorse spectrograph NIRSpec and 50% of the mid-infrared instrument MIRI that was designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with NASA's Jet Propulsion Laboratory (JPL) and the University of Arizona.

Webb is an international partnership between NASA, European Space Agency (ESA) and the Canadian Space Agency (CSA).


Image Credit: NASA, ESA, CSA, and STScI, J. DePasquale (STScI)
Duration: 48 seconds
Release Date: Feb. 20, 2025


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In Lunar Orbit! Blue Ghost Week 5 Update | Firefly Aerospace

In Lunar Orbit! Blue Ghost Week 5 Update | Firefly Aerospace

Firefly Aerospace update: "There are ten days left in our lunar roadtrip and Blue Ghost has traveled 2.2 million miles so far and downlinked 18.7 GB of data! Our Ghost Riders have already accomplished so many milestones, but there are still more to come. Catch our week 5 update on what's next as we prepare to land on the Moon on March 2."

Firefly Aerospace is targeting no earlier than 3:45 a.m. EST on Sunday, March 2, 2025, to land the Blue Ghost lunar lander on the Moon. This is part of NASA’s Commercial Lunar Payload Services (CLPS) initiative and Artemis campaign to establish a long-term lunar presence. 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/

NASA continues to work with multiple American companies to deliver science and technology to the lunar surface through the agency’s CLPS initiative. This pool of companies may bid on contracts for end-to-end lunar delivery services, including payload integration and operations, launching from Earth, and landing on the surface of the Moon.


Video Credit: Firefly Aerospace
Duration: 7 minutes
Release Date: Feb. 20, 2025


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NASA Artemis II Moon Rocket: Booster Stacking | Kennedy Space Center

NASA Artemis II Moon Rocket: Booster Stacking | Kennedy Space Center

Technicians with Exploration Ground Systems integrate the right forward segment atop the center forward segment on NASA’s SLS (Space Launch System) Moon rocket booster inside the Vehicle Assembly Building’s High Bay 3 at Kennedy Space Center in Florida on Friday, Feb. 14, 2025.
Engineers with NASA’s Exploration Ground Systems complete stacking operations on the twin SLS (Space Launch System) solid rocket boosters for Artemis II by integrating the nose cones atop the forward assemblies inside the Vehicle Assembly Building’s High Bay 3 at NASA’s Kennedy Space Center in Florida on Wednesday, Feb. 19, 2025.
Technicians with Exploration Ground Systems integrate the right forward segment atop the center forward segment on NASA’s SLS (Space Launch System) Moon rocket booster inside the Vehicle Assembly Building’s High Bay 3 at Kennedy Space Center in Florida on Friday, Feb. 14, 2025.
Inside High Bay 3 of the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida, technicians with the agency’s Exploration Ground Systems integrate the left forward center booster segment for the NASA’s SLS (Space Launch System) rocket onto the left center center segment atop the mobile launcher on Thursday, Jan. 30, 2025.
Inside High Bay 3 of the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida, technicians with the agency’s Exploration Ground Systems integrate the left forward center booster segment for the NASA’s SLS (Space Launch System) rocket onto the left center center segment atop the mobile launcher on Thursday, Jan. 30, 2025.
Technicians with NASA’s Exploration Ground Systems complete the integration of the left forward segment to the center forward segment on mobile launcher 1 inside the Vehicle Assembly Building at the agency’s Kennedy Space Center in Florida on Friday, Feb. 7, 2025.
Technicians with NASA’s Exploration Ground Systems complete the integration of the left forward segment to the center forward segment on mobile launcher 1 inside the Vehicle Assembly Building at the agency’s Kennedy Space Center in Florida on Friday, Feb. 7, 2025.
Technicians transport the right forward segment for NASA’s SLS (Space Launch System) Moon rocket boosters from the Rotation Processing and Surge Facility to NASA’s Vehicle Assembly Building in Florida on Monday, Feb. 15, 2025.

Technicians with the Exploration Ground Systems team are integrating solid rocket booster segments  for NASA’s Artemis II Space Launch System (SLS) Moon rocket inside the Vehicle Assembly Building’s High Bay 3 at Kennedy Space Center in Florida. 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 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:

Image Credit: NASA/Cory S. Huston
Capture Dates: Jan. 30-Feb. 19, 2025

#NASA #Space #Moon #ArtemisProgram #ArtemisIIMission #ArtemisII #NASASLS #SLSRocket #SRB #SolidRocketBoosters #NorthropGrumman #Astronauts #MoonToMars #Science #DeepSpaceExploration #SpaceExploration #HumanSpaceflight #VAB #ExplorationGroundSystems #EGS #MSFC #KSC #MerrittIsland #Spaceport #Florida #UnitedStates #STEM #Education

Rapid-Fire Light Show from Milky Way's Central Black Hole | Webb Telescope

Rapid-Fire Light Show from Milky Way's Central Black Hole | Webb Telescope

NASA’s James Webb Space Telescope has captured the most detailed look yet at the heart of our galaxy. Sagittarius A*, the supermassive black hole at its core, is constantly flaring with no breaks.

Webb’s Near Infrared Camera (NIRCam) observed the black hole for a year, revealing unpredictable bursts of light. Scientists believe smaller flickers come from turbulence, while the biggest flares result from magnetic fields colliding.

These findings help us better understand how black holes shape their surroundings. Sagittarius A* is more active than expected, offering a rare look at the forces driving our galaxy.

Read more:  https://science.nasa.gov/missions/webb/webb-reveals-rapid-fire-light-show-from-milky-ways-central-black-hole/

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).


Video Credit: NASA
Duration: 2 minutes
Release Date: Feb. 20, 2025


#NASA #ESA #Astronomy #Space #Science #Stars #SupermassiveBlackHoles #SagittariusA #SgrA #Sagittarius #Constellation #MilkyWayGalaxy #Astrophysics #Universe #JamesWebbSpaceTelescope #JWST #NIRCam #InfraredAstronomy #NearInfrared #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video