Thursday, December 18, 2025

Post-impact Dust Clouds cs1 & cs2 around Star Fomalhaut | Hubble Space Telescope

Post-impact Dust Clouds cs1 & cs2 around Star Fomalhaut | Hubble Space Telescope

This composite NASA/European Space Agency Hubble Space Telescope image shows the debris ring and dust clouds cs1 and cs2 around the star Fomalhaut. For comparison, dust cloud cs1, imaged in 2012, is pictured with dust cloud cs2, imaged in 2023. The dashed circles mark the location of these clouds. When dust cloud cs2 suddenly appeared, astronomers quickly noticed they had witnessed the violent collision of two massive objects. Previously thought to be a planet, cs1 is now classified as a similar debris cloud. In this image, Fomalhaut itself is masked out to allow the fainter features to be seen. Its location is marked by the white star.

This image was created from Hubble data from proposal #17139 (P. Kalas).

Image Description: Image labeled Fomalhaut system, Hubble Space Telescope. A grainy orange oval ring tilts slightly from upper right to lower left. At two o’clock, a white box outlines the ring’s edge and white lines extend to a larger pullout at lower right. Two spots are labeled cs1 2013 and cs2 2023. Inside the ring is a black circle with a white star symbol in the middle.


Credit: NASA, ESA, P. Kalas (UC Berkeley), J. DePasquale (STScI)
Release Date: Dec. 18, 2025

#NASA #ESA #Astronomy #Space #Science #Star #Fomalhaut #ObjectCollisions #DustCloudcs1 #DustCloudcs2 #AsteroidBelts #CircumstellarDiscs #Exoplanets #PiscisAustrinus #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

Asteroids Found Colliding at Nearby Star for First Time | Hubble Space Telescope

Asteroids Found Colliding at Nearby Star for First Time | Hubble Space Telescope

This episode highlights a historical milestone: catastrophic collisions in a nearby planetary system were witnessed for the first time by astronomers using the NASA/European Space Agency Hubble Space Telescope. 

Hubble captured the violent collision of two massive objects around the star Fomalhaut. This extraordinary event is unlike anything in our own present-day solar system that we know of. The video shows the sequence of events leading up to the creation of dust cloud cs2 around the star Fomalhaut. In the opening frames, Fomalhaut appears in the top left corner. Two white dots, located in the bottom right corner, represent the two massive objects in orbit around Fomalhaut. These objects approach each other and collide, resulting in a huge debris cloud that initially resembles an exoplanet as seen in reflected light. Years later, starlight is able to push the dust cloud outward from the star. 

Fomalhaut is the brightest star in the southern constellation of Piscis Austrinus, the Southern Fish, and one of the most luminous stars in the night sky.

Distance from Earth: ~25 light years


Credit: European Space Agency (ESA)
Directed by: Bethany Downer and Nico Bartmann
Editing: Nico Bartmann
Web and technical support: Enciso Systems
Written by: Bethany Downer Music: Stan Dart - Organic Life
Footage and photos: NASA, ESA, STScI, R. Crawford (STScI), P. Kalas (UC Berkeley), J. DePasquale (STScI), L. Calçada (ESO), N. Bartmann (ESA/Hubble)
Duration: 1 minute, 19 seconds
Release Date: Dec. 18, 2025

#NASA #ESA #Astronomy #Space #Science #Star #Fomalhaut #ObjectCollisions #DustCloudcs2 #AsteroidBelts #CircumstellarDiscs #Exoplanets #PiscisAustrinus #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education #Animation #HD #Video

Hints of Planets in "Baby Star" Systems | Europe's Gaia Space Telescope

Hints of Planets in "Baby Star" Systems | Europe's Gaia Space Telescope

Ever wondered how planetary systems like our own Solar System form? 
Thanks to the European Space Agency’s Gaia space telescope, we are getting a unique peek behind the cosmic curtain into these dusty environments. In this collage, we see the images of thirty-one baby star systems. All of the systems are centered around very young stars that have recently collapsed from vast clouds of gas and dust. After the clouds collapsed under their own gravity, they spun faster and flattened into discs with hot, dense centers. These became the stars, sometimes multiple stars were formed. The discs around them are called protoplanetary discs. The 31 baby systems are shown here in orange-purple, as seen by the Atacama Large Millimeter Array (ALMA) ground-based telescope. Astronomers expect the remaining material in protoplanetary discs to clump together to form planets, but until now it is been very difficult to spot them because of all the dust and gas present in discs. To date, very few planets have been detected around forming stars.

The collage also shows our own Solar System for reference on the bottom right corner, as it is predicted to have looked at an age of one million years, with the Sun at its center (not visible).

Enter Gaia.

In 31 out of 98 young star systems, Gaia has detected subtle motions that suggest the presence of unseen companions. For seven of these systems, the observed motions are consistent with objects of planetary mass. In eight systems, the data best match the presence of brown dwarfs—objects larger than planets but smaller than stars. The remaining sixteen systems likely have additional stars around.

Gaia’s predicted locations of these companions in the systems are shown in cyan. In the reference image of our baby Solar System, Jupiter’s orbit is also shown in cyan. Gaia discovered the companions in the baby star systems thanks to its unique ability to sense the gravitational tug or ‘wobble’ a planet or companion induces on a star. This technique had already been used to find companions around older stars. However, now, for the first time, a team of astronomers led by Miguel Vioque of the European Southern Observatory (ESO), Germany, has used this Gaia technique to find planets and companions around stars that are still forming.

The all-sky, large-scale nature of the Gaia survey enabled the team to study hundreds of forming stars and identify companions across large samples for the first time. This in contrast to costly ground-based searches that can only target a few stars at a time.

This ability of Gaia is benefiting the field of star and planet formation. The companions that the telescope has already found, can now be followed up by telescopes like the NASA/European Space Agency/Canadian Space Agency James Webb Space telescope that can study the inner discs of the baby systems in more detail.

With Gaia’s upcoming fourth data release, many more hidden planets are expected to be uncovered.

This new finding has been described in ‘Astrometric view of companions in the inner dust cavities of protoplanetary disks’ by M. Vioque et al., accepted for publication in Astronomy & Astrophysics.

Image Description: A collage of 32 glowing discs on a black background. Each disc shows concentric rings in vivid colours: purple, orange, and yellow, with bright cyan centres. The discs vary in size and orientation, creating a striking pattern of circular and elliptical shapes.

ESA's Gaia Mission:

Credits: ESO, ESA/Gaia/DPAC, M. Vioque et al.; CC BY-SA 3.0 IGO
Release Date: Dec. 18, 2025

#NASA #ESA #Space #Astronomy #Science #GaiaMission #GaiaSpaceTelescope #Stars #StellarNurseries #StarFormation #ProtoplanetaryDiscs #Exoplanets #PlanetarySystems #MilkyWayGalaxy #Cosmos #Universe #ALMA #ESO #Chile #Europe #STEM #Education

The Fomalhaut Triple Star System: Visualizing a Violent Collision | STScI

The Fomalhaut Triple Star System: Visualizing a Violent Collision | STScI

Hubble captured the violent collision of two massive objects around the star Fomalhaut. This extraordinary event is unlike anything in our own present-day solar system that we know of. The video shows the sequence of events leading up to the creation of dust cloud cs2 around the star Fomalhaut. In the opening frames, Fomalhaut appears in the top left corner. Two white dots, located in the bottom right corner, represent the two massive objects in orbit around Fomalhaut. These objects approach each other and collide, resulting in a huge debris cloud that initially resembles an exoplanet as seen in reflected light. Years later, starlight is able to push the dust cloud outward from the star. 

Fomalhaut is the brightest star in the southern constellation of Piscis Austrinus, the Southern Fish, and one of the most luminous stars in the night sky.

Distance from Earth: ~25 light years


Video Credits: NASA, ESA, Ralf Crawford Space Telescope Science Institute (STScI)
Duration: 35 seconds
Release Date: Dec. 18, 2025

#NASA #ESA #Astronomy #Space #Science #Star #Fomalhaut #ObjectCollisions #DustCloudcs2 #AsteroidBelts #CircumstellarDiscs #Exoplanets #PiscisAustrinus #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education #Animation #HD #Video

The Fomalhaut Triple Star System: Witnessing the "Destruction of Worlds" | Hubble

The Fomalhaut Triple Star System: Witnessing the "Destruction of Worlds" | Hubble

NASA’s Hubble Space Telescope has captured a rare and violent event unfolding around the nearby star Fomalhaut, an apparent collision between two large bodies in a distant planetary system. This discovery sheds light on the chaotic processes that may have shaped our own solar system billions of years ago. With support from both Hubble and the James Webb Space Telescope, astronomers are now closely monitoring the aftermath.

Fomalhaut is the brightest star in the southern constellation of Piscis Austrinus, the Southern Fish, and one of the brightest stars in the night sky.

Distance from Earth: ~25 light years


Credit: NASA's Goddard Space Flight Center 
Paul Morris: Lead Producer
Animation: Space Telescope Science Institute (STScI)
Duration: 3 minutes
Release Date: Dec. 18, 2025

#NASA #ESA #Astronomy #Space #Science #Star #Fomalhaut #AsteroidBelts #CircumstellarDiscs #Exoplanets #PiscisAustrinus #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education #Animation #HD #Video

Close-up: Dwarf Galaxy Markarian 178 in Ursa Major | Hubble

Close-up: Dwarf Galaxy Markarian 178 in Ursa Major | Hubble

The glittering blue galaxy in this Hubble Space Telescope picture is a blue compact dwarf galaxy called Markarian 178 (Mrk 178). This galaxy, substantially smaller than our own Milky Way, lies 13 million light-years away in the constellation Ursa Major (The Great Bear). Mrk 178 is one of more than 1,500 Markarian galaxies. These galaxies get their name from the Armenian astrophysicist Benjamin Markarian. He compiled a list of galaxies that were surprisingly bright in ultraviolet light.

While the bulk of the galaxy is blue owing to an abundance of young, hot stars with little dust shrouding them, Mrk 178 gets a red hue from a collection of massive stars that are especially concentrated in the brightest, reddish region near the galaxy’s edge. This azure cloud is home to a large number of rare objects called Wolf–Rayet stars. Wolf–Rayet stars are massive stars that are casting off their atmospheres through powerful winds. Because Mrk 178 contains so many Wolf–Rayet stars, the bright emission lines from these stars’ hot stellar winds are etched upon the galaxy’s spectrum. Particularly ionized hydrogen and oxygen appear as a red color to Mrk 178 in this photo, observed using Hubble’s specialized light filters.

Massive stars enter the Wolf–Rayet phase just before they collapse into black holes or neutron stars. Because Wolf–Rayet stars last for only a few million years, researchers know that something must have triggered a recent burst of star formation in Mrk 178. At first glance, it is not clear what could be the cause—Mrk 178 does not seem to have any close galactic neighbors that could have stirred up its gas to form new stars. Instead, researchers suspect that a gas cloud crashed into Mrk 178, or its gas may have been disturbed as the galaxy swims through the intergalactic medium, lighting up this tiny galaxy with a ripple of bright new stars.

Image Description: A pale blue dwarf galaxy seen on the black backdrop of space with faraway galaxies. The galaxy itself resembles a fuzzy cloud of tightly-packed stars with a broad halo of stars dispersed around it. Several small, glowing patches of gas are spread across the galaxy’s core, where very hot stars are concentrated.


Credit: ESA/Hubble & NASA, F. Annibali, S. Hong
Duration: 30 seconds
Release Date: Dec. 8, 2025


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #WolfRayetStars #Galaxies #Markarian178 #Mrk178 #DwarfGalaxies #UrsaMajor #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Close-up: Spiral Galaxy NGC 4388 in Virgo | Hubble

Close-up: Spiral Galaxy NGC 4388 in Virgo | Hubble


A sideways spiral galaxy shines in this Hubble Space Telescope picture. Located about 60 million light-years away in the constellation Virgo (The Maiden), NGC 4388 is a resident of the Virgo galaxy cluster. The Virgo cluster contains more than a thousand galaxies and is the nearest large galaxy cluster to the Milky Way.

NGC 4388 is tilted at an extreme angle relative to our point of view, giving us a nearly edge-on vantage point. This perspective reveals a curious feature that was not visible in a previous Hubble image of this galaxy released in 2016: a plume of gas from the galaxy’s nucleus, here seen billowing out from the galaxy’s disc towards the lower-right corner of the image. However, where did this outflow come from, and why does it glow?

The answer likely lies in vast stretches that separate the galaxies of the Virgo cluster. Though the space between the galaxies appears to be empty, this space is actually occupied by hot wisps of gas called the intracluster medium. As NGC 4388 journeys within the cluster, it plunges through the intracluster medium. The pressure from the hot intracluster gas whisks away the gas from within NGC 4388’s disc, causing it to trail behind as NGC 4388 moves.

The source of the energy that ionizes this gas cloud and causes it to glow is more uncertain. Researchers suspect that a portion of the energy comes from the center of the galaxy, where a supermassive black hole has spun the gas around it into a superheated disc. The blazing radiation from this disc might ionize the gas closest to the galaxy, while shock waves might be responsible for ionizing the filaments of gas farther out.

This image incorporates new data including several additional wavelengths of light to bring the ionized gas cloud into view. The data used to create this image come from several observing programs that aim to illuminate galaxies with active black holes at their centers.

Image Description: A spiral galaxy seen nearly edge-on. Its disk is filled with red and blue lights from star-forming nebulae and clusters of hot stars, respectively, as well as thick dark clouds of dust that block the strong white light from its center. A faint, glowing halo of gas surrounds the disc, fading into the black background. A bluish plume of gas also extends from the galaxy’s core to the lower-right of the image.


Credit: ESA/Hubble & NASA, S. Veilleux, J. Wang, J. Greene
Duration: 30 seconds
Release Date: Dec. 15, 2025

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #NGC4388 #SpiralGalaxies #VirgoGalaxyCluster #VirgoCluster #Virgo #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Blue Origin NS-37 Crewed Flight: Michaela (Michi) Benthaus Pre-launch Profile

Blue Origin NS-37 Crewed Flight: Michaela (Michi) Benthaus Pre-launch Profile

Blue Origin's next New Shepard crewed flight, NS-37 is scheduled to lift off from Launch Site One in West Texas no earlier than on Thursday, December 18, 2025. Michaela (Michi) Benthaus will become the first wheelchair user to cross the Kármán line. Her story, advocacy, and passion are evident in everything she does. She is expanding the boundaries of human spaceflight.

Fly to space: https://www.blueorigin.com/new-shepard/fly


Video Credit: Blue Origin
Duration: 3 minutes
Release Date: Dec. 18, 2025

#NASA #Space #BlueOrigin #NewShepard #NewShepardRocket #NewShepardCrewCapsule #NS37Mission #NS37Crew #CommercialAstronauts #MichaelaMichiBenthaus #CommercialSpace #LaunchSiteOne #Texas #UnitedStates #FortheBenefitofEarth #JeffBezos #STEM #Education #HD #Video

Globular Cluster Messier 79 in Lepus: A snowstorm of stars | Hubble

Globular Cluster Messier 79 in Lepus: A snowstorm of stars | Hubble

It is beginning to look a lot like Christmas in this NASA/European Space Agency Hubble Space Telescope image of a blizzard of stars, resembling a swirling storm in a snow globe.

These stars make up the globular cluster Messier 79, located about 40,000 light-years from Earth in the constellation of Lepus (The Hare). Globular clusters are gravitationally bound groupings of up to one million stars. These giant “star globes” contain examples of the oldest stars in our galaxy. Messier 79 is no exception; it contains about 150,000 stars, packed into an area measuring just roughly 120 light-years across.

This 11.7-billion-year-old star cluster was first discovered by French astronomer Pierre Méchain in 1780. Méchain reported the finding to his colleague Charles Messier, who included it in his catalog of non-cometary objects: The Messier catalog. About four years later, using a larger telescope than Messier’s, William Herschel was able to resolve the stars in Messier 79 and described it as a “globular star cluster.”

In this sparkling Hubble image, Sun-like stars appear yellow-white and the reddish stars are bright giants that are in the final stages of their lives. Most of the blue stars sprinkled throughout the cluster are aging “helium-burning” stars that have exhausted their hydrogen fuel and are now fusing helium in their cores.


Credit: NASA and ESA
Acknowledgement: S. Djorgovski (Caltech) and F. Ferraro (University of Bologna)
Release Date: Dec. 18, 2017


#NASA #Hubble #Astronomy #Space #Science #Stars #StarClusters #GlobularClusters #Messier79 #M79 #Lepus #Constellations #MilkyWayGalaxy #Cosmos #Universe #HST #HubbleSpaceTelescope #ESA #Europe #GSFC #STScI #UnitedStates #STEM #Education

Wednesday, December 17, 2025

A Tour of the International Space Station | NASA's Johnson Space Center

A Tour of the International Space Station NASA's Johnson Space Center

What's it like to float through the International Space Station?

Come along with us for a guided tour! 

Our astronauts in low Earth orbit recorded this tour on Oct. 10, 2022, while NASA's SpaceX Crew-4 and Crew-5 missions were aboard.

As you glide through the ISS, pop-ups will appear highlighting each part of the station and what it is used for—wrapping up with a view of Earth and space through SpaceX's Dragon capsule. 

For more than 25 years, humans have been living and working on the International Space Station 24/7, helping us learn how to live in space (and prepare for missions to the Moon and Mars) while doing scientific research to make life better back on Earth.

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, Chris Williams

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

Credit: NASA
Duration: 15 minutes
Release Date: Dec. 17, 2025

#NASA #Space #ISS #Science #Planets #Earth #AstronautVideography #Astronauts #Japan #日本 #宇宙航空研究開発機構 #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #UnitedStates #STEM #Education #HD #Video

NASA’s Perseverance Mars Rover Ready to Roll for Miles in Years Ahead

NASA’s Perseverance Mars Rover Ready to Roll for Miles in Years Ahead

NASA’s Perseverance Mars rover captured this view of a location nicknamed “Mont Musard” on Sept. 8, 2025. Made up of three images, the panorama also captures another region, “Lac de Charmes,” where the rover’s team will be looking for more rock core samples to collect in the year ahead. 
Image Credit: NASA/JPL-Caltech/ASU/MSSS 

The rover has been acing a long-term series of durability tests, making the most of its enhanced navigation capabilities, and ferreting out new findings about Mars’ geologic past.

After nearly five years on Mars, NASA’s Perseverance rover has traveled almost 25 miles (40 kilometers), and the mission team has been busy testing the rover’s durability and gathering new science findings on the way to a new region nicknamed “Lac de Charmes,” where it will be searching for rocks to sample in the coming year.

Like its predecessor Curiosity that has been exploring the Gale Crater region of Mars since 2012, Perseverance was made for the long haul. NASA’s Jet Propulsion Laboratory in Southern California built Perseverance and leads the mission. It has continued testing the rover’s parts here on Earth to make sure the six-wheeled scientist will be strong for years to come. This past summer, JPL certified that the rotary actuators that turn the rover’s wheels can perform optimally for at least another 37 miles (60 kilometers); comparable brake testing is underway as well.

Over the past two years, engineers have extensively evaluated nearly all the vehicle’s subsystems in this way, concluding that they can operate until at least 2031.

“These tests show the rover is in excellent shape,” said Perseverance’s deputy project manager, Steve Lee of JPL, who presented the results on Wednesday at the American Geophysical Union’s annual meeting, the largest gathering of planetary scientists in the United States. “All the systems are fully capable of supporting a very long-term mission to extensively explore this fascinating region of Mars.”

Perseverance has been driving through Mars’ Jezero Crater, the site of an ancient lake and river system, where it has been collecting scientifically compelling rock core samples. In fact, in September, the team announced that a sample from a rock nicknamed “Cheyava Falls” contains a potential fingerprint of past microbial life.

More efficient roving

In addition to a hefty suite of six science instruments, Perseverance packs more autonomous capabilities than past rovers. A paper published recently in IEEE Transactions on Field Robotics highlights an autonomous planning tool called Enhanced Autonomous Navigation, or ENav. The software looks up to 50 feet (15 meters) ahead for potential hazards, then chooses a path without obstacles and tells Perseverance’s wheels how to steer there.

Engineers at JPL meticulously plan each day of the rover’s activities on Mars. However, once the rover starts driving, it is on its own and sometimes has to react to unexpected obstacles in the terrain. Past rovers could do this to a certain degree, but not if these obstacles were clustered near each other. They also could not react as far in advance, resulting in the vehicles driving slower while approaching sand pits, rocks, and ledges. In contrast, ENav’s algorithm evaluates each rover wheel independently against the elevation of terrain, trade-offs between routes, and “keep-in” or “keep-out” areas marked by human operators for the path ahead.

“More than 90% of Perseverance’s journey has relied on autonomous driving, making it possible to quickly collect a diverse range of samples,” said JPL autonomy researcher Hiro Ono, a paper lead author. “As humans go to the Moon and even Mars in the future, long-range autonomous driving will become more critical to exploring these worlds.”

New science

A paper published Wednesday in Science details what Perseverance discovered in the “Margin Unit,” a geologic area at the margin, or inner edge, of Jezero Crater. The rover collected three samples from that region. Scientists think these samples may be particularly useful for showing how ancient rocks from Mars’ deep interior interacted with water and the atmosphere, helping create conditions supportive for life.

From September 2023 to November 2024, Perseverance ascended 1,312 feet (400 meters) of the Margin Unit, studying rocks along the way— especially those containing the mineral olivine. Scientists use minerals as timekeepers because crystals within them can record details about the precise moment and conditions in which they formed.

Jezero Crater and the surrounding area holds large reserves of olivine that forms at high temperatures, typically deep within a planet, and offers a snapshot of what was going on in the planet’s interior. Scientists think the Margin Unit’s olivine was made in an intrusion, a process where magma pushes into underground layers and cools into igneous rock. In this case, erosion later exposed that rock to the surface, where it could interact with water from the crater’s ancient lake and carbon dioxide that was abundant in the planet’s early atmosphere.

Those interactions form new minerals called carbonates that can preserve signs of past life, along with clues as to how Mars’ atmosphere changed over time.

“This combination of olivine and carbonate was a major factor in the choice to land at Jezero Crater,” said the new paper’s lead author, Perseverance science team member Ken Williford of Blue Marble Space Institute of Science in Seattle. “These minerals are powerful recorders of planetary evolution and the potential for life.”

Together, the olivine and carbonates record the interplay between rock, water, and atmosphere inside the crater, including how each changed over time. The Margin Unit’s olivine appeared to have been altered by water at the base of the unit, where it would have been submerged. Nevertheless, the higher Perseverance went, the more the olivine bore textures associated with magma chambers, like crystallization, and fewer signs of water alteration.

As Perseverance leaves the Margin Unit behind for Lac de Charmes, the team will have the chance to collect new olivine-rich samples and compare the differences between the two areas.

Celebrating 4+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

Managed for NASA by Caltech, NASA’s Jet Propulsion Laboratory in Southern California built and manages operations of the Perseverance rover on behalf of the agency’s Science Mission Directorate as part of NASA’s Mars Exploration Program portfolio.


Credit: NASA's Jet Propulsion Laboratory/Caltech
Release Date: Dec. 17, 2025

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #STEM #Education 

NASA Perseverance Mars Rover’s View of Record-Breaking Drive | JPL

NASA Perseverance Mars Rover’s View of Record-Breaking Drive | JPL

This video shows the Perseverance Mars Rover’s point of view during a record-breaking drive that occurred June 19, 2025, the 1,540th Martian day, or sol, of the mission.

Perseverance rover was traveling northbound and covered 1,350.7 feet (411.7 meters) on that sol, over the course of about 4 hours and 24 minutes. This distance eclipsed its previous record of distance traveled in a single sol: 1,140.7 feet (347.7 meters), achieved on April 3, 2023 (Sol 753). 

An inset seen to the right of the video shows the rover’s position on an orbital map.

Prior to Perseverance’s arrival at Mars, NASA’s Opportunity rover held the single-sol drive-distance record, having covered 718.5 feet (219 meters) on March 20, 2005 (Sol 410).

The rover tracks seen in the video are from Perseverance’s two previous southbound traverses on May 18 and 19, 2025 (sols 1,509 and 1,510). 

This video was created by stitching together 300 image pairs from the rover’s navigation cameras (navcams). The images were captured at the rate of one image every 16 feet (5 meters) for the first third of the traverse, and then one every 3.3 feet (1 meter) for the remaining two-thirds. 

The navcam image pairs were combined with rover data on orientation, wheel speed, and steering angle, as well as data from Perseverance’s inertial measurement unit, and placed into a 3D virtual environment. The result is this reconstruction of the rover’s record drive with virtual frames inserted about every 4 inches (0.1 meters) of drive progress. 

The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach. This includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

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

Celebrating 4+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars


Video Credit: NASA/JPL-Caltech
Duration: 1 minute, 24 seconds
Release Date: Dec. 17, 2025

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #STEM #Education #HD #Video

NASA Astronaut Jonny Kim Returns to Houston | Johnson Space Center

NASA Astronaut Jonny Kim Returns to Houston | Johnson Space Center

NASA astronaut Jonny Kim returned to Earth on Tuesday, December 9, 2025, concluding an eight-month science mission aboard the International Space Station. This was Kim’s first spaceflight. Kim and Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky of Russia orbited Earth 3,920 times and traveled nearly 104 million miles over the course of their 245-day mission. The Soyuz MS-27 spacecraft launched and docked with the International Space Station on April 8, 2025. After the Soyuz MS-27 spacecraft landed in Kazakhstan, Kim boarded a NASA Gulfstream V that took him back to Ellington Field in Houston, Texas, while Ryzhikov and Zubritsky departed for their training base in Star City, Russia. Kim's flight landed in Houston on December 10. As he stepped off the plane, he was greeted by NASA leadership, family, and his fellow astronauts. 


Video Credit: NASA's Johnson Space Center
Duration: 2 minutes, 46 seconds
Release Date: Dec. 17, 2025


#NASA #Space #ISS #Science #Planets #Earth #CrewSpacecraft #SoyuzMS27Spacecraft #Astronauts #JonnyKim #JAXA #Japan #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition73 #JSC #Houston #UnitedStates #STEM #Education #HD #Video

Geminid Meteor Shower 2025: View from Iran

Geminid Meteor Shower 2025: View from Iran

Astrophotographer Khosro Jafarizadeh: "The Geminid meteor shower is one of the most spectacular astronomical events of the year, lighting up the night sky with bright and fast meteors. Observing this celestial phenomenon over the ancient fire temple Atashkooh in the city of Delijan-Iran creates a breathtaking combination of history and astronomy. The fire temple, a symbol of ancient Persian culture and spirituality, stands silently beneath the stars as meteors streak across the sky. This moment beautifully connects the deep past of human civilization with the vast universe above, reminding us of humanity’s long-standing fascination with the heavens."

Meteors come from leftover comet particles and bits from asteroids. When these objects come around the Sun, they leave a dusty trail behind them. Every year Earth passes through these debris trails. This allows the bits to collide with our atmosphere where they disintegrate to create fiery and colorful streaks in the sky. Unlike most meteor showers which originate from comets, the Geminids originate from an Apollo asteroid named 3200 Phaethon. 

Learn about the Geminid Meteor shower:

Iran, officially the Islamic Republic of Iran and also known as Persia, is a country in West Asia. It borders Iraq to the west, Turkey, Azerbaijan, and Armenia to the northwest, the Caspian Sea to the north, Turkmenistan to the northeast, Afghanistan to the east, Pakistan to the southeast, and the Gulf of Oman and the Persian Gulf to the south. 

Image Credit: Khosro Jafarizadeh
Location: Atashkuh, Delijan, Iran
Khosro's website: 

#NASA #Space #Astronomy #Science #Stars #SolarSystem #Planet #Earth #Meteors #MeteorShowers #Geminids #GeminidMeteorShower #Asteroids #3200Phaethon #Astrophotography #KhosroJafarizadeh #Astrophotographers #Atashkuh #Delijan #Iran #Persia #History #STEM #Education

Meet NASA's X-59 Test Pilot Jim “Clue” Less | Armstrong Flight Research Center

Meet NASA's X-59 Test Pilot Jim “Clue” Less Armstrong Flight Research Center

Get to know one of the NASA X-59 test pilots working on the Quesst mission—Jim Less, call sign “Clue.” What inspired him to become a test pilot? Does he sing karaoke? Learn about his pre-flight routine and what his career would be if he was not a test pilot.  

The X-59 quiet supersonic aircraft builds on decades of supersonic flight research and is the centerpiece of NASA’s Quesst mission. The vast amount of data collected over the years has given designers the tools they needed to craft the shape of the X-59. The goal is to enable the aircraft to fly at supersonic speeds and reduce a loud sonic boom to a quieter “sonic thump.” Follow the X-59 team as they take on the exciting journey of building the X-59 and working toward quiet supersonic flight.

The X-59’s engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.
The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.

For more information about the X-59 and NASA's Quesst mission, visit www.nasa.gov/quesst

NASA's Armstrong Flight Research Center (AFRC): https://www.nasa.gov/armstrong/


Video Credit: NASA's Armstrong Flight Research Center (AFRC)
Duration: 2 minutes
Release Date: Dec. 17, 2025


#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #X59Pilot #JimClueLess #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #NASAArmstrong #AFRC #Edwards #California #UnitedStates #STEM #Education #HD #Video

China's Commercial Reusable Rocket Achieves Key Breakthrough in First Flight

China's Commercial Reusable Rocket Achieves Key Breakthrough in First Flight

 

The first test flight of China's independently developed Zhuque-3 reusable rocket, also the country's first attempt to recover an orbital stage of a carrier rocket, has made important breakthrough despite a final-stage failure, said Dai Zheng, commander in chief of the Zhuque-3 mission.

The Zhuque-3 is a large-capacity, low-cost, reusable liquid launch vehicle independently developed by China to deploy large-scale constellations.

The Zhuque-3 rocket blasted off from the Dongfeng commercial space innovation pilot zone, near the Jiuquan Satellite Launch Center (JSLC) in northwest China.

After ignition and liftoff, the first and second stages of the rocket separated in about 130 seconds. The second stage continued to complete the orbital insertion mission, while the first stage began its return journey.

The reuse section appeared in people's sight on time. Nevertheless, its first-stage booster suffered anomalous combustion during recovery, failing to achieve a soft touchdown on the landing pad.

The specific causes are under investigation, according to Dai, also the CEO of LandSpace, the rocket's designer, who gave an exclusive interview to the China Central Television (CCTV) in Beijing.

"This launch was actually China's first attempt to recover the first stage of an orbital-deployed launch vehicle. From the very beginning, we didn't expect the maiden flight to be a guaranteed success, it was more of an experimental and exploratory endeavor, and the result is slightly regrettable," said Dai.

Getting a rocket from supersonic speed to a perfectly intact landing on the ground is an extremely difficult task for rocket control, and the retrieved footage from the rocket showed that Zhuque-3 is not far from success, according to Dai.

"After separation, it underwent a high-altitude, high-angle attitude adjustment. After the attitude adjustment, it ignited at an altitude of 80 kilometers. This high-altitude ignition phase is actually very successful. When it entered the lower 40-kilometer range, the engine was shut down. Then it entered the aerodynamic gliding phase, during which the rocket descended at a supersonic speed, which was very fast at this point, and we had to rely on the grid fins on the rocket and the onboard control system to control the rocket," he said.

"From 40 kilometers to the final three kilometers above the ground, the supersonic descent phase, the aerodynamic control during the phase were flawless. At three kilometers above the ground, a landing ignition was required, somewhat like an emergency brake. As the altitude dropped to zero, the speed essentially decreased to zero. Only then could the landing legs extend to absorb the final impact, allowing the rocket to land intact. This is an extremely challenging maneuver for rocket control. Our final attempt to brake failed, so it didn't function as a brake, and ultimately it crashed at the edge of the landing zone, approximately 40 meters from the designated touchdown center," said Dai.

Although the mission was not entirely successful, for Dai and his team, the successful entry into orbit is also very meaningful.

"The primary objective of this mission was to verify the rocket's ability to reach the designated orbit. It shows that our rocket is able to subsequently provide services to satellite customers. Recovery is a very important means for a rocket company to reduce costs, but for our customers, their requirement is you deliver their cargo, their payload, their satellite, to the intended operational orbit. Whether the rocket can be reused is not their concern. In fact, we didn't launch the rocket with a real payload this time, but with a dummy payload instead. For the rocket industry, especially for a private commercial rocket company like ours, a successful flight is essential to demonstrate the rocket's capability before we can sell it. This is actually an industry practice," said Dai.

By comparison, SpaceX's first landing test occurred in September 2013 on the sixth flight of a Falcon 9 and maiden launch of the v1.1 rocket version. Between 2013 to 2016, sixteen test flights were conducted, only six of these achieved a soft landing and recovery of the first-stage booster. 

SpaceX CEO Elon Musk has commented on the Landspace Zhuque-3's design: "They have added aspects of Starship, such as use of stainless steel and methalox, to a Falcon 9 architecture, which would enable it to beat Falcon 9 . . ."


Video Credit: CCTV
Duration: 3 minutes
Release Date: Dec. 16, 2025

#NASA #Space #Satellites #Earth #LEO #China #中国 #LandSpace #蓝箭 #DaiZheng #Zhuque3Rocket #Zhuque3 #ReusableRockets #LaunchVehicles #MethaneLiquidOxygen #Methalox #JSLC  #JiuquanSatelliteLaunchCenter #酒泉卫星发射中心 #InnerMongolia #CommercialSpace #CommercialSpaceflight #STEM #Education #HD #Video