Monday, October 12, 2026

NASA’s Perseverance Mars Rover Sets Off-World Record for Total Distance Driven

NASA’s Perseverance Mars Rover Sets Off-World Record for Total Distance Driven

The animated orbital-map view in this video shows the route NASA’s Perseverance Mars rover has taken from time of its 2021 landing to Oct. 11, 2026—the day it broke the off-world driving record previously held by the agency’s Opportunity rover. As of that date, Perseverance has driven over 28 miles (45 kilometers). 

The six-wheeled geologist has in less than six years surpassed a mark set by the agency’s Opportunity rover that explored the Red Planet for nearly 15 years.

NASA’s Perseverance Mars rover has driven farther than any vehicle ever has on the surface of another world. On Oct. 11, the rover’s odometer reached 28.10 miles (45.22 kilometers), eclipsing the record of 28.06 miles (45.16 kilometers) set by NASA’s Opportunity rover that explored Mars from 2004 to 2018. Perseverance reached the mark on the 2,006th Martian day, or sol, of its mission, covering in five and a half years a distance that took Opportunity almost 15.

The milestone came as Perseverance traveled toward an area called “Idubi” through the region off the western rim of Jezero Crater nicknamed “Lac de Charmes,” where the rover is investigating what may be among the oldest terrain ever explored in the solar system. The rocks and terrain of Lac de Charmes are so ancient that their Earthly equivalents have long since been erased by erosion and plate tectonics (Mars does not have tectonic plates), and Idubi is where the science team hopes to find traces of ancient hydrothermal systems.

Much of the credit belongs to Perseverance’s self-driving capability. Using an autonomous navigation system known as AutoNav, the rover images the terrain while rolling, builds a 3D map of hazards, and plots its course between waypoints selected by rover planners on Earth—a capability the team calls “thinking while driving.” Perseverance can do all that at or near its top speed, covering as much as 1,351 feet (412 meters) in a single sol. The six-wheeled scientist has driven more than 90% of its total distance using AutoNav to evaluate the terrain, compared with about 5% for the first Martian AutoNav system on Opportunity and its twin, Spirit. Where NASA’s first Mars rover, Sojourner, assessed the path ahead using 20 measurement points, Perseverance processes 600,000 with every look.

“It is an honor to be working on Perseverance at a moment when the technology has evolved to the point that drives like these are routine,” said Steven Lee, the project manager of the Curiosity and Perseverance rovers at NASA’s Jet Propulsion Laboratory in Southern California. “The original mission called for no more than 12.4 miles of driving. We’ve blown well past that, and with all mobility systems fully operational and favorable extended-ground-life test results, we expect Perseverance to keep adding to this record for many years to come.”

NASA recently approved the mission’s first extension that began in October and will carry Perseverance’s exploration of the crater rim through roughly the end of 2028.

Perseverance’s record caps nearly three decades of NASA rover operations on Mars, each mission driving farther and more capably than the last.

The microwave-oven-size Sojourner rover covered about 330 feet (100 meters) during its 83-sol mission in 1997. The golf-cart-size twins Spirit and Opportunity arrived in 2004 with 90-sol prime missions. Spirit logged 4.8 miles (7.7 kilometers) before succumbing to the Martian winter in 2010. Opportunity kept rolling for 5,111 sols, completing the first extraterrestrial marathon in 2015 and setting the record Perseverance has now surpassed. The agency’s Curiosity rover, which landed in Gale Crater in 2012 and remains hard at work, has logged more than 23.65 miles (38.07 kilometers).

“The rover that broke this record did so by making its own decisions about the path. Given the autonomy to just go, Perseverance is a better driver than the one that landed, and we’re not done,” Mark Maimone, deputy team chief for robotic operations on Perseverance. “Our newest software teaches Perseverance to steer less and roll more, and to check its own position against orbital maps mid-drive. The next frontier is sunlight itself. Glare in the navigation cameras is why we park by mid-afternoon if we’re driving toward the Sun, and if we can teach the rover to see past those artifacts, every rover that follows gets a longer working day.”

The extraterrestrial off-road driving record is not limited to Mars: Lunar driving records were broken earlier in the journey. Perseverance rolled past both the 22.2 miles (35.7 kilometers) covered by Apollo 17 astronauts Gene Cernan and Harrison Schmitt in 1972 and the 24.2 miles (39 kilometers) driven by the Soviet Union’s Lunokhod 2 rover in 1973.

Setting distance records is just a bonus. Stamina and longer drives are putting more geologic diversity within reach faster—more outcrops examined and more of the Red Planet’s history read from its rocks. As a result, Perseverance has reached an ancient lakebed and a fossilized river system, where the rover found a potential biosignature at a rock called “Cheyava Falls.” Meanwhile, another ancient habitat—hydrothermal—may await.

Perseverance has collected 29 rock and regolith samples spanning the crater floor, a delta fan formed by a long-gone river, and now the crater rim. In the latter region, it has been exploring impact-generated rocks about 4 billion years old, from a chapter of planetary history almost entirely erased on Earth.

After Lac de Charmes, the rover will continue along the crater rim and head south during the extended mission towards Rainbow Falls, a 328-foot-wide (100-meter-wide) block of ancient crust uplifted by the impact that created Jezero.

Managed for NASA by Caltech, JPL 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.

For more information on NASA's Mars missions, visit: mars.nasa.gov

Video Credit: NASA's Jet Propulsion Laboratory-Caltech
Duration: 2 minutes
Release Date: Oct. 12, 2026


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

Planet Mars and The Beehive Cluster under Auroral Curtain over Sweden

Planet Mars and The Beehive Cluster under Auroral Curtain over Sweden

Astrophotographer Petr Horálek: "During Saturday's G3 geomagnetic storm, one detail was somewhat overlooked: the planet Mars was at its closest angular proximity to the center of the M44 Beehive (or Praesepe) open star cluster. While this "meeting" event itself was visible from many parts of the world only in the early morning hours, there were regions where it could be observed for a significant portion of the night—specifically north of the Arctic Circle, where this beautiful celestial clustering appeared very low on the horizon due to the high ecliptic latitude. I was fortunate to be in a location with a clear view near Lansjärv, Sweden, where this lovely celestial encounter unfolded directly beneath the 'curtain' of an exceptionally bright aurora. Its brilliance was so intense that it beautifully illuminated the landscape on an otherwise moonless night. A truly rare sight!"

The Beehive Cluster (also known as Messier 41, M41 or NGC 2287) is an open star cluster in the constellation Canis Major. Located approximately four degrees south of Sirius, it forms a roughly equilateral triangle with Sirius and Nu2 Canis Majoris, visible together in binoculars. The cluster spans an area comparable to the size of the full Moon and contains about a hundred stars, including several red giants and white dwarfs.

Known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

Sweden, formally the Kingdom of Sweden, is a Nordic country located on the Scandinavian Peninsula in Northern Europe. It borders Norway to the west and north, and Finland to the east.

Image Credit: Petr Horálek
Location: Lansjarv, Sweden
Petr's website: https://www.petrhoralek.com
Release Date: Oct. 10, 2026


#NASA #Space #Astronomy #Science #Stars #StarClusters #BeehiveCluster #Planets #Mars #Earth #Aurora #AuroraBorealis #NorthernLights #SolarSystem #Sun #Astrophotography #PetrHorálek #Astrophotographer #Lansjärv #Sweden #Sverige #STEM #Education

Aurora Borealis on Ice over Finland

Aurora Borealis on Ice over Finland

Astrophotographer Karsten Berger: "The clear icy surface of the frozen lake offered a rare opportunity to capture this reflection."

Known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

Finland is a Nordic country in Northern Europe. It borders Sweden to the northwest, Norway to the north, and Russia to the east, with the Gulf of Bothnia to the west and the Gulf of Finland to the south, opposite Estonia. Levi is located in Finnish Lapland. At a latitude of 67.8° north, it is approximately 170 km (110 mi) north of the Arctic Circle.

Image Credit: Karsten Berger
Location: Levi, Finland
Dates: Oct. 12, 2026

#NASA #Space #Astronomy #Science #Planets #Earth #Aurora #AuroraBorealis #NorthernLights #SolarSystem #Sun #Astrophotography #KarstenBerger #Astrophotographer #Levi #Finland #Suomi #STEM #Education

Welcome Home, ESA Astronaut Sophie Adenot! | International Space Station

Welcome Home, ESA Astronaut Sophie Adenot! | International Space Station

European Space Agency astronaut Sophie Adenot has arrived back in Europe, landing in Cologne, Germany.


After 237 days and over 3,700 orbits around Earth aboard the International Space Station, European Space Agency (ESA) astronaut Sophie Adenot of France is back on Earth! Following a handover to Crew-13, Sophie and her Crew-12 crewmates undocked on October 7, 2026, and splashed down off the coast of California the next day.

From Ellington Field in Houston, Sophie boarded a French Air and Space Force Airbus A330 MRTT Phénix bound for ESA’s European Astronaut Center (EAC) in Cologne, Germany. She landed at 04:21 GMT/06:21 CEST on October 10 and was warmly welcomed by family, friends, colleagues, journalists and representatives from ESA Member States.

Now back in Europe, Sophie will begin her post-flight data collection and rehabilitation while readjusting to life on Earth after the longest mission in space by a European astronaut so far.

Welcome home, Sophie!



Expedition 75 Crew
Station Commander: Pyotr Dubrov 
Roscosmos (Russia) Flight Engineers:
Anna Kikina,
Sergey Teteryatnikov
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Anil Menon, Jessica Watkins, Luke Delaney 

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: European Space Agency (ESA)
Release Date: Oct. 12, 2026



#NASA #Space #Science #ISS #Planets #Earth #Crew12 #Astronauts #SophieAdenot #France #Europe #ESA #Cosmonauts #AndreyFedyaev #Russia #Россия #Roscosmos #Роскосмос #Europe #ESA #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education

This Week at Roscosmos—Russia's Space Agency: Aist-2T, Crew-12 & Board Meetin

This Week at Roscosmos—Russia's Space Agency: Aist-2T, Crew-12 & Board Meeting

▪️ A meeting of the Roscosmos Supervisory Board was held at the National Space Center named after the world's first female cosmonaut, Vera Tereshkova.

▪️ Roscosmos cosmonaut Andrei Fedyayev returned from the ISS on the Crew Dragon spacecraft.

▪️ Roscosmos and Rostec presented the first 3D images of Earth from the Aist-2T satellites

Roscosmos cosmonaut Andrei Fedyayev successfully splashed down in the Pacific Ocean with his fellow crew members as part of NASA's SpaceX Crew-12 on October 8, 2026. He completed 237 days at the International Space Station. Fedyayev has visited the International Space Station twice on a SpaceX Crew Dragon spacecraft. 

Roscosmos cosmonaut Pyotr Dubrov accepted command of the International Space Station from NASA astronaut Jessica Meir as part of the Expedition 75 Mission after a ceremony on Sunday, October 4.

The Aist (Russian: Аист, meaning "Stork") satellites are a series of Russian microsatellites developed primarily by students, postgraduates, and researchers at Samara National Research University (formerly Samara State Aerospace University, SGAU) in collaboration with TsSKB-Progress (now part of Roscosmos).

Spektr-RG (Спектр-РГ), also called Spectrum-X-Gamma, SRG and SXG, is a Russian–German high-energy astrophysics space observatory launched in 2019. The spacecraft entered an orbit around the Sun, circling the Sun-Earth L2 Lagrangian point in a halo orbit, about 1.5 million kilometers away from Earth. The primary instrument of the mission is eROSITA, built by the Max Planck Institute for Extraterrestrial Physics (MPE) in Germany. It is designed to conduct a seven-year x-ray survey, the first in the medium x-ray band less than 10 keV energies, and the first to map an estimated 100,000 galaxy clusters. This survey may detect new clusters of galaxies and active galactic nuclei. The second instrument, ART-XC, is a Russian high-energy x-ray telescope capable of detecting supermassive black holes.

Follow the International Space Station's Expedition 75 Mission:

Expedition 75 Crew
Station Commander: Pyotr Dubrov 
Roscosmos (Russia) Flight Engineers:
Anna Kikina,
Sergey Teteryatnikov
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Anil Menon, Jessica Watkins, Luke Delaney 

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.


Video Credit: Roscosmos
Duration: 3 minutes
Date: Oct. 12, 2026

#NASA #Space #Science #Astronomy #Satellites #Aist2T #EarthObservation #SpektrRG #ISS #Planets #Earth #SpaceXCrewDragonSpacecraft #Crew12 #Astronauts #Europe #ESA #Cosmonauts #AndreyFedyaev #Russia #Россия #Roscosmos #Роскосмос #Europe #ESA #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education #HD #Video

Welcome Home, ESA Astronaut Sophie Adenot! | International Space Station

Welcome Home, ESA Astronaut Sophie Adenot! | International Space Station

After 237 days and over 3,700 orbits around Earth aboard the International Space Station, European Space Agency astronaut Sophie Adenot of France is back on Earth! Following a handover to Crew-13, Sophie and her Crew-12 crewmates undocked on October 7, 2026, and splashed down off the coast of California the next day.

Now back in Europe, Sophie will begin her post-flight data collection and rehabilitation while readjusting to life on Earth after the longest mission in space by a European astronaut so far.

Welcome home, Sophie!


Expedition 75 Crew
Station Commander: Pyotr Dubrov 
Roscosmos (Russia) Flight Engineers:
Anna Kikina,
Sergey Teteryatnikov
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Anil Menon, Jessica Watkins, Luke Delaney 

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: European Space Agency (ESA)
Duration: 3 minutes
Release Date: Oct. 12, 2026



#NASA #Space #Science #ISS #Planets #Earth #Crew12 #Astronauts #SophieAdenot #France #Europe #ESA #Cosmonauts #AndreyFedyaev #Russia #Россия #Roscosmos #Роскосмос #Europe #ESA #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education #HD #Video

Planet Mars: Preparing Europe's Rosalind Franklin Rover for a First Drive | ESA

Planet Mars: Preparing Europe's Rosalind Franklin Rover for a First Drive | ESA

Of course, before the European Space Agency's Rosalind Franklin can explore the planet Mars, it has to get off its lander. Engineers are rehearsing this on Earth using a full-size rover model and Mars-like terrain. The test recreates challenges Rosalind Franklin will face on the Red Planet from reduced gravity and a 20-degree incline to uneven ground and obstacles beneath its ramps.

Scheduled for launch in 2028, Rosalind Franklin is set to arrive on Mars in 2030.

ESA’s ExoMars program will deliver the European Rosalind Franklin Rover, tasked with searching for traces of life and with characterizing the shallow subsurface environment.

The ExoMars Rosalind Franklin Mission (EXM-RFM) includes important contributions from NASA: the launch service, the lander’s descent engines, Radioisotope Heating Units (RHUs) for the Rover’s thermal control, and components of the MOMA instrument. The mission’s launch is scheduled for late 2028. RFM will reach Mars after a journey of approximately two years, longer than the usual 9 months. This trajectory has been chosen to ensure that touchdown takes place during the northern-hemisphere spring to guarantee plenty of sunlight on the Rover’s solar panels.

The main scientific objective of Rosalind Franklin is to search for signs of past and present life. To achieve this goal, the mission will land at an ancient site—rich in sedimentary deposits (clay minerals) that formed in the presence of abundant liquid water—and explore the area in a quest for finding morphological and chemical biosignatures.

After landing, Rosalind Franklin will deploy its solar panels and locomotion system. Ground control will study the surroundings to choose directions for travel. The Rover can use one of two sets of descent ramps to reach the surface. Once on the ground, Rosalind Franklin will move away from the lander to start its traverse, identify, reach, and investigate scientifically promising locations.

The Rover is equipped with a drill to collect samples at and below the surface. The drill has a maximum vertical reach of 2 meters (~6.5 feet). Scientifically, this is very important because it is in the subsurface that organic molecules (some of which could be biosignatures) are preserved from the ravages of ionizing radiation prevailing at the top. The deepest anyone has explored for organic molecules on Mars is ~15 cm—a record still held today by NASA's Viking landers from the 1970s. Therefore, the 2-m drill will allow us to explore for the first time Mars’s third dimension: depth.

The Rosalind Franklin Rover will carry a set of eight instruments collectively referred to as “the Pasteur payload”. They will be utilized to explore the landing site, identify targets for close-up studies, characterize the shallow subsurface, and analyze samples obtained with the drill.


Video Credit: European Space Agency (ESA)
Duration: 1 minute, 44 seconds
Release Date: Oct. 12, 2026

#NASA #ESA #Space #Astronomy #Science #Planets #Mars #ExoMars #PlanetaryRovers #RosalindFranklin ##EXMRFM #Geology #Astrobiology #Europe #STEM #Education #HD #Video

Shenzhou-23 Space Science Experiments & In-Orbit Training | China Space Station

Shenzhou-23 Space Science Experiments & In-Orbit Training | China Space Station

The China Manned Space Agency (CMSA) on Sunday released its weekly update on the Shenzhou-23 mission, reporting that the crew continued to conduct scientific research and platform maintenance aboard the Tiangong Space Station.

Nearly five months into their mission, the three astronauts—Zhu Yangzhu, Zhang Zhiyuan and Lai Ka-ying—have steadily advanced space science and experiment tasks including experiments in microgravity physical science.

Last week, the crew replaced and processed experimental samples within the high-temperature materials experiment cabinet according to schedule.

In-orbit rendezvous and docking training was also carried out, during which the three astronauts completed image recognition exercises under various initial conditions using a metacognitive training system.

Additionally, the trio studied the spaceflight handbook and crew-equipment operating guidelines as planned.

For space-station maintenance, the crew conducted routine inspections and servicing of the regenerative environmental control and life-support system and related equipment. They also took inventory of medical supplies, organized materials and cleaned the interior of the cabinet.

The astronauts also exercised using equipment, such as a bone-loss countermeasure device and a neuromuscular stimulator, to mitigate the physiological effects of weightlessness.

The three astronauts were sent into space aboard the Shenzhou-23 spacecraft on May 24.

Shenzhou-23 Crew
Zhu Yangzhu 朱杨柱, Commander & Flight Engineer (second spaceflight)
Zhang Zhiyuan 张志远, Pilot (first spaceflight)
Lai Ka-ying/Li Jiaying 黎家盈, Payload Specialist (first spaceflight) [Hong Kong SAR]

Video Credit: CCTV
Duration: 1 minute
Release Date: Oct. 11, 2026

#NASA #Space #Science #China #中国 #Shenzhou23Mission #神舟二十三号 #Shenzhou23 #Taikonauts #Astronauts #ZhuYangzhu #ZhangZhiyuan #LiJiaying #LaiKaying #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #MicrogravityExperiments #SpaceLaboratory #CMSA #中国载人航天工程办公室 #HumanSpaceflight #STEM #Education #HD #Video

Sunday, October 11, 2026

Auroras after Solar Activity | International Space Station

Auroras after Solar Activity | International Space Station

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about aurora: 
https://science.nasa.gov/sun/auroras/

Two main types of explosions occur on the sun—solar flares and coronal mass ejections. Unlike the energy and x-rays produced in a solar flare that can reach Earth at the speed of light in eight minutes, coronal mass ejections (CMEs) are giant clouds of solar material that take one to three days to reach Earth. Once at Earth, these ejections, can impact satellites in space or interfere with radio communications. 


Expedition 75 Crew
Station Commander: Pyotr Dubrov 
Roscosmos (Russia) Flight Engineers:
Anna Kikina,
Sergey Teteryatnikov
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Anil Menon, Jessica Watkins, Luke Delaney 

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.


Credits: NASA's Johnson Space Center, A. Menon
Duration: 53 seconds
Date: Oct. 10, 2026

#NASA #Space #Science #ISS #Sun #CMEs #SolarSystem #Planets #Earth #Auroras #Astronauts #ESA #Europe #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #Europe #ESA #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education #HD #Video

Coronal Mass Ejection Hits Earth: Auroras Last Night | International Space Station

Coronal Mass Ejection Hits Earth: Auroras Last Night | International Space Station


Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about aurora: 
https://science.nasa.gov/sun/auroras/

Two main types of explosions occur on the sun—solar flares and coronal mass ejections. Unlike the energy and x-rays produced in a solar flare that can reach Earth at the speed of light in eight minutes, coronal mass ejections (CMEs) are giant clouds of solar material that take one to three days to reach Earth. Once at Earth, these ejections, can impact satellites in space or interfere with radio communications. 


Expedition 75 Crew
Station Commander: Pyotr Dubrov 
Roscosmos (Russia) Flight Engineers:
Anna Kikina,
Sergey Teteryatnikov
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Anil Menon, Jessica Watkins, Luke Delaney 

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.


Credits: NASA's Johnson Space Center, A. Menon
Date: Oct. 10, 2026

#NASA #Space #Science #ISS #Sun #CMEs #SolarSystem #Planets #Earth #Auroras #Astronauts #ESA #Europe #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #Europe #ESA #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education

Journey to Galaxy Centaurus A—A Galactic Merger | Victor Blanco Telescope

Journey to Galaxy Centaurus A—A Galactic Merger | Victor Blanco Telescope

This zoom shows a spectacular portrait of Centaurus A that was captured with the Dark Energy Camera (DECam) on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile. The galaxy Centaurus A, located over 12 million light-years away in the direction of the southern-hemisphere constellation Centaurus (The Centaur), is the leading light of this striking image. This image provides a view of the luminous glow of stars and dark tendrils of dust that hide the bright center of the galaxy. This dust is the result of a past galactic collision, where a giant elliptical galaxy merged with a smaller spiral galaxy. As well as large amounts of gas and dust, Centaurus A’s dust lane contains widespread star formation, as indicated by the red clouds of hydrogen and by the large numbers of faint blue stars visible at each end of the dust lane.

Centaurus A was discovered in 1826 by Scottish astronomer James Dunlop from his home in Parramatta, in New South Wales, Australia.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/DOE/NSF/AURA 
Acknowledgments: 
PI: M. Soraisam (University of Illinois at Urbana-Champaign/NSF NOIRLab) 
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab) & D. de Martin (NSF NOIRLab)
Duration: 1 minute
Release Date: Aug. 31, 2021

#NASA #Astronomy #Space #Science #Galaxies #CentaurusA #NGC5128 #Caldwell77 #InteractingGalaxies #BlackHoles #CentaurusConstellation #MilkyWayGalaxy #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #SouthAmerica #Europe #STEM #Education #HD #Video

Close-up: Galaxy Centaurus A—A Galactic Merger | Victor Blanco Telescope

Close-up: Galaxy Centaurus A—A Galactic Merger | Victor Blanco Telescope

The galaxy Centaurus A, located over 12 million light-years away in the direction of the southern-hemisphere constellation Centaurus (The Centaur), is the leading light of this striking image. This image provides a view of the luminous glow of stars and dark tendrils of dust that hide the bright center of the galaxy. This dust is the result of a past galactic collision, where a giant elliptical galaxy merged with a smaller spiral galaxy. As well as large amounts of gas and dust, Centaurus A’s dust lane contains widespread star formation, as indicated by the red clouds of hydrogen and by the large numbers of faint blue stars visible at each end of the dust lane.

Centaurus A was discovered in 1826 by Scottish astronomer James Dunlop from his home in Parramatta, in New South Wales, Australia.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/DOE/NSF/AURA 
Acknowledgments: 
PI: M. Soraisam (University of Illinois at Urbana-Champaign/NSF NOIRLab) 
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab) & D. de Martin (NSF NOIRLab)
Duration: 46 seconds
Release Date: Aug. 31, 2021

#NASA #Astronomy #Space #Science #Galaxies #CentaurusA #NGC5128 #Caldwell77 #InteractingGalaxies #BlackHoles #CentaurusConstellation #MilkyWayGalaxy #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #SouthAmerica #Europe #STEM #Education #HD #Video

Galaxy Centaurus A: The Result of a Galactic Merger | Victor Blanco Telescope

Galaxy Centaurus A: The Result of a Galactic Merger | Victor Blanco Telescope

The galaxy Centaurus A, located over 12 million light-years away in the direction of the southern-hemisphere constellation Centaurus (The Centaur), is the leading light of this striking image. This image provides a view of the luminous glow of stars and dark tendrils of dust that hide the bright center of the galaxy. This dust is the result of a past galactic collision, where a giant elliptical galaxy merged with a smaller spiral galaxy. As well as large amounts of gas and dust, Centaurus A’s dust lane contains widespread star formation, as indicated by the red clouds of hydrogen and by the large numbers of faint blue stars visible at each end of the dust lane.

Centaurus A was discovered in 1826 by Scottish astronomer James Dunlop from his home in Parramatta, in New South Wales, Australia.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/DOE/NSF/AURA 
Acknowledgments: 
PI: M. Soraisam (University of Illinois at Urbana-Champaign/NSF NOIRLab) 
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab) & D. de Martin (NSF NOIRLab) 
Release Date: Aug. 31, 2021

#NASA #Astronomy #Space #Science #Galaxies #CentaurusA #NGC5128 #Caldwell77 #InteractingGalaxies #BlackHoles #CentaurusConstellation #MilkyWayGalaxy #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #SouthAmerica #Europe #STEM #Education

Expedition 75 Crew Photos | International Space Station

Expedition 75 Crew Photos | International Space Station

The official portrait of the seven‑member Expedition 75 crew that now live and work aboard the International Space Station. From left, are Roscosmos cosmonaut Sergey Teteryatnikov (Russia); NASA astronaut Anil Menon; Station commander & Roscosmos cosmonaut Pyotr Dubrov (Russia); NASA astronaut Luke Delaney; Roscosmos cosmonaut Anna Kikina (Russia); NASA astronaut Jessica Watkins; and Canadian Space Agency (CSA) astronaut Joshua Kutryk

Eight Expedition 75 crew members gather inside the International Space Station’s Destiny laboratory module for a daily planning conference at the end of their shift. Clockwise from left are NASA astronaut Jessica Meir, Roscosmos cosmonauts Sergey Teteryatnikov and Anna Kikina of Russia, Canadian Space Agency astronaut Joshua Kutryk, European Space Agency astronaut Sophie Adenot, and NASA astronauts Jessica Watkins, Luke Delaney, and Jack Hathaway.

Two crews swapping places aboard the International Space Station pose together for a portrait inside the station’s Kibo laboratory module. In the front row are the members of NASA’s SpaceX Crew‑12 mission with, from left, Roscosmos cosmonaut Andrey Fedyaev (Russia), NASA astronauts Jack Hathaway and Jessica Meir, and European Space Agency astronaut Sophie Adenot. Hathaway and Meir hold a photograph of SpaceX personnel standing in front of a Falcon 9 rocket. In the back are the Crew‑13 members with Roscosmos cosmonaut Sergey Teteryatnikov (Russia), NASA astronauts Luke Delaney and Jessica Watkins, and Canadian Space Agency astronaut Joshua Kutryk.


Expedition 75 Crew
Station Commander: Pyotr Dubrov 
Roscosmos (Russia) Flight Engineers:
Anna Kikina,
Sergey Teteryatnikov
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Anil Menon, Jessica Watkins, Luke Delaney 

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.


Credits: NASA's Johnson Space Center, A. Menon
Dates: Oct. 4-7, 2026

#NASA #Space #Science #ISS #Planets #Earth #Astronauts #ESA #Europe #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #Europe #ESA #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education

Lunar Farside | NASA's Lunar Reconnaissance Orbiter (2009-2026)

Lunar Farside | NASA's Lunar Reconnaissance Orbiter (2009-2026)

Tidally locked in synchronous rotation, the Moon always presents its familiar nearside to denizens of planet Earth. From lunar orbit, the Moon's farside can become familiar, though. In fact this sharp picture, a mosaic from the Lunar Reconnaissance Orbiter's wide angle camera, is centered on the lunar farside. Part of a global mosaic of over 15,000 images acquired between November 2009 and February 2011, the highest resolution version shows features at a scale of 100 meters per pixel. Surprisingly, the rough and battered surface of the farside looks very different from the nearside covered with smooth dark lunar maria. A likely explanation is that the farside crust is thicker, making it harder for molten material from the interior to flow to the surface and form dark, smooth maria.

Learn more about LRO:
https://science.nasa.gov/mission/lro/

NASA's Lunar Reconnaissance Orbiter has made a 3-D map of the Moon's surface at 100-meter resolution and 98.2% coverage (excluding polar areas in deep shadow), including 0.5-meter resolution images of Apollo landing sites.

LRO has been studying the Moon from up close since 2009, making it the longest-lived lunar orbiting mission ever. The orbiter has mapped the Moon’s surface and measured its temperature, composition, and radiation environment in unprecedented detail. Data from LRO enables NASA, and our international and commercial partners, to select locations on the lunar surface where spacecraft and astronauts can safely land. The orbiter is also helping NASA identify areas near the Moon’s South Pole with crucial resources like water and extended sunlight that provides power for equipment and supports exploration activities.


Image Credit: NASA/GSFC/Arizona State University
Text Credit: J. Stopar
Authors & editors: Jerry Bonnell, Cecilia Chirenti, Robert Nemiroff, Keighley Rockcliffe
A service of the Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center, NASA Science Activation & Michigan Technological University (MTU)
Release Date: Oct. 10, 2026


#NASA #Space #Astronomy #Science #Earth #Moon #FarSide #Geology #Geoscience #LRO #LunarOrbiter #LROC #SpaceRobotics #SpaceTechnology #NASAGoddard #GSFC #ASU #UnitedStates #SolarSystem #LunarExploration #STEM #Education #APoD

South Korea's KSLV-II ('Nuri') Rocket Prelaunch | Korea AeroSpace Administration

South Korea's KSLV-II ('Nuri') Rocket Prelaunch | Korea AeroSpace Administration

South Korea's 200-ton, three-stage kerosene and liquid oxygen (LOX) KSLV-II rocket launched a record 15 satellites on its fifth flight: five NeonSat Earth observation smallsats, South Korea's first constellation launch, plus ten university-built CubeSats on Oct 7, 2026, at 12:25pm Korea Standard Time (KST) from the Naro Space Center in Goheung, south of the capital Seoul. Despite one cubesat failing to deploy, this marked a significant milestone for South Korea’s space program.

The Korean Space Launch Vehicle-II (KSLV-II) ('Nuri') rocket was built by Hanwha Aerospace. Nuri, means “world” in Korean.

This was the first time that Nuri has deployed multiple main satellites in a single flight. The five NeonSats are the start of South Korea's first constellation launched on its own rocket. Each one weighs under 100 kg (220 pounds) and can spot objects about 1 meter across. Five more go up on Nuri's sixth flight next year. Once all ten are deployed, South Korea can image the entire peninsula three or more times a day.


Video Credit: Korea Aerospace Research Institute (KARI)
Duration: 44 seconds
Date: Oct. 6, 2026

#NASA #KASA #KARI #Space #Science #Earth #Satellites #EarthObservation #RemoteSensing #Rockets #KSLVII #KSLVIIRocket #Nuri #누리 #HanwhaAerospace #한화에어로스페이스 #LG #SpaceTechnology #CommercialSpace #NaroSpaceCenter #Goheung #SouthKorea #대한민국 #Spaceports #STEM #Education #HD #Video