Tuesday, October 06, 2026

NASA's SpaceX Crew-12 Prepares for Earth Return | International Space Station

NASA's SpaceX Crew-12 Prepares for Earth Return | International Space Station

NASA's SpaceX Crew-12 members gather for a portrait in the pressure suits they will wear when they depart the International Space Station inside the SpaceX Dragon spacecraft. From left, Roscosmos cosmonaut and mission specialist Andrey Fedyaev of Russia, NASA astronauts Jack Hathaway and Jessica Meir, Crew-12 pilot and commander respectively, and European Space Agency (ESA) astronaut and mission specialist Sophie Adenot.
European Space Agency (ESA) astronaut and NASA's SpaceX Crew-12 mission specialist Sophie Adenot poses for a portrait while wearing the pressure suit she will wear when she departs the International Space Station inside the SpaceX Dragon spacecraft. 

European Space Agency astronaut and NASA's SpaceX Crew-12 mission specialist Sophie Adenot poses for a portrait while wearing the pressure suit she will wear when she departs the International Space Station inside the SpaceX Dragon spacecraft.
Roscosmos cosmonaut and NASA's SpaceX Crew-12 mission specialist Andrey Fedyaev of Russia poses for a portrait while wearing the pressure suit he will wear when he departs the International Space Station inside the SpaceX Dragon spacecraft.
NASA astronaut and NASA's SpaceX Crew-12 pilot Jack Hathaway poses for a portrait while wearing the pressure suit he will wear when he departs the International Space Station inside the SpaceX Dragon spacecraft.
European Space Agency astronaut and Expedition 75 flight engineer Sophie Adenot of France looks at the Earth below from the cupola, the International Space Station's "window to the world." Just outisde the cupola is the Russian Soyuz MS-29 spacecraft from Roscosmos docked to the Prichal module. 

NASA's SpaceX Crew-12 emblem

NASA astronauts Jessica Meir and Jack Hathaway will respectively command and pilot Dragon when it undocks from the Harmony module’s space-facing port at 8:05 a.m. EDT on Wednesday, October 7, 2026. Mission specialists Sophie Adenot of the European Space Agency (ESA) and Andrey Fedyaev of Roscosmos will ride back to Earth with the NASA duo for a parachute-assisted splashdown in the Pacific Ocean at 11:34 a.m. on Thursday where NASA and SpaceX support personnel will retrieve Dragon and greet the crew. Their return to Earth will represent the completion of NASA’s SpaceX Crew-12 mission after 237 days in space.

The homebound quartet has finalized packing Dragon with personal items, cargo, and scientific samples that began a couple of weeks ago. The returning crew also prepared drink bags combined with salt tablets that they will consume before reentering Earth’s atmosphere. Fluid loading is a part of every crew’s return to Earth and helps the body adjust to gravity after a long duration spaceflight.


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov,
Sergey Teteryatnikov
European Space Agency Flight Engineer: Sophie Adenot
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Jack Hathaway, 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.


Image Credits: NASA's Johnson Space Center, NASA astronaut Anil Menon, European Space Agency (ESA)
Image Dates: Sept. 21-22, 2026

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

NASA’s Curiosity Rover Catches Stunning Martian Dawn | Jet Propulsion Laboratory

NASA’s Curiosity Rover Catches Stunning Martian Dawn | Jet Propulsion Laboratory

The captivating shapes of wind-carved crags called yardangs are revealed in this zoomed-in crop of a broader panorama captured by NASA’s Curiosity Mars rover on Aug. 11, 2026. Scientists are eager to learn more about how the yardang layer formed. 

Image Description: A stark, grayish-tan Martian landscape features jagged rock formations and rolling mountain ridges beneath a pale, hazy sky.

A broad, panoramic view of a stark, grayish-tan Martian landscape features jagged rock formations and rolling mountain ridges beneath a hazy sky. Features in the front are darker while distant rock formations are washed in pale light.


NASA’s Curiosity Mars rover captured this view looking back at the floor of Gale Crater on Sept. 5, 2026. Just nine days prior, the rover had marked 1 kilometer of elevation gain above the crater floor since beginning its ascent of Mount Sharp in 2014.
Image Description: A wide panoramic view of a rocky, reddish-brown Martian valley framed by rugged hills under a hazy sky, with a portion of NASA’s Curiosity Mars visible on the far right.

This artist’s concept shows Mount Sharp, the 3-mile-tall (5-kilometer-tall) mountain that NASA’s Curiosity has been ascending since 2014. The location of the yardang layer, which the rover recently captured from a distance, is indicated by an ellipse annotation on the mountain’s northwestern shoulder. 
Image Description: A 3D topographical map shows a large Martian crater with a prominent central mountain peak, encircled by a black oval highlighting a specific region near the base of the mound.

A newly released panorama captured by NASA’s Curiosity rover offers the most detailed view yet of distant, wind-carved Martian cliffs, highlighting features the mission’s scientists have long been waiting to see up close. The scene was snapped at 8:30 a.m. local Mars time, showing striking blue hues in the foreground as bright morning light illuminates crags known as yardangs on the horizon.

This panorama was captured by Curiosity’s Mastcam on Aug. 11, 2026, the 4,982nd Martian day, or sol, of the mission, and comprises six individual images that were stitched together after being sent to Earth. Unlike most of Curiosity’s Mastcam images, this one was processed without white balancing, preserving the early morning appearance.

The yardang layer extends roughly 10 miles (16 kilometers) across the northwestern reaches of Mount Sharp, a 3-mile-tall (5-kilometer-tall) mountain that Curiosity has been ascending since 2014. In fact, the rover recently passed another milestone in its ascent, reaching 0.6 miles (1 kilometer) of elevation—the most ever climbed on Mars. As it draws ever-closer to the yardangs, mission scientists expect to get even more amazing imagery—and, they hope, answers to how these cliffs were created.

Mount Sharp is made up of layers, each recording a distinct period of Mars’ history. By studying them, scientists have been able to learn more about lakes and streams that covered this part of the Red Planet billions of years ago. Eventually, the water dried up and left salty minerals behind. After new material stopped settling on the mountain, part of it may have been stripped away by wind, giving rise to the yardangs.

“The yardang layer looks out of place. It’s the wrong color, the layers tilt at an odd angle, and it almost appears plastered on,” said Ashwin Vasavada, Curiosity project scientist of NASA’s Jet Propulsion Laboratory in Southern California. “But that’s what makes it exciting to reach. No one is sure exactly what created this layer, but one idea is it may be ash deposited by ancient volcanic eruptions.”

Curiosity is in the second year of its fifth extended mission. It started with an exploration of the spiderweb-like boxwork ridges. The rover will spend most of the next year or so driving through layers enriched with sulfates and carbonates, both signs of ancient drying on the surface. During 2027, scientists hope to reach the base of the yardangs, where Curiosity will be able to use its robotic arm to collect one-of-a-kind data on these mysterious features.

Curiosity was built by NASA's Jet Propulsion Laboratory (JPL), managed by Caltech in Pasadena, California. NASA JPL leads the mission on behalf of the agency’s Science Mission Directorate in Washington as part of its Mars Exploration Program portfolio. Malin Space Science Systems in San Diego built and operates Mastcam.

Celebrating 14+ Years on Mars (2012-2026)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

To learn more about Curiosity, visit: https://science.nasa.gov/mission/msl-curiosity/

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


Image Credit: NASA/JPL-Caltech/MSSS/ESA/DLR/FU Berlin
Image Dates: Aug. 11 & Sept. 5, 2026
Release Date: Oct. 6, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #Yardangs #CuriosityRover #Sol4982 #MSL #MountSharp #GaleCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #MarsExploration #SolarSystem #STEM #Education

Astronaut Pikachu gets a private tour | International Space Station

Astronaut Pikachu gets a private tour | International Space Station

Earlier this year, our astronaut Sophie Adenot gave astronaut Pikachu a special tour of the International Space Station as part of the Pokémon × European Space Agency (ESA) partnership. Now, as World Space Week 2026 begins, space fans can continue the adventure through Pokémon-themed exhibitions at science museums across Europe.

Learn more about World Space Week 2026: https://www.worldspaceweek.org

ESA and Pokémon are teaming up to inspire the next generation of explorers. Whether through science or imagination, discovery begins with curiosity.

Learn more about the ESA-Pokémon partnership here: https://bit.ly/4rO47Rv

Pokémon is a Japanese media franchise consisting of video games, animated series and films, a trading card game, and other related media. The franchise takes place in a shared universe where humans co-exist with special creatures, a large variety of species endowed with special powers.

Follow Sophie’s mission on the εpsilon page: https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/epsilon 


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov, 
Sergey Teteryatnikov
European Space Agency Flight Engineer: Sophie Adenot
Canadian Space Agency (CSA) Flight Engineer: Joshua Kutryk
NASA Flight Engineers: Jack Hathaway, 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: European Space Agency (ESA)
Duration: 2 minutes
Release Date: Oct. 6, 2026  

#NASA #Space #Science #Astronomy #ISS #Earth #Cupola #PokemonxESA #WorldSpaceWeek2026 #Pikachu #ピカチュウ #Pokemon #ポケモン #Japan #日本 #Children #Toys #Astronauts #SophieAdenot #France #CNES #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education #HD #Video

The Milky Way: View from Utah

The Milky Way: View from Utah



Astrophotographer Cary Bahora: "I'm 60 and never seen so many stars as I did in the extremely remote Henry Mountains of Utah at 10,500 ft. It was amazing walking around seeing clearly only by starlight. Two pics looking south. Other looking north. And is that a galaxy in the lower right on the northward looking pic?"

Generally speaking, the best time to see the Milky Way galaxy is during the Milky Way season from February to October, usually between 00:00 and 5:00, and on nights with a New Moon. This, however, will vary depending on the hemisphere, your latitude, and other factors like the moon phase.

The Henry Mountains is a mountain range located in the southeastern portion of the U.S. state of Utah that runs in a generally north-south direction, extending over a distance of about 30 miles (48 km). 

Utah is a landlocked state in the Mountain West subregion of the Western United States. It is one of the Four Corners states, sharing a border with Arizona, Colorado, and New Mexico. It also borders Wyoming to the northeast, Idaho to the north, and Nevada to the west.


Image Credit: Cary Bahora
Location: Henry Mountains, Utah, United States
Date: Oct. 1, 2026

#NASA #Astronomy #Space #Science #SolarSystem #Stars #SagittariusConstellation  #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #CaryBahora #Astrophotographers #HenryMountains #Utah #UnitedStates #STEM #Education

The Northern Lights over Reykjavik, Iceland

The Northern Lights over Reykjavik, Iceland

Astrophotographer Wioleta Gorecka: "This time, I wanted to capture the aurora borealis in the center of Reykjavík. It is not an easy task due to light pollution; the aurora needs to be strong enough to be visible and allow for a proper exposure. I managed to capture the shot just as the famous Hallgrímskirkja church was illuminated in pink—a symbol of the fight against breast cancer. The colors harmonized beautifully."

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 auroras: 
https://science.nasa.gov/sun/auroras/

Iceland is a Nordic island country between the Arctic Ocean and the North Atlantic Ocean, located on the Mid-Atlantic Ridge between Europe and North America. Reykjavík is the capital and largest city of Iceland. It is located on the southern shore of the Faxaflói bay in southwest Iceland and has a latitude of 64°08′ N, making it the world's northernmost capital of a sovereign state.

Image Credit: Wioleta Gorecka
Location: Reykjavik, Hallgrimskirkja
Wioleta's website: https://instagram.com/wiola.gorecka?igshid=ff0xckzefdlb
Release Date: Oct. 5, 2026

#NASA #Astronomy #Space #Science #Sun #SolarSystem #SolarWind #Planet #Earth #Magnetosphere #GeomagneticStorms #Aurora #AuroraBorealis #NorthernLights #Astrophotography #WioletaGorecka #Astrophotographers #Reykjavík #Iceland #Ísland #STEM #Education

Journey to The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

Journey to The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

This video takes the viewer on a journey through space to a technicolor dreamscape. It reveals a new image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. It portrays a stellar nursery known as NGC 7129, a nebula that holds numerous protostars and stars within its fields of gas and dust. Webb captured infrared light that pierces through the dense matter that scatters or absorbs other types of light. This region, rife with stellar objects at various stages of their lives, offers an opportunity to explore how stars shape their surrounding environment.

Also known as the Flower Bud Nebula or Small Cluster Nebula, NGC 7129 is a reflection nebula located about 3,300 light years away in the constellation Cepheus. A young open cluster is responsible for illuminating the surrounding nebula. The region to the left of the central star is filled with hot, atomic hydrogen gas. This creates a golden glow, while the region to the right is packed with cooler, molecular hydrogen. Embedded protostars in the rightmost region eject outflows that shock and heat the region, giving certain areas a red hue and a clumpy texture. Many of these red outflows, ejected as protostars accumulate mass, are visible throughout the image.

The central star and the stars embedded within the golden region are at a more mature stage in their life cycle than the protostars growing to the right of the central star. Their heat breaks down the molecular hydrogen into atoms, driving variations in temperature and color. The coldest, densest gas, where protostars have yet to form, is shown in grey.


Credit: ESA/Webb, NASA, CSA, WIYN and NOIRLab, NSF, AURA, DSS2, A. Pagan (STScI), N. Bartmann (ESA/Webb),  E. Slawik, N. Risinger, T. A. Rector, H. Schweiker, M. Zamani (ESA/Webb)
Duration: 1 minute, 30 seconds
Release Date: Oct. 6, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #Protostars #Nebulae #StellarNurseries #NGC7129 #FlowerBudNebula #SmallClusterNebula #CepheusConstellation #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #Europe #NASAGoddard #STScI #UnitedStates #CSA #Canada #STEM #Education #HD #Video

Close-up: The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

Close-up: The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

A technicolor dreamscape is revealed in this new image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. It portrays a stellar nursery known as NGC 7129, a nebula that holds numerous protostars and stars within its fields of gas and dust. Webb captured infrared light that pierces through the dense matter that scatters or absorbs other types of light. This region, rife with stellar objects at various stages of their lives, offers an opportunity to explore how stars shape their surrounding environment.

Also known as the Flower Bud Nebula or Small Cluster Nebula, NGC 7129 is a reflection nebula located about 3,300 light years away in the constellation Cepheus. A young open cluster is responsible for illuminating the surrounding nebula. The region to the left of the central star is filled with hot, atomic hydrogen gas. This creates a golden glow, while the region to the right is packed with cooler, molecular hydrogen. Embedded protostars in the rightmost region eject outflows that shock and heat the region, giving certain areas a red hue and a clumpy texture. Many of these red outflows, ejected as protostars accumulate mass, are visible throughout the image.

The central star and the stars embedded within the golden region are at a more mature stage in their life cycle than the protostars growing to the right of the central star. Their heat breaks down the molecular hydrogen into atoms, driving variations in temperature and color. The coldest, densest gas, where protostars have yet to form, is shown in grey.


Credit: NASA, ESA, CSA, STScI, N. Bartmann (ESA/Webb)
Image Processing: A. Pagan (STScI)
Duration: 30 seconds
Release Date: Oct. 6, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #Protostars #Nebulae #StellarNurseries #NGC7129 #FlowerBudNebula #SmallClusterNebula #CepheusConstellation #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #Europe #NASAGoddard #STScI #UnitedStates #CSA #Canada #STEM #Education #HD #Video

The Flower Bud Nebula: NGC 7129 in Cepheus | James Webb Space Telescope

The Flower Bud Nebula: NGC 7129 in Cepheus | James Webb Space Telescope

The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope’s Near-InfraRed Camera (NIRCam) has revealed many protostars and stars within the glowing gases of NGC 7129. Also known as the Flower Bud Nebula or Small Cluster Nebula, NGC 7129 is a reflection nebula located about 3,300 light years away in the constellation Cepheus. A young open cluster is responsible for illuminating the surrounding nebula. The region to the left of the central star is filled with hot, atomic hydrogen gas. This creates a golden glow, while the region to the right is packed with cooler, molecular hydrogen. Embedded protostars in the rightmost region eject outflows that shock and heat the region, giving certain areas a red hue and a clumpy texture. Many of these red outflows, ejected as protostars accumulate mass, are visible throughout the image.

The central star and the stars embedded within the golden region are at a more mature stage in their life cycle than the protostars growing to the right of the central star. Their heat breaks down the molecular hydrogen into atoms, driving variations in temperature and color. The coldest, densest gas, where protostars have yet to form, is shown in grey.

Image Description: A young star cluster filled with many stars that display Webb’s unique eight-pronged diffraction pattern. At its center is a yellow star which sports the largest diffraction pattern. To the left of the star, there is a region filled with yellow dust and gas that extends from the star to the left border of the image. This yellow region extends from the bottom, covering about two-thirds of the image. The yellow region has several blue stars of different sizes embedded within. The top third lies outside of the yellow region. It holds a few bright protostars within dense gray gas. Those stars illuminate the gas, making it appear blue. A few red outflows from other protostars are visible above this grayish-blue region. To the right of the central star, there is a clumpy, flame-like plume of red dust and gas with protostars that emit a soft white light within. The plume is surrounded by more dense gray gas and dust. There are several background galaxies strewn throughout the image.


Credit: NASA, ESA, CSA, STScI
Image Processing: A. Pagan (STScI)
Release Date: Oct. 6, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #Protostars #Nebulae #StellarNurseries #NGC7129 #FlowerBudNebula #SmallClusterNebula #CepheusConstellation #Cosmos #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #Europe #NASAGoddard #STScI #UnitedStates #CSA #Canada #STEM #Education

Monday, October 05, 2026

Swirling Spiral Galaxy Messier 83 in Hydra (radio telescope view) | ALMA

Swirling Spiral Galaxy Messier 83 in Hydra (radio telescope view) | ALMA

Like a portal to another dimension, a hypnotizing swirl is featured in this picture of the spiral galaxy Messier 83 (M83), also known as the Southern Pinwheel, located approximately 15 million light-years away. It is one of the brightest galaxies in the night sky, but this image––taken with the Atacama Large Millimeter/submillimeter Array (ALMA). ALMA does not show how M83 looks in the light our eyes can see. Instead, it depicts the light emitted by cold gas molecules, the ingredients of star formation.

Nicolas-Louis de Lacaille discovered M83 on February 17, 1752, at the Cape of Good Hope.

Astronomers are interested in molecular gas clouds as virtually all stars are born from their collapse. Once stars form, they heat up their surroundings, making it harder for gas to condense and form further stars. This, combined with galactic dynamics that continually stirs gas, controls the growth of galaxies. ALMA allows astronomers to map how the density and temperature of these gas clouds change at locations within a galaxy, such as the central regions, the spiral arms, or the space between them. This in turn helps us understand star formation in a variety of galactic environments. The European Southern Observatory (ESO) is an ALMA partner. 

M83 closely resembles our own galaxy, the Milky Way. Since M83 appears nearly face-on in the sky, astronomers enjoy a privileged view to study whether the recipe to turn gas into stars is universal or changes within M83.

Image Description: This image shows an object made of two spiral arms connected at the center, in shades of orange against a black background. The object is brightest at the center and along the spiral arms. The spirals are composed of cloud-like threads that become more diffuse further away from the center of the image, spreading out like loose tufts of wool.

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF), and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the National Science and Technology Council (NSTC) in Taiwan, and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).

ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of ALMA's construction, commissioning, and operation. 


Learn more about the Atacama Large Millimeter/submillimeter Array (ALMA):
https://www.almaobservatory.org/en/about-alma/

Credit: ALMA(ESO/NAOJ/NRAO)/J. Koda et al.
Release Date: Oct. 5, 2026

#NASA #Astronomy #Science #Space #Messier83 #M83 #SouthernPinwheelGalaxy #NGC5236 #SpiralGalaxies #HydraConstellation #Cosmos #Universe #ALMA #RadioAstronomy #Chile #NSF #AUI #NRAO #UnitedStates #NAOJ #Japan #ESO #Europe #STEM #Education

The Sombrero Galaxy's Tidal Streams: Messier 104 in Virgo | View from Namibia

The Sombrero Galaxy's Tidal Streams: Messier 104 in Virgo | View from Namibia


A deep image of the Sombrero galaxy reveals surprises. Messier 104 (M104) is named the Sombrero galaxy because, on shorter exposures, it looks like a hat. A key defining feature of this huge galaxy is a dark brim of dust that circles the disk galaxy's center. A much longer exposure, however, brings up a hairy past where a bright, hazy halo is revealed that extends well past the central disk and contains many unresolved stars. Surprisingly, in this stellar haze, structures can be seen that include a diagonal ring. These structures and tidal streams provide fresh evidence that M104 had a violent past and is surely the result of collisions and mergers of smaller galaxies. Light takes about 30 million years to reach us from the Sombrero galaxy. It fully spans about 150 thousand light years across. This image was taken over seven days in mid-2026 from Namibia.

Namibia, officially the Republic of Namibia, is a country in southern Africa. Its borders include the Atlantic Ocean to the west, Angola and Zambia to the north, Botswana to the east and South Africa to the south; in the northeast, approximating a quadripoint, Zimbabwe lies less than 200 meters (660 feet) away along the Zambezi River near Kazungula, Zambia.


Credit & Copyright: Engelbert Vollmer
Engelbert's website: https://app.astrobin.com/u/Fox368
Authors & Editors: Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti, 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. 5, 2026

#NASA #Astronomy #Space #Science #Galaxies #Messier104 #M104 #NGC4594 #SombreroGalaxy #VirgoConstellation #Cosmos #Universe #Astrophotographers #EngelbertVollmer #Astrophotography #NASAGoddard #MTU #UnitedStates #STEM #Education #APoD

Aurora Borealis over Four Mile Lake in Alberta, Canada

Aurora Borealis over Four Mile Lake in Alberta, Canada




Astrophotographer John David McKinnon: "The Aurora Borealis dancing over Four Mile Lake on a perfectly peaceful fall night."

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/

Alberta is a province in Canada. It is a part of Western Canada and is one of the three prairie provinces. Alberta is bordered by British Columbia to its west, Saskatchewan to its east, the Northwest Territories to its north, and the U.S. state of Montana to its south.

Canada is a country in North America. Its ten provinces and three territories extend from the Atlantic Ocean to the Pacific Ocean and northward into the Arctic Ocean, making it the second-largest country by total area with the longest coastline of any country. Its border with the United States is the longest international land border.

Image Credit: John David McKinnon 
Location: Four Mile Lake, Dënéndeh, Alberta, Canada
Date: Oct. 2, 2026

#NASA #Astronomy #Space #Science #Stars #Sun #SolarSystem #Planets #Earth #Aurorae #AuroraBorealis #NorthernLights #MagneticFields #Magnetosphere #SolarWind #Astrophotography #JohnDavidMcKinnon #Astrophotographers #CitizenScience #FourMileLake #Dënéndeh #Alberta #Canada #NorthAmerica #STEM #Education

Planet Mars Images: Sept. 30-Oct. 5, 2026 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: Sept. 30-Oct. 5, 2026 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1999
Mars 2020 - sol 1999
Mars 2020 - sol 1999
Mars 2020 - sol 1999
Mars 2020 - sol 1994
Mars 2020 - sol 1994
Mars 2020 - sol 1994
MSL - sol 5032

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Celebrating 14+ Years on Mars (2012-2026)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 5+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020
Landing: Feb. 18, 2021, Jezero Crater, Mars

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

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Release Dates: Sept. 30-Oct. 5, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #MarsExploration #SolarSystem #STEM #Education

Dying Star Creates Brand New Planet | Hubble Space Telescope

Dying Star Creates Brand New Planet | Hubble Space Telescope

What if a star’s death could give rise to an entirely new planet?

Astronomers revisiting decades-old observations from NASA’s Hubble Space Telescope found an unexpected chemical clue around a white dwarf: niobium, a heavy element forged during the final stages of a star’s life. 

Combined with observations from other NASA missions, the evidence points to an intriguing possibility: a Jupiter-sized world may have formed from material expelled when the star died.

If confirmed, this “second-generation” planet could reveal that the death of a star is not always the end of its planetary system. It may result in the beginning of a new one.


Credit: NASA's Goddard Space Flight Center 
Paul Morris: Lead Producer
Cassandra Morris: Narrator
Video Credits:
Tracks Stars. They Look Like Meteors Video by NikitaMaykov via Pond5
White Dwarf and Exoplanet Animations created by Chris Smith and Scott Wiessinger
Death Valley National Park Milky Way Galaxy Time Lapse Night Sky Above Telescope Video by Lovemushroom via Pond5
Duration: 2 minutes, 35 seconds
Release Date: Oct. 5, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #WhiteDwarfStars #Niobium #StellarEvolution #PlanetarySystems #Cosmos #Universe #HubbleSpaceTelescope #HST #NASAGoddard #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Crew-12 Farewell & Change of Command Ceremony | International Space Station

Crew-12 Farewell & Change of Command Ceremony | International Space Station

Aboard the International Space Station, Crew-12 NASA astronauts Jessica Meir and Jack Hathaway as well as European Space Agency astronaut Sophie Adenot and Roscosmos cosmonaut Andrey Fedyaev of Russia, provided farewell remarks on Oct. 4, 2026, ahead of their upcoming departure from the space station.

Joining Crew-12 for the farewell remarks were NASA astronauts Jessica Watkins, Luke Delaney, and Anil Menon as well as Canadian Space Agency astronaut Josh Kutryk and Roscosmos cosmonauts Sergey Teteryatnikov, Andrey Fedyaev, Pyotr Dubrov, and Anna Kikina of Russia. Following the farewell remarks a change of command ceremony took place where Meir handed over command of the space station to Dubrov. 

Crew-12 is slated to undock on Oct. 5 and splash down off the coast of California Oct. 6 after completing a long-duration science mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration missions. Such research benefits people on Earth and lays the groundwork for future human exploration through the agency’s Artemis missions that will send astronauts to the Moon to prepare for future expeditions to Mars.


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jack Hathaway, Anil Menon

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: NASA's Johnson Space Center
Duration: 10 minutes
Date: Oct. 4, 2026


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

Sunday, October 04, 2026

Planetary Nebula IC 4634 in Ophiuchus: Glowing Waves | Hubble

Planetary Nebula IC 4634 in Ophiuchus: Glowing Waves | Hubble

This striking Hubble image of the planetary nebula IC 4634 reveals two shining, S-shaped ejections from a dying star. This star, awash in glowing material at the center of the picture, bloated as it aged and launched its outer layers off into space. The star’s very hot, exposed core has since beamed intense ultraviolet radiation at these lost shells of gas, making them glow in rich colors.

This process has been far from orderly or calm, however, as revealed by the distinct, separate waves of thrown-off gases. One is more distant and therefore was spewed first, followed by a more recently ejected tide of matter that formed the tighter S-shape. The result is remarkably symmetric on each side of the central star.

The NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2 (WFPC2) captured this image of IC 4634. It is found more than about 7,500 light-years away in the constellation of Ophiuchus (the Serpent Holder). IC 4634 and other objects like it are known as planetary nebulae due to their appearance through early telescopes as rounded, faintly luminous discs similar to the distant planets Uranus and Neptune. 

This picture was created from images through five filters (F487N, F502N, F574M, F656N and F658N) that captured light emitted by elements in the gaseous features. The total aggregate exposure time was 4,000 seconds and the field of view is just 29 arcseconds across.


Credit: European Space Agency/Hubble and NASA
Release Date: May 10, 2010


#NASA #ESA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #IC4634 #OphiuchusConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #HubbleWFPC2 #NASAGoddard #STScI #UnitedStates #Europe #STEM #Education

Close-up: Nebula NGC 7380 in Cepheus | Kitt Peak National Observatory

Close-up: Nebula NGC 7380 in Cepheus | Kitt Peak National Observatory

NGC 7380 is a typical star-forming region in the direction of an outer spiral arm of our galaxy (around 7,000 light years distant). It is a young open cluster of stars in the northern circumpolar constellation of Cepheus, discovered by Caroline Herschel in 1787. This field contains many young energetic stars that make the natal gas surrounding them glow an intense pink/red. The majority of stars in this newly formed group are out of the field to the upper left. Their winds and radiation sculpt clouds of gas and dust into the mountainous ridges seen here. The darkest parts of this image are foreground clouds of dust thick enough to extinct the light beyond them. Also note the bright star (left of center) that is in a bluish bubble of gas. This may be a Wolf-Rayet star beginning to blow a bubble. Other famous examples of this action include The Bubble Nebula and Thor's Helmut.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.


Credit: KPNO/NOIRLab/NSF/AURA/Kris Sandburg and Peter Jacobs/Adam Block
Release Date: June 11, 2014

#NASA #Space #Astronomy #Science #Nebulae #NGC7380 #WizardNebula #CepheusConstellation #MilkyWayGalaxy #Cosmos #Universe #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education