Thursday, August 07, 2025

Interstellar Comet 3I/ATLAS | Hubble Space Telescope

Interstellar Comet 3I/ATLAS | Hubble Space Telescope

A team of astronomers has taken the sharpest picture of the unexpected interstellar comet 3I/ATLAS so far, using the crisp vision of the NASA/European Space Agency Hubble Space Telescope. This visible light image was captured by the Hubble Space Telescope’s Wide Field Camera on July 21, 2025.

Hubble's observations are allowing astronomers to more accurately estimate the size of the comet’s solid icy nucleus. The upper limit on the diameter of the nucleus is 5.6 kilometers, though it could be as small as 320 meters across, researchers report.
The Hubble images put tighter constraints on the nucleus size compared to previous ground-based estimates. However, the solid heart of the comet cannot be directly seen by Hubble at the present time.

3I/ATLAS is traveling through our Solar System at roughly 210,000 kilometers per hour—the highest velocity ever recorded for a Solar System visitor. This breathtaking sprint is evidence that the comet has been drifting through interstellar space for many billions of years. The gravitational slingshot effect from innumerable stars and nebulae the comet passed added momentum, ratcheting up its speed. The longer 3I/ATLAS was out in space, the higher its speed grew.

Hubble also captured a dust plume ejected from the Sun-warmed side of the comet, and the hint of a dust tail streaming away from the nucleus. Hubble’s data yields a dust-loss rate consistent with comets that are first detected around 480 million kilometers from the Sun. This behavior is much like the signature of previously seen Sun-bound comets originating within our Solar System. Of course, the major difference is that this interstellar visitor originated in another Solar System in our Milky Way galaxy.

This comet was discovered by the Asteroid Terrestrial-impact Last Alert System (ATLAS) on July 1, 2025, at a distance of 675 million kilometers from the Sun. 3I/ATLAS should remain visible to ground-based telescopes through September 2025, before it will pass too close to the Sun to be observed. It is expected to reappear on the other side of the Sun by early December.

The scale bar is labeled in arcseconds. This is a measure of angular distance on the sky. One arcsecond is equal to an angular measurement of 1/3600 of one degree. There are 60 arcminutes in a degree and 60 arcseconds in an arcminute (the full Moon has an angular diameter of about 30 arcminutes). The actual size of an object that covers one arcsecond on the sky depends on its distance from the telescope.

The north and east compass arrows show the orientation of the image on the sky. Note that the relationship between north and east on the sky (as seen from below) is flipped relative to direction arrows on a map of the ground (as seen from above).


Credit: NASA, ESA, D. Jewitt (UCLA)
Image Processing: J. DePasquale (STScI)
Release Date: Aug. 7, 2025

#NASA #Astronomy #Hubble #Space #Science #InterstellarObjects #InterplanetaryBodies #InterstellarComets #InterstellarComet3I #Comet3I #SolarSystem #Planets #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #ESA #Europe #Infographics #STEM #Education 

Interstellar Visitor is Fastest Comet Ever Recorded | NASA Goddard

Interstellar Visitor is Fastest Comet Ever Recorded | NASA Goddard

NASA's Hubble Space Telescope just captured an incredible image of interstellar comet 3I/ATLAS racing through our solar system at 130,000 mph!

This cosmic wanderer from beyond our solar system may have been traveling for billions of years before astronomers spotted it.

Learn what this ancient visitor may reveal about our galaxy's history and why scientists are racing to study it before its close encounter with the Sun in 2025.


Credit: NASA's Goddard Space Flight Center
Paul Morris: Lead Producer
Video Credits:
Halley’s Comet Animation via Pond5
Milky Way Timelapse via Pond5
Comet Grazing the Sun (Tsuchinshan-ATLAS)
Exocomets in Solar System
ESO/L. Calçada/N. Risinger
Comets orbiting White Dwarf Star
ESA/Hubble, NASA, ESO, M. Kornmesser
Oumuamua Image
ESA/Hubble, NASA, ESO, M. Kornmesser
Duration: 4 minutes
Release Date: Aug. 7, 2025

#NASA #Astronomy #Space #Science #InterstellarObjects #InterplanetaryBodies #Comets #InterstellarComet3I #3IATLAS #SolarSystem #Planets #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #ESA #Europe #STEM #Education #HD #Video

A Martian Vista Clear as Day | NASA's Perseverance Rover

A Martian Vista Clear as Day | NASA's Perseverance Rover

This is a natural color view of a location called “Falbreen" acquired on May 26, 2025 by NASA's Perseverance Rover.
Captured at a location called “Falbreen,” this enhanced-color mosaic features deceptively blue skies and the 43rd rock abrasion (the white patch at center-left) of the NASA Perseverance rover’s mission at Mars. The 96 images stitched together to create this panoramic view were acquired on May 26, 2025.

The imaging team of NASA’s Perseverance Mars rover took advantage of clear skies on the Red Planet to capture one of the sharpest panoramas of its mission so far. Visible in the mosaic, stitched together from 96 images taken at a location the science team calls “Falbreen,” is a rock that appears to lie on top of a sand ripple, a boundary line between two geologic units, and hills as distant as 40 miles (65 kilometers) away. The enhanced-color version shows the Martian sky to be remarkably clear and deceptively blue, while in the natural-color version, it is reddish.

The rover’s Mastcam-Z instrument captured the images on May 26, 2025, the 1,516th Martian day, or sol, of Perseverance’s mission that began in February 2021 on the floor of Jezero Crater. Perseverance reached the top of the crater rim late last year.

“The relatively dust-free skies provide a clear view of the surrounding terrain,” said Jim Bell, Mastcam-Z’s principal investigator at Arizona State University in Tempe. “And in this particular mosaic, we have enhanced the color contrast, which accentuates the differences in the terrain and sky.”

Buoyant Boulder
One detail that caught the science team’s attention is a large rock that appears to sit atop a dark, crescent-shaped sand ripple to the right of the mosaic’s center, about 14 feet (4.4 meters) from the rover. Geologists call this type of rock a “float rock” because it was more than likely formed someplace else and transported to its current location. Whether this one arrived by a landslide, water, or wind is unknown, but the science team suspects it got here before the sand ripple formed.

The bright white circle just left of center and near the bottom of the image is an abrasion patch. This is the 43rd rock Perseverance has abraded since it landed on Mars. Two inches (5 centimeters) wide, the shallow patch is made with the rover’s drill and enables the science team to see what’s beneath the weathered, dusty surface of a rock before deciding to drill a core sample that would be stored in one of the mission’s titanium sample tubes.

The rover made this abrasion on May 22, 2025, and performed proximity science (a detailed analysis of Martian rocks and soil) with its arm-mounted instruments two days later. The science team wanted to learn about Falbreen because it is situated within what may be some of the oldest terrain Perseverance has ever explored—perhaps even older than Jezero Crater.

Tracks from the rover’s journey to the location can be seen toward the mosaic’s right edge. About 300 feet (90 meters) away, they veer to the left, disappearing from sight at a previous geologic stop the science team calls “Kenmore.”

A little more than halfway up the mosaic, sweeping from one edge to the other, is the transition from lighter-toned to darker-toned rocks. This is the boundary line, or contact, between two geologic units. The flat, lighter-colored rocks nearer to the rover are rich in the mineral olivine, while the darker rocks farther away are believed to be much older clay-bearing rocks.

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

Learn more about NASA's Perseverance Mars rover: https://science.nasa.gov/mission/mars-2020-perseverance/

Image Credit: NASA/JPL-Caltech/ASU/MSSS
Image Date: May 26, 2025
Release Date: Aug. 6, 2025


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

City Lights of Southeast Asia with Lightning Flashes | International Space Station

City Lights of Southeast Asia with Lightning Flashes | International Space Station

The International Space Station soars 259 miles above Cambodia in this long-duration photograph revealing star trails, lightning storms, and the city lights of Southeast Asia streaking below.

Cambodia, officially the Kingdom of Cambodia, is a country in Mainland Southeast Asia. It is bordered by Thailand to the northwest, Laos to the north, and Vietnam to the east, and has a coastline along the Gulf of Thailand in the southwest. 


Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineers (Japan): Takuya Onishi, Kimiya Yui
Roscosmos (Russia) Flight Engineers: Kirill Peskov, Alexey Zubritskiy, Oleg Platonov
NASA Flight Engineers: Anne McClain, Nichole Ayers, Jonny Kim, Zena Cardman, Mike Fincke

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science

For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)

Image Credit: NASA's Johnson Space Center 
Date: June 21, 2025 


#NASA #Space #ISS #Science #Planet #Earth #Atmosphere #Airglow #SoutheastAsia #Cambodia #Meteorology #Weather #LightningStorms #Astronauts #UnitedStates #Japan #日本 #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education

SpaceX Starship Multi-engine Static Test Fire Pre-10th Flight | Starbase Texas

SpaceX Starship Multi-engine Static Test Fire Pre-10th Flight | Starbase Texas

This was the first Starship to be static fired on the orbital launch mount that was modified by engineers and technicians at Starbase Texas.

Read SpaceX's Ninth Test Flight Report: 

SpaceX’s Starship spacecraft and Super Heavy rocket—collectively referred to as Starship—represent a fully reusable transportation system designed to carry crew and cargo to Earth orbit, the Moon, Mars and beyond. Starship is currently the "world’s most powerful launch vehicle ever developed", capable of carrying up to 150 metric tonnes fully reusable and 250 metric tonnes expendable.

Key Starship Parameters:
Height: 123m/403ft
Diameter: 9m/29.5ft
Payload to LEO: 100–150t (fully reusable)

"Starship is essential to both SpaceX’s plans to deploy its next-generation Starship system as well as for NASA, which will use a lunar lander version of Starship for landing astronauts on the Moon during the Artemis III mission through the Human Landing System (HLS) program."

Learn more about Starship:

Download the Free Starship User Guide (PDF):


Video Credit: Space Exploration Technologies Corporation (SpaceX)
Duration: 39 seconds
Date: Aug. 3, 2025

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #Starship #StarshipSpacecraft #Starship10 #StarshipTestFlight10 #SuperHeavyBooster #SuperHeavyRocket #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #StarbaseTexas #Texas #UnitedStates #STEM #Education #HD #Video

Wednesday, August 06, 2025

Close-up: The Tarantula Nebula in nearby Large Magellanic Cloud Galaxy | Hubble

Close-up: The Tarantula Nebula in nearby Large Magellanic Cloud Galaxy | Hubble

A scene from a star-forming factory shines in this NASA/European Space Agency Hubble Space Telescope picture. It captures incredible details in the dusty clouds in a star-forming region called the Tarantula Nebula. What is possibly the most amazing aspect of this detailed image is that this nebula is not even in our galaxy. Instead, it is in the Large Magellanic Cloud (LMC), a dwarf galaxy that is located about 160,000 light-years away in the constellations Dorado and Mensa. 

The Large Magellanic Cloud is the largest of the dozens of small satellite galaxies that orbit the Milky Way. The Tarantula Nebula is the largest and brightest star-forming region in the Large Magellanic Cloud, and within the entire group of nearby galaxies that the Milky Way belongs to.

The Tarantula Nebula is home to the most massive stars known—a portion are roughly 200 times as massive as our Sun. The scene pictured here is located away from the center of the nebula, where there is a super star cluster called R136, but very close to a rare type of star called a Wolf–Rayet star. Wolf–Rayet stars are massive stars that have lost their outer shell of hydrogen and are extremely hot and luminous, powering dense and furious stellar winds.

This nebula is a frequent target for Hubble, whose multiwavelength capabilities are critical for capturing sculptural details in the nebula’s dusty clouds. The data used to create this image come from an observing program called Scylla. It is named for a multi-headed sea monster from the Greek myth of Ulysses. The Scylla program was designed to complement another Hubble observing program called Ultraviolet Legacy library of Young Stars as Essential Standards (ULYSSES). It targets massive young stars in the Small and Large Magellanic Clouds, while Scylla investigates the structures of gas and dust that surround these stars.

Image Description: A nebula. The top-left is dense with layers of fluffy pink and greenish clouds. Long strands of green clouds stretch out from here; a faint layer of translucent blue dust combines with them to create a three-dimensional scene. A sparse network of dark dust clouds in the foreground adds reddish-black patches atop the nebula. Blue-white and orange stars, from our galaxy and beyond, are spread amongst the clouds.


Credit: ESA/Hubble & NASA, C. Murray, N. Bartmann (ESA/Hubble)
Duration: 30 seconds
Release Date: Aug. 4, 2025

#NASA #Astronomy #Hubble #Space #Science #Nebulae #TarantulaNebula #StellarNursery #Stars #WolfRayetStars #Dorado #Constellation #LargeMagellanicCloud #LMC #DwarfGalaxies #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #ESA #Europe #STEM #Education #HD #Video

Earthbound: Japanese Astronaut Takuya Onishi | International Space Station

Earthbound: Japanese Astronaut Takuya Onishi | International Space Station

Expedition 73 flight engineer and Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi: "The Earth . . . everything feels so nostalgic."

NASA astronauts Anne McClain and Nichole Ayers, along with JAXA astronaut Takuya Onishi and Roscosmos cosmonaut Kirill Peskov of Russia are preparing to return to Earth inside their Dragon spacecraft they launched to the station in as Crew-10 members.


Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineers (Japan): Takuya Onishi, Kimiya Yui
Roscosmos (Russia) Flight Engineers: Kirill Peskov, Alexey Zubritskiy, Oleg Platonov
NASA Flight Engineers: Anne McClain, Nichole Ayers, Jonny Kim, Zena Cardman, Mike Fincke

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science

For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)

Image Credit: T. Onishi/JAXA
Date: Aug. 5, 2025


#NASA #Space #ISS #Science #Planet #Earth #Crew10 #Astronauts #TakuyaOnishi #日本 #Japan #宇宙航空研究開発機構 #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #UnitedStates #STEM #Education

Moon Minute: Artemis II Ascent Abort Recovery Training | Kennedy Space Center

Moon Minute: Artemis II Ascent Abort Recovery Training | Kennedy Space Center

Here's the latest update for NASA's Artemis campaign. NASA rehearsed recovery procedures for an ascent abort scenario off the coast of Florida. 

The Artemis II crew will be sent on a ten-day Moon journey no earlier than April 2026.

The Artemis II test flight is the first crewed flight under NASA’s Artemis campaign and is another step toward missions on the lunar surface and helping the agency prepare for future human missions to Mars.

The Artemis II test flight will be sending NASA astronauts Victor Glover, Christina Koch, and Reid Wiseman, as well as Canadian Space Agency (CSA) astronaut Jeremy Hansen, on a ten-day journey around the Moon and back.

Check the NASA Artemis II Mission page for updates:

Follow updates on the Artemis blog: 

Video Credit: NASA's Kennedy Space Center
Duration: 1 minute
Release Date: Aug. 6, 2025 

#NASA #Space #Science #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #ArtemisIICrewModule #Astronauts #AstronautTraining #CrewedMission #DeepSpace #MoonToMars #SpaceEngineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #UnitedStates #Europe #STEM #Education #HD #Video

Planet Mars Images: Aug. 4-6, 2025 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: Aug. 4-6, 2025 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - Sol 1585
Mars 2020 - Sol 1584
Mars 2020 - Sol 1585
Mars 2020 - Sol 1584
Mars 2020 - Sol 1585
Mars 2020 - Sol 1585
MSL - Sol 4621
MSL - Sol 4620

Celebrating 13+ Years on Mars (2012-2024)
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 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

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

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Dates: Aug. 4-6, 2025

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

Gas & Dust Surround Unique Red Supergiant Star Stephenson 2 DFK 52 | ESO

Gas & Dust Surround Unique Red Supergiant Star Stephenson 2 DFK 52 | ESO


This picture is reminiscent of the 3D images that you require flimsy paper red and cyan glasses to properly view. What we are seeing in this photo is actually a red supergiant star expelling a cloud of gas and dust as it nears the end of its life. These nebulae are common around supergiant stars; however, this particular cloud presents an unexpected and considerable mystery for astronomers. 

This is the largest cloud of ejected material to have been found around a supergiant star at an enormous 1.4 light years across. Astronomers studied this star, Stephenson 2 DFK 52, with the Atacama Large Millimeter/submillimeter Array (ALMA) while studying other supergiants in its vicinity. DFK 52 is rather similar to Betelgeuse, another famous red supergiant, so they were expecting to see a similar cloud around it. However, if DFK 52 was as close to us as Betelgeuse is, the cocoon around it would be as wide in the sky as a third of a full Moon.  

These new ALMA observations allow astronomers to measure how much material surrounds the star and how fast it is moving. The parts that are moving towards us are highlighted in blue, and the sections that are moving away, in red. The data show that about 4,000 years ago the star went through an episode of extreme mass shedding, and then slowed down to its current rate, more similar to that of Betelgeuse. DFK 52 is estimated to be 10-15 times more massive than the Sun, and by now it has already lost 5-10% of its mass. 

It is still a mystery as to how the star managed to expel so much material in such a short timeframe. Could it be an odd interaction with a companion star? Why is the shape of the cloud so unusually complex? Are there more supergiants like this out there? Deciphering why DFK 52 has already shed so much material will help astronomers understand how it will meet its end—a supernova explosion sometime in the next million years.

Image Description: A fuzzy ball of gas and dust is central in this image with sections overlapping of red and blue. The background is completely black. In the center towards the top of the cloud is a lighter patch of whitish red. This is where the red supergiant is.


Credit: ALMA (ESO/NAOJ/NRAO)/M. Siebert et al.
Release Date: Aug. 4, 2025


#NASA #ESO #Space #Astronomy #Science #Stars #RedSupergiants #Nebulae #CircumstellarMaterials #Stephenson2DFK52 #Stephenson2DFK52A #Scutum #Constellation #MilkyWayGalaxy #Cosmos #Universe #ALMA #NRAO #UnitedStates #NAOJ #Japan #日本 #STEM #Education

NASA Astronaut Nichole Ayers: Hair Wash Day | International Space Station

NASA Astronaut Nichole Ayers: Hair Wash Day | International Space Station

To wash their hair in space, astronauts can use a special no-rinse shampoo, a water-filled pouch with a one-way valve, and a towel. They squirt warm water onto their scalp and work it through to the ends of their hair, applying the shampoo and then drying it with a towel. The water used in the process is recycled. This method ensures that astronauts maintain their hygiene needs while living in space. 

Astronaut Nichole Ayers NASA Biography:


Expedition 73 Crew
Station Commander: JAXA Flight Engineer Takuya Onishi
JAXA Flight Engineer: Kimiya Yui
Roscosmos (Russia) Flight Engineers: Kirill Peskov, Sergey Ryzhikov, Alexey Zubritskiy, Oleg Platonov

NASA Flight Engineers: Anne McClain, Nichole Ayers, Jonny Kim, Zena Cardman, Mike Fincke

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science

For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)

Video Credit: NASA's Johnson Space Center 
Duration: 2 minutes
Release Date: Aug. 4, 2025


#NASA #Space #ISS #Science #Planet #Earth #Crew10 #Astronauts #NicholeAyers #HairWashing #WashingHair #UnitedStates #Japan #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education #HD #Video

NASA’s SpaceX Crew-10: Exploring Science | International Space Station

NASA’s SpaceX Crew-10: Exploring Science | International Space Station

During their mission on the International Space Station, NASA astronauts Anne McClain, Nichole Ayers, Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov of Russia performed numerous investigations to advance our understanding of biology, Earth science, human research, physical sciences, and technology, providing the foundation for continuing human exploration beyond low Earth orbit to the Moon and Mars.

Learn more about NASA’s SpaceX Crew-10 science mission:
https://go.nasa.gov/4m0yU9Z

Follow Expedition 73:
https://blogs.nasa.gov/spacestation/

Expedition 73 Crew
Station Commander: JAXA Flight Engineer Takuya Onishi
JAXA Flight Engineer: Kimiya Yui
Roscosmos (Russia) Flight Engineers: Kirill Peskov, Sergey Ryzhikov, Alexey Zubritskiy, Oleg Platonov

NASA Flight Engineers: Anne McClain, Nichole Ayers, Jonny Kim, Zena Cardman, Mike Fincke
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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science

For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)

Video Credit: NASA's Johnson Space Center 
Duration: 3 minutes
Release Date: Aug. 5, 2025


#NASA #Space #ISS #Science #Planet #Earth #Crew10 #Astronauts #NicholeAyers #AnneMcClain #JonnyKim #UnitedStates #TakuyaOnishi #Japan #JAXA #Cosmonauts #KirillPeskov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education #HD #Video

Highlights of Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope

Highlights of Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope

Abell 3667—an actively merging galaxy cluster—is featured in this image assembled from over 28 hours of observations with the 570-megapixel Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory, a Program of NSF NOIRLab. This collage shows examples of Abell 3667's interesting features.

1. Jellyfish Galaxy JO171
Similar to the iconic Hoag’s Object, JO171 is an example of a ring galaxy, characterized by a completely detached ring of young stars surrounding a central old spheroid. JO171’s fall into the dense Abell 3667 galaxy cluster is stripping it of gas, creating the striking jellyfish-like tendrils seen trailing off to one side of the galaxy. Analysis of the galaxy’s stellar population and its gas and stellar dynamics shows that the origin of the ring is related to an interaction with another galaxy in the distant past, prior to its accretion onto Abell 3667. More recently, since infall into the cluster, the gas in the ring has been stripped by ram pressure, causing the quenching of star formation in the stripped half of the ring. This is the first observed case of ram-pressure stripping in action in a ring galaxy. Both of the events (accretion and stripping) caused dramatic transformations in this galaxy.

2. Jellyfish Galaxy LEDA 64246
LEDA 64246 is another example of extended galaxy tails formed by ram-pressure stripping. Their blue glow indicates that the stripping has triggered star formation in the trails.

3. Brightest cluster galaxy IC 4965 and infalling group
The central galaxy in this cutout is referred to as the brightest cluster galaxy (BCG). The formation of BCGs has been an astronomical mystery for decades. The mystery has been partially answered by the detection of intracluster light. This provides evidence that BCGs generally form through the gradual stripping of stars from less massive galaxies in the cluster, which then accrete onto the BCG.

4. Seyfert Galaxy NGC 6862
NGC 6862 is a Seyfert galaxy that is partially obscured by Milky Way cirrus, or integrated flux nebulae.

Credit: CTIO/NOIRLab/NSF/AURA
Acknowledgment: PI: Anthony Englert (Brown University)
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Release Date: Aug. 5, 2025

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell3667 #JellyfishGalaxies #SeyfertGalaxies #Pavo #Constellation #DarkMatter #IntraclusterLight #Astrophysics #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #DECam #DOE #AURA #UnitedStates #STEM #Education

Tuesday, August 05, 2025

Deep View of Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope

Deep View of Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope


The final image shows Abell 3667—an actively merging galaxy cluster. It was assembled from over 28 hours of observations with the 570-megapixel Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory, a Program of NSF NOIRLab.

Within Abell 3667, two smaller galaxy clusters are actively merging together, evidenced by the glowing bridge (yellow) of stars stretching across the center of this image. This bridge connects the hearts of the two galaxy clusters, known as their brightest cluster galaxies, and forms out of material stripped from the galaxies as they merge to form one massive conglomerate. 

Galaxy clusters are among the largest structures in our Universe, consisting of hundreds or thousands of galaxies that have become gravitationally bound together over billions of years. Astrophysicists have long been eager to understand the formation of these imposing structures. The histories of galaxy clusters not only help us understand how the Universe formed, but they also provide constraints on the properties of dark matter—an invisible material that does not emit or reflect light and is found in high concentrations around clusters of galaxies.

One clue astronomers look for to understand the history of a galaxy cluster is intracluster light—the faint glow emitted by stars that have been stripped from their original galaxies by the immense gravity of a forming galaxy cluster. These stars serve as whispering evidence of past galactic interactions, though most existing telescopes and cameras struggle to capture them.

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


Credit: CTIO/NOIRLab/NSF/AURA
Acknowledgment: PI: Anthony Englert (Brown University)
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Duration: 1 minute
Release Date: Aug. 5, 2025

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell3667 #Pavo #Constellation #DarkMatter #IntraclusterLight #Astrophysics #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #DECam #DOE #AURA #UnitedStates #STEM #Education #HD #Video

Journey to Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope

Journey to Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope



The final image shows Abell 3667—an actively merging galaxy cluster. It was assembled from over 28 hours of observations with the 570-megapixel Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory, a Program of NSF NOIRLab.

Within Abell 3667, two smaller galaxy clusters are actively merging together, evidenced by the glowing bridge (yellow) of stars stretching across the center of this image. This bridge connects the hearts of the two galaxy clusters, known as their brightest cluster galaxies, and forms out of material stripped from the galaxies as they merge to form one massive conglomerate. 

Galaxy clusters are among the largest structures in our Universe, consisting of hundreds or thousands of galaxies that have become gravitationally bound together over billions of years. Astrophysicists have long been eager to understand the formation of these imposing structures. The histories of galaxy clusters not only help us understand how the Universe formed, but they also provide constraints on the properties of dark matter—an invisible material that does not emit or reflect light and is found in high concentrations around clusters of galaxies.

One clue astronomers look for to understand the history of a galaxy cluster is intracluster light—the faint glow emitted by stars that have been stripped from their original galaxies by the immense gravity of a forming galaxy cluster. These stars serve as whispering evidence of past galactic interactions, though most existing telescopes and cameras struggle to capture them.

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


Credit: CTIO/NOIRLab/NSF/AURA
Acknowledgment: PI: Anthony Englert (Brown University)
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Duration: 1 minute
Release Date: Aug. 5, 2025

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell3667 #Pavo #Constellation #DarkMatter #IntraclusterLight #Astrophysics #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #DECam #DOE #AURA #UnitedStates #STEM #Education #HD #Video

Close-up: Merging Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope

Close-up: Merging Galaxy Cluster Abell 3667 in Pavo | Victor Blanco Telescope

Abell 3667—an actively merging galaxy cluster—is featured in this image assembled from over 28 hours of observations with the 570-megapixel Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory, a Program of NSF NOIRLab.

Within Abell 3667, two smaller galaxy clusters are actively merging together, evidenced by the glowing bridge (yellow) of stars stretching across the center of this image. This bridge connects the hearts of the two galaxy clusters, known as their brightest cluster galaxies, and forms out of material stripped from the galaxies as they merge to form one massive conglomerate. 

Galaxy clusters are among the largest structures in our Universe, consisting of hundreds or thousands of galaxies that have become gravitationally bound together over billions of years. Astrophysicists have long been eager to understand the formation of these imposing structures. The histories of galaxy clusters not only help us understand how the Universe formed, but they also provide constraints on the properties of dark matter—an invisible material that does not emit or reflect light and is found in high concentrations around clusters of galaxies.

One clue astronomers look for to understand the history of a galaxy cluster is intracluster light—the faint glow emitted by stars that have been stripped from their original galaxies by the immense gravity of a forming galaxy cluster. These stars serve as whispering evidence of past galactic interactions, though most existing telescopes and cameras struggle to capture them.

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


Credit: CTIO/NOIRLab/NSF/AURA
Acknowledgment: PI: Anthony Englert (Brown University)
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Duration: 30 seconds
Release Date: Aug. 5, 2025

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell3667 #Pavo #Constellation #DarkMatter #IntraclusterLight #Astrophysics #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #DECam #DOE #AURA #UnitedStates #STEM #Education #HD #Video