Saturday, November 11, 2023

A Red Arc of Light & The Milky Way over France

A Red Arc of Light & The Milky Way over France

This broad, luminous red arc was a surprising visitor to partly cloudy evening skies over northern France. Captured extending toward the zenith in a west-to-east mosaic of images from November 5, 2023,the faint atmospheric ribbon of light is an example of a Stable Auroral Red (SAR) arc. The rare night sky phenomenon was also spotted at unusually low latitudes around world, along with more dynamic auroral displays during an intense geomagnetic storm. 

SAR arcs and their relation to auroral emissions have been explored by citizen science and satellite investigations. From altitudes substantially above the normal auroral glow, the deep red SAR emission is thought to be caused by strong heating due to currents flowing in planet Earth's inner magnetosphere. Beyond this SAR, the Milky Way arcs above the cloud banks along the horizon, a regular visitor to night skies over northern France.


Image Credit & Copyright: Julien Looten

Julien's website: 

https://www.flickr.com/photos/julienlooten/

Release Date: Nov. 11, 2023


#NASA #Space #Astronomy #Science #Planet #Earth #Atmosphere #AtmosphericOptics #Physics #NorthernLights #StableAuroralRed #SAR #Stars #MilkyWayGalaxy #France #Astrophotography #JulienLooten #Astrophotographer #CitizenScience #STEM #Education #APoD

NASA Sounding Rocket Launches into Alaskan Aurora

NASA Sounding Rocket Launches into Alaskan Aurora


A sounding rocket launched from Poker Flat Research Range in Fairbanks, Alaska, Nov. 8, 2023, carrying the DISSIPATION mission. The rocket launched into aurora and successfully captured data to understand how auroras heat the atmosphere and cause high-altitude winds.

The teams continue to support a second sounding rocket launch for BEAM-PIE, a mission for Los Alamos National Laboratory that will use an electron beam to create radio waves, measuring how atmospheric conditions modulate them. The data is key to interpreting measurements from many other missions. 


NASA’s Sounding Rockets Program, funded by NASA’s Heliophysics Division, is managed at the agency’s Wallops Flight Facility in Virginia, under NASA’s Goddard Space Flight Center in Greenbelt, Maryland.


Image Credit: NASA/Lee Wingfield

Image Date: Nov. 8, 2023


#NASA #Astronomy #Space #Science #Suborbital #Earth #Sun #Heliophysics #PokerFlatResearchRange #Fairbanks #Alaska #SoundingRocket #RocketLaunch #DissipationMission #Aurora #AuroraBorealis #NorthernLights #GSFC #NASAGoddard #WFF #UnitedStates #STEM #Education

Friday, November 10, 2023

Planet Jupiter Profile | Hubble Space Telescope

Planet Jupiter Profile | Hubble Space Telescope

Jupiter is the fifth planet from our Sun and is, by far, the largest planet in the solar system—more than twice as massive as all the other planets combined.

Jupiter's stripes and swirls are actually cold, windy clouds of ammonia and water, floating in an atmosphere of hydrogen and helium. Jupiter’s iconic Great Red Spot is a giant storm bigger than Earth that has raged for hundreds of years.

Jupiter is named for the king of the ancient Roman gods.​

Learn more: https://science.nasa.gov/jupiter


Credits: NASA, European Space Agency (ESA)

Duration: 15 seconds

Release Date: Aug. 2, 2021


#NASA #ESA #Space #Astronomy #Science #Hubble #Jupiter #Planet #Atmosphere #Weather #Meteorology #GreatRedSpot #SolarSystem #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Planet Jupiter in Ultraviolet | Hubble Space Telescope

Planet Jupiter in Ultraviolet | Hubble Space Telescope

This image from the NASA/European Space Agency Hubble Space Telescope shows the planet Jupiter in a color composite of ultraviolet wavelengths. The Great Red Spot appears red to the human eye, however in this ultraviolet image it appears darker because high altitude haze particles absorb light at these wavelengths. The reddish, wavy polar hazes are absorbing slightly less of this light due to differences in either particle size, composition, or altitude. The data used to create this ultraviolet image is part of a Hubble proposal that looked at Jupiter’s stealthy superstorm system. Hubble has a long history of observing the outer planets. From the Comet Shoemaker-Levy 9 impacts to studying Jupiter's storms, Hubble's decades-long career and unique vantage point provide astronomers with valuable data to chart the evolution of this dynamic planet.

Hubble’s ultraviolet-observing capabilities allow astronomers to study the short, high-energy wavelengths of light beyond what the human eye can see. Ultraviolet light reveals fascinating cosmic phenomena, including light from the hottest and youngest stars embedded in local galaxies; the composition, densities, and temperatures of the material between stars; and the evolution of galaxies.

This is a false-color image because the human eye cannot detect ultraviolet light. Therefore, colors in the visible light spectrum were assigned to the images, each taken with a different ultraviolet filter. In this case, the assigned colors for each filter are: Blue: F225W, Green: F275W, and Red: F343N.


Credits: NASA, ESA, M. Wong (University of California - Berkeley), G. Kober (NASA/Catholic University of America); CC BY 4.0

Release Date: Nov. 7, 2023


#NASA #ESA #Space #Astronomy #Science #Hubble #Jupiter #Planet #Atmosphere #Weather #Meteorology #Ultraviolet #SolarSystem #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Autumn in Japan | Earth from Space | Europe's Copernicus Sentinel-3 Satellite

Autumn in Japan | Earth from Space Europe's Copernicus Sentinel-3 Satellite

This image, from the Copernicus Sentinel-3 mission on Nov. 1, 2023, captures the colors of autumn over the Japanese archipelago.

Japan is made up of thousands of islands stretching over 2,500 km through the western Pacific Ocean. Almost all of the land area, however, is taken up by the country’s four main islands, three of which are pictured in this image. From north to south we see Honshu, the largest island extending in a northeast–southwest arc, Shikoku, just beneath the lower part of Honshu, and Kyushu at the bottom.

The image also shows how Japan is mainly mountainous and about 68% of the land area is covered by forest. Cooler temperatures and fewer daylight hours triggered the autumn foliage. This shows up here in shades of brown and red, particularly in forests in the upper part of the image. The colors depend on the various tree species, local weather, altitude and orientation of the slopes.

Urban areas and cultivated land stand out in sharp contrast in tones of grey. The largest area on the eastern coast of Honshu is Japan’s capital Tokyo. This metropolitan area—commonly known as Greater Tokyo—stretches around Tokyo Bay and is home to about 37 million people, making it the largest megacity in the world. Other urban areas, visible moving south along the Pacific coast of Honshu, are Nagoya and Osaka.

Honshu is also home to the country’s highest mountain Mount Fuji, a volcano that has been dormant since 1707. Its snow-capped summit can be spotted as a small white dot near the Pacific coast, about 100 km southwest of Tokyo.

Another volcano, visible with a plume of smoke pouring from its summit, is Sakurajima on the southern island of Kyushu. Formerly an island-volcano in the middle of Kagoshima Bay, it is now a peninsula after a powerful eruption in 1914 connected it with the Osumi Peninsula to the east.

Copernicus Sentinel-3 satellites carry four sensors working together, making it the most complex so far of all the Sentinel missions. The Ocean and Land Color Instrument used to create this image offers new eyes on Earth, monitoring ocean ecosystems, supporting crop management and agriculture, and providing estimates of atmospheric aerosol and clouds.

Learn more about Copernicus Sentinel satellites:

https://sentinels.copernicus.eu/web/sentinel/home


Image Credit: Copernicus Sentinel data (2023), processed by ESA, CC BY-SA 3.0 IGO

Image Date: Nov. 1, 2023

Release Date: Nov. 10, 2023


#NASA #ESA #Space #Science #Satellite #Sentinel3Satellite #Planet #Earth #Japan #日本 #Autumn #Autumn2023 #Europe #EarthObservation #RemoteSensing #FalseColor #STEM #Education

Celebrating the NASA Worm Logo | This Week @NASA | Week of Nov. 10, 2023

Celebrating the NASA Worm Logo | This Week @NASA | Week of Nov. 10, 2023

Celebrating the NASA worm, NASA telescopes spot a record-breaking black hole, and the first science images from a new space observatory . . . a few of the stories to tell you about—This Week at NASA!


Credit: National Aeronautics and Space Administration (NASA)

Video Producer & Editor: Andre Valentine

Narrator: Emanuel Cooper

Duration: 2 minutes, 35 seconds

Release Date: Nov. 10, 2023


#NASA #Space #Astronomy #Science #NASALogo #ESAEuclid #GalaxyUHZ1 #Abell2744 #Constellation #Sculptor #Universe #ChandraObservatory #Xray #MSFC #JWST #SpaceTelescopes #ESA #GSFC #STScI #UnitedStates #ESA #CSA #STEM #Education #HD #Video

NASA's Space to Ground: Night Launch | Week of Nov. 10, 2023

NASA's Space to Ground: Night Launch | Week of Nov. 10, 2023

 

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. SpaceX’s Dragon spacecraftcarrying about 6,500 pounds of critical science, hardware, and crew suppliesis on its way to the International Space Station following a successful launch from NASA’s Kennedy Space Center in Florida. The company’s Falcon 9 rocket lifted off from Launch Complex 39A at 8:28 p.m. EST Thursday, Nov. 9, 2023, on SpaceX’s 29th resupply services mission for NASA to the orbiting laboratory.

The mission marks the ninth flight on the Commercial Resupply Services-2 SpaceX contract and the second flight of this Dragon, which previously flew on NASA’s SpaceX 26th resupply services mission.
Dragon now is safely in orbit, and its solar arrays have deployed. A series of thruster firings will help Dragon reach the space station at approximately 5:20 a.m. on Saturday, Nov. 11. Upon its arrival, it will dock autonomously to the space-facing port of the station’s Harmony module, with NASA astronauts Jasmin Moghbeli and Loral O’Hara monitoring operations.

Follow Expedition 70 Updates:

https://blogs.nasa.gov/spacestation/

Expedition 70 Crew

Station Commander: Andreas Mogensen of the European Space Agency (Denmark)

Roscosmos (Russia): Oleg Kononenko, Nikolai Chub, Konstantin Borisov

JAXA: Flight Engineer Satoshi Furukawa (Japan)

NASA: Jasmin Moghbeli, Loral O'Hara (USA)

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. The ISS has been the most politically complex space exploration program ever undertaken.

Learn more about the important research being operated on Station:

For more information about STEM on Station:

https://www.nasa.gov/stemonstation


Credit: NASA's Johnson Space Center (JSC)

Duration: 2 minutes, 46 seconds

Release Date: Nov. 9, 2023


#NASA #Space #Astronomy #Science #ISS #Earth #CRS29 #SpaceX #DragonSpacecraft #HumanSpaceflight #Astronauts #LoralOHara #JasminMoghbelli #AndreasMogensen #SatoshiFurukawa #JAXA #Japan #ESA #Europe #UnitedStates #Cosmonauts #Russia #Роскосмос #SpaceLaboratory #Expedition70 #STEM #Education #HD #Video

NASA's SpaceX CRS-29 Falcon 9 Launch | International Space Station

NASA's SpaceX CRS-29 Falcon 9 Launch | International Space Station






Falcon 9’s first stage landing

The SpaceX Falcon 9 rocket carrying the Dragon spacecraft lifts off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida on Thursday, Nov. 9, 2023, on the company’s 29th commercial resupply services mission for the agency to the International Space Station. Liftoff was at 8:28 p.m. EST. Dragon will deliver 6,500 pounds of scientific research, technology demonstrations, crew supplies, and hardware to the space station to support its Expedition 70 crew, including NASA’s Integrated Laser Communications Relay Demonstration Low Earth Orbit User Modem and Amplifier Terminal (ILLUMA-T) and Atmospheric Waves Experiment (AWE). 

Following stage separation, Falcon 9’s first stage (B1081) landed on Landing Zone 1 (LZ-1) at Cape Canaveral Space Force Station, having previously supported the Crew-7 mission.

The spacecraft is expected to spend about a month attached to the orbiting outpost before it returns to Earth with research and return cargo, splashing down off the coast of Florida. 


Image Credits: NASA/Francisco Martin/SpaceX

Image Date: Nov. 9, 2023


#NASA #Space #ISS #Earth #Science #SpaceX #Falcon9Rocket #DragonSpacecraft #CRS29 #CommercialResupplyServices #Astronauts #Cosmonauts #HumanSpaceflight #SpaceTechnology #SpaceLaboratory #Spaceport #CapeCanaveral #Florida #UnitedStates #Russia #Japan #Expedition70 #STEM #Education


Thursday, November 09, 2023

NASA's SpaceX CRS-29 Falcon 9 Launch | International Space Station

NASA's SpaceX CRS-29 Falcon 9 Launch | International Space Station

A SpaceX Falcon 9 rocket launched NASA's CRS-29 Dragon cargo spacecraft from Launch Complex 39A (LC-39A) at NASA’s Kennedy Space Center in Florida, on Nov. 9, 2023, at 8:28pm EST. The CRS-29 Dragon cargo spacecraft is scheduled to autonomously dock to the International Space Station on Nov. 11, 2023, at approximately 05:20am EST. Following stage separation, Falcon 9’s first stage (B1081) landed on Landing Zone 1 (LZ-1) at Cape Canaveral Space Force Station, having previously supported the Crew-7 mission. CRS-29 is the second flight for this Dragon spacecraft, which previously flew CRS-26 to the International Space Station. 


Credit: NASA/SpaceX

Duration: 5 minutes

Release Date: Nov. 9, 2023


#NASA #Space #ISS #Earth #Science #SpaceX #Falcon9Rocket #DragonSpacecraft #CRS29 #CommercialResupplyServices #Astronauts #Cosmonauts #HumanSpaceflight #SpaceTechnology #SpaceLaboratory #Spaceport #CapeCanaveral #Florida #UnitedStates #Russia #Japan #Expedition70 #STEM #Education #HD #Video

NASA Science: SpaceX's 29th Cargo Resupply Mission | International Space Station

NASA Science: SpaceX's 29th Cargo Resupply Mission | International Space Station

The 29th SpaceX commercial resupply services (CRS) mission for NASA carries scientific experiments and technology demonstrations, including studies of enhanced optical communications and measurement of atmospheric waves. The uncrewed SpaceX Dragon spacecraft is scheduled to launch to the International Space Station from the agency’s Kennedy Space Center in Florida no earlier than 8:28 p.m. EST Thursday, Nov. 9, 2023, from Kennedy’s Launch Complex 39A.

Details: https://go.nasa.gov/402KJSA


Credit: National Aeronautics and Space Administration (NASA)

Duration: 1 minute

Release Date: Oct. 23, 2023 


#NASA #Space #ISS #Earth #Science #SpaceX #Falcon9Rocket #DragonSpacecraft #CRS29 #CommercialResupplyServices #Astronauts #Cosmonauts #HumanSpaceflight #SpaceTechnology #SpaceLaboratory #Spaceport #CapeCanaveral #Florida #UnitedStates #Russia #Japan #Expedition70 #STEM #Education #HD #Video

NASA SpaceX CRS-29 Falcon 9 & Dragon Pre-Launch | Kennedy Space Center

NASA SpaceX CRS-29 Falcon 9 & Dragon Pre-Launch | Kennedy Space Center







In preparation for SpaceX’s 29th commercial resupply services launch to the International Space Station for NASA, the company’s Falcon 9 rocket, with the Dragon spacecraft atop, was raised to a vertical position at Kennedy Space Center’s Launch Complex 39A in Florida on Wednesday, Nov. 8, 2023. The mission will carry scientific research, technology demonstrations, crew supplies, and hardware to the space station to support its Expedition 70 crew, including NASA’s Integrated Laser Communications Relay Demonstration Low Earth Orbit User Modem and Amplifier Terminal (ILLUMA-T) and Atmospheric Waves Experiment (AWE). 

Liftoff is scheduled for no earlier than 8:28 p.m. EST Thursday, Nov. 9, 2023, from Kennedy’s Launch Complex 39A.

Credit: Space Exploration Technologies Corp. (SpaceX)

Image Date: Nov. 8, 2023


#NASA #Space #ISS #Earth #SpaceX #Falcon9Rocket #DragonSpacecraft #CRS29 #CommercialResupplyServices #ElonMusk #GwynneShotwell #Astronauts #Cosmonauts #HumanSpaceflight #SpaceTechnology #Engineering #Spaceport #CapeCanaveral #Florida #UnitedStates #Russia #Japan #InternationalCooperation #Expedition70 #STEM #Education

NASA's "Espacio A Tierra" | Caminata espacial de noviembre: 3 de noviembre 2023

NASA's "Espacio A Tierra" | Caminata espacial de noviembre: 3 de noviembre 2023

Espacio a Tierra, la versión en español de las cápsulas Space to Ground de la NASA, te informa semanalmente de lo que está sucediendo en la Estación Espacial Internacional. 

Ciencia de la NASA: https://ciencia.nasa.gov

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: https://www.nasa.gov/suscribete


Credit: NASA's Johnson Space Center (JSC)

Duration: 3 minutes

Release Date: Nov. 9, 2023


#NASA #Space #Astronomy #Science #ISS #Earth #NASAenespañol #español #HumanSpaceflight #Astronauts #EVA #Spacewalk #LoralOHara #JasminMoghbeli #AndreasMogensen #SatoshiFurukawa #JAXA #Japan #ESA #Europe #UnitedStates #Cosmonauts #Russia #Роскосмос #SpaceLaboratory #Expedition70 #STEM #Education #HD #Video

"Mothra" Star in Galaxy Cluster MACS0416 | Webb & Hubble Space Telescopes

"Mothra" Star in Galaxy Cluster MACS0416 | Webb & Hubble Space Telescopes


This image of galaxy cluster MACS0416 highlights one particular gravitationally lensed background galaxy that existed about 3 billion years after the big bang. That galaxy contains a transient, or object that varies in observed brightness over time, that the science team nicknamed “Mothra”.

Mothra is a star that is magnified by a factor of at least 4,000 times. The team believes that Mothra is magnified not only by the gravity of galaxy cluster MACS0416, but also by an object known as a “milli-lens” that likely weighs about as much as a globular star cluster.

Image Description: A field of galaxies on the black background of space. In the middle, stretching from left to right, is a collection of dozens of yellowish spiral and elliptical galaxies that form a foreground galaxy cluster. Among them are distorted linear features created when the light of a background galaxy is bent and magnified through gravitational lensing. At center left, a particularly prominent example stretches vertically about three times the length of a nearby galaxy. It is outlined by a white box, and a lightly shaded wedge leads to an enlarged view at the bottom right. The linear feature is reddish and curves gently. It is studded with about a half dozen bright clumps. One such spot near the middle of the feature is labelled “Mothra".


Credit: NASA, ESA, CSA, STScI, J. Diego (Instituto de Física de Cantabria, Spain), J. D’Silva (U. Western Australia), A. Koekemoer (STScI), J. Summers & R. Windhorst (ASU), and H. Yan (U. Missouri).

Release Date: Nov. 9, 2023


#NASA #Space #Hubble #JWST #Astronomy #Science #Galaxies #GalaxyCluster #MACS0416 #Star #Mothra #Eridanus #Constellation #Cosmos #Universe #HST #SpaceTelescopes #ESA #GSFC #STScI #UnitedStates #ESA #CSA #STEM #Education

Pan of Galaxy Cluster MACS0416 | Webb & Hubble Space Telescopes

Pan of Galaxy Cluster MACS0416 | Webb & Hubble Space Telescopes

This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope with visible-light data from the NASA/European Space Agency Hubble Space Telescope. To make the image, in general the shortest wavelengths of light were color-coded blue, the longest wavelengths red, and intermediate wavelengths green. The resulting wavelength coverage, from 0.4 to 5 microns, reveals a vivid landscape of galaxies that could be described as one of the most colorful views of the universe ever created.

MACS0416 is a galaxy cluster located about 4.3 billion light-years from Earth, meaning that the light from it that we see now left the cluster shortly after the formation of our Solar System. This cluster magnifies the light from more distant background galaxies through gravitational lensing. As a result, the research team has been able to identify magnified supernovae and even very highly magnified individual stars.

Those colors give clues to galaxy distances: the bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant, or else contain copious amounts of dust, as best detected by Webb. The image reveals a wealth of details that it is only possible to capture by combining the power of both space telescopes.


Credit: NASA, ESA, CSA, STScI, J. Diego (Instituto de Física de Cantabria, Spain), J. D’Silva (U. Western Australia), A. Koekemoer (STScI), J. Summers & R. Windhorst (ASU), and H. Yan (U. Missouri), N. Bartmann (ESA/Webb)

Duration: 30 seconds

Release Date: Oct. 31, 2023


#NASA #Space #Hubble #JWST #Astronomy #Science #Galaxies #GalaxyCluster #MACS0416 #Eridanus #Constellation #Cosmos #Universe #HST #SpaceTelescopes #Optical #Infrared #ESA #GSFC #STScI #UnitedStates #ESA #CSA #STEM #Education #HD #Video

Galaxy Cluster MACS0416 | Webb & Hubble Space Telescopes

Galaxy Cluster MACS0416 | Webb & Hubble Space Telescopes

This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope with visible-light data from the NASA/European Space Agency Hubble Space Telescope. To make the image, in general the shortest wavelengths of light were color-coded blue, the longest wavelengths red, and intermediate wavelengths green. The resulting wavelength coverage, from 0.4 to 5 microns, reveals a vivid landscape of galaxies that could be described as one of the most colorful views of the universe ever created.

Image Description: A field of galaxies on the black background of space. In the middle is a collection of dozens of yellowish spiral and elliptical galaxies that form a foreground galaxy cluster. Among them are distorted linear features, which mostly appear to follow invisible concentric circles curving around the center of the image. The linear features are created when the light of a background galaxy is bent and magnified through gravitational lensing. A variety of brightly colored, red and blue galaxies of various shapes are scattered across the image, making it feel densely populated.

MACS0416 is a galaxy cluster located about 4.3 billion light-years from Earth, meaning that the light from it that we see now left the cluster shortly after the formation of our Solar System. This cluster magnifies the light from more distant background galaxies through gravitational lensing. As a result, the research team has been able to identify magnified supernovae and even very highly magnified individual stars.

Those colors give clues to galaxy distances: the bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant, or else contain copious amounts of dust, as best detected by Webb. The image reveals a wealth of details that it is only possible to capture by combining the power of both space telescopes.


Image Credit: NASA, ESA, CSA, STScI, J. Diego (Instituto de Física de Cantabria, Spain), J. D’Silva (U. Western Australia), A. Koekemoer (STScI), J. Summers & R. Windhorst (ASU), and H. Yan (U. Missouri)

Release Date: Nov. 9, 2023


#NASA #Space #Hubble #JWST #Astronomy #Science #Galaxies #GalaxyCluster #MACS0416 #Eridanus #Constellation #Cosmos #Universe #HST #SpaceTelescopes #ESA #GSFC #STScI #UnitedStates #ESA #CSA #STEM #Education

Wednesday, November 08, 2023

The Hamburger Galaxy: NGC 3628 in Leo | Víctor Blanco Telescope

The Hamburger Galaxy: NGC 3628 in Leo | Víctor Blanco Telescope


NGC 3628, sometimes nicknamed the Hamburger Galaxy or Sarah's Galaxy, is an unbarred spiral galaxy about 35 million light-years away in the constellation Leo. Extending to the left of NGC 3628 for around 300,000 light-years is a ‘tidal tail’—an elongated region of stars that arises as a result of gravitational interaction with another galaxy. Embedded within this tidal tail is the ultra-compact dwarf galaxy known as NGC 3628-UCD1.

NGC 3628 was discovered by William Herschel in 1784. Along with M65 and M66, NGC 3628 forms the Leo Triplet, a small group of galaxies. Notice the broad and obscuring band of dust located along the outer edge of its spiral arms, effectively transecting the galaxy to the view from Earth.

This image was captured by the US Department of Energy’s (DOE) Dark Energy Camera mounted on the National Science Foundation’s (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of NSF’s NOIRLab.


Credit: CTIO/NOIRLab/DOE/NSF/AURA

Image Processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani (NSF’s NOIRLab), & D. de Martin (NSF’s NOIRLab)

Release Date: Nov. 8, 2023


#NASA #Gemini #Astronomy #Space #Science #Galaxies #Galaxy #NGC3628 #HamburgerGalaxy #SarahsGalaxy #SpiralGalaxy #TidalTail #DwarfGalaxy #NGC3628UCD1 #Leo #Constellation #Cosmos #Universe #Observatory #VictorBlancoTelescope #Optical #CTIO #NOIRLab #AURA #NSF #DOE #UnitedStates #STEM #Education