NASA's Artemis I Moon Rocket Launch | Kennedy Space Center

NASA's Artemis I Moon Rocket Launch | Kennedy Space Center

NASA’s Space Launch System rocket carrying the Orion spacecraft launches on the Artemis I flight test, Wednesday, Nov. 16, 2022, from Launch Complex 39B at NASA’s Kennedy Space Center in Florida. NASA’s Artemis I mission is the first integrated flight test of the agency’s deep space exploration systems: the Orion spacecraft, Space Launch System (SLS) rocket, and ground systems. SLS and Orion launched at 1:47am ET from Launch Pad 39B at the Kennedy Space Center. 

The first in a series of increasingly complex missions, Artemis I will be an uncrewed flight test that will provide a foundation for human deep space exploration, and demonstrate NASA's commitment and capability to extend human existence to the Moon and beyond.  It will travel 280,000 miles from Earth, thousands of miles beyond the Moon over the course of about a three-week mission. Orion will stay in space longer than any ship for astronauts has done without docking to a space station and return home faster and hotter than ever before.

On the Artemis III Mission, NASA will land the first woman and the first person of color on the surface of the Moon, paving the way for a long-term lunar presence and serving as a steppingstone on the way to Mars. 

Learn more about Artemis I at:

https://www.nasa.gov/specials/artemis

https://www.nasa.gov/artemis-1

Credit: NASA/Bill Ingalls

Image Date: November 16, 2022

#NASA #ESA #Space #Moon #Artemis #ArtemisI #Orion #Spacecraft #SLS #Rocket #DeepSpace #Astronauts #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #KSC #KennedySpaceCenter #Florida #UnitedStates #Europe #STEM #Education

NASA Artemis I Moon Rocket Prelaunch: Tanking Underway | Kennedy Space Center

NASA Artemis I Moon Rocket Prelaunch: Tanking Underway | Kennedy Space Center

NASA’s Space Launch System (SLS) rocket with the Orion spacecraft aboard is seen atop the mobile launcher at Launch Pad 39B, Tuesday, Nov. 15, 2022, as the Artemis I launch teams load more than 700,000 gallons of cryogenic propellants including liquid hydrogen and liquid oxygen as the launch countdown progresses at NASA’s Kennedy Space Center in Florida. NASA’s Artemis I flight test is the first integrated test of the agency’s deep space exploration systems: the Orion spacecraft, SLS rocket, and supporting ground systems. Launch of the uncrewed flight test is targeted for no earlier than no earlier Nov. 16 at 1:04 a.m. EST. 

The first in a series of increasingly complex missions, Artemis I will be an uncrewed flight test that will provide a foundation for human deep space exploration, and demonstrate NASA's commitment and capability to extend human existence to the Moon and beyond.  It will travel 280,000 miles from Earth, thousands of miles beyond the Moon over the course of about a three-week mission. Orion will stay in space longer than any ship for astronauts has done without docking to a space station and return home faster and hotter than ever before.

On the Artemis III Mission, NASA will land the first woman and the first person of color on the surface of the Moon, paving the way for a long-term lunar presence and serving as a steppingstone on the way to Mars. 

Learn more about Artemis I at:

https://www.nasa.gov/specials/artemis

https://www.nasa.gov/artemis-1

Credit: NASA/Joel Kowsky/Keegan Barber

Image Date: Nov. 15, 2022

#NASA #ESA #Space #Moon #Artemis #ArtemisI #Orion #Spacecraft #SLS #Rocket #DeepSpace #Astronauts #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #KSC #KennedySpaceCenter #Florida #UnitedStates #Europe #STEM #Education

Creating Black Hole Jets with a NASA Supercomputer | NASA Goddard

Creating Black Hole Jets with a NASA Supercomputer | NASA Goddard

NASA Goddard astrophysicists Ryan Tanner and Kim Weaver have used the NASA Center for Climate Simulation's Discover supercomputer to simulate weak jets produced by monster black holes, which can weigh up to billions of times the Sun's mass. As matter falls toward the black hole, some of it accelerates to near light speed and diverts into a narrow pair of jets flowing in opposite directions. In the grandest examples, these jets extend hundreds of thousands of light-years and are easily detected features in radio. 

However, weaker jets, which are more difficult to detect, can greatly impact the central regions of their host galaxies. Astronomers suspected weak jets might be responsible for unusual gas motions or otherwise unexplainable optical and X-ray emission in some black-hole-powered galaxies. 

So Tanner and Weaver simulated weak jets under realistic conditions for a galaxy about the mass of our own Milky Way. To represent the gas distribution and properties related to the black hole's activity, they referenced spiral galaxies such as NGC 1386, NGC 3079, and NGC 4945. 

Tanner modified existing astrophysical hydrodynamics code to explore how the jets and the gas impact each other across 26,000 light-years of space, or about a quarter the diameter of the Milky Way, and 600,000 years of time. From the full set of 100 simulations, the team selected 19—which consumed 800,000 core hours on Discover—for publication. 

The final form of these outflows depends mainly on their interactions with large, dense gas clouds in the galaxy's central region. These clouds can disrupt, deflect, split, or even suppress the jet. This atlas of simulations provides an important touchstone for better understanding how weaker, less apparent jets modify their galaxies.

Credit: NASA's Goddard Space Flight Center (GSFC)

Scott Wiessinger (KBRwyle): Producer

Amogh Thakkar: Lead Producer

Francis Reddy (University of Maryland College Park): Science Writer

Ryan Tanner (The Catholic University of America): Visualizer

Kim Weaver (NASA/GSFC): Interviewee

Ryan Tanner (The Catholic University of America): Interviewee

Ryan Tanner (The Catholic University of America): Scientist

Kim Weaver (NASA/GSFC): Scientist

Amogh Thakkar: Lead Videographer

Amogh Thakkar: Lead Video Editor

Sophia Roberts (AIMM): Lead Videographer

Scott Wiessinger (KBRwyle): Editor

Duration: 8 minutes

Release Date: November 15, 2022

#NASA #Astronomy #Space #Science #BlackHoles #BlackHoleJets #Galaxies #MilkyWayGalaxy #Supercomputers #Simulations #Astrophysics #Cosmos #Universe #GSFC #UnitedStates #STEM #Education #HD #Video

NASA Artemis I Moon Rocket Prelaunch: Tanking Underway | Kennedy Space Center

NASA Artemis I Moon Rocket Prelaunch: Tanking Underway | Kennedy Space Center

NASA’s Space Launch System (SLS) rocket with the Orion spacecraft aboard is seen atop the mobile launcher at Launch Pad 39B, Tuesday, Nov. 15, 2022, as the Artemis I launch teams are loading over 700,000 gallons of cryogenic propellants including liquid hydrogen and liquid oxygen as the launch countdown progresses at NASA’s Kennedy Space Center in Florida. NASA’s Artemis I flight test is the first integrated test of the agency’s deep space exploration systems: the Orion spacecraft, SLS rocket, and supporting ground systems. Launch of the uncrewed flight test is targeted for no earlier than no earlier Nov. 16 at 1:04 a.m. EST.

The first in a series of increasingly complex missions, Artemis I will be an uncrewed flight test that will provide a foundation for human deep space exploration, and demonstrate NASA's commitment and capability to extend human existence to the Moon and beyond.  It will travel 280,000 miles from Earth, thousands of miles beyond the Moon over the course of about a three-week mission. Orion will stay in space longer than any ship for astronauts has done without docking to a space station and return home faster and hotter than ever before.

On the Artemis III Mission, NASA will land the first woman and the first person of color on the surface of the Moon, paving the way for a long-term lunar presence and serving as a steppingstone on the way to Mars. 

Learn more about Artemis I at:

https://www.nasa.gov/specials/artemis

https://www.nasa.gov/artemis-1

Credit: NASA/Joel Kowsky

Image Date: Nov. 15, 2022

#NASA #ESA #Space #Moon #Artemis #ArtemisI #Orion #Spacecraft #SLS #Rocket #DeepSpace #Astronauts #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #KSC #KennedySpaceCenter #Florida #UnitedStates #Europe #STEM #Education

Zoom-in on Nearest Black Hole to Earth | NOIRLab

Zoom-in on Nearest Black Hole to Earth | NOIRLab

Zoom-in on the closest-known black hole to Earth. This is the first unambiguous detection of a dormant stellar-mass black hole in the Milky Way. Its close proximity to Earth, a mere 1,600 light-years away, offers an intriguing target of study to advance our understanding of the evolution of binary systems.

Credit: International Gemini Observatory/NOIRLab/NSF/AURA/Digitized Sky Survey 2/N. Bartmann/D. De Martin

Duration: 1 minute

Release Date: November 15, 2022

#NASA #ESA #Astronomy #Space #Science #Gaia #Spacecraft #Star #GaiaBH1 #BlackHole #Ophiuchus #Constellation #MilkyWayGalaxy #Cosmos #Universe #GeminiNorthTelescope #NOIRLab #AURA #NSF #Hawaii #UnitedStates #STEM #Education #HD #Video

Astronomers Discover Closest Black Hole to Earth | NOIRLab

Astronomers Discover Closest Black Hole to Earth | NOIRLab

Cosmoview 57: Astronomers using the International Gemini Observatory, operated by the National Science Foundation’s NOIRLab, have discovered the closest-known black hole to Earth. This is the first unambiguous detection of a dormant stellar-mass black hole in the Milky Way. Its close proximity to Earth, a mere 1,600 light-years away, offers an intriguing target of study to advance our understanding of the evolution of binary systems.

Black holes are the most extreme objects in the Universe. Supermassive versions of these unimaginably dense objects likely reside at the centers of all large galaxies. Stellar-mass black holes—which weigh approximately five to 100 times the mass of the Sun—are much more common, with an estimated 100 million in the Milky Way alone. Only a handful have been confirmed to date, however, and nearly all of these are ‘active’—meaning they shine brightly in X-rays as they consume material from a nearby stellar companion, unlike dormant black holes which do not. 

Astronomers using the Gemini North telescope on Hawai‘i, one of the twin telescopes of the International Gemini Observatory, operated by NSF’s NOIRLab, have discovered the closest black hole to Earth, which the researchers have dubbed Gaia BH1. This dormant black hole is about 10 times more massive than the Sun and is located about 1,600 light-years away in the constellation Ophiuchus, making it three times closer to Earth than the previous record holder, an X-ray binary in the constellation of Monoceros. The new discovery was made possible by making exquisite observations of the motion of the black hole’s companion, a Sun-like star that orbits the black hole at about the same distance as the Earth orbits the Sun. 

“Take the Solar System, put a black hole where the Sun is, and the Sun where the Earth is, and you get this system,” explained Kareem El-Badry, an astrophysicist at the Center for Astrophysics | Harvard & Smithsonian and the Max Planck Institute for Astronomy, and the lead author of the paper describing this discovery. 

Though there are likely millions of stellar-mass black holes roaming the Milky Way Galaxy, those few that have been detected were uncovered by their energetic interactions with a companion star. As material from a nearby star spirals in toward the black hole, it becomes superheated and generates powerful X-rays and jets of material. If a black hole is not actively feeding (i.e., it is dormant) it simply blends in with its surroundings.

Credit: NOIRLab

Duration: 1 minute, 24 seconds

Release Date: November 15, 2022

#NASA #ESA #Astronomy #Space #Science #Gaia #Spacecraft #Star #GaiaBH1 #BlackHole #Ophiuchus #Constellation #MilkyWayGalaxy #Cosmos #Universe #GeminiNorthTelescope #NOIRLab #AURA #NSF #Hawaii #UnitedStates #Art #Illustration #STEM #Education #HD #Video

NASA's Artemis I Moon Rocket Prelaunch | Kennedy Space Center

NASA's Artemis I Moon Rocket Prelaunch | Kennedy Space Center

The Moon is seen rising above NASA’s Space Launch System (SLS) rocket with the Orion spacecraft aboard at Launch Pad 39B as preparations for launch continue, Monday, Nov. 14, 2022, at NASA’s Kennedy Space Center in Florida. NASA’s Artemis I flight test is the first integrated test of the agency’s deep space exploration systems: the Orion spacecraft, SLS rocket, and supporting ground systems. 

NASA’s Space Launch System rocket and Orion spacecraft will lift off from Launch Complex 39B no earlier than November 16 at 1:04 a.m. EST. on a mission beyond the Moon and back to Earth.

Live coverage of briefings and events will air on NASA Television, the NASA app, and the agency’s website at: https://www.nasa.gov/nasalive

3:30 p.m. (EST)– Coverage of the cryogenic fueling of the Space Launch System for launch on the Artemis I mission

10:30 p.m. (EST) – Coverage of the launch of the Space Launch System and the Orion spacecraft on the Artemis I mission (Launch scheduled at 1:04 a.m. EST Nov. 16)

EST = Eastern Standard Time

The first in a series of increasingly complex missions, Artemis I will be an uncrewed flight test that will provide a foundation for human deep space exploration, and demonstrate NASA's commitment and capability to extend human existence to the Moon and beyond.  It will travel 280,000 miles from Earth, thousands of miles beyond the Moon over the course of about a three-week mission. Orion will stay in space longer than any ship for astronauts has done without docking to a space station and return home faster and hotter than ever before.

On the Artemis III Mission, NASA will land the first woman and the first person of color on the surface of the Moon, paving the way for a long-term lunar presence and serving as a steppingstone on the way to Mars. 

Learn more about Artemis I at:

https://www.nasa.gov/specials/artemis

https://www.nasa.gov/artemis-1

Credit: NASA/Bill Ingalls

Release Date: Nov. 14, 2022

#NASA #ESA #Space #Moon #Artemis #ArtemisI #Orion #Spacecraft #SLS #Rocket #DeepSpace #Astronauts #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #KSC #KennedySpaceCenter #Florida #UnitedStates #Europe #STEM #Education

NASA’s Artemis I Moon Rocket Launch Set to Make History

NASA’s Artemis I Moon Rocket Launch Set to Make History

A quick recap of NASA’s history in space exploration segueing to Artemis serves as the opening video for the launch broadcast for the agency’s Artemis I Moon mission. The broadcast originates from Kennedy Space Center in Florida, where NASA’s Space Launch System rocket and Orion spacecraft will lift off from Launch Complex 39B no earlier than November 16 on a mission beyond the Moon and back to Earth.

Live coverage of briefings and events will air on NASA Television, the NASA app, and the agency’s website at: https://www.nasa.gov/nasalive

3:30 p.m. (EST)– Coverage of the cryogenic fueling of the Space Launch System for launch on the Artemis I mission

10:30 p.m. (EST) – Coverage of the launch of the Space Launch System and the Orion spacecraft on the Artemis I mission (Launch scheduled at 1:04 a.m. EST Nov. 16)

The first in a series of increasingly complex missions, Artemis I will be an uncrewed flight test that will provide a foundation for human deep space exploration, and demonstrate NASA's commitment and capability to extend human existence to the Moon and beyond.  It will travel 280,000 miles from Earth, thousands of miles beyond the Moon over the course of about a three-week mission. Orion will stay in space longer than any ship for astronauts has done without docking to a space station and return home faster and hotter than ever before.

On the Artemis III Mission, NASA will land the first woman and the first person of color on the surface of the Moon, paving the way for a long-term lunar presence and serving as a steppingstone on the way to Mars. 

Learn more about Artemis I at:

https://www.nasa.gov/specials/artemis

https://www.nasa.gov/artemis-1

Credits: National Aeronautics and Space Administration (NASA)

Produced and Edited by Oxcart and Sami Aziz

Duration: 1 minute 19 seconds

Release Date: November 14, 2022

#NASA #ESA #Space #Moon #Artemis #ArtemisI #Orion #Spacecraft #SLS #Rocket #DeepSpace #Astronauts #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #KSC #KennedySpaceCenter #Florida #UnitedStates #Europe #STEM #Education #HD #Video

Wide-field View of Overlapping Galaxies NGC 3314 (ground-based view)

Wide-field View of Overlapping Galaxies NGC 3314 (ground-based view)

This image shows a wide field of view around the overlapping galaxy pair NGC 3314. While the two galaxies look as if they are in the midst of a collision, this is in fact a trick of perspective: the two are in chance alignment from our vantage point.

Distance: 150 million light years

Credit: NASA, European Space Agency (ESA), Digitized Sky Survey 2 

Acknowledgement: Davide de Martin

Release Date: June 14, 2012

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxy #Galaxies #NGC3314 #NGC3314A #NGC3314B #Hydra #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

Zoom into Overlapping Galaxies: NGC 3314 | Hubble

Zoom into Overlapping Galaxies: NGC 3314 | Hubble

This video begins with an image of the whole night sky, before zooming in to the constellation of Hydra and the curious pair of galaxies cataloged as NGC 3314. These two galaxies are actually separated by around 20 million light years, even if from our vantage point they look like they are in the midst of a collision. The video ends with detailed Hubble observations of the two galaxies.

Distance: 150 million light years

Credit: NASA, ESA, Digitized Sky Survey 2, N. Risinger

Duration: 1 minute

Release Date: June 14, 2012

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxy #Galaxies #NGC3314 #NGC3314A #NGC3314B #Hydra #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video

Panning across Overlapping Galaxies: NGC 3314 | Hubble

Panning across Overlapping Galaxies: NGC 3314 | Hubble

This video pans across Hubble observations of NGC 3314A and NGC 3314B, a pair of galaxies in the constellation Hydra. While they might look like they are in the midst of a cosmic collision, they are in fact separated by around 20 million light-years of space. The overlap is simply a trick of perspective.

Distance: 150 million light years

Credit: NASA, European Space Agency (ESA), W. Keel (University of Alabama)

Duration: 1 minute

Release Date: June 14, 2012

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxy #Galaxies #NGC3314 #NGC3314A #NGC3314B #Hydra #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video

Pair of Overlapping Galaxies: NGC 3314 | Hubble

Pair of Overlapping Galaxies: NGC 3314 | Hubble

The NASA/European Space Agency Hubble Space Telescope has produced an incredibly detailed image of a pair of overlapping galaxies called NGC 3314. While the two galaxies look as if they are in the midst of a collision, this is in fact a trick of perspective: the two are in chance alignment from our vantage point.

Distance: 150 million light years

Credit: NASA, European Space Agency (ESA), the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and W. Keel (University of Alabama)

Release Date: June 14, 2012

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxy #Galaxies #NGC3314 #NGC3314A #NGC3314B #Hydra #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

Panning across a "Clouded Vision": Dense Core CB 130-3 | Hubble

Panning across a "Clouded Vision": Dense Core CB 130-3 | Hubble

A small, dense cloud of gas and dust called CB 130-3 blots out the center of this image from the NASA/European Space Agency Hubble Space Telescope. CB 130-3 is an object known as a dense core, a compact agglomeration of gas and dust. This particular dense core is in the constellation Serpens, and seems to billow across a field of background stars.

Image Description: This image shows an irregularly-shaped bright orange object composed of dense gas and dust, which appears darker and more compact at the center. This dense cloud, called CB 130-3, is outlined by thinner gas and dust in light shades of blue. The background shows a multitude of bright stars against a black background.

Dense cores like CB 130-3 are the birthplaces of stars, and as such are of particular interest to astronomers. During the collapse of these cores enough mass can accumulate in one place to reach the temperatures and densities required to ignite hydrogen fusion, marking the birth of a new star. While it may not be obvious from this image, a compact object teetering on the brink of becoming a fully fledged star is embedded deep within CB 130-3.

Astronomers used Hubble’s Wide Field Camera 3 to better understand the environment surrounding this fledgling star. As this image shows, the density of CB 130-3 is not constant; the outer edges of the cloud consist of only tenuous wisps, whereas at its core CB 130-3 blots out background light entirely. The gas and dust making up CB 130-3 affect not only the brightness but also the color of background stars, with stars towards the center the cloud appearing redder than their counterparts at the outskirts of this image. Astronomers used Hubble to measure this reddening effect and chart out the density of CB 130-3, providing insights into the inner structure of this stellar nursery.

Credit: ESA/Hubble, NASA & STScI, C. Britt, T. Huard  

Duration: 30 seconds

Release Date:  Nov. 11, 2022

#NASA #ESA #Hubble #Astronomy #Space #Science #CB1303 #LDN507 #Cloud #Gas #Dust #Object #StellarNursery #SerpensCauda #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video

Clouded Vision: Dense Core CB 130-3 | Hubble

Clouded Vision: Dense Core CB 130-3 | Hubble

A small, dense cloud of gas and dust called CB 130-3 blots out the center of this image from the NASA/European Space Agency Hubble Space Telescope. CB 130-3 is an object known as a dense core, a compact agglomeration of gas and dust. This particular dense core is in the constellation Serpens, and seems to billow across a field of background stars.

Image Description: The image shows an irregularly-shaped bright orange object composed of dense gas and dust, which appears darker and more compact at the center. This dense cloud, called CB 130-3, is outlined by thinner gas and dust in light shades of blue. The background shows a multitude of bright stars against a black background.

Dense cores like CB 130-3 are the birthplaces of stars, and as such are of particular interest to astronomers. During the collapse of these cores enough mass can accumulate in one place to reach the temperatures and densities required to ignite hydrogen fusion, marking the birth of a new star. While it may not be obvious from this image, a compact object teetering on the brink of becoming a fully fledged star is embedded deep within CB 130-3.

Astronomers used Hubble’s Wide Field Camera 3 to better understand the environment surrounding this fledgling star. As this image shows, the density of CB 130-3 is not constant; the outer edges of the cloud consist of only tenuous wisps, whereas at its core CB 130-3 blots out background light entirely. The gas and dust making up CB 130-3 affect not only the brightness but also the color of background stars, with stars towards the center the cloud appearing redder than their counterparts at the outskirts of this image. Astronomers used Hubble to measure this reddening effect and chart out the density of CB 130-3, providing insights into the inner structure of this stellar nursery.

Credit: European Space Agency/Hubble, NASA & STScI, C. Britt, T. Huard, A. Pagan

Release Date: November 14, 2022

#NASA #ESA #Hubble #Astronomy #Space #Science #CB1303 #LDN507 #Cloud #Gas #Dust #Object #StellarNursery #SerpensCauda #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

Zooming in on Two Galaxies in a Ghostly Embrace: Arp-Madore 2026-424 | Hubble

Zooming in on Two Galaxies in a Ghostly Embrace: Arp-Madore 2026-424 | Hubble

This video gives the viewer a closer look at the Arp-Madore 2026-424 (AM 2026-424) from the NASA/European Space Agency Hubble Space Telescope. This image shows the collision of two galaxies of equal size and was taken on June 19, 2019, in visible light by the telescope’s Advanced Camera for Surveys. 

Residing 704 million light-years from Earth, this system is cataloged as Arp-Madore 2026-424 (AM 2026-424) in the Arp-Madore “Catalog of Southern Peculiar Galaxies and Associations”.

Credit: NASA, European Space Agency (ESA), J. Dalcanton, B.F. Williams, and M. Durbin (University of Washington)

Duration: 50 seconds

Release Date: October 28, 2019

#NASA #ESA #Astronomy #Space #Science #Galaxies #ESO28519 #ArpMadore2026424 #AM2026424 #Microscopium #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video

Pan across Two Galaxies in a Ghostly Embrace: Arp-Madore 2026-424 | Hubble

Pan across Two Galaxies in a Ghostly Embrace: Arp-Madore 2026-424 | Hubble

This video pans over Arp-Madore 2026-424 (AM 2026-424) as observed by the NASA/European Space Agency Hubble Space Telescope. This image shows the collision of two galaxies of equal size and was taken on June 19, 2019, in visible light by the telescope’s Advanced Camera for Surveys. 

Residing 704 million light-years from Earth, this system is cataloged as Arp-Madore 2026-424 (AM 2026-424) in the Arp-Madore “Catalog of Southern Peculiar Galaxies and Associations.”

Credit: NASA, European Space Agency (ESA), J. Dalcanton, B.F. Williams, and M. Durbin (University of Washington)

Duration: 20 seconds

Release Date: November 20, 2019

#NASA #ESA #Astronomy #Space #Science #Galaxies #ESO28519 #ArpMadore2026424 #AM2026424 #Microscopium #Constellation #Cosmos #Universe #Telescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video