Reflection Nebula vdB31 in Auriga | Schulman Telescope

Reflection Nebula vdB31 in Auriga | Schulman Telescope

The dark dust clouds of vdB31, illuminated by and reflecting the light of the bright blue star AB Aurigae. It is an extremely young star just 4 million or so years old, still in the process of settling down after its birth. It has more than twice the mass of the Sun, and is fiercely hot and luminous, visible in binoculars despite its distance of well over 500 light years.

AB Aurigae is so hot it puts out most of its light in the blue part of the spectrum. Moreover, the tiny grains of silicates and carbon tend to let red light pass by them even while blue light tends to be scattered off them—sent in semi-random directions. These factors combine to create the incredibly lovely blue glow to the dust hanging in space around the star. Without it, the wisps and filaments in the dust would be invisible to our eyes.

The 0.81 m (32 in) Schulman Telescope is a Ritchey-Chrétien reflector built by RC Optical Systems and installed in 2010. It is operated by the Mount Lemmon SkyCenter and is Arizona's largest dedicated public observatory. The Schulman Telescope was designed from inception for remote control over the Internet by amateur and professional astrophotographers worldwide. It is currently the world's largest telescope dedicated for this purpose.

Image Credit: Adam Block

Caption Credit: Phil Plait

Image Date: Jan. 1, 2013

#NASA #Astronomy #Space #Nebulae #Nebula #ReflectionNebula #vdB31 #Star #ABAurigae #Auriga #Constellation #MilkyWayGalaxy #Cosmos #Universe #UA #MountLemmonObservatory #SchulmanTelescope #Arizona #UnitedStates #STEM #Education

Reflection Nebula VdB 38 in Orion | Schulman Telescope

Reflection Nebula VdB 38 in Orion | Schulman Telescope

VdB 38, also known as Sh-2 263, is a single-emission, fragmentary reflection nebula, visible in the Orion constellation. The star of the nebula gas light is HD 34989, a magnitude 5,78 magnitude-star blue-blue star, well visible to the naked eye on clearer nights. 

The cloud appears distinct in a shining part for reflection of the star light, and in fact, shows a markedly blue color, and a part on the background that appears ionized and has a reddish light. Part of the gas cloud that is part of vdB 38 is not illuminated and looks like a dark nebula masking the light coming from the behind-the-scenes stars; This obscured part returns the abbreviation LDN 1588 (B223). The distance between the cloud and the star would be approximately 736 light years according to parallax studies, which would place them in the most peripheral regions of the Orion Complex.

The 0.81 m (32 in) Schulman Telescope is a Ritchey-Chrétien reflector built by RC Optical Systems and installed in 2010. It is operated by the Mount Lemmon SkyCenter and is Arizona's largest dedicated public observatory. The Schulman Telescope was designed from inception for remote control over the Internet by amateur and professional astrophotographers worldwide. It is currently the world's largest telescope dedicated for this purpose.

Image Credit & Copyright: Adam Block/Mount Lemmon SkyCenter/University of Arizona

Caption Credit: Mark Hanson

Image Date: Jan. 1, 2013

#NASA #Astronomy #Space #Nebulae #Nebula #ReflectionNebula #VdB38 #Sh2263 #LDN1588 #Star #HD34989 #Orion #Constellation #MilkyWayGalaxy #Cosmos #Universe #UA #MountLemmonObservatory #SchulmanTelescope #Arizona #UnitedStates #STEM #Education

Expedition 69 Space Station Crew Talks with WBTS-TV Boston, AccuWeather

Expedition 69 Space Station Crew Talks with WBTS-TV Boston, AccuWeather 

Aboard the International Space Station, Expedition 69 Flight Engineers Woody Hoburg and Steve Bowen of NASA discussed life and work aboard the orbital outpost during an in-flight interview June 29, 2023, with WBTS-TV (NBC, Boston) and AccuWeather. Hoburg and Bowen are in the midst of a long-duration 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, which will send astronauts to the Moon to prepare for future expeditions to Mars.

Follow Expedition 69 updates here:

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

Expedition 69 Crew (May 2023)

Station Commander: Sergey Prokopyev of Roscosmos (Russia)

Roscosmos (Russia): Flight Engineers Dmitri Petelin & Andrey Fedyaev

Flight Engineer Sultan Alneyadi of the United Arab Emirates (UAE)

NASA: Flight Engineers Frank Rubio, Stephen Bowen, Warren Hoburg

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.

Credit: NASA's Johnson Space Center (JSC)

Duration: 21 minutes

Release Date: June 29, 2023

#NASA #Space #Earth #Science #ISS #Astronauts #StephenBowen #WoodyHoburg #Cosmonauts #HumanSpaceflight #UnitedStates #Russia #Россия #Роскосмос #UAE #MicrogravityResearch #SpaceResearch #SpaceLaboratory #UNOOSA #InternationalCooperation #Expedition69 #STEM #Education #HD #Video

Planet Venus in Ultraviolet: Japan's Venus Climate Orbiter | JAXA

Planet Venus in Ultraviolet: Japan's Venus Climate Orbiter  | JAXA

    

Why is Venus so different from Earth? To help find out, Japan launched the Akatsuki spacecraft which entered orbit around Venus late in 2015 after an unplanned five-year adventure around the inner Solar System. Even though Akatsuki was past its original planned lifetime, the spacecraft and instruments were operating so well that much of its original mission was reinstated. Also known as the Venus Climate Orbiter, Akatsuki's instruments investigated unknowns about Earth's sister planet, including whether volcanoes are still active, whether lightning occurs in the dense atmosphere, and why wind speeds greatly exceed the planet's rotation speed. 

In this image taken by Akatsuki's UVI camera, the day-side of Venus is seen shown with planet-scale V-shaped cloud pattern. The image displays three ultraviolet colors and indicates a dip in the relative abundance of sulfur dioxide shown in faint blue. Analyses of Akatsuki images and data has shown, among other discoveries, that Venus has equatorial jet similar to Earth's jet stream.

Akatsuki (あかつき, 暁, "Dawn"), also known as the Venus Climate Orbiter (VCO) and Planet-C, is a Japanese (JAXA) spacecraft tasked to study the atmosphere of Venus. By using five different cameras, working at several wavelengths, Akatsuki is studying the stratification of the atmosphere, atmospheric dynamics, and cloud physics. It was launched aboard an H-IIA 202 rocket on May 20, 2010.

Image Credit & Copyright: JAXA/ISAS/DARTS/Planet-C Project Team

Processing Credit & Copyright: Dr. Mehmet Hakan

Release Date: June 23, 2023

#NASA #JAXA #Space #Astronomy #Science #Planet #Venus #Atmosphere #EquatorialJet #SulfurDioxide  #Ultraviolet #Meteorology #Weather #Clouds #Ultraviolet #VenusClimateOrbiter #VCO #Akatsuki #あかつき #PlanetC #Spacecraft #Japan #日本  #SolarSystem #SpaceExploration #宇宙航空研究開発機構 #MehmetHakan #CitizenScience #STEM #Education #APoD

Neighboring Irregular Galaxy ESO 174-1 in Centaurus | Hubble

Neighboring Irregular Galaxy ESO 174-1 in Centaurus | Hubble

The highly irregular galaxy ESO 174-1, which resembles a lonely, hazy cloud against a backdrop of bright stars, dominates this image from the NASA/European Space Agency Hubble Space Telescope. ESO 174-1 lies around 11 million light-years from Earth and consists of a bright cloud of stars and a faint, meandering tendril of dark gas and dust.

Credit: European Space Agency (ESA)/Hubble & NASA, R. Tully  

Duration: 30 seconds

Release Date: July 3, 2023

#NASA #ESA #Hubble #Astronomy #Space #Science #Hubble #Galaxies #Galaxy #ESO1741 #IrregularGalaxy #Centaurus #Constellation #Cosmos #Universe #HST #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video

Serene Supernova Aftermath: Galaxy UGC 11860 in Pegasus | Hubble

Serene Supernova Aftermath: Galaxy UGC 11860 in Pegasus | Hubble

The spiral galaxy UGC 11860 seems to float serenely against a field of background galaxies in this image from the NASA/European Space Agency Hubble Space Telescope. UGC 11860 lies around 184 million light-years away in the constellation Pegasus, and its untroubled appearance can be deceiving. This galaxy recently played host to an almost unimaginably energetic stellar explosion.

A supernova explosion—the catastrophically violent end of a massive star’s life—was detected in UGC 11860 in 2014 by a robotic telescope dedicated to scouring the skies for transient astronomical phenomena—astronomical objects which are only visible for a short period of time. Two different teams of astronomers used Hubble’s Wide Field Camera 3 to search through the aftermath and unpick the lingering remnants of this vast cosmic explosion.

Image Description: A spiral galaxy, a fuzzy oval tilted diagonally and partially towards the viewer. The center glows in warm colors, and has two prominent spiral arms around it, with bright points of star formation. The galaxy is central in a field of small stars and galaxies on a dark background.

One team explored UGC 11860 to understand more about the progenitor star systems that eventually meet their demise in supernovae. The unimaginably energetic environment during supernova explosions is predominantly responsible for forging the elements between silicon and nickel on the periodic table. This means that understanding the influence of progenitor star systems’ masses and compositions is vital to explaining how many of the chemical elements here on Earth originated.

The other group of astronomers used Hubble to follow up supernovae that were detected by robotic telescopes. These automated eyes on the sky function without the intervention of humans, and capture transient events in the night sky. Robotic telescopes allow astronomers to detect everything from unexpected asteroids to rare, unpredictable supernovae, and can identify intriguing objects that can then be investigated in more detail by powerful telescopes such as Hubble.

Credit: European Space Agency (ESA)/Hubble & NASA, A. Filippenko, J. D. Lyman

Release Date: July 3, 2023

#NASA #ESA #Astronomy #Space #Hubble #Galaxies #Galaxy #UGC11860 #Spiral #Supernova #Pegasus #Constellation #Cosmos #Universe #HST #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Galaxy NGC 3256 in Vela | Hubble & Webb Space Telescope Views

Galaxy NGC 3256  in Vela | Hubble & Webb Space Telescope Views

The peculiar galaxy NGC 3256 takes center stage in the two images featured in this video. This distorted galaxy is the wreckage of a head-on collision between two spiral galaxies which likely occurred 500 million years ago, and it is studded with clumps of young stars which were formed as gas and dust from the two galaxies collided.

The first image contains data from the NASA/European Space Agency Hubble Space Telescope’s Advanced Camera for Surveys and Wide Field Camera 3. Here the visible light lays out in detail the dark threads of dust and molecular gas that spin around the centers of the two merged galaxies. Many of the young, infrared-emitting stars produced by the collision are obscured in visible wavelengths by this dark dust.

The second image contains data from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope, using both the Near-InfraRed Camera and the Mid-InfraRed Instrument. The collision that produced NGC 3256 spurred an enormous burst of star formation, and these new stars radiate enormously brightly in infrared wavelengths as seen here. Learn more about this image here.

Credit: ESA/Webb, NASA & CSA, L. Armus, N. Bartmann (ESA/Webb)  

Duration: 30 seconds

Release Date: July 3, 2023

#NASA #ESA #Astronomy #Space #Science #JWST #Hubble #Galaxies #Galaxy #NGC3256 #Vela #Constellation #HydraCentaurusSupercluster #Cosmos #Universe #HST #SpaceTelescopes #GSFC #STScI #UnitedStates #CSA #Canada #Europe #STEM #Education #HD #Video

Zoom into Galaxy NGC 3256 in Vela | James Webb Space Telescope

Zoom into Galaxy NGC 3256 in Vela | James Webb Space Telescope

This video takes the viewer on a journey through space to the peculiar galaxy NGC 3256. This Milky Way-sized galaxy lies about 120 million light-years away in the constellation Vela, and is a denizen of the Hydra-Centaurus Supercluster.

This distorted galaxy is the wreckage of a head-on collision between two spiral galaxies which likely occurred 500 million years ago, and it is studded with clumps of young stars which were formed as gas and dust from the two galaxies collided.

Credit: ESA/Webb, NASA & CSA, L. Armus, N. Bartmann (ESA/Webb)

Duration: 53 seconds

Release Date: July 3, 2023

#NASA #ESA #Astronomy #Space #Science #JWST #Galaxies #Galaxy #NGC3256 #Vela #Constellation #HydraCentaurusSupercluster #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #CSA #Canada #Europe #STEM #Education #HD #Video

Pan of Galaxy NGC 3256 | James Webb Space Telescope

Pan of Galaxy NGC 3256 | James Webb Space Telescope

This video features the peculiar galaxy NGC 3256 as seen by the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. This Milky Way-sized galaxy lies about 120 million light-years away in the constellation Vela, and is a denizen of the Hydra-Centaurus Supercluster.

NGC 3256 may seem peaceful, a swirl of tightly entwined spiral arms set in a hazy cloud of light, but this image shows the aftermath of an ancient cosmic clash. This distorted galaxy is the wreckage of a head-on collision between two equally massive spiral galaxies which astronomers estimate to have met around 500 million years ago. The tumultuous past of NGC 3256 is captured in the long tendrils of bright gas and stars which extend outwards from the main body of the galaxy. These luminous tendrils are called tidal tails, and are studded with young stars which were formed as gas and dust from the two galaxies collided.

Credit: ESA/Webb, NASA & CSA, L. Armus, N. Bartmann (ESA/Webb)

Duration: 30 seconds

Release Date: July 3, 2023

#NASA #ESA #Astronomy #Space #Science #JWST #Galaxies #Galaxy #NGC3256 #Vela #Constellation #HydraCentaurusSupercluster #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #CSA #Canada #Europe #STEM #Education #HD #Video

Clash of the Titans: Galaxy NGC 3256 | James Webb Space Telescope

Clash of the Titans: Galaxy NGC 3256 | James Webb Space Telescope

The peculiar galaxy NGC 3256 dominates this image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. This Milky Way-sized galaxy lies about 120 million light-years away in the constellation Vela, and is a denizen of the Hydra-Centaurus Supercluster.

NGC 3256 may seem peaceful, a swirl of tightly entwined spiral arms set in a hazy cloud of light, but this image shows the aftermath of an ancient cosmic clash. This distorted galaxy is the wreckage of a head-on collision between two equally massive spiral galaxies which astronomers estimate to have met around 500 million years ago. The tumultuous past of NGC 3256 is captured in the long tendrils of shining dust and stars which extend outwards from the main body of the galaxy. The striking red and orange regions spread across the galaxy contain young stars created in the merger that are irradiating small dust grains, which then emit infrared light that is captured in astonishing detail by Webb’s instruments. Further out, there are extended tidal features, which are mostly stars pulled out of the galaxies when they collided.

Image Description: A large, face-on spiral galaxy. The core is radiating very brightly. Streaks of dust glow intensely red, in the center and across most of the galaxy. This gas is surrounded by a dark grey halo made of the galaxy’s stars. The halo stretches out into a tidal tail at the upper-left, and another at the bottom. Small stars and galaxies surround the spiral galaxy, on a black background.

If you were asked to picture a galaxy collision, you might picture stars careening into one another with catastrophically explosive results. In reality, the spaces between the stars in a galaxy are vast; when galaxies collide, their clouds of stars pass through one another and mingle like two clouds of smoke. The gas and dust in colliding galaxies does interact, however, and with spectacular results. The galactic collision that created NGC 3256 triggered a luminous burst of star formation that can be seen in the brightest portions of this image. These infant stars shine most brightly at infrared wavelengths, light which can penetrate through obscuring dust in the galaxy, and which makes the stars perfect subjects for Webb.

This observation is one of several which take a detailed look at the physics of star formation and black hole growth in nearby merging galaxies, hoping to transform astronomers' understanding of galactic evolution. Capturing a selection of luminous infrared galaxies like NGC 3256 will help the astronomical community to understand how Webb can unravel the complex histories of nearby star-forming galaxies.

This image contains data from Webb’s Near-InfraRed Camera and Mid-InfraRed Instrument, which—as the names suggest—capture NGC 3256 in stunning detail at infrared wavelengths. 

Credit: ESA/Webb, NASA & CSA, L. Armus, A. Evans

Release Date: July 3, 2023

#NASA #ESA #Astronomy #Space #Science #JWST #Galaxies #Galaxy #NGC3256 #Vela #Constellation #HydraCentaurusSupercluster #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #CSA #Canada #Europe #STEM #Education

Planetary Nebula NGC 2346 in Monoceros | Kitt Peak National Observatory

Planetary Nebula NGC 2346 in Monoceros | Kitt Peak National Observatory

Butterfly in the sky . . . but why? It is thought that this intriguing shape was formed by two different processes. First of all there are two stars that play the "starring" role. This pair used to orbit one another at a casual distance, but then one of them evolved into a red giant star and enveloped the other one. This means the swallowed star orbited inside of the red giant! This process both caused the two to move close together and eject a ring of gas in the process. Then strong winds from the stars blew gas perpendicular to the ring to form the wings of the "butterfly." Currently these two stars are so close they orbit each other in a period of 16 days. NGC 2346 is between 2000-3000 light years away (and perhaps 1/2 light year in extent).

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. Kitt Peak National Observatory (KPNO) in Arizona is a program of the National Science Foundation’s NOIRLab.

Credit: KPNO/NOIRLab/NSF/AURA/Doug Matthews and Charles Betts/Adam Block

Release Date: June 19, 2014

#NASA #ESA #Astronomy #Space #Hubble #Nebulae #Nebula #PlanetaryNebula #Stars #RedGiantStar #WhiteDwarfStar #BinaryStarSystem #Monoceros #Constellation #MilkyWayGalaxy #Cosmos #Universe #KPNO #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Planetary Nebula NGC 2346 in Monoceros | Schulman Telescope

Planetary Nebula NGC 2346 in Monoceros | Schulman Telescope

NGC 2346 is a so-called "planetary nebula," which is ejected from Sun-like stars near the ends of their lives. NGC 2346 is remarkable because its central star is known to be actually a very close pair of stars, orbiting each other every 16 days. It is believed that the binary star was originally more widely separated. However, when one component of the binary evolved, expanded in size, and became a red-giant star, it literally swallowed its companion star. The companion star then spiralled downwards inside the red giant, and in the process spewed out gas into aring around the binary system. Later on, when the hot core of the red giant was exposed, it developed a faster stellar wind, which emerged perpendicularly to the ring and inflated two huge "bubbles". This two-stage process is believed to have resulted in the butterfly-like shape of the nebula. NGC 2346 lies about 2,000 light-years away from us, and is about one-third of a light-year in size.

The 0.81 m (32 in) Schulman Telescope is a Ritchey-Chrétien reflector built by RC Optical Systems and installed in 2010. It is operated by the Mount Lemmon SkyCenter and is Arizona's largest dedicated public observatory. The Schulman Telescope was designed from inception for remote control over the Internet by amateur and professional astrophotographers worldwide. It is currently the world's largest telescope dedicated for this purpose.

Credit: Adam Block

Release Date: Nov. 1, 2012

#NASA #ESA #Astronomy #Space #Hubble #Nebulae #Nebula #PlanetaryNebula #Stars #RedGiantStar #WhiteDwarfStar #BinaryStarSystem #Monoceros #Constellation #MilkyWayGalaxy #Cosmos #Universe #UA #MountLemmonObservatory #SchulmanTelescope #Arizona #UnitedStates #Europe #STEM #Education

Planetary Nebula NGC 2346 in Monoceros | Hubble

Planetary Nebula NGC 2346 in Monoceros | Hubble

NGC 2346 is a so-called "planetary nebula," which is ejected from Sun-like stars which are near the ends of their lives. NGC 2346 is remarkable because its central star is known to be actually a very close pair of stars, orbiting each other every 16 days. It is believed that the binary star was originally more widely separated. However, when one component of the binary evolved, expanded in size, and became a red-giant star, it literally swallowed its companion star. The companion star then spiralled downwards inside the red giant, and in the process spewed out gas into aring around the binary system. Later on, when the hot core of the red giant was exposed, it developed a faster stellar wind, which emerged perpendicularly to the ring and inflated two huge "bubbles". This two-stage process is believed to have resulted in the butterfly-like shape of the nebula. NGC 2346 lies about 2,000 light-years away from us, and is about one-third of a light-year in size.

Credit: NASA/European Space Agency and The Hubble Heritage Team (AURA/STScI)

Release Date: Oct. 7, 1999

#NASA #ESA #Astronomy #Space #Hubble #Nebulae #Nebula #PlanetaryNebula #Stars #RedGiantStar #WhiteDwarfStar #BinaryStarSystem #Monoceros #Constellation #MilkyWayGalaxy #Cosmos #Universe #HST #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

A Cosmic Butterfly’s Delicate Wings: Planetary Nebula NGC 2346 | NOIRLab

A Cosmic Butterfly’s Delicate Wings: Planetary Nebula NGC 2346 | NOIRLab

The Gemini Observatory 8-meter telescope in Chile obtained this high resolution infrared image of the bipolar planetary nebula NGC 2346 and its molecular hydrogen gas. The image is about 1 arc minute on a side: north is up, east is to the left. In contrast, the size of the full moon is 30 arc minutes. 

NGC 2346 is informally known as the Butterfly Nebula. Its most remarkable characteristics are its unusually cool central star, which is a spectroscopic binary, and its unusual shape—like an hourglass. This object is at a distance of 2,300 light-years from our Sun in the constellation Monoceros.

This pair of stars used to orbit one another at a casual distance, but then one of them evolved into a red giant star and enveloped the other one. This means the swallowed star orbited inside of the red giant! This process caused the two to move close together and to eject a ring of gas in the process. Then strong winds from the stars blew gas perpendicular to the ring to form the wings of the "butterfly." Currently these two stars are so close they orbit each other in a period of only 16 days. The two stars are closer together than our Sun and planet Mercury.

Credit: NOIRLab

Release Date: July 9, 2015

#NASA #Astronomy #Space #Science #Nebulae #Nebula #PlanetaryNebula #Stars #RedGiantStar #WhiteDwarfStar #BinaryStarSystem #Monoceros #Constellation #Cosmos #Universe #GeminiSouthObservatory #Chile #Telescope #Infrared #AdaptiveOpticsImager #NOIRLab #AURA #NSF #UnitedStates #STEM #Education

Zooming into Galactic Home of Gamma-ray Burst 151229A | NOIRLab

Zooming into Galactic Home of Gamma-ray Burst 151229A | NOIRLab

The Gemini North telescope has revealed the previously unrecognized galactic home of the gamma-ray burst identified as GRB 151229A. Astronomers calculate that this gamma-ray burst, which lies in the direction of the constellation Capricornus, occurred approximately 9 billion years ago.

The Gemini North telescope is located on Hawaii‘s Maunakea as part of the international community of observatories built to take advantage of the superb atmospheric conditions on this long-dormant volcano which rises about 4214 meters (13,825 feet) into the dry, stable air of the Pacific.

Credit: NOIRLab/NSF/AURA

Image Processing: M. Zamani (NSF’s NOIRLab) & D. de Martin (NSF’s NOIRLab)

Duration: 1 minute, 13 seconds

Release Date: June 29, 2023

#NASA #Astronomy #Space #Science #Galaxy #GammaRayBurst #GRB151229A #Capricornus #Constellation #Astrophysics #Cosmos #Universe #GeminiTelescope #NOIRLab #NSF #AURA #Hawaii #UnitedStates #STEM #Education #HD #Video

Hidden Galaxy Home to Gamma-ray Burst 9 Billion Years Ago | NOIRLab

Hidden Galaxy Home to Gamma-ray Burst 9 Billion Years Ago | NOIRLab

This image captured by the Gemini North telescope reveals the previously unrecognized galactic home of the gamma-ray burst identified as GRB 151229A. GRBs are the most powerful class of explosions in the universe. Astronomers calculate that this gamma-ray burst, which lies in the direction of the constellation Capricornus, occurred approximately 9 billion years ago.

The Gemini North telescope is located on Hawaii‘s Maunakea as part of the international community of observatories built to take advantage of the superb atmospheric conditions on this long-dormant volcano which rises about 4214 meters (13,825 feet) into the dry, stable air of the Pacific. 

Credit: International Gemini Observatory/NOIRLab/National Science Foundation (NSF)/Association of Universities for Research in Astronomy (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: July 26, 2022

#NASA #Astronomy #Space #Science #Galaxy #GammaRayBurst #GRB151229A #Capricornus #Constellation #Astrophysics #Cosmos #Universe #GeminiTelescope #NOIRLab #NSF #AURA #Hawaii #UnitedStates #STEM #Education