Thursday, July 20, 2023

Dark Nebula LDN 673 in Aquila | Schulman Telescope

Dark Nebula LDN 673 in Aquila | Schulman Telescope

Lynds’ Dark Nebula 673 (or LDN 673) is located in the constellation Aquila, the Eagle. This dark nebula is at a distance of about 600 light years. Expansive molecular clouds in the Aquila rift make the distant stars appear reddish, while the very dense LDN 673 nebula completely blocks the starlight. You can find LDN 673 in the summer skies near bright star Altair and the Summer Triangle (Coordinates: RA 19h 20m 55s) in the northern hemisphere.

Sometimes it is what you do not see that makes a picture interesting. In this case, starlight in the thick of the Milky Way is being obliterated by dust and soot that makes up the dark lanes of our galaxy.  LDN673 is a molecular cloud of gigantic proportions—it is around 67 trillion kilometers across. Such molecular clouds are places where stars are born, and there may be enough matter in this regions to form hundreds of thousands of new stars.

The Aquila Rift forms a great mass of dark molecular clouds along the summer Milky Way through the constellations Aquila, Serpens, and eastern Ophiuchus. Many of them have been identified and catalogued in 1962 by B.T. Lynds in his "Catalogue of dark nebulae". 

Together with the Vulpecula Rift and the Cygnus Rift or Northern Coalsack, the Aquila Rift is part of the so-called Great Rift (also Dark Rift, or Dark River), which is a series of overlapping, non-luminous, molecular dust clouds that are located between the Solar System and the Sagittarius Arm of the Milky Way Galaxy.

The Great Rift appears as a dark lane that obscures the bright star fields behind it, splitting the crowded plane of our Milky Way galaxy into two as seen from Earth. These clouds are estimated to contain about 1 million solar masses of plasma and dust.


Image Data: Schulman 32-inch RCOS Telescope

Camera SBIG STX16803

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/Mount Lemmon SkyCenter/University of Arizona

Release Date: April 1, 2012


#NASA #Astronomy #Space #Nebulae #MolecularClouds #Nebula #DarkNebula #LDN673 #Aquila #Constellation #MilkyWayGalaxy #Cosmos #Universe #UA #MountLemmonObservatory #SchulmanTelescope #Arizona #UnitedStates #STEM #Education

Galactic Neighbors: Galaxies M81 & M82 in Ursa Major | NOIRLab

Galactic Neighbors: Galaxies M81 & M82 in Ursa Major | NOIRLab


This image was obtained with the wide-field view of the Mosaic camera on the KPNO 0.9m-meter telescope at Kitt Peak National Observatory. M81 (the spiral galaxy on the left) and M82 (the galaxy on the right) are two relatively nearby galaxies that are gravitationally interacting with each other. This interaction is triggering the formation of new stars in M82 at a massive rate, which can be seen from the filaments of red hydrogen gas in the galaxy. The very faint irregular dwarf galaxy Holmberg IX can barely be seen above M81. The image was generated with observations in B (blue), V (cyan), R (green), I (orange) and Hydrogen-Alpha (red). In this image, North is right, East is up.

Distance between M81 & M82: 150,000 light years

M81 & M82 Distance to Earth: 12 million light years

 

Credit: T.A. Rector (University of Alaska Anchorage) and NOIRLab/National Science Foundation (NSF)/Association of Universities for Research in Astronomy (AURA)

Release Date: June 30, 2020


#NASA #Astronomy #Space #Science #Stars #Galaxies #Galaxy #Messier82 #M82 #CigarGalaxy #StarburstGalaxy #IrregularGalaxy #Messier81 #M81 #SpiralGalaxy #UrsaMajor #Constellation #Cosmos #Universe #KPNO #Arizona #UnitedStates #Europe #STEM #Education

Starburst Galaxy Messier 82 | Kitt Peak National Observatory

Starburst Galaxy Messier 82 | Kitt Peak National Observatory

Messier 82 (M82) is one of the most irregular galaxies in our galactic neighborhood. Due to a recent interaction with the neighboring M81 galaxy, M82 has tremendous amounts of star formation taking place. The image shows reddened outflows of material that extend hundreds and thousands of light years away from core of the galaxy. Curiously, this galaxy is exceedingly bright in visible wavelengths of light, but even brighter in emissions at radio wavelengths.

Distance: 13 million light years


Credit: KPNO/NOIRLab/National Science Foundation (NSF)/Association of Universities for Research in Astronomy (AURA)/Steve Peterson/ Katy Garmany

Release Date: Feb. 20, 2014


#NASA #Astronomy #Space #Science #Stars #Galaxy #Messier82 #M82 #CigarGalaxy #StarburstGalaxy #IrregularGalaxy #UrsaMajor #Constellation #Cosmos #Universe #KPNO #Arizona #UnitedStates #Europe #STEM #Education

NASA's "Espacio a Tierra" | Momento decisivo: 14 de julio de 2023

NASA's "Espacio a Tierra" | Momento decisivo: 14 de julio de 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.

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

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


Credit: NASA's Johnson Space Center (JSC)

Duration: 4 minutes

Release Date: July 19, 2023


#NASA #Space #ISS #Earth #Science #NASAenespañol #español #Astronauts #FrankRubio #LongDurationSpaceflight #StephenBowen #WoodyHoburg #SultanAlneyadi #UAE #MBRSC #Cosmonauts #HumanSpaceflight #Technology #Russia #Роскосмос #Microgravity #SpaceResearch #SpaceLaboratory #UnitedStates #Expedition69 #STEM #Education #HD #Video

NASA OSIRIS-REx Asteroid Mission: Preparing for Sample Return to Earth

NASA OSIRIS-REx Asteroid Mission: Preparing for Sample Return to Earth

NASA’s OSIRIS-REx, the first U.S. mission to collect a sample from an asteroid, will return to Earth on Sept. 24, 2023, with material from asteroid Bennu. When it arrives, the OSIRIS-REx spacecraft will release the sample capsule for a safe landing in the Utah desert. The primitive material from Bennu—rocks and dust collected from the asteroid’s surface in 2020—will offer generations of scientists a window into the time when the Sun and planets were forming about 4.5 billion years ago. 


Follow sample-delivery updates on the OSIRIS-REx blog: https://blogs.nasa.gov/osiris-rex/

OSIRIS-REx Mission: http://www.asteroidmission.org


Credit: NASA's Goddard Space Flight Center/Scientific Visualization Studio

James Tralie (ADNET):

Lead Producer

Lead Editor

Walt Feimer (KBRwyle):

Animator

Michael Lentz (KBRwyle):

Animator

Jonathan North (KBRwyle):

Animator

Adriana Manrique Gutierrez (KBRwyle):

Animator

Krystofer Kim (KBRwyle):

Animator

Kel Elkins (USRA):

Visualizer

Duration: 36 seconds

Release Date: July 20, 2023


#NASA #Astronomy #Space #Science #OSIRISRExMission #OSIRISRExSpacecraft #Asteroids #AstreroidBennu #ToBennuAndBack #Organics #Minerals #Mapping #SampleReturn #SpaceTechnology #GSFC #CSA #JAXA #Japan #日本 #UnitedStates #SolarSystem #SpaceExploration #STEM #Education #Animation #HD #Video

How NASA Unlocks The Moon's Mysteries | NASA Goddard

How NASA Unlocks The Moon's Mysteries | NASA Goddard

The Lunar Reconnaissance Orbiter spacecraft continues gathering a wide variety of data on our Moon using its suite of scientific instruments. The information collected has led to many scientific discoveries that have shed light on the Moon's history, composition, and potential for future exploration with the upcoming Artemis missions. This video highlights some of those recent discoveries that involve impact craters, volcanic activity, and the Moon's South Pole.


Video Credit: NASA’s Goddard Space Flight Center (GSFC)

Produced and Edited by: David Ladd (AIMM) 

Data Visualizations by: Ernie Wright (USRA) 

LRO spacecraft animations by: Adriana Manrique Gutierrez (KBRwyle)


Credit: NASA Goddard (GSFC)

Duration: 3 minutes, 46 seconds

Release Date: July 20, 2023


#NASA #Space #Astronomy #Science #Moon #Geology #Lunar #LRO #Orbiter #Spacecraft #ArtemisProgram  #SpaceTechnology #SpaceEngineering #NASAGoddard #GSFC #UnitedStates #STEM #Education #Animations #Visualizations #HD #Video

Boulders from NASA DART Spacecraft Impact with Asteroid Dimorphos | Hubble

Boulders from NASA DART Spacecraft Impact with Asteroid Dimorphos | Hubble



This NASA/European Space Agency (ESA) Hubble Space Telescope image of the asteroid Dimorphos was taken on December 19, 2022, nearly four months after the asteroid was impacted by NASA’s DART (Double Asteroid Redirection Test) mission. Hubble’s sensitivity reveals a few dozen boulders knocked off the asteroid by the force of the collision. These are among the faintest objects Hubble has ever photographed inside the Solar System. The ejected boulders range in size from 1 meter to 6.7 meters across, based on Hubble photometry. They are drifting away from the asteroid at around a kilometer per hour. The discovery yields invaluable insights into the behavior of a small asteroid when it is hit by a projectile for the purpose of altering its trajectory.

Image Description: The bright white object at lower left is the asteroid Dimorphos. It has a blue dust tail extending diagonally to the upper right. A cluster of blue dots surrounds the asteroid. These are boulders that were knocked off the asteroid when, on September 26, 2022, NASA deliberately slammed the half-ton DART impactor spacecraft into the asteroid as a test of what it would take to deflect some future asteroid from hitting Earth. Hubble photographed the slow-moving boulders in December 2022.

Dimorphos is a natural satellite or moon of the near-Earth asteroid 65803 Didymos, with which it forms a binary system. Dimorphos has a diameter of 177 meters (581 ft) across its longest extent. Before the impact with NASA's DART spacecraft, Dimorphos had a shape of an oblate spheroid with a surface covered in boulders, but virtually no craters.


Credit: NASA, European Space Agency (ESA), D. Jewitt (UCLA)

Release Date: July 20, 2023


#NASA #ESA #Hubble #Astronomy #Space #Science #SolarSystem #Asteroids #AsteroidDimorphos #Boulders #Asteroid65803Didymos #DARTSpacecraft #Earth #PlanetaryDefense #Cosmos #Universe #HST #HubbleSpaceTelescope #Europe #GSFC #STScI #UnitedStates #Infographic #Illustration #STEM #Education

Messier 82: The Cigar Galaxy in Ursa Major | Hubble

Messier 82: The Cigar Galaxy in Ursa Major | Hubble


This a mosaic image of the magnificent starburst galaxy, Messier 82 (M82). This galaxy is remarkable for its webs of shredded clouds and flame-like plumes of glowing hydrogen blasting out from its central regions where young stars are being born 10 times faster than they are inside in our Milky Way Galaxy.

Distance: 13 million light years


Credit: NASA, European Space Agency (ESA) and the Hubble Heritage Team (STScI/AURA). Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI) and P. Puxley (NSF)

Release Date: April 24, 2006


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #Galaxies #Galaxy #Messier82 #M82 #CigarGalaxy #StarburstGalaxy #IrregularGalaxy #UrsaMajor #Constellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Wednesday, July 19, 2023

Carbon-rich Dust Grains Found in First Billion Years of Universe | Webb Telescope

Carbon-rich Dust Grains Found in First Billion Years of Universe | Webb Telescope

This image highlights the location of the galaxy JADES-GS-z6 in a portion of an area of the sky known as GOODS-South, which was observed as part of the JWST Advanced Deep Extragalactic Survey, or JADES. 

The galaxy JADES-GS-z6, along with others in this region, were part of a Webb study by an international team of astronomers, who observed the chemical signature of carbon-rich dust grains at redshift ~7. This is roughly equivalent to one billion years after the birth of the Universe. Similar observational signatures have been observed in the much more recent Universe, attributed to complex, carbon-based molecules known as polycyclic aromatic hydrocarbons (PAHs). It is not thought likely, however, that PAHs would have developed within the first billion years of cosmic time. Therefore, this observation suggests the exciting possibility that Webb may have observed a different species of carbon-based molecule: possibly minuscule graphite- or diamond-like grains produced by the earliest stars or supernovae. This observation suggests exciting avenues of investigation into both the production of cosmic dust and the earliest stellar populations in our Universe, and was made possible by Webb’s unprecedented sensitivity.

Image Description: This image shows a deep galaxy field, featuring thousands of galaxies of various shapes and sizes. A cutout indicates a particular galaxy, known as JADES-GS-z6, which was a research target for this result. It appears as a blurry smudge of blue, red and green.

The team’s research indicates that this particular galaxy showed significant dust obscuration and has undergone substantial metal enrichment relative to galaxies with similar mass at the same redshift. The team also believes the galaxy's visible color gradient may indicate a peculiar geometrical alignment of stars and dust.

The galaxy is shown zoomed in on a region measuring roughly 1x1 arcseconds, which is a measure of angular distance on the sky. One arcsecond is equal to 1/3600 of one degree of arc (the full Moon has an angular diameter of about 0.5 degrees). The actual size of an object that covers one arcsecond on the sky depends on its distance from the telescope.


Credit: ESA/Webb, NASA, ESA, CSA, B. Robertson (UC Santa Cruz), B. Johnson (Center for Astrophysics, Harvard & Smithsonian), S. Tacchella (University of Cambridge, M. Rieke (Univ. of Arizona), D. Eisenstein (Center for Astrophysics, Harvard & Smithsonian), A. Pagan (STScI)

Release Date: July 19, 2023


#NASA #ESA #Astronomy #Space #Science #JWST #Galaxies #Galaxy #JADESGSz6 #GOODSSouth #CarbonRichDust #CarbonBasedMolecules #Fornax #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #CSA #Canada #Europe #Infographic #STEM #Education

Meet the Samples: Ha'ahóni and Atsá (Samples 8 & 9) | NASA/JPL

Meet the Samples: Ha'ahóni and Atsá (Samples 8 & 9) | NASA/JPL

Meet two of the Martian samples that have been collected and are awaiting return to Earth as part of the Mars Sample Return campaign. As of late June 2023, NASA’s Mars Perseverance rover has collected and sealed 20 scientifically selected samples inside pristine tubes. The next stage is to get them back for study.

Considered one of the highest priorities by the scientists in the Science and Astrobiology Decadal Survey 2023-2032, Mars Sample Return would be the first mission to return samples from another planet and provides the best opportunity to reveal the early evolution of Mars, including the potential for ancient life. NASA is teaming with the European Space Agency (ESA) on this important endeavor.


Learn more about Samples No. 8 and 9—“Ha'ahóni” and “Atsá,” two rock samples collected by Perseverance near its original landing site in Jezero Crater. These rock cores were drilled from a boulder that is among the more pristine igneous rocks the rover has sampled. Perseverance found igneous rocks, which form as lava or magma solidifies, throughout the crater floor. Samples No. 8 and 9 potentially represent a unique chapter in the history of Jezero Crater and were the last samples the rover collected on the crater floor before moving on to explore the nearby ancient river delta.

Read about all the carefully selected samples:

https://mars.nasa.gov/mars-rock-samples

Learn more about the Mars Sample Return campaign: 

https://mars.nasa.gov/msr 


A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, as well as be the first mission to collect and cache Martian rock and regolith (broken rock and dust).


Credit: NASA/Jet Propulsion Laboratory (JPL)-Caltech

Duration: 1 minute 22 seconds 

Release Date: July 19, 2023


#NASA #ESA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #Mars2020 #PerseveranceRover #JezeroCrater #Haahóni #Atsá #MarsSampleReturn #MSR #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #Europe #MoonToMars #STEM #Education #HD #Video

Orbital Sunrise above Earth's Pacific Ocean | International Space Station

Orbital Sunrise above Earth's Pacific Ocean | International Space Station


The International Space Station was soaring into an orbital sunrise 259 miles above the U.S. territory of Guam in the Pacific Ocean at the time of this photograph.

Follow Expedition 69 updates here:

Expedition 69 Crew (July 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)
Image Date: July 15, 2023

#NASA #Space #ISS #Planet #Earth #Sun #Sunrise #Orbital #Atmosphere #PacificOcean #Guam #Science #Astronauts #Cosmonauts #HumanSpaceflight #SpaceTechnology #UnitedStates #Russia #Роскосмос #UAE #SpaceResearch #SpaceLaboratory #OverviewEffect #OrbitalPerspective #Expedition69 #InternationalCooperation #STEM #Education

The Final Pre-launch Tests | High Above Down Under | NASA Goddard

The Final Pre-launch Tests | High Above Down Under | NASA Goddard

Episode 4: The Final Tests | Follow two NASA rocket teams as they launch from Australia to study our nearest stellar neighbors—Alpha Centauri A & B—on a quest to understand how stars make the planets around them suitable for life

In this episode, we will answer that question and check in on the rockets as they make their final preparation to launch into space.

Learn more about NASA’s Sounding Rockets Program:

https://www.nasa.gov/soundingrockets


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

Additional footage: Office of the Chief Minister of the Northern Territory government, Equatorial Launch Australia

Additional graphics: Vecteezy

Host: Miles Hatfield (NASA/GSFC) 

Writers/Videographers: 

Miles Hatfield (NASA/GSFC) 

Mara Johnson-Groh (NASA/GSFC) 

Producers: 

Beth Anthony (NASA/GSFC) 

Joy Ng (NASA/GSFC) 

Lacey Young (NASA/GSFC) 

Animators: 

Walt Feimer (NASA/GSFC) 

Jenny McElligott (NASA/GSFC) 

Scientific Advisor: 

Kevin France (CU Boulder/LASP/SISTINE)

Special thanks to:

Equatorial Launch Australia

Gumatj Corporation Ltd.

Office of the Chief Minister of the Northern Territory government

Release Date: July 19, 2023


#NASA #Space #Astronomy #Science #Stars #Exoplanets #Planets #AlphaCentauriA #AlphaCentauriB #UtravioletLight #Astrobiology #SoundingRockets #RocketLaunches #TeamSistine #TeamDeuce #ArnhemSpaceCentre #Australia #NorthernTerritory #Host #MilesHatfield #GSFC #NASAWallops #WFF #STEM #Education #Animation #HD #Video

What's Going on with the Hole in the Earth's Ozone Layer? We Asked a NASA Expert

What's Going on with the Hole in the Earth's Ozone Layer? We Asked a NASA Expert

What's going on with the hole in the ozone layer?

Thanks to a global effort to regulate ozone-depleting substances, the ozone hole is showing signs of recovery and is projected to return to a healthy level by mid-century. Well done, world.

However, at NASA, scientists continue to monitor its progress. NASA Goddard’s Qing Liang explains more. Background info:

https://go.nasa.gov/3DhEBvp

 

Credit: National Aeronautics and Space Administration (NASA)

Producers: Scott Bednar, Jessica Wilde

Editor: James Lucas

Duration: 1 minute, 42 seconds

Release Date: July 19, 2023


#NASA #Space #Satellites #Planet #Earth #Atmosphere #SouthPole #Antarctica #OzoneHole #OzoneLayer #Star #Sun #UltravioletLight #UltravioletRadiation #UVRadiation #HumanHealth #HealthHazard #MontrealProtocol #NASAGoddard #GSFC #UnitedStates #STEM #Education #HD #Video

Zooming in on PDS 70 System: Host to Planet PDS 70b & Possible Trojan | ESO

Zooming in on PDS 70 System: Host to Planet PDS 70b & Possible Trojan | ESO


This sequence takes the viewer towards the southern constellation of Centaurus. We zoom in on the orange dwarf star PDS 70, which is located about 400 light-years away and has at least two planets orbiting it. The final shot shows the spectacular new image, taken with the Atacama Large Millimeter/submillimeter Array (ALMA) of the PDS 70 system, where the planet PDS 70b and its Trojan cloud of debris are in the same orbit around the central star.


Credit: European Southern Observatory (ESO)/L. Calçada/ALMA (ESO/NAOJ/NRAO)/Balsalobre-Ruza et al.

Duration: 50 seconds

Release Date: July 19, 2023


#NASA #ESO #Space #Astronomy #Science #DwarfStarPDS70 #PDS70System #Planets #Exoplanets #PlanetPDS70b #PlanetPDS70c #CircumstellarDisc #Centaurus #Constellation #Cosmos #Universe #ALMA #AtacamaDesert #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

Does this Exoplanet have a “Sibling” Sharing the Same Orbit? | ESO

Does this Exoplanet have a “Sibling” Sharing the Same Orbit? | ESO

ESOcast 263 Light: Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have found  the possible ‘sibling’ of a planet orbiting a distant star. This video summarizes the discovery. The system features a star at its center, around which the planet PDS 70b (highlighted with a solid yellow circle) is orbiting. On the same orbit as PDS 70b, indicated by a solid yellow ellipse, astronomers have detected a cloud of debris (circled by a yellow dotted line) that could be the building blocks of a new planet or the remnants of one already formed. The ring-like structure that dominates the image is a circumstellar disc of material, out of which planets are forming. There is in fact another planet in this system: PDS 70c, seen at 3 o’clock right next to the inner rim of the disc.


Credit: European Southern Observatory (ESO)

Directed by: Angelos Tsaousis and Martin Wallner.

Editing: Angelos Tsaousis.

Web and technical support: Gurvan Bazin and Raquel Yumi Shida.

Written by: Claudia Sciarma and Tom Howarth.

Footage and photos: ESO / L. Calçada, M. Kornmesser, Angelos Tsaousis, C. Malin ( christophmalin.com ), ALMA (ESO/NAOJ/NRAO)/UHD Team/Balsalobre-Ruza et al.

Scientific consultant: Paola Amico, Mariya Lyubenova.

Duration: 1 minute, 28 seconds

Release Date: July 19, 2023


#NASA #ESO #Space #Astronomy #Science # #DwarfStarPDS70 #PDS70System #Planets #Exoplanets #PlanetPDS70b #PlanetPDS70c #CircumstellarDisc #ALMA #AtacamaDesert #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

Messier 81: Optical, Ultraviolet & Infrared Views Combined | Hubble/GALEX/Spitzer

Messier 81: Optical, Ultraviolet & Infrared Views Combined | Hubble/GALEX/Spitzer


This image combines data from the Hubble Space Telescope, the Spitzer Space Telescope and the Galaxy Evolution Explorer (GALEX) missions. The GALEX ultraviolet data were from the far-UV portion of the spectrum (135 to 175 nanometres). The Spitzer infrared data were taken with the IRAC 4 detector (8 microns). The Hubble data were taken at the blue portion of the spectrum.

Messier 81 (M81) is a spiral-shaped system of stars, dust, and gas clouds—the galaxy's arms wind all the way down into the nucleus. M81 is located 11.6 million light-years away. The M81 galaxy's large size and relatively high brightness make it a popular target for amateur astronomers. In the midsts of this galaxy is the supernova 1993J which was recently found to have a companion star which had been hidden in the glow of the supernova for 21 years. 


Credit: NASA, European Space Agency (ESA) and A. Zezas (Harvard-Smithsonian Centre for Astrophysics); GALEX data: NASA, JPL-Caltech, GALEX Team, J. Huchra et al. (Harvard-Smithsonian Centre for Astrophysics); Spitzer data: NASA/JPL/Caltech/Harvard-Smithsonian Centre for Astrophysics.

Release Date: May 28, 2007


#NASA #ESA #Astronomy #Space #Galaxies #Galaxy #Messier81 #M81 #NGC3031 #BodesGalaxy #SpiralGalaxy #UrsaMajor #Constellation #MilkyWayGalaxy #Cosmos #Universe #HST #Spitzer #Infrared  #GALEX #Ultraviolet #SpaceTelescopes #STScI #GSFC #UnitedStates #Europe #STEM #Education