HubbleSite - Picture Album: Star Cluster NGC 2074 in the Large Magellanic Cloud by Biljana Love
Biljana Love
Biljana Love HubbleSite - Picture Album: Star Cluster NGC 2074 in the Large Magellanic Cloud
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Star Cluster NGC 2074 in the Large Magellanic Cloud Hubble... by Damian Pelser
Damian Pelser
Damian Pelser Star Cluster NGC 2074 in the Large Magellanic Cloud Hubble...
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HubbleSite - Picture Album: Taken Under the �Wing� of the Small Magellanic Cloud by Fran Land
Fran Land
Fran Land HubbleSite - Picture Album: Taken Under the �Wing� of the Small Magellanic Cloud
landscapes
HubbleSite - Picture Album: N 180B in the Large Magellanic Cloud by Biljana Love
Biljana Love
Biljana Love HubbleSite - Picture Album: N 180B in the Large Magellanic Cloud
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Astronomy Picture of the Day: 01/18/14 - Dancing Squid      This is NGC 1760 (also known as N11 or the Dancing Squid nebula), one of the most massive, active star-forming regions located in our local corner of the universe. More specifically, this region belongs to the northern part of a neighboring dwarf-galaxy of the Milky Way; a little place you may know of as the Large Magellanic Cloud.      The intricate network of interlinking cosmic by maryellen
maryellen
maryellen Astronomy Picture of the Day: 01/18/14 - Dancing Squid This is NGC 1760 (also known as N11 or the Dancing Squid nebula), one of the most massive, active star-forming regions located in our local corner of the universe. More specifically, this region belongs to the northern part of a neighboring dwarf-galaxy of the Milky Way; a little place you may know of as the Large Magellanic Cloud. The intricate network of interlinking cosmic
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Star Cluster NGC 2074 Mousepads you will get best price offer lowest prices or diccount couponeDiscount Deals
        
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nmas
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Star Cluster NGC 2074 Mousepads
Star Cluster NGC 2074 Samsung Galaxy SIII Cover in each seller & make purchase online for cheap. Choose the best price and best promotion as you thing Secure Checkout you can trust Buy bestDiscount Deals
        
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jedjbjob
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Star Cluster NGC 2074 Samsung Galaxy SIII Cover
Starburst Cluster NGC 1929 in the Large Magellanic Cloud This cluster is creating shockwave “superbubbles” that are triggering chain reactions of supernova explosions. This image is a composite of three light wavelengths, X-rays are represented as blue, visible light as yellow, and infra-red light as red. by allie
allie
allie Starburst Cluster NGC 1929 in the Large Magellanic Cloud This cluster is creating shockwave “superbubbles” that are triggering chain reactions of supernova explosions. This image is a composite of three light wavelengths, X-rays are represented as blue, visible light as yellow, and infra-red light as red.
Whedonverse
NGC 2818  It may look like a seahorse, but the dark object is actually a pillar of smoky dust about 20 light-years long. The structure occurs in our neighbouring Large Magellanic Cloud, in a star-forming region near the Tarantula Nebula. by grace
grace
grace NGC 2818 It may look like a seahorse, but the dark object is actually a pillar of smoky dust about 20 light-years long. The structure occurs in our neighbouring Large Magellanic Cloud, in a star-forming region near the Tarantula Nebula.
Astronomy
Hubble images remarkable double cluster located in the Large Magellanic Cloud.     Credit: ESA, NASA and Martino Romaniello (European Southern Observatory, Germany) by bessie
bessie
bessie Hubble images remarkable double cluster located in the Large Magellanic Cloud. Credit: ESA, NASA and Martino Romaniello (European Southern Observatory, Germany)
SPACE
NGC 602 is a young, bright open cluster of stars located in the Small Magellanic Cloud (SMC), a satellite galaxy to the Milky Way. Radiation and shock waves from the stars have pushed away much of the lighter surrounding gas and dust that compose the nebula known as N90, and this in turn has triggered new star formation in the ridges (or "elephant trunks") of the nebula. by caroline.c
caroline.c
caroline.c NGC 602 is a young, bright open cluster of stars located in the Small Magellanic Cloud (SMC), a satellite galaxy to the Milky Way. Radiation and shock waves from the stars have pushed away much of the lighter surrounding gas and dust that compose the nebula known as N90, and this in turn has triggered new star formation in the ridges (or "elephant trunks") of the nebula.
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magellanic cloud by roseann
roseann
roseann magellanic cloud
clouds
The star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 that extends one degree on the sky in the direction of the Scorpius constellation. Part of the nebula is ionised by the youngest (bluest) heavy stars in Pismis 24. The intense ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder. by marguerite
marguerite
marguerite The star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 that extends one degree on the sky in the direction of the Scorpius constellation. Part of the nebula is ionised by the youngest (bluest) heavy stars in Pismis 24. The intense ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
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Nebula near NGC 2074, Hubble by Quella
Quella
Quella Nebula near NGC 2074, Hubble
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region of star cluster NGC 6611, from The Celestial Handbook, by Robert Burnham Jr., 1966 by imelda
imelda
imelda region of star cluster NGC 6611, from The Celestial Handbook, by Robert Burnham Jr., 1966
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A Halo for NGC 6164 Image Credit & Copyright: Don Goldman Explanation: Beautiful emission nebula NGC 6164 was created by a rare, hot, luminous O-type star, some 40 times as massive as the Sun. Seen at the center of the cosmic cloud, the star is a mere 3 to 4 million years old. In another three to four million years the massive star will end its life in a supernova explosion. Spanning around 4 light-years, the nebula itself has a bipolar symmetry. by allie
allie
allie A Halo for NGC 6164 Image Credit & Copyright: Don Goldman Explanation: Beautiful emission nebula NGC 6164 was created by a rare, hot, luminous O-type star, some 40 times as massive as the Sun. Seen at the center of the cosmic cloud, the star is a mere 3 to 4 million years old. In another three to four million years the massive star will end its life in a supernova explosion. Spanning around 4 light-years, the nebula itself has a bipolar symmetry.
Whedonverse
Star cluster Pismis 24 hang over the dusty clouds of NGC 6357 by Errcomp
Errcomp
Errcomp Star cluster Pismis 24 hang over the dusty clouds of NGC 6357
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Amazing Space Photos ~ Pacman Nebula  In visible light, the star-forming cloud known as NGC 281 in the constellation of Cassiopeia appears by da_names_ellie
da_names_ellie
da_names_ellie Amazing Space Photos ~ Pacman Nebula In visible light, the star-forming cloud known as NGC 281 in the constellation of Cassiopeia appears
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10% SALE - Necklace Copper The Seahorse of the Large Magellanic Cloud Galaxy Jewelry Universe Space Pendant Necklaces Gift by timegemstone
timegemstone
timegemstone 10% SALE - Necklace Copper The Seahorse of the Large Magellanic Cloud Galaxy Jewelry Universe Space Pendant Necklaces Gift
Necklace
This photo, released by NASA and the European Space Agency to commemorate the Hubble Space Telescope’s completion of 100,000th orbit around the Earth in its 18th year of exploration and discovery, scientists have aimed Hubble to take a snapshot of a dazzling region of celestial birth and renewal. In the image, a small portion of the nebula star cluster NGC 2074, located 170,000 light-years away, can be observed. by martha
martha
martha This photo, released by NASA and the European Space Agency to commemorate the Hubble Space Telescope’s completion of 100,000th orbit around the Earth in its 18th year of exploration and discovery, scientists have aimed Hubble to take a snapshot of a dazzling region of celestial birth and renewal. In the image, a small portion of the nebula star cluster NGC 2074, located 170,000 light-years away, can be observed.
Pink
magellanic cloud #Stars and #Space images from the #Hubble telescope. by mamie
mamie
mamie magellanic cloud #Stars and #Space images from the #Hubble telescope.
Amazing Places
Star cluster Pismis 24 hang over the dusty clouds of NGC 6357 #Stars and #Space images from the #Hubble telescope. by nusa159
nusa159
nusa159 Star cluster Pismis 24 hang over the dusty clouds of NGC 6357 #Stars and #Space images from the #Hubble telescope.
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HubbleSite - Picture Album: Galaxy Cluster MACS J0717 by Biljana Love
Biljana Love
Biljana Love HubbleSite - Picture Album: Galaxy Cluster MACS J0717
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M45: The Pleiades Star Cluster by gina
gina
gina M45: The Pleiades Star Cluster
The Space
-- NGC 7822: a young star-forming region in Cepheus --  Hot, young stars and cosmic pillars of gas and dust seem to crowd into NGC 7822. At the edge of a giant molecular cloud toward the northern constellation Cepheus, the glowing star forming region lies about 3,000 light-years away. - Image Credit: Manuel Fernández Suarez -  Image enhancement: Jean-Baptiste Faure by oldrose
oldrose
oldrose -- NGC 7822: a young star-forming region in Cepheus -- Hot, young stars and cosmic pillars of gas and dust seem to crowd into NGC 7822. At the edge of a giant molecular cloud toward the northern constellation Cepheus, the glowing star forming region lies about 3,000 light-years away. - Image Credit: Manuel Fernández Suarez - Image enhancement: Jean-Baptiste Faure
Night Time & Sunsets
Young Stars Sculpt Gas with Powerful Outflows in the Small Magellanic Cloud by Skylar Seed
Skylar Seed
Skylar Seed Young Stars Sculpt Gas with Powerful Outflows in the Small Magellanic Cloud
Hubble
Once thought to be part of the Orion nebula, the star cluster NGC 1980 is actually a separate entity, scientists say. It appears around the brightest star seen at the bottom of this image, iota Ori. The disks around the star are the result of internal light reflection in the camera optics. by mavis
mavis
mavis Once thought to be part of the Orion nebula, the star cluster NGC 1980 is actually a separate entity, scientists say. It appears around the brightest star seen at the bottom of this image, iota Ori. The disks around the star are the result of internal light reflection in the camera optics.
Ideas for the house
Cotton Candy Nebula  - The nebula known as N11, complete with sparkly star clusters embedded in fluffy pink clouds of gas. This exceptionally energetic star-forming region, also known as the Bean Nebula, extends over 1,000 light-years in the Large Magellanic Cloud.  Three generations of star formation have created shells of gas and dust which are being blown away by radiation from the newborn stars. by babegotback
babegotback
babegotback Cotton Candy Nebula - The nebula known as N11, complete with sparkly star clusters embedded in fluffy pink clouds of gas. This exceptionally energetic star-forming region, also known as the Bean Nebula, extends over 1,000 light-years in the Large Magellanic Cloud. Three generations of star formation have created shells of gas and dust which are being blown away by radiation from the newborn stars.
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It's the bubble versus the cloud. NGC 7635, the Bubble Nebula, is being pushed out by the stellar wind of massive central star BD+602522. by Nina Maltese
Nina Maltese
Nina Maltese It's the bubble versus the cloud. NGC 7635, the Bubble Nebula, is being pushed out by the stellar wind of massive central star BD+602522.
library
Stellar cluster NGC 2467 and its surrounds, located in the constellation Puppis ("The Stern"). A few million years old at most, it is a very active stellar nursery, where new stars are born continuously from large clouds of dust and gas. The image contains open clusters Haffner 18 (center) & Haffner 19 (middle right) and vast areas of ionised gas. The bright star at the center of the largest pink region is HD 64315, a massive young star helping to shape the structure of the whole nebular region. by batjas88
batjas88
batjas88 Stellar cluster NGC 2467 and its surrounds, located in the constellation Puppis ("The Stern"). A few million years old at most, it is a very active stellar nursery, where new stars are born continuously from large clouds of dust and gas. The image contains open clusters Haffner 18 (center) & Haffner 19 (middle right) and vast areas of ionised gas. The bright star at the center of the largest pink region is HD 64315, a massive young star helping to shape the structure of the whole nebular region.
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NGC 6193 & NGC 6188 (Curtis-Schmidt telescope at Cerro Tololo Inter-American Ob. Chile). NGC 6188 is an emission nebula located about 4000 ly away in the constel. Ara. The bright open cluster NGC 6193 is responsible for a region of reflection nebulosity w/in NGC6188Nebula of Stars and Colorful Gas - Long, Tall, Vertical Pins by bitz
bitz
bitz NGC 6193 & NGC 6188 (Curtis-Schmidt telescope at Cerro Tololo Inter-American Ob. Chile). NGC 6188 is an emission nebula located about 4000 ly away in the constel. Ara. The bright open cluster NGC 6193 is responsible for a region of reflection nebulosity w/in NGC6188Nebula of Stars and Colorful Gas - Long, Tall, Vertical Pins
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