Mikulski Archive for Space Telescopes (MAST) archive.stsci.edu send questions to: archive@stsci.edu Search position in form ra,dec in decimal degrees Search diameter in decimal degrees MAST STPR_SIAP Search: 8 row(s) returned!name of image file RA from center of image array Dec from center of image array URL of image file OPO-designated ID General descriptive title Name of object(s) (semi-colon separated list) Full caption and related text. Sample list of datasets used to create image, with at least one dataset listed for each bandpass. Note this is not always a complete list of exposures used. URL of press release images page at HubbleSite File size in kilobytes Distance to source in light years, or a redshift Comments regarding Distance (if any) Size of image (x y); Reference coordinates for the image (RA;Dec). Reference pixel position for the image (x;y). Typically defined at the image center. Semi-colon separated list of approximate total exposure times per bandpass. Approximate exposure start times of exposures within a specific bandpass in a semi-colon separated list. Image scale in deg/pixel for each axis (as a concatenated string) CD matrix (values concatenated into a single character field) Mime type of file coordinate system reference frame Equinox celestial projection used Bandpass Designations Spectral bands using a controlled vocabulary, one for each bandpass Notes on Spectral bands approximate central wavelength or frequency of each bandpass Instrument(s) used to obtain exposures Link to related press release page Organization responsible for creating image Short description of the full press release caption. Acknowledgments for image creator(s) Date file was generated or made available Type of processing performed as defined by SIAP. All values are currently "V" indicating images are for display only, not for numerical analysis. Number of axes Average of start dates that were specified for each bandpass in MJD. Note only one start date is specified for each bandpass even when multiple files were included for a given bandpass. Average of mean wavelengths from each bandpass in meters. Highest mean bandpass in meters for specified colors. Lowest mean bandpass in meters for specified colors. Units for wavelengths.
hs-2008-02-b-full-jpg.jpg149.375249169.2787976http://archive.stsci.edu/pub/stpr/hs-2008-02-b-full-jpg.jpgSTScI-PRC-2008-02-bHubble View of Arp's LoopArp's Loop;A0952+69A Hubble Space Telescope image of an area in the neighborhood of the interacting galaxies, M81 and M82, which lie 12 million light-years away in the constellation Ursa Major. The gravity from each galaxy dramatically affected the other during their last close encounter, 200 million years ago. Gas density waves rippling around M81 make it a grand design spiral. M82 is undergoing a starburst at its core, creating glowing fingers of hydrogen. The visible light Hubble image shows bright blue star clusters found along a wispy bridge of gas that was tidally stretched between the two galaxies, and a third companion galaxy. Turbulence in the normally low-density gas may have enhanced the density locally to trigger starbirth. The so-called "blue blobs" are clumped together in a structure called Arp's Loop. Hubble reveals the clusters contain the equivalent of five Orion Nebulae. Hubble's Advanced Camera for Surveys imaged the region in blue and infrared light in September of 2006.J9RA1B010 J9RA1B020http://hubblesite.org/newscenter/archive/releases/2008/02/image/b2242370000012 million light-years (3.6 Megaparsecs)2586.0 1935.0149.3752491 69.27879761294.0 968.52250 22652006-09-22 2006-09-221.3902e-05 1.3902008e-05-1.1866504188e-05 -7.2270075932e-06 -7.1871389407e-06 1.1875865591e-05image/jpegICRSJ2000TANg IOptical OpticalGalaxy &gt Dwarf September 22,2006475 814ACS ACShttp://hubblesite.org/newscenter/archive/releases/2008/02Space Telescope Science Institute Office of Public OutreachArp's Loop, imaged by the Hubble Space Telescope. It is located 12 million light-years away in the constellation Ursa Major.NASA, ESA, and D. de Mello (Catholic University of America and GSFC;NASA, ESA, and the Hubble Heritage Team (STScI/AURA)2011-03-17 00:00:00V254000.0006.445e-78.140e-74.750e-7meters
hs-2008-02-b-full-tif.tif149.375249169.2787976http://archive.stsci.edu/pub/stpr/hs-2008-02-b-full-tif.tifSTScI-PRC-2008-02-bHubble View of Arp's LoopArp's Loop;A0952+69A Hubble Space Telescope image of an area in the neighborhood of the interacting galaxies, M81 and M82, which lie 12 million light-years away in the constellation Ursa Major. The gravity from each galaxy dramatically affected the other during their last close encounter, 200 million years ago. Gas density waves rippling around M81 make it a grand design spiral. M82 is undergoing a starburst at its core, creating glowing fingers of hydrogen. The visible light Hubble image shows bright blue star clusters found along a wispy bridge of gas that was tidally stretched between the two galaxies, and a third companion galaxy. Turbulence in the normally low-density gas may have enhanced the density locally to trigger starbirth. The so-called "blue blobs" are clumped together in a structure called Arp's Loop. Hubble reveals the clusters contain the equivalent of five Orion Nebulae. Hubble's Advanced Camera for Surveys imaged the region in blue and infrared light in September of 2006.J9RA1B010 J9RA1B020http://hubblesite.org/newscenter/archive/releases/2008/02/image/b13476370000012 million light-years (3.6 Megaparsecs)2586.0 1935.0149.3752491 69.27879761294.0 968.52250 22652006-09-22 2006-09-221.3902e-05 1.3902008e-05-1.1866504188e-05 -7.2270075932e-06 -7.1871389407e-06 1.1875865591e-05image/tiffICRSJ2000TANg IOptical OpticalGalaxy &gt Dwarf September 22,2006475 814ACS ACShttp://hubblesite.org/newscenter/archive/releases/2008/02Space Telescope Science Institute Office of Public OutreachArp's Loop, imaged by the Hubble Space Telescope. It is located 12 million light-years away in the constellation Ursa Major.NASA, ESA, and D. de Mello (Catholic University of America and GSFC;NASA, ESA, and the Hubble Heritage Team (STScI/AURA)2011-03-17 00:00:00V254000.0006.445e-78.140e-74.750e-7meters
hs-2008-02-d-full-jpg.jpg149.377418669.0497878http://archive.stsci.edu/pub/stpr/hs-2008-02-d-full-jpg.jpgSTScI-PRC-2008-02-dDwarf Galaxy Holmberg IXHolmberg IX;UGC 5336This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so-called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud. It is suspected that the dwarf galaxy was created as a result of a galactic interaction between M81 and neighboring galaxy M82. The bluish-white fuzz in the space surrounding M81 and Holmberg IX is new star formation triggered by gravitational interactions between the two galaxies.J9CM06010 J9CM06020http://hubblesite.org/newscenter/archive/releases/2008/02/image/d5233370000012 million light-years (3.6 Megaparsecs)3779.0 3993.0149.3774186 69.04978781890.5 1997.54768 47682006-03-23 2006-03-231.38997e-05 1.3899689e-051.1431104938e-05 7.9072304857e-06 7.8939877325e-06 -1.1431406649e-05image/jpegICRSJ2000TANV IOptical OpticalGalaxy &gt Dwarf March 23, 2006555 814ACS ACShttp://hubblesite.org/newscenter/archive/releases/2008/02Space Telescope Science Institute Office of Public OutreachDwarf galaxy, Holmberg IX, as imaged by the Hubble Space Telescope. It is located 12 million light-years away in the constellation Ursa Major.NASA, ESA, and D. de Mello (Catholic University of America and GSFC;NASA, ESA, and the Hubble Heritage Team (STScI/AURA)2011-03-17 00:00:00V253817.0006.845e-78.140e-75.550e-7meters
hs-2008-02-d-full-tif.tif149.377418669.0497878http://archive.stsci.edu/pub/stpr/hs-2008-02-d-full-tif.tifSTScI-PRC-2008-02-dDwarf Galaxy Holmberg IXHolmberg IX;UGC 5336This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so-called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud. It is suspected that the dwarf galaxy was created as a result of a galactic interaction between M81 and neighboring galaxy M82. The bluish-white fuzz in the space surrounding M81 and Holmberg IX is new star formation triggered by gravitational interactions between the two galaxies.J9CM06010 J9CM06020http://hubblesite.org/newscenter/archive/releases/2008/02/image/d38791370000012 million light-years (3.6 Megaparsecs)3779.0 3993.0149.3774186 69.04978781890.5 1997.54768 47682006-03-23 2006-03-231.38997e-05 1.3899689e-051.1431104938e-05 7.9072304857e-06 7.8939877325e-06 -1.1431406649e-05image/tiffICRSJ2000TANV IOptical OpticalGalaxy &gt Dwarf March 23, 2006555 814ACS ACShttp://hubblesite.org/newscenter/archive/releases/2008/02Space Telescope Science Institute Office of Public OutreachDwarf galaxy, Holmberg IX, as imaged by the Hubble Space Telescope. It is located 12 million light-years away in the constellation Ursa Major.NASA, ESA, and D. de Mello (Catholic University of America and GSFC;NASA, ESA, and the Hubble Heritage Team (STScI/AURA)2011-03-17 00:00:00V253817.0006.845e-78.140e-75.550e-7meters
hs-2008-35-d-full-jpg.jpg150.8393668.73424http://archive.stsci.edu/pub/stpr/hs-2008-35-d-full-jpg.jpgSTScI-PRC-2008-35-dANGST Survey Galaxy - NGC 3077NGC 3077NASA's Hubble Space Telescope has imaged the galaxy NGC 3077. The dark clumps of material scattered around the bright nucleus of NGC 3077 are pieces of wreckage from the galaxy's interactions with its larger neighbors. NGC 3077 is a member of the M81 group of galaxies and it resides 12.5 million light-years from Earth. This galaxy is part of a detailed survey called the ACS Nearby Galaxy Survey Treasury program (ANGST). The survey explored a region called the "Local Volume," which resides beyond the Local Group of galaxies, an even nearer collection of a few dozen galaxies within about 3 million light-years of our Milky Way Galaxy.J9RA84010:J9RA84020 J9RA84030http://hubblesite.org/newscenter/archive/releases/2008/35/image/d502400000013 million light-years1491.0 830.0150.8393600 68.7342400746.5 416.01570 1596 16222006-09-21 2006-09-21 2006-09-212.42936e-05 2.429361e-05-2.181089819e-05 -1.1084268188e-05 -1.1006262587e-05 2.1617550459e-05image/jpegICRSJ2000TANg V IOptical Optical OpticalSeptember 21, 2006475 606 814ACS ACS ACShttp://hubblesite.org/newscenter/archive/releases/2008/35Space Telescope Science Institute Office of Public OutreachNASA's Hubble Space Telescope has imaged NGC 3077 as part of the ACS Nearby Galaxy Survey Treasury (ANGST) survey. This galaxy which is located 13 million light-years away.NASA, ESA, J. Dalcanton and B. Williams (University of Washington)2011-03-17 00:00:00V253999.0006.317e-78.140e-74.750e-7meters
hs-2008-35-d-full-tif.tif150.8393668.73424http://archive.stsci.edu/pub/stpr/hs-2008-35-d-full-tif.tifSTScI-PRC-2008-35-dANGST Survey Galaxy - NGC 3077NGC 3077NASA's Hubble Space Telescope has imaged the galaxy NGC 3077. The dark clumps of material scattered around the bright nucleus of NGC 3077 are pieces of wreckage from the galaxy's interactions with its larger neighbors. NGC 3077 is a member of the M81 group of galaxies and it resides 12.5 million light-years from Earth. This galaxy is part of a detailed survey called the ACS Nearby Galaxy Survey Treasury program (ANGST). The survey explored a region called the "Local Volume," which resides beyond the Local Group of galaxies, an even nearer collection of a few dozen galaxies within about 3 million light-years of our Milky Way Galaxy.J9RA84010:J9RA84020 J9RA84030http://hubblesite.org/newscenter/archive/releases/2008/35/image/d3248400000013 million light-years1491.0 830.0150.8393600 68.7342400746.5 416.01570 1596 16222006-09-21 2006-09-21 2006-09-212.42936e-05 2.429361e-05-2.181089819e-05 -1.1084268188e-05 -1.1006262587e-05 2.1617550459e-05image/tiffICRSJ2000TANg V IOptical Optical OpticalSeptember 21, 2006475 606 814ACS ACS ACShttp://hubblesite.org/newscenter/archive/releases/2008/35Space Telescope Science Institute Office of Public OutreachNASA's Hubble Space Telescope has imaged NGC 3077 as part of the ACS Nearby Galaxy Survey Treasury (ANGST) survey. This galaxy which is located 13 million light-years away.NASA, ESA, J. Dalcanton and B. Williams (University of Washington)2011-03-17 00:00:00V253999.0006.317e-78.140e-74.750e-7meters
hs-2010-05-a-full-jpg.jpg146.834442267.9088931http://archive.stsci.edu/pub/stpr/hs-2010-05-a-full-jpg.jpgSTScI-PRC-2010-05-aStar-Birth Party Almost Over in NGC 2976NGC 2976NGC 2976 resides on the fringe of the M81 group of galaxies, located about 12 million light-years away in the constellation Ursa Major. This image, taken with NASA's Hubble Space Telescope, shows that the galaxy does not look like a typical spiral galaxy. In the galaxy's inner region, there are no obvious spiral arms. Dusty filaments running through the disk show no clear spiral structure. A raucous interaction with a neighboring group of hefty galaxies stripped away some gas and funneled the rest to the galaxy's inner region, fueling star birth about 500 million years ago. At the same time, the galaxy's outer regions stopped making stars because the gas ran out. Now, the inner disk is almost out of gas as new stars burst to life, shrinking the star-formation region to a small area of about 5,000 light-years around the core. The Hubble image can resolve hundreds of thousands of individual stars. What look like grains of sand in the image are actually single stars.J9RA57010 J9RA57020 J9RA57030http://hubblesite.org/newscenter/archive/releases/2010/05/image/a2944--3337.0 2331.0146.8344422 67.90889311669.5 1166.51570 1596 16222006-12-30 2006-12-30 2006-12-301.39134e-05 1.3913445e-058.3800560819e-06 -1.1094266444e-05 -1.1102296974e-05 -8.3964994332e-06image/jpegICRSJ2000TANg V IOptical Optical OpticalDecember 27, 2006 - January 10, 2007475 606 814ACS ACS ACShttp://hubblesite.org/newscenter/archive/releases/2010/05Space Telescope Science Institute Office of Public OutreachThe star-birth party is almost over in NGC 2976, located in the Ursa Major constellationNASA, ESA, and J. Dalcanton and B. Williams (University of Washington, Seattle)2011-03-17 00:00:00V254099.0006.317e-78.140e-74.750e-7meters
hs-2010-05-a-full-tif.tif146.834442267.9088931http://archive.stsci.edu/pub/stpr/hs-2010-05-a-full-tif.tifSTScI-PRC-2010-05-aStar-Birth Party Almost Over in NGC 2976NGC 2976NGC 2976 resides on the fringe of the M81 group of galaxies, located about 12 million light-years away in the constellation Ursa Major. This image, taken with NASA's Hubble Space Telescope, shows that the galaxy does not look like a typical spiral galaxy. In the galaxy's inner region, there are no obvious spiral arms. Dusty filaments running through the disk show no clear spiral structure. A raucous interaction with a neighboring group of hefty galaxies stripped away some gas and funneled the rest to the galaxy's inner region, fueling star birth about 500 million years ago. At the same time, the galaxy's outer regions stopped making stars because the gas ran out. Now, the inner disk is almost out of gas as new stars burst to life, shrinking the star-formation region to a small area of about 5,000 light-years around the core. The Hubble image can resolve hundreds of thousands of individual stars. What look like grains of sand in the image are actually single stars.J9RA57010 J9RA57020 J9RA57030http://hubblesite.org/newscenter/archive/releases/2010/05/image/a19839--3337.0 2331.0146.8344422 67.90889311669.5 1166.51570 1596 16222006-12-30 2006-12-30 2006-12-301.39134e-05 1.3913445e-058.3800560819e-06 -1.1094266444e-05 -1.1102296974e-05 -8.3964994332e-06image/tiffICRSJ2000TANg V IOptical Optical OpticalDecember 27, 2006 - January 10, 2007475 606 814ACS ACS ACShttp://hubblesite.org/newscenter/archive/releases/2010/05Space Telescope Science Institute Office of Public OutreachThe star-birth party is almost over in NGC 2976, located in the Ursa Major constellationNASA, ESA, and J. Dalcanton and B. Williams (University of Washington, Seattle)2011-03-17 00:00:00V254099.0006.317e-78.140e-74.750e-7meters