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2741. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9C047376-08CE-4F93-B7C2-0E14B08042F2%7D
. An image of the globular star cluster M80 (NGC 6093) made using the Hubble Space Telescope. M80 contains hundreds of thousands of stars and is one of 147 globular clusters known to be associated with the Milky Way. The Hubble Heritage Team/AURA/STScI/NASA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9C047376-08CE-4F93-B7C2-0E14B08042F2%7D -- 3.3 Кб -- 10.04.2016
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2742. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B80A8FF9B-5975-4151-9959-AA912A3CB325%7D
. Saturn peaks this month when it lies opposite the Sun in our sky and shines brightly in central Virgo near blue-white Spica. Astronomy: Roen Kelly
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B80A8FF9B-5975-4151-9959-AA912A3CB325%7D -- 3.1 Кб -- 10.04.2016
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2743. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7EFA25D7-791E-49AC-B2B3-3A187461C7E4%7D
. A theoretical model of a galaxy like the Milky Way, showing trails of stars torn from disrupted satellite galaxies that have merged with the central galaxy. The region shown is about 1 million light-years on a side; the Sun is just 25,000 light-years from the center of the galaxy and would appear close to the center of this picture. K. Johnston/J. Bullock
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7EFA25D7-791E-49AC-B2B3-3A187461C7E4%7D -- 3.5 Кб -- 10.04.2016
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2744. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B78CD630D-C628-450D-B70F-3DF9E53A29CD%7D
The red colors in this image show the galaxy M66 as it appears at the submillimeter wavelength of 850 microns, while the white background shows the galaxy as it appears in visible light. Regions of cold dust that appear as dark streaks in the white image glow brightly in the red image. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B78CD630D-C628-450D-B70F-3DF9E53A29CD%7D -- 3.9 Кб -- 10.04.2016
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2745. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B699C92B1-A1A0-4EF8-906A-53ECF197CE9B%7D
. This 2006 Hubble Space Telescope optical image shows the belt of dust and debris (bright oval) surrounding the star Fomalhaut and the planet (inset) that orbits the star every 872 years and sculpts the inner edge of the belt. A coronagraph on the Advanced Camera for Surveys blocks out the light of the star (center), which is 100 million times brighter than the planet. Paul Kalas, UC Berkeley/STScI
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B699C92B1-A1A0-4EF8-906A-53ECF197CE9B%7D -- 3.6 Кб -- 10.04.2016
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2746. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6586F26C-4393-490B-BB50-E054534ED65F%7D
. A composite image of the colliding galaxies Arp 82, taken by the Spitzer Space Telescope (red), NASA's Galaxy Evolution Explorer (blue), and SARA telescope (green). NASA/JPL-Caltech/ETSU
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6586F26C-4393-490B-BB50-E054534ED65F%7D -- 3.1 Кб -- 10.04.2016
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2747. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B605FAE68-6141-4631-8E24-4C4B1C33ACC1%7D
. SOFIAтАЩs mid-infrared image of M42 (right) with comparison images of the same region made at other wavelengths by the Hubble Space Telescope (left) and European Southern Observatory (middle). Visible-light image: NASA/ESA/HST/AURA/STScI/OтАЩDell Wong; Near-IR image: ESO/McCaughrean et al.; Mid-IR image: NASA/DLR/SOFIA/USRA/DSI/FORCAST Team
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B605FAE68-6141-4631-8E24-4C4B1C33ACC1%7D -- 3.4 Кб -- 10.04.2016
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2748. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3ED50826-6946-4FC5-8E40-E418933B26F6%7D
. The locations of STEREOтАУA, STEREOтАУB and SDO relative to the Sun and Earth in 2011. Credit: NRL
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3ED50826-6946-4FC5-8E40-E418933B26F6%7D -- 2.9 Кб -- 10.04.2016
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2749. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B21957736-67FE-4201-A1C2-A26542FA6270%7D
. The white dwarf in the AE Aquarii system is the first star of its type known to give off pulsar-like pulsations that are powered by its rotation and particle acceleration. Casey Reed
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B21957736-67FE-4201-A1C2-A26542FA6270%7D -- 3.1 Кб -- 10.04.2016
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2750. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0887D22C-FE14-420D-A6C6-AFE600148258%7D
The top images show coronal cells as viewed from above by STEREO-B (on the left) and SDO (on the right). Their diameters are about 18,000 miles (29,000 kilometers). The bottom images show the same region as viewed almost simultaneously from the sides by STEREO-B (on the left) and SDO (on the right). The bottom views show the plumes as if they were leaning away from each observatory, the way a giant pillar would look if seen from the side. ... Credit: NASA/STEREO/SDO/NRL ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0887D22C-FE14-420D-A6C6-AFE600148258%7D -- 4.0 Кб -- 10.04.2016
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2751. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEBF5D4F3-3099-4674-84E7-0F96BDBAE87C%7D
Astronomers have discovered a massive cluster of young galaxies forming in the distant universe. The growing galactic metropolis, named COSMOS-AzTEC3, is the most distant known massive "proto-cluster" of galaxies, lying about 12.6 billion light-years from Earth. ... The other dots in this picture are stars or galaxies that are not members of the cluster тАФ most of them are located closer to us than the cluster, but some are farther away. The two brightest spots are stars. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEBF5D4F3-3099-4674-84E7-0F96BDBAE87C%7D -- 4.2 Кб -- 10.04.2016
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2752. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEA20A2A2-1BAA-41BA-8493-E075F250A793%7D
. Illustration of the gravitational lensing measurement of the cosmic expansion speed. The accelerated expansion increases the distance to the quasar, giving rise to higher chance of having a massive galaxy close to the light path to produce gravitational lensing. Credit: Kavli IPMU
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEA20A2A2-1BAA-41BA-8493-E075F250A793%7D -- 3.3 Кб -- 10.04.2016
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2753. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD5E6C5E0-A3E3-4E62-885F-0B62468F8C5F%7D
The Gemini South laser guide star тАЬconstellationтАЭ (upper left) is captured in this image. ... The yellow-orange beam is caused by scattering of the laser's light by Earth's lower atmosphere. The 30-second exposure was obtained January 21-22, 2011, using a 500mm f/5.6 Celestron telescope with a Canon Rebel XT camera at an ISO setting of 1600. Gemini Observatory/AURA ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD5E6C5E0-A3E3-4E62-885F-0B62468F8C5F%7D -- 4.2 Кб -- 10.04.2016
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2754. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC2376ACE-0F32-4DB9-B777-0D8BDD3F434E%7D
. Image of SDSSJ1226-0006, a new gravitationally lensed quasar discovered in this survey. The quasar image in the original image of the Sloan Digital Sky Survey, which has been used for the actual survey to identify gravitational lensing, looks only slightly extended, but the Hubble Space Telescope image clearly exhibits two distinct quasar images (white) as well as a massive galaxy in between the quasar images (orange) that produces gravitational lensing.
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC2376ACE-0F32-4DB9-B777-0D8BDD3F434E%7D -- 3.7 Кб -- 10.04.2016
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2755. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBFCBD4D4-A452-4F55-80C3-FCB2310C5569%7D
. Seeing baby dwarf galaxies. NASA/JPL-Calech/DSS
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBFCBD4D4-A452-4F55-80C3-FCB2310C5569%7D -- 2.8 Кб -- 10.04.2016
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2756. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBD369CCC-DBBD-4BD0-9667-10BDAE7E7386%7D
. The loose, patchy arms of M33 correlate with its pint-sized 1,500-solar-mass central black hole. T.A. Rector/M. Hanna (NRAO/AUI/NOAO/AURA/NSF
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBD369CCC-DBBD-4BD0-9667-10BDAE7E7386%7D -- 3.0 Кб -- 10.04.2016
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2757. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC0F9837-AD22-41EC-8EB1-EB372FF12DA3%7D
. NGC 253 is one of the brightest spiral galaxies in the sky, and also one of the dustiest. The whole galaxy is shown here as observed with the WFI instrument, while the insert shows a close-up of the central parts as observed with the NACO instrument on ESO's Very Large Telescope and the ACS on the NASA/ESA Hubble Space Telescope. ESO
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC0F9837-AD22-41EC-8EB1-EB372FF12DA3%7D -- 3.4 Кб -- 10.04.2016
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2758. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB87A2AA4-D65D-448D-B183-03C11BA7F9A4%7D
. The Andromeda Galaxy has tightly wound spiral arms and a beefy black hole weighing 170 million Suns. Conrad Jung
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB87A2AA4-D65D-448D-B183-03C11BA7F9A4%7D -- 2.9 Кб -- 10.04.2016
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2759. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA0278431-A8E0-413E-A8C6-BEF6EA1415A3%7D
This series of images shows the interaction of a white dwarf star with a black hole. As it passes the black hole, the white dwarf becomes strongly compressed and heated (top left), triggering an explosion. Most of the stellar mass is ejected into space (the "bubble" in the upper right part of the debris in the top right image), while the rest (the cusp-like part of the image) falls toward the black hole. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA0278431-A8E0-413E-A8C6-BEF6EA1415A3%7D -- 3.9 Кб -- 10.04.2016
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2760. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B910EA67C-BFD5-43F8-B501-F94A213E335B%7D
. Some scientists suspect that the x-ray afterglow following a gamma-ray burst is produced when a jet of high-energy particles shooting from a black hole (itself the remnant of an exploded star) slams into the expanding supernova shell. CXC / M. Weiss
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B910EA67C-BFD5-43F8-B501-F94A213E335B%7D -- 3.2 Кб -- 10.04.2016
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