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2241. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B335A46AB-0838-44A6-AC12-C8B1691BC2AC%7D
. Kepler 78b // Cristina Sanchis Ojeda
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B335A46AB-0838-44A6-AC12-C8B1691BC2AC%7D -- 2.8 Кб -- 10.04.2016
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2242. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1AEEB647-C5A4-4262-B3C3-6120D6A5A8B3%7D
. Rock fins up to about 1 foot (30 centimeters) tall dominate this scene from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Opportunity. // Image credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1AEEB647-C5A4-4262-B3C3-6120D6A5A8B3%7D -- 3.1 Кб -- 10.04.2016
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2243. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B06DDA4BE-98C8-444E-9D28-E720175E85E1%7D
. Artist's conception of SS Cygni double-star system. "Normal" red-dwarf star, left, has material pulled from it onto swirling disk surrounding compact white-dwarf star, right. Outbursts occur when the disk becomes unstable. // Bill Saxton, NRAO/AUI/NSF
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B06DDA4BE-98C8-444E-9D28-E720175E85E1%7D -- 3.3 Кб -- 10.04.2016
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2244. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B05023674-C274-410B-BED5-4BF672A99A56%7D
. Streaming out from the center of the galaxy M87 like a cosmic searchlight is one of nature's most amazing phenomena, a black-hole-powered jet of sub-atomic particles traveling at nearly the speed of light. In this Hubble Space Telescope image, the blue of the jet contrasts with the yellow glow from the combined light of billions of unseen stars and the yellow, point-like globular clusters that make up this galaxy. // Credit: NASA and the Hubble Heritage Team
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B05023674-C274-410B-BED5-4BF672A99A56%7D -- 3.7 Кб -- 10.04.2016
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2245. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B018A8D1C-B06B-48EE-B2A5-55F50BFDF99A%7D
... The picture in the top left shows the SDSS-III view of a small part of the sky, centered on the galaxy M33. The middle top picture is a further zoom-in on M33, showing the spiral arms of this galaxy, including the blue knots of intense star formation known as "HII regions." The top right-hand picture is a further zoom into M33 showing the object NGC 604, which is one of the largest HII regions in that galaxy. ... M. Blanton and the SDSS-III ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B018A8D1C-B06B-48EE-B2A5-55F50BFDF99A%7D -- 4.5 Кб -- 10.04.2016
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2246. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF9C27049-E488-4657-92A8-7276BE85E80B%7D
. This image of the Venus southern hemisphere illustrates the terminator тАФ the transitional region between the dayside (left) and nightside of the planet (right). The south pole is near the terminator, just above the center of the image. The complex atmosphere that surrounds the planet is also clearly visible. // Credits: ESA/MPS, Katlenburg-Lindau, Germany
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF9C27049-E488-4657-92A8-7276BE85E80B%7D -- 3.5 Кб -- 10.04.2016
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2247. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF7DA4136-B42F-48E1-B86A-1D236C35BE5F%7D
. A family portrait of the PH1 planetary system. PH1 is depicted in this artist's rendition with the pair of eclipsing stars it orbits. The planet transits in front the larger of the two stars approximately every 138 days. Off in the distance, well beyond PH1's orbit, resides a second pair of stars bound to the planetary system. // Credit: Haven Giguere/Yale Univ.
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF7DA4136-B42F-48E1-B86A-1D236C35BE5F%7D -- 3.5 Кб -- 10.04.2016
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2248. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD7E1ED49-171F-4B33-B854-450AEF6EBD72%7D
. Close-up of olivine crystals seen inside a meteorite found on Earth that originated from a partly melted solar system asteroid. The yellow olivine crystals are on the order of a few millimeters to centimeters in size and are held together by an alloy of iron and nickel. In contrast, the olivine crystals found in pristine comets, such as in the material measured in the Beta Pictoris system by ESAтАЩs Herschel space observatory, are iron-poor but magnesium-rich. // Credit: J. Debosscher, KU Leuven
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD7E1ED49-171F-4B33-B854-450AEF6EBD72%7D -- 3.8 Кб -- 10.04.2016
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2249. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD25B149A-DE39-4B2D-87DC-15583D015C8D%7D
. LADEE star tracker image with Golgi and Zinner Craters. NASA Ames
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD25B149A-DE39-4B2D-87DC-15583D015C8D%7D -- 2.9 Кб -- 10.04.2016
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2250. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBFE78C9B-2CC9-471C-A8F5-7325FD669FAE%7D
. LADEE star tracker image with Krieger and Toscanelli Craters. NASA Ames
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBFE78C9B-2CC9-471C-A8F5-7325FD669FAE%7D -- 2.9 Кб -- 10.04.2016
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2251. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC8EF0A5-0360-4884-8A71-93C4AD539C7C%7D
XMM-Newton observation of the core of the massive cluster Cyg OB2 located in the constellation Cygnus, 4,700 light-years from Earth. The cluster contains massive O-type stars that shine brightly in X-rays. Cyg OB2 #9 is seen as the bright star just below the central star, and in 2008 was determined to be a binary system. ... Hundreds of lower mass stars also fill the field of view, which spans nearly 22 x 16 arcminutes. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC8EF0A5-0360-4884-8A71-93C4AD539C7C%7D -- 4.2 Кб -- 10.04.2016
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2252. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBBFB27CA-195C-4B11-B88D-9ADD8E902491%7D
. Mars Express image of the moons Phobos (foreground) and Deimos (background). // Credit: ESA/DLR/FU Berlin (G. Neukum)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBBFB27CA-195C-4B11-B88D-9ADD8E902491%7D -- 2.9 Кб -- 10.04.2016
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2253. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB9EE55B0-CAE6-4B31-993F-19E554C98F62%7D
. The cratered plains of Saturn's moon Rhea are visible in this image obtained by NASA's Cassini spacecraft November 21, 2009. NASA/JPL/Space Science Institute
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB9EE55B0-CAE6-4B31-993F-19E554C98F62%7D -- 3.0 Кб -- 10.04.2016
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2254. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB6A70F8C-77E0-4BEE-9D4D-B0113598506E%7D
. ArtistтАЩs impression of the exoplanet Tau Bo?Єtis b. Credit: ESO
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB6A70F8C-77E0-4BEE-9D4D-B0113598506E%7D -- 2.9 Кб -- 10.04.2016
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2255. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB380223F-AB19-476B-9100-6FC07F0F1259%7D
. This artist's conception illustrates a storm of comets around a star near our own, called Eta Corvi. Evidence for this barrage comes from NASA's Spitzer Space Telescope whose infrared detectors picked up indications that one or more comets was recently torn to shreds after colliding with a rocky body. Credit: NASA/JPL-Caltech
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB380223F-AB19-476B-9100-6FC07F0F1259%7D -- 3.4 Кб -- 10.04.2016
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2256. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB0AA6BDD-9DAC-43CC-80B8-8C0B5C5EC81C%7D
. Mercury reaches the peak of of its 2012 evening appearance March 5, when it lies farthest from the Sun and climbs highest in the twilight sky. NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB0AA6BDD-9DAC-43CC-80B8-8C0B5C5EC81C%7D -- 3.2 Кб -- 10.04.2016
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2257. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BADB6EA5C-8F59-4221-97CE-D724FFBB42D2%7D
. A giant black hole in the center of the galaxy 4C+29.30 is generating two powerful jets of particles. By combining X-rays (blue), optical (gold), and radio (pink) data, astronomers get a full picture of what is happening. // X-ray: NASA/CXC/SAO/A.Siemiginowska et al; Optical: NASA/STScI; Radio: NSF/NRAO/VLA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BADB6EA5C-8F59-4221-97CE-D724FFBB42D2%7D -- 3.5 Кб -- 10.04.2016
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2258. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA12449A7-09DF-45B7-BBD9-11C2B9FB68CD%7D
Relationship between the diameter and cumulative number of bodies larger than the size obtained from the observed asteroids. ... The red circles show the diameter range used for evaluation of the distribution slope, which indicates the asteroid population. ... The slope changes at one kilometer, a shift that asteroids near the ecliptic plane also show. The blue and green lines show the estimated slope of asteroids in diameter ranges smaller and larger than one kilometer, respectively. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA12449A7-09DF-45B7-BBD9-11C2B9FB68CD%7D -- 4.6 Кб -- 10.04.2016
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2259. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9EA3409A-2625-4307-91BB-3756FD875C7C%7D
. LADEE star tracker image with Wollaston P Crater and Mons Herodotus. NASA Ames
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9EA3409A-2625-4307-91BB-3756FD875C7C%7D -- 3.0 Кб -- 10.04.2016
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2260. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B99DA6B1B-1F4A-4E86-B7C2-C8105B044046%7D
. Post-lunar cataclysm diagram of our solar system. Credit: LPI/Marchi/Bottke/Kring/Morbidelli
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B99DA6B1B-1F4A-4E86-B7C2-C8105B044046%7D -- 2.9 Кб -- 10.04.2016
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