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1921. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0BACD4C9-BF47-4221-946D-813A94F3A303%7D
. Mars Phoenix lander captured this image June 5, 2008 — its 11th day on the Red Planet. This view shows two trenches, Dodo (left) and Baby Bear (right), dug by the lander's robotic arm. Dodo was a test dig, but Baby Bear was collected as an analysis sample. NASA/JPL-Caltech/UA/Texas A&M
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0BACD4C9-BF47-4221-946D-813A94F3A303%7D -- 3.4 Кб -- 10.04.2016
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1922. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B01594279-F5DD-491E-899C-F8CA17E4EB56%7D
. Titan's surface shows ample evidence for drainage channels and dry lake beds that occasionally fill with liquid methane. The Huygens probe took this panoramic mosaic as it descended through the moon's windy atmosphere. ESA / NASA / University of Arizona
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B01594279-F5DD-491E-899C-F8CA17E4EB56%7D -- 3.2 Кб -- 10.04.2016
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1923. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFFF32241-AC6D-447A-9EEB-A587E7D13842%7D
. Warm, low-density material within Enceladus rises toward the surface at the moonтАЩs south pole. This heats the satelliteтАЩs icy shell and creates the hot spot and ice geysers the Cassini spacecraft detected in 2005. NASA /JPL / Space Science Institute
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFFF32241-AC6D-447A-9EEB-A587E7D13842%7D -- 3.3 Кб -- 10.04.2016
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1924. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEEAD1C6E-8508-42A4-A319-A546C2603935%7D
. Sequences of cyclic sedimentary rock layers exposed in an unnamed crater in Arabia Terra, Mars. Topography, Caltech; HiRISE Image, NASA/JPL/University of Arizona
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEEAD1C6E-8508-42A4-A319-A546C2603935%7D -- 3.0 Кб -- 10.04.2016
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1925. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEC59E6B2-7C04-4B13-9580-30B98362D9FF%7D
. Phoenix's Surface Stereo Imager took this false color image on Sol 72, the 72nd martian day after landing. It shows a soil sample from a trench informally called Rosy Red after being delivered to a gap between partially opened doors on the lander's TEGA. NASA/JPL-Caltech/University of Arizona/Texas A&M University
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEC59E6B2-7C04-4B13-9580-30B98362D9FF%7D -- 3.4 Кб -- 10.04.2016
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1926. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDFC320FD-7A59-4B5C-85A8-16BCD368A8F7%7D
. This photograph from June 2008, shows the robotic arm on NASA's Phoenix Mars Lander carrying a scoop of martian soil bound for the spacecraft's microscope. NASA/JPL-Caltech/University of Arizona
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDFC320FD-7A59-4B5C-85A8-16BCD368A8F7%7D -- 3.1 Кб -- 10.04.2016
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1927. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDBAE43D7-6158-474A-BC44-41E116D8CF46%7D
. This image shows Snow White in a patch of martian soil near the center of a polygonal surface feature, called Cheshire Cat. NASA/JPL-Caltech/University of Arizona/Texas A&M University/NASA Ames
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDBAE43D7-6158-474A-BC44-41E116D8CF46%7D -- 3.1 Кб -- 10.04.2016
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1928. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDACEF3F5-187A-4246-B4A0-E51F0A0AE24A%7D
. Dust devils in 3D: These images show the first (above) and second (below) dust devils imaged by Spirit. The dust devils are located top center in both images. Use red/blue stereo glasses to see the 3D effect. NASA / JPL / Cornell / Francis Reddy
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDACEF3F5-187A-4246-B4A0-E51F0A0AE24A%7D -- 3.2 Кб -- 10.04.2016
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1929. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD4C3ADCF-01E1-457B-B01E-72BD4CFD44A0%7D
. Nine days before it entered orbit, Cassini spacecraft captured this exquisite natural-color view of Saturn's rings. Cassini's narrow-angle camera took the images that make up this composition on June 21, from 4 million miles (6.4 million kilometers) away from the Ringed Planet. The scale is 23 miles (38 km) per pixel. NASA / JPL / Space Science Institute
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD4C3ADCF-01E1-457B-B01E-72BD4CFD44A0%7D -- 3.5 Кб -- 10.04.2016
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1930. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD494517F-8D7E-4ABD-B28A-87047D923650%7D
. Mimas drifts along in its orbit against the azure backdrop of Saturn's northern latitudes in this true-color view. The long, dark lines on the atmosphere are shadows cast by the planet's rings. NASA/JPL / Space Science Institute
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD494517F-8D7E-4ABD-B28A-87047D923650%7D -- 3.2 Кб -- 10.04.2016
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1931. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC152B6C0-91DD-42CE-8590-BF9C4A3DF893%7D
. This bright terrain is cut by channels that are variable in width; they form both radial and branching networks. This Cassini Synthetic Aperture Radar image of Titan was taken on Sept. 7, 2005, at a distance of 2,000 kilometers (1,250 miles). NASA/JPL
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC152B6C0-91DD-42CE-8590-BF9C4A3DF893%7D -- 3.3 Кб -- 10.04.2016
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1932. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBD08E3F9-CFB0-4AAE-B68F-A8380034C3F8%7D
. This Huygens image of Titan's surface merges a view from the camera's side-looking imager with one from the medium-resolution imager. The biggest water-ice rocks measure about 6 inches (15cm) across. ESA / NASA / JPL / University of Arizona
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBD08E3F9-CFB0-4AAE-B68F-A8380034C3F8%7D -- 3.2 Кб -- 10.04.2016
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1933. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB7572E02-FA3A-4F5B-B2A8-4AA78DA581BB%7D
. The circle marks the spot of the newly discovered moon S/2004 S 11, one of 13 new moons found orbiting Saturn. Of the 13 moons, S 11 lies closest to the planet, but it's still more than 10 million miles (16 million km) away. D. Jewitt and S. Sheppard (Hawaii) and J. Kleyna (Cambridge)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB7572E02-FA3A-4F5B-B2A8-4AA78DA581BB%7D -- 3.3 Кб -- 10.04.2016
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1934. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA0A59D26-4D84-4C11-BADC-62F9E4AD2BFF%7D
. This Synthetic Aperture Radar image of the surface of Saturn's moon Titan was obtained by the Cassini spacecraft on Sept. 7, 2005. The bright, rough region on the left side of the image seems to be topographically high terrain that is cut by channels and bays. NASA/JPL
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA0A59D26-4D84-4C11-BADC-62F9E4AD2BFF%7D -- 3.3 Кб -- 10.04.2016
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1935. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B94F7B224-0DBE-4F82-9837-A89034CA1E3E%7D
. This image shows the outer C and inner B rings, respectively, from left to right, with the inner B ring beginning a little more than halfway across the image. The general pattern is from dirty (red) particles to ice (turquoise) at greater distances from Saturn. NASA / Univ. Colorado, LASP
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B94F7B224-0DBE-4F82-9837-A89034CA1E3E%7D -- 3.3 Кб -- 10.04.2016
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1936. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B91540C6F-5A82-4827-BAB7-6B49C473FD67%7D
. Binary stars, like the ones depicted in this artist's drawing, will lose their orbital energy by generating gravity waves, according to Einstein's theory of General Relativity. The NASA/ESA/LISA satellites are designed to detect these waves. Planetary scientists will be able to use this data to gather useful information about near-Earth asteroids. NASA/courtesy of nasaimages.org
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B91540C6F-5A82-4827-BAB7-6B49C473FD67%7D -- 3.5 Кб -- 10.04.2016
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1937. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8FE77ECD-61F5-4255-BE00-6C60B3DDB47E%7D
. This image shows a microscopic view of fine-grained material at the tip of the Robotic Arm scoop aboard NASA's Phoenix Mars Lander on June 20, 2008. The image shows small clumps of fine, fluffy, red soil particles. NASA/JPL-Caltech/University of Arizona/Max Planck Institute
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8FE77ECD-61F5-4255-BE00-6C60B3DDB47E%7D -- 3.3 Кб -- 10.04.2016
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1938. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8D2AC258-2B3F-43F9-A4CC-499B6A90A406%7D
. Pack-ice-like plates cover the ground in Mars' southern Elysium Planitia, a possible relic of an ice-covered sea. A team of planetary geologists think some of the ice probably is still in the ground. The image frame spans about 25 miles (40 km), and the scale of the features matches that of pack ice on Earth. ESA / DLR / FU Berlin, G. Neukum
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8D2AC258-2B3F-43F9-A4CC-499B6A90A406%7D -- 3.5 Кб -- 10.04.2016
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1939. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8954EAFE-204D-475A-90BB-781A056571AE%7D
. This 180-degree panorama shows the southward vista from the location where Spirit is spending its third martian winter inside Mars' Gusev Crater . NASA/JPL/Cornell
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8954EAFE-204D-475A-90BB-781A056571AE%7D -- 3.1 Кб -- 10.04.2016
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1940. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B80C3B55C-03D4-4839-A009-06060B4785D5%7D
. Huygens took this panoramic image of Titan's surface from altitudes ranging between 11 and 5 miles (17 and 8 km). The probe landed at the center of the circle. ESA / NASA / JPL / University of Arizona
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B80C3B55C-03D4-4839-A009-06060B4785D5%7D -- 3.1 Кб -- 10.04.2016
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