Oil bubbles inside water base form patterns

Oil bubbles inside water base form patterns
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Yellow gem under the microscope. Closeup macro photography.
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Cratering and Grooved Terrain on Ganymede
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GASTRALIA Dermal bones of the ventral wall of a Plesiosaurus. Geology Museum. Rapid City State of South Dakota. U.S.
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This image, taken Jan. 26, 2012, shows the back shell of NASA's Phoenix Mars Lander spacecraft after its second Martian arctic winter.
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Ganymede's Varied Terrain
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Dune fields in the high southern latitudes of Mars tell a mostly similar story during local summer. The dark dunes grow warmer than the surrounding bright plains because they absorb more sunlight. Dust devils form over the warm dunes but then dance out over the plains, spinning and performing pirouettes and leaving conspicuous dark tracks as bright dust is lifted from the surface. Loops in the tracks can often be used to discern the direction traveled by the dust devils, where in some cases, one track clearly overprints the other.
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This image is a still frame, created from images taken by NASA's Cassini spacecraft, shows white oval storms in Jupiter's southern hemisphere that rotate counterclockwise, similar to the larger Great Red Spot.
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A88448 U12P MISSION CYBER FAC MINEBACK & RECOVERY STALLER (PROJECT ENGINEER) APR 7 88 EG&G/NTS PHOTO LAB Publication Date: 4/7/1988 EDGERTON, GERMESHAUSEN & GRIER; EG&G; EQUIPMENT; EQUIPMENT & INSTRUMENTS; FAC MINEBACK & RECOVERY; INSTRUMENTS; INSTRUMENTS & EQUIPMENT; MISSION CYBER; NEVADA; NEVADA TEST SITE; NTS; NUCLEAR ENERGY TECHNOLOGY; NUCLEAR TESTING; NUCLEAR TESTS; TEST SITES; UGT; UNDERGROUND; UNDERGROUND TESTING; U12P MISSION CYBER historical images. 1972 - 2012. Department of Energy. National Nuclear Security Administration. Photographs Related to Nuclear Weapons Testing at the Nevada Test Site.
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This observation from NASA's Mars Reconnaissance Orbiter show it is late summer in the Southern hemisphere, so the Sun is low in the sky and subtle topography is accentuated in orbital images. We see many shallow pits in the bright residual cap of carbon dioxide ice (also called Swiss cheese terrain ). There is also a deeper, circular formation that penetrates through the ice and dust. This might be an impact crater or it could be a collapse pit.
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In this image, NASA's Mars Reconnaissance Orbiter (MRO) observes an impact crater with associated bright deposits that at first glance give the appearance of seasonal frost or ice accumulations. MRO has an onboard spectrometer called CRISM that can distinguish between ices and other minerals. Unfortunately, there is currently no coverage of this particular spot. However, it can be deduced through several lines of evidence that this is, in fact, not ice. Just like Earth, Mars experiences seasons that change as the planet orbits the Sun. Seasonal changes are most apparent at the higher latitudes. As these regions in each hemisphere enter their respective summer seasons, the Sun rises higher in the Martian sky causing frost and ice to sublimate, and illuminate more features across the landscape. As the high latitudes of each hemisphere move toward their respective winters, the days (called sols ) grow shorter and the sun hangs low on the horizon, giving rise to prolonged periods of cold,
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Meristem, light micrograph
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ISS006-E-26946 (16 February 2003) --- View of surface tension demonstration using water that is being held in place by a metal loop. Astronaut Donald R. Pettit, Expedition Six NASA ISS science officer, photographed these demonstrations for educational purposes. The experiment took place in the Destiny laboratory on the International Space Station (ISS).
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A88107 U12P MISSION CYBER POST SHOT G-SAC JOHN WEYDERT (PROJECT ENGINEER) JAN 11 88 EG&G/NTS PHOTO LAB Publication Date: 1/11/1988 EDGERTON, GERMESHAUSEN & GRIER; EG&G; EQUIPMENT; EQUIPMENT & INSTRUMENTS; GSAC; INSTRUMENTS; INSTRUMENTS & EQUIPMENT; MISSION CYBER; MISSION CYBER POST SHOT; NEVADA; NEVADA TEST SITE; NTS; NUCLEAR ENERGY TECHNOLOGY; NUCLEAR TESTING; NUCLEAR TESTS; TEST SITES; UGT; UNDERGROUND; UNDERGROUND TESTING; U12P MISSION CYBER POST SHOT historical images. 1972 - 2012. Department of Energy. National Nuclear Security Administration. Photographs Related to Nuclear Weapons Testing at the Nevada Test Site.
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The ultimate origin of the sediment that forms Martian dunes has long been debated. While sand dunes on Earth are primarily sourced by quartz-bearing components of granitic continental crust, it's often suggested that sand on Mars derives from eroded volcanic flows or sedimentary deposits, but exact sources are often vague. This image reveals a unique situation where this small dune field occurs along the summit of the large 1-mile-tall mound near the center of Juventae Chasma. The layered mound slopes are far too steep for dunes to climb, and bedform sand is unlikely to come from purely airborne material. Instead, the mound's summit displays several dark-toned, mantled deposits that are adjacent to the dunes and appear to be eroding into fans of sandy material. Along with local HiRISE images, spectral data from other instruments on MRO have confirmed such units are likely to be the sand source for these mound summit dunes and reveal how landscape evolution on Mars might occur. More in
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Image Number: 1848-66605300Royalty FreeCredit Line:Hulya Koca/imageBROKER/SuperStockCollection:imageBROKERStory:Microscopic and Planetary TexturesContributor:Hulya KocaModel Release:NoProperty Release:NoResolution:5584×3723
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