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Coffee Shoppe
Posted On: 06/11/2013 5:26:44 PM
Post# of 63836
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Posted By: PoemStone


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  • Thursday, June 13: NASA Historian Bill Barry: "The Space Program Under Presidents Nixon and Ford," UStream, Noon EDT






  • Martian Dune Marks May Be Tracks of Dry-Ice Sleds


    Several types of downhill flow features have been observed on Mars. This image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter is an example of a type called



    NASA research indicates hunks of frozen carbon dioxide -- dry ice -- may glide down some Martian sand dunes on cushions of gas similar to miniature hovercraft, plowing furrows as they go.

    Researchers deduced this process could explain one enigmatic class of gullies seen on Martian sand dunes by examining images from NASA's Mars Reconnaissance Orbiter (MRO) and performing experiments on sand dunes in Utah and California.








    • Several types of downhill flow features have been observed on Mars. This image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter is an example of a type called

      Dune Marks




    • Permafrost zones occupy nearly a quarter of the exposed land area of the Northern Hemisphere. NASA's Carbon in Arctic Reservoirs Vulnerability Experiment is probing deep into the frozen lands above the Arctic Circle in Alaska to measure emissions of the greenhouse gases carbon dioxide and methane.

      Arctic Climate




    • The Sculptor galaxy is seen in a new light, in this composite image from NASA's Nuclear Spectroscopic Telescope Array (NuSTAR) and the European Southern Observatory in Chile. Image credit: NASA/JPL-Caltech/JHU

      Black Hole




    • This illustration shows a newfound reservoir of stellar fuel discovered by the Herschel space observatory (red). Image credit: ESA/NASA/JPL-Caltech

      Pools of Gas




    • An M-class flare appears on the lower right of the sun on June 7, 2013. This image was captured by NASA’s Solar Dynamics Observatory in the 131 Angstrom wavelength, a wavelength of UV light that is particularly good for seeing flares and that is typically colorized in teal. Caption: NASA/SDO

      Solar Flare



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