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            "release_date": "2017-03-30T14:00:00-04:00",
            "title": "MAVEN Reveals Mars Argon Loss to Space",
            "description": "Infographic explaining the MAVEN argon results. Enlarge or click \"download\" for print-resolution versions. Also available in text-readable PDF for the visually impaired. || MAVEN_Argon_Infographic_print.jpg (1024x450) [159.1 KB] || MAVEN_Argon_Infographic.jpg (7500x3300) [4.1 MB] || MAVEN_Argon_Infographic.png (7500x3300) [27.0 MB] || MAVEN_Argon_Infographic_searchweb.png (320x180) [72.3 KB] || MAVEN_Argon_Infographic_thm.png (80x40) [5.0 KB] || MAVEN_Argon_Infographic.tif (7500x3300) [27.2 MB] || maven-reveals-mars-argon-loss-to-space.hwshow || ",
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            "result_type": "Hyperwall Visual",
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            "title": "Sloshing Supernovas",
            "description": "Cassiopeia A, one of astronomy’s most famous supernova remnants, was created when a massive star blew up leaving behind a dense stellar corpse and its ejected remains. How supernovas explode, however, has been a mystery for a long time. With the help of NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR), scientists have been able to see into the heart of a supernova explosion for the first time, by detecting high-energy X-rays emitted by the radioactive isotope titanium-44. This image of Cas A shows titanium concentrated in clumps at the remnant's center (in blue). The irregular distribution of the clumps strongly suggests that material at the heart of the exploding star literally “sloshed” around, thereby allowing the shockwave to escape the core of the collapsing star and blast off the star’s outer layers. This NuSTAR map shows high-energy X-rays generated by titanium-44, shown here in blue. Lower-energy X-rays from non-radioactive material, imaged previously with NASA's Chandra X-ray Observatory, are shown in red, yellow and green. || ",
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            "title": "Sample Analysis at Mars (SAM)",
            "description": "Sample Analysis at Mars (SAM) is a suite of instruments developed for use on the Mars Science Laboratory. By looking for evidence of water, carbon, and other important building blocks of life in the Mars soil and atmosphere, this suite will help answer one of humankind's biggest questions about the planet: did it ever support life? SAM was designed and built in an international collaboration between Goddard Space Flight Center, the Jet Propulsion Laboratory, the University of Paris, and Honeybee Robotics. This video series highlights the mission, its objectives, and some of Goddard's contributors to the project. || ",
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            "url": "http://svs.gsfc.nasa.gov/20064/",
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            "title": "Model for Coronal Mass Ejections",
            "description": "A coronal mass ejection (CME) is a massive burst of solar wind, other light isotope plasma, and magnetic fields rising above the solar corona or being released into space. || CME_640x480_pre.00002_print.jpg (1024x768) [45.1 KB] || CME_640x480_thm.png (80x40) [4.5 KB] || CME_640x480_pre.jpg (320x240) [3.1 KB] || CME_320x240_pre.jpg (320x240) [2.9 KB] || CME_320x240_pre_searchweb.jpg (320x180) [11.8 KB] || CME_NTSC.webmhd.webm (960x540) [1.1 MB] || 720x486_4x3_30 (720x486) [32.0 KB] || CME_640x480.mpg (640x480) [10.7 MB] || CME_NTSC.m2v (720x480) [17.2 MB] || a010066_seq.mpg (720x480) [8.2 MB] || a010066_H264_640x480.mp4 (640x480) [7.1 MB] || CME_320x240.mpg (320x240) [2.8 MB] || ",
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