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            "id": 10679,
            "url": "https://svs.gsfc.nasa.gov/10679/",
            "result_type": "Produced Video",
            "release_date": "2010-11-02T09:00:00-04:00",
            "title": "Using Color to Search for Alien Earths",
            "description": "NASA astronomer Lucy McFadden and UCLA graduate Carolyn Crow recently made a discovery that will help identify characteristics of extrasolar planets, such as the compositions of their surfaces and atmospheres. By comparing the reflected red, blue, and green light from planets in our solar system, a team led by Crow and McFadden was able to group the planets according to their similarities. As it turns out, the planets fall into very distinct regions on this plot, where the vertical direction indicates the relative amount of blue light, and the horizontal direction the relative amount of red light. This technique works even when the source of the reflected light is visible only as a point, like exoplanets appear when observed through a telescope. Therefore, scientists can use it to identify earthlike planets more easily. || ",
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            "url": "https://svs.gsfc.nasa.gov/10536/",
            "result_type": "Produced Video",
            "release_date": "2009-12-02T06:00:00-05:00",
            "title": "Suzaku: Intergalactic Prospector",
            "description": "Recently astronomers used the Suzaku orbiting X-ray observatory, operated jointly by NASA and the Japanese space agency, to discover the largest known reservoir of rare metals in the universe.  Suzaku detected the elements chromium and manganese while observing the central region of the Perseus galaxy cluster. The metallic atoms are part of the hot gas, or \"intergalactic medium,\" that lies between galaxies. Exploding stars, or supernovas, forge the heavy elements. The supernovas also create vast outflows, called superwinds. These galactic gusts transport heavy elements into the intergalactic void. || ",
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