{
    "count": 3,
    "next": null,
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    "results": [
        {
            "id": 11366,
            "url": "https://svs.gsfc.nasa.gov/11366/",
            "result_type": "Produced Video",
            "release_date": "2013-10-24T00:00:00-04:00",
            "title": "Colossal Glow",
            "description": "Scientists first observed Saturn’s auroras in 1979. Decades later, these shimmering ribbons of light still fascinate. For one thing they’re magnificently tall, rising hundreds of miles above the planet’s poles. And unlike on Earth where bright displays fizzle after only a few hours, auroras on Saturn can shine for days. Auroras are produced when speeding particles accelerated by the sun’s energy collide with gases in a planet’s atmosphere. The gases fluoresce, emitting flashes of light at different wavelengths. Watch the video to see an edge-on view of Saturn’s northern and southern lights courtesy of NASA’s Hubble Space Telescope. || ",
            "hits": 62
        },
        {
            "id": 11365,
            "url": "https://svs.gsfc.nasa.gov/11365/",
            "result_type": "Produced Video",
            "release_date": "2013-10-22T00:00:00-04:00",
            "title": "New Planet",
            "description": "Scientists estimate more than 100 billion planets exist beyond our solar system. These alien worlds, known as exoplanets, orbit distant stars located light-years from Earth. One such planet is called HD 189733b. A gas giant slightly larger than Jupiter, HD 189733b circles its star from a distance of only 3 million miles. That's 13 times closer than Mercury is to our sun. As a result, temperatures in its atmosphere approach 2,000°F. Astronomers discovered HD 189733b in 2005 after observing its parent star dimming with every pass, or transit, of the planet. We now know from follow-up observations by NASA’s Hubble Space Telescope that HD 189733b is blue in color. Watch the video to learn more. || ",
            "hits": 61
        },
        {
            "id": 11352,
            "url": "https://svs.gsfc.nasa.gov/11352/",
            "result_type": "Produced Video",
            "release_date": "2013-09-05T00:00:00-04:00",
            "title": "Waveless Lakes",
            "description": "Lakes on another world are strange enough. But lakes without waves? Scientists studying Titan, Saturn’s largest moon, have never seen a wave in the hundreds of liquid pools discovered at its poles. Some of these pools are comparable in size to Earth’s biggest lakes. However, unlike our planet, Titan's lakes are not made of water. Data collected by NASA’s Cassini spacecraft show they're filled with a mix of methane, ethane and other complex hydrocarbons. Such molecules freeze at very low temperatures and can still exist as a liquid in Titan’s frigid minus 290°F weather. Cassini has surveyed Titan since it arrived at the Saturn system in 2004. Any wave, even millimeters high, would appear as a bright spot in its radar images. So why isn’t the surf up on these alien lakes? Researchers have put forth a new theory that may explain their calm surface. Watch the video to learn more. || ",
            "hits": 47
        }
    ]
}