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    "title": "Supermassive Black Holes",
    "description": "In this video NuSTAR (Nuclear Spectroscopic Telescope Array) lead scientist Peter Boorman explains how the NuSTAR penetrates thick gas and dust to reveal black holes that other telescopes can’t see. \r\n\r\nThis video was prepared for use on the NASA Hyperwall from content originally published at [https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/](https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/)",
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            "description": "NuSTAR (the Nuclear Spectroscopic Telescope Array) is a NASA Small Explorer mission launched in 2012 and the first telescope in orbit to create images by focussing light in the high-energy X-ray (3 – 79 keV) region of the electromagnetic spectrum. NuSTAR is an active mission, coordinationing with other X-ray missions and responding to the rapidly changing X-ray sky. Its unique capabilities enable the study of a wide range of scientific targets, from supermassive black holes to our very own Sun.  \r\n\r\nIn this video NuSTAR lead scientist Peter Boorman explains how the NuSTAR space telescope penetrates thick gas and dust to reveal black holes that other telescopes can’t see. \r\n\r\nThis video was prepared for use on the NASA Hyperwall from content originally published at [https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/](https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/)",
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            "description": "Most supermassive black holes in the universe are hiding, but NASA’s NuSTAR mission can find them by using high-energy X-rays. \r\n**NASA/JPL-Caltech/Goddard Space Flight Center Conceptual Image Lab**",
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    "credits": [
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            "people": [
                {
                    "name": "Marit Jentoft-Nilsen",
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            "id": 31273,
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            "page_type": "Hyperwall Visual",
            "title": "NASA Telescopes Chase Down \"Green Monster\" in Star's Debris",
            "description": "Animations of images originally published at https://chandra.harvard.edu/photo/2024/casa/ and https://www.nasa.gov/image-article/nasa-telescopes-chase-down-green-monster-in-stars-debris/.Astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure called the “Green Monster”. Composite images from Chandra, Webb, Hubble, NuSTAR, and Spitzer reveal where elements such as silicon, iron, and titanium are located. Comparing where certain elements are with the location of the blast wave, researchers conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it. || ",
            "release_date": "2024-01-31T00:00:00-05:00",
            "update_date": "2025-06-23T00:34:54.913535-04:00",
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