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    "url": "https://svs.gsfc.nasa.gov/14619/",
    "page_type": "Produced Video",
    "title": "Black Hole with Accretion Disk Visualization",
    "description": "This visualization shows the strange ways that light is gravitationally warped in the region around a black hole surrounded by a rapidly-rotating disk of gas and dust. The distortions seen in this image are due to the physics of general relativity, which informs us how the path of light is deflected in the presence of a gravitational field. The material forming a black hole has been compressed to densities so high that it is hidden within an “event horizon,” beyond which the gravitational field is so strong that nothing, not even light, can escape. Outside of this event horizon light paths will bend sharply, and even loop around the black hole, under the influence of the intense gravitational fields.The speed at which material, in what is known as an accretion disk, orbits the black hole increases with proximity. The orbital speed of material closest to the event horizon approaches the speed of light. This produces an effect known as “relativistic doppler beaming” which enhances the brightness of material moving towards us along our line of sight, and correspondingly dims the brightness of material moving away.The gravitational warping of the light from background stars is strong, creating the effect of a powerful lens. Light from the region directly behind the black hole forms an “Einstein Ring” that encircles the event horizon. Inside this ring we find an inverted view of the entire sky, which is increasingly distorted. The inner black disk is known as the black hole’s “shadow” which appears slightly larger than the actual location of the event horizon due to the distortion of the light paths.The light from the orbiting material is likewise distorted, making the flat accretion disk appear to bend completely around the black hole’s shadow and have the disk behind the black hole appear to be both above and below it. Yet despite these strange visual distortions that change with viewing angle, the accretion disk itself physically remains flat.These illustrations depict what is known as a “Schwarzschild” black hole, made from material that had no overall rotation. A black hole created from rapidly spinning material retains a sense of this rotation and displays additional asymmetries not pictured here; this is known as a “Kerr” black hole.The appearance of a black hole like this is “scale invariant,” meaning that the way light warps around it will appear the same, regardless of the mass of the object. The only thing that changes is the overall size of the distortions and shadow. Thus a black hole ten times as massive as the one shown here, viewed from ten times further away, would look exactly the same.These animations show qualitatively correct depictions of light distortion around a black hole that use a simplified optical model for the effect, rather than full general relativistic ray-tracing code. || ",
    "release_date": "2024-07-17T10:00:00-04:00",
    "update_date": "2024-07-02T11:22:58.202069-04:00",
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        "alt_text": "This movie shows the approach to a black hole surrounded by an accretion disk. Ripples and waves in the disk are caused by turbulent instabilities in the orbiting material, which is hottest and brightest along the inner edge of the disk.",
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        "height": 576,
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    "main_credits": {
        "Visualizations by": [
            {
                "name": "Robert Hurt",
                "employer": "Caltech-IPAC"
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        "Produced by": [
            {
                "name": "Keith Miller",
                "employer": "Caltech-IPAC"
            },
            {
                "name": "Chelsea Gohd",
                "employer": "NASA/JPL"
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        "Written by": [
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                "name": "Robert Hurt",
                "employer": "Caltech-IPAC"
            }
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    "progress": "Complete",
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                        "alt_text": "This abstract movie highlights the ways light is warped by the gravity of a black hole. It sits in an environment inscribed with latitude and longitude lines, and is orbited by a rainbow-colored disk. The colors can help interpret how light paths are affected by the black hole. For instance, the background is colored to be orange above the black hole and blue below it, but inside the “Einstein Ring” we see the colors are inverted, coming from opposite sides of the sky. Similarly, the color coding of the surrounding disk highlights the inverted view of the underside of the disk seen close to the black hole.",
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        {
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            "url": "https://svs.gsfc.nasa.gov/14620/",
            "page_type": "Produced Video",
            "title": "Isolated Black Hole Visualization",
            "description": "This visualization shows the strange ways that light is gravitationally warped in the region around a black hole. The distortions seen in this image are due to the physics of general relativity, which informs us how the path of light is deflected in the presence of a gravitational field. The material forming a black hole has been compressed to densities so high that it is hidden within an “event horizon,” beyond which the gravitational field is so strong that nothing, not even light, can escape. Outside of this event horizon light paths will bend sharply, and even loop around the black hole, under the influence of the intense gravitational fields.The gravitational warping of the light from background stars is strong, creating the effect of a powerful lens. Light from the region directly behind the black hole forms an “Einstein Ring” that encircles the event horizon. Inside this ring we find an inverted view of the entire sky, which is increasingly distorted. The inner black disk is known as the black hole’s “shadow” which appears slightly larger than the actual location of the event horizon due to the distortion of the light paths.These illustrations depict what is known as a “Schwarzschild” black hole, made from material that had no overall rotation. A black hole created from rapidly spinning material retains a sense of this rotation and displays additional asymmetries not pictured here; this is known as a “Kerr” black hole.The appearance a black hole like this is “scale invariant,” meaning that the way light warps around it will appear the same, regardless of the mass of the object. The only thing that changes is the overall size of the distortions and shadow. Thus a black hole ten times as massive as the one shown here, viewed from ten times further away, would look exactly the same.These animations show qualitatively correct depictions of light distortion around a black hole that use a simplified optical model for the effect, rather than full general relativistic ray-tracing code. || ",
            "release_date": "2024-07-17T10:00:00-04:00",
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                "alt_text": "In this video the camera orbits around a bare black hole, getting closer to it over time. The black hole is only seen because of the way light warps around it. Note how an inverted view of the sky appears inside the “Einstein Ring” surrounding the black hole’s shadow. Features that are about to move into the left side of the frame can first be seen slowly moving away from the right side of the black hole’s shadow. ",
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            "title": "What is a black hole? Astro-Investigates Ep. 1",
            "description": "Black holes - what are they really? Learn this and more with “Astro-Investigates,” the video series that explores and explains big astrophysics topics with the help of NASA scientists. In this episode, you’ll hear from: Joanna Piotrowska - Astrophysicist at Caltech Varoujan Gorjian - NASA Research Astronomer Daniel Stern - NASA Astrophysicist Michele Vallisneri - NASA Theoretical physicist To learn more about black holes and NASA missions studying these mysterious objects, visit: [https://science.nasa.gov/universe/bla...](https://science.nasa.gov/universe/black-holes/) || JPL_Explainers_BH_FINAL.00096_print.jpg (1024x576) [76.6 KB] || JPL_Explainers_BH_FINAL.00096_searchweb.png (320x180) [61.4 KB] || JPL_Explainers_BH_FINAL.en_US.srt [9.2 KB] || JPL_Explainers_BH_FINAL.en_US.vtt [8.7 KB] || JPL_Explainers_BH_FINAL.mp4 (1920x1080) [812.8 MB] || JPL_Explainers_BH_FINAL_NoText.mp4 (1920x1080) [815.1 MB] || ",
            "release_date": "2024-07-17T10:00:00-04:00",
            "update_date": "2024-07-22T09:57:54.712206-04:00",
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                "media_type": "Image",
                "alt_text": "Black holes - what are they really? Learn this and more with “Astro-Investigates,” the video series that explores and explains big astrophysics topics with the help of NASA scientists. In this episode, you’ll hear from: Joanna Piotrowska - Astrophysicist at Caltech Varoujan Gorjian - NASA Research Astronomer Daniel Stern - NASA Astrophysicist Michele Vallisneri - NASA Theoretical physicist To learn more about black holes and NASA missions studying these mysterious objects, visit: [https://science.nasa.gov/universe/bla...](https://science.nasa.gov/universe/black-holes/)",
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    "products": [
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            "id": 14802,
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            "title": "Earth to Space: A National Symphony Orchestra Concert",
            "description": "Explore the vastness of space with music inspired by the planets, stars, and beyond! In anticipation of the upcoming voyage of Artemis II, the National Symphony Orchestra celebrates the discoveries and beauty of space through music and images produced by NASA. Explore this page to learn more about the visuals used in the Kennedy Center's 2025 Earth to Space Festival NSO Family Concert.",
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                "alt_text": "This artist's concept shows how the universe might have looked when it was less than a billion years old, about 7 percent of its current age. Star formation voraciously consumed primordial hydrogen, churning out myriad stars at an unprecedented rate. NASA’s Nancy Grace Roman Space Telescope will peer back to the universe’s early stages to understand how it transitioned from being opaque to the brilliant starscape we see today.\rCredit: NASA, ESA, and A. Schaller (for STScI)\rAlt text: This illustration depicts a mesmerizing and chaotic cosmic scene, filled with misshapen clumps and twists of white and purplish material on a black background. Most of the clumps are small, but a particularly large conglomeration extends from the lower-right of the frame up to the middle and nearly all the way across to the left side, sort of like billowing clouds. It's full of bulbous shapes outlined with glowing lavender tendrils. Bright groups of stars are concentrated in the center of each lobe, and also scattered more sparsely throughout the surrounding area.",
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