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    "title": "Orion Nebula from Hubble",
    "description": "Orion Nebula from Hubble (2006) || orion_nebula-hst-9000x9000_print.jpg (1024x1024) [161.5 KB] || orion_nebula-hst-9000x9000.png (9000x9000) [79.3 MB] || orion_nebula-hst-9000x9000_searchweb.png (320x180) [85.2 KB] || orion_nebula-hst-9000x9000_thm.png (80x40) [6.3 KB] || orion-nebula-from-hubble.hwshow [218 bytes] || ",
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            "description": "This dramatic image offers a peek inside a cavern of roiling dust and gas where thousands of stars are forming. The image, taken by the Advanced Camera for Surveys (ACS) aboard NASA's Hubble Space Telescope, represents the sharpest view ever taken of this region, called the Orion Nebula. More than 3,000 stars of various sizes appear in this image. Some of them have never been seen in visible light. These stars reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that are reminiscent of the Grand Canyon.<br><br>The Orion Nebula is a picture book of star formation, from the massive, young stars that are shaping the nebula to the pillars of dense gas that may be the homes of budding stars. The bright central region is the home of the four heftiest stars in the nebula. The stars are called the Trapezium because they appear in a trapezoid pattern. Ultraviolet light unleashed by these stars is carving a cavity in the nebula and potentially disrupting the growth of hundreds of smaller stars. Located near the Trapezium stars are stars still young enough to have disks of material encircling them. These disks are called protoplanetary disks or \"proplyds\" and are too small to see clearly in this image. The disks are the building blocks of solar systems.<br><br>The bright glow at upper left is from M43, a small region being shaped by a massive, young star's ultraviolet light. Astronomers call the region a miniature Orion Nebula because only one star is sculpting the landscape. The Orion Nebula has four such stars. Next to M43 are dense, dark pillars of dust and gas that point toward the Trapezium. These pillars are resisting erosion from the Trapezium's intense ultraviolet light. The glowing region on the right reveals arcs and bubbles formed when stellar winds - streams of charged particles ejected from the Trapezium stars - collide with material.<br><br>The faint red stars near the bottom are the myriad brown dwarfs that Hubble spied for the first time in the nebula in visible light. Sometimes called \"failed stars,\" brown dwarfs are cool objects that are too small to be ordinary stars because they cannot sustain nuclear fusion in their cores the way our Sun does. The dark red column, below, left, shows an illuminated edge of the cavity wall.<br><br>The Orion Nebula is 1,400 light-years away, one of the nearest star-forming regions to Earth. Astronomers used 520 Hubble images, taken in five colors, to make this picture. They also added ground-based photos to fill out the nebula. The ACS mosaic covers approximately the apparent angular size of the full moon.<br><br>The Orion observations were taken between 2004 and 2005.",
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            "title": "For More Information",
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            "description": "See [http://hubblesite.org/news_release/news/2006-01](http://hubblesite.org/news_release/news/2006-01)",
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            "people": [
                {
                    "name": "Massimo Robberto",
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    "related": [
        {
            "id": 13983,
            "url": "https://svs.gsfc.nasa.gov/13983/",
            "page_type": "Produced Video",
            "title": "Hubble's Field Guide to Nebulae",
            "description": "Nebulae are some of the most resplendent objects in the universe, but it’s easy to confuse which one is an “emission nebula,” and which one is an “absorption nebula.”  Thankfully, this “Field Guide” will give you a quick rundown so you can impress all of your friends with your Nebulae Knowledge! And thanks to the Hubble Space Telescope, we can study all sorts of nebulae in all of their magnificent forms. For more information, visit https://nasa.gov/hubble. Additional Credits:Photo Logo Opener by Tony Ivonin via Motion ArrayMusic Credits: “Himalayan Temple” by Jan Pham Huu Tri [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music || ",
            "release_date": "2021-11-01T09:55:00-04:00",
            "update_date": "2023-05-03T13:43:47.378149-04:00",
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                "filename": "13983_Nebula_Guide_WIDE_PRINT.jpg",
                "media_type": "Image",
                "alt_text": "Master VersionHorizontal version. This is for use on any YouTube or non-YouTube platform where you want to display the video horizontally.",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        },
        {
            "id": 13320,
            "url": "https://svs.gsfc.nasa.gov/13320/",
            "page_type": "Produced Video",
            "title": "Hubble Shows Torrential Outflows from Infant Stars May Not Stop Them from Growing",
            "description": "Though our galaxy is an immense city of at least 200 billion stars, the details of how they formed remain largely cloaked in mystery. Scientists know that stars form from the collapse of huge hydrogen clouds that are squeezed under gravity to the point where nuclear fusion ignites. But only about 30 percent of the cloud’s initial mass winds up as a newborn star. Where does the rest of the hydrogen go during such a terribly inefficient process?For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Additional Visualizations:Zoom In To Star Formation: ESA, Silicon WorldsWide Image of Orion Complex: Image courtesy of Rogelio Bernal Andreo, DeepSkyColors.comHerschel and Rosette Nebula: ESA - C. CarreauSpace Cloud: ESA/Hubble (M. Kornmesser & L. L. Christensen)Zoom out of Milky Way: ESA, Silicon WorldsMusic Credits: \"Winter Solstice\" by Laetitia Frenod [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM], and Universal Production Music. || ",
            "release_date": "2021-03-18T08:55:00-04:00",
            "update_date": "2023-05-03T13:44:16.107648-04:00",
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                "filename": "13320_ORION_WIDE_PRINT.jpg",
                "media_type": "Image",
                "alt_text": "Master VersionHorizontal version. This is for use on any YouTube or non-YouTube platform where you want to display the video horizontally.",
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                "height": 1080,
                "pixels": 2073600
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        },
        {
            "id": 30775,
            "url": "https://svs.gsfc.nasa.gov/30775/",
            "page_type": "Hyperwall Visual",
            "title": "Hubble and Spitzer Composite of the Orion Nebula",
            "description": "Hubble and Spitzer collaborate to show hundreds of baby stars and strong stellar winds shaping the gas and dust of the Orion Nebula || orion_nebula_vis_ir-hst_sst-3240x3240_print.jpg (1024x1024) [228.6 KB] || orion_nebula_vis_ir-hst_sst-3240x3240.png (3240x3240) [10.9 MB] || orion_nebula_vis_ir-hst_sst-6000x6000.png (6000x6000) [41.2 MB] || orion_nebula_vis_ir-hst_sst-3240x3240_searchweb.png (320x180) [107.4 KB] || orion_nebula_vis_ir-hst_sst-3240x3240_thm.png (80x40) [22.7 KB] || hubble-and-spitzer-composite-of-the-orion-nebula.hwshow [346 bytes] || ",
            "release_date": "2006-01-11T00:00:00-05:00",
            "update_date": "2024-10-10T00:26:15.741212-04:00",
            "main_image": {
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                "media_type": "Image",
                "alt_text": "Hubble and Spitzer collaborate to show hundreds of baby stars and strong stellar winds shaping the gas and dust of the Orion Nebula",
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