{"id":12718,"date":"2024-12-16T12:00:30","date_gmt":"2024-12-16T16:00:30","guid":{"rendered":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/nasas-webb-finds-planet-forming-disks-lived-longer-in-early-universe\/"},"modified":"2024-12-16T12:00:30","modified_gmt":"2024-12-16T16:00:30","slug":"nasas-webb-finds-planet-forming-disks-lived-longer-in-early-universe","status":"publish","type":"post","link":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/nasas-webb-finds-planet-forming-disks-lived-longer-in-early-universe\/","title":{"rendered":"NASA\u2019s Webb Finds Planet-Forming Disks Lived Longer in Early Universe"},"content":{"rendered":"<h2 style=\"text-align: center;\">NASA\u2019s Webb Finds Planet-Forming Disks Lived Longer in Early Universe<\/h2>\n<p><!-- no image --><\/p>\n<div class=\" hds-module hds-module-full wp-block-nasa-blocks-secondary-navigation\">\n<div class=\"hds-secondary-navigation-wrapper z-top width-100 padding-0\">\n<div class=\"hds-secondary-navigation 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width-full maxw-full color-mode-dark hds-module hds-module-full wp-block-nasa-blocks-article-hero-header\">\n<div class=\"hds-cover-wrapper width-full maxw-full minh-tablet grid-container minh-tablet flex-column padding-0\">\n<div class=\"hds-foreground-wrapper display-flex flex-direction-column\">\n<div class=\"grid-container grid-container-block margin-top-auto width-full maxw-desktop-lg padding-y-9 padding-x-3 desktop:padding-x-3 z-400\">\n<div class=\"z-400 grid-col-12 tablet:grid-col-12 desktop:grid-col-7 z-400\">\n<div class=\"margin-0\">\n<div class=\"label color-spacesuit-white margin-bottom-2\">7 Min Read<\/div>\n<h1 class=\"heading-41 line-height-md color-spacesuit-white-important\">\n\t\t\t\t\t\t\t\tNASA\u2019s Webb Finds Planet-Forming Disks Lived Longer in Early Universe\t\t\t\t\t\t\t<\/h1>\n<\/div>\n<\/div>\n<div class=\"grid-col-12 tablet:grid-col-12 desktop:grid-col-5\"><\/div>\n<div class=\"skrim-overlay skrim-left mobile-skrim-top z-200\"><\/div>\n<figure class=\"hds-media-background  \"><img fetchpriority=\"high\" decoding=\"async\" width=\"1829\" height=\"2000\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1829&#038;h=2000&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"The center of the image contains arcs of orange and pink that form a boat-like shape. One end of these arcs points to the top right of the image, while the other end point toward the bottom left. Another plume of orange and pink expands from the center to the top left of the image. To the right of this plume is a large cluster of white stars. There are various other white stars and a few galaxies of different sizes spread throughout the image. Ten, small, yellow circles overlaid at various points across the image indicate the positions of the ten stars surveyed in this study.\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1829&#038;h=2000&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1829w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=274&#038;h=300&#038;fit=crop&#038;crop=faces%2Cfocalpoint 274w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=768&#038;h=840&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=936&#038;h=1024&#038;fit=crop&#038;crop=faces%2Cfocalpoint 936w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1405&#038;h=1536&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1405w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=366&#038;h=400&#038;fit=crop&#038;crop=faces%2Cfocalpoint 366w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=549&#038;h=600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 549w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=823&#038;h=900&#038;fit=crop&#038;crop=faces%2Cfocalpoint 823w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1097&#038;h=1200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1097w\" sizes=\"(max-width: 1829px) 100vw, 1829px\" loading=\"eager\"><\/figure>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"padding-y-3 padding-x-3\">\n<div class=\"grid-container grid-container-block padding-x-0\"><figcaption class=\"hds-caption maxw-mobile desktop:padding-x-3\">\n<div class=\"hds-caption-text p-sm margin-0 color-carbon-30\">\n<div><figcaption>This is a James Webb Space Telescope image of NGC 346, a massive star cluster in the Small Magellanic Cloud, a dwarf galaxy that is one of the Milky Way\u2019s nearest neighbors.<\/figcaption><\/div>\n<\/div>\n<div class=\"hds-credits color-spacesuit-white-important\">\n\t\t\t\t\t\t<span>Credits: <\/span><br \/>\n\t\t\t\t\t\t<span>NASA, ESA, CSA, STScI, Olivia C. Jones (UK ATC), Guido De Marchi (ESTEC), Margaret Meixner (USRA)<\/span>\n\t\t\t\t\t<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>NASA\u2019s James Webb Space Telescope just solved a conundrum by proving a controversial finding made with the agency\u2019s Hubble Space Telescope more than 20 years ago.<\/p>\n<p>In 2003, <a href=\"https:\/\/hubblesite.org\/contents\/news-releases\/2003\/news-2003-19.html\" target=\"_blank\" rel=\"noreferrer noopener\">Hubble provided evidence<\/a> of a massive planet around a very old star, almost as old as the universe. Such stars possess only small amounts of heavier elements that are the building blocks of planets. This implied that some planet formation happened when our universe was very young, and those planets had time to form and grow big inside their primordial disks, even bigger than Jupiter. But how? This was puzzling.<\/p>\n<p>To answer this question, researchers used Webb to study stars in a nearby galaxy that, much like the early universe, lacks large amounts of heavy elements. They found that not only do some stars there have planet-forming disks, but that those disks are longer-lived than those seen around young stars in our Milky Way galaxy.<\/p>\n<p>\u201cWith Webb, we have a really strong confirmation of what we saw with Hubble, and we must rethink how we model planet formation and early evolution in the young universe,\u201d said study leader Guido De Marchi of the European Space Research and Technology Centre in Noordwijk, Netherlands.<\/p>\n<h2 class=\"wp-block-heading\">Image A: Protoplanetary Disks in NGC 346 (NIRCam Image)<\/h2>\n<div class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-wide\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1829&#038;h=2000&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" width=\"1829\" height=\"2000\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1829&#038;h=2000&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"The center of the image contains arcs of orange and pink that form a boat-like shape. One end of these arcs points to the top right of the image, while the other end point toward the bottom left. Another plume of orange and pink expands from the center to the top left of the image. To the right of this plume is a large cluster of white stars. There are various other white stars and a few galaxies of different sizes spread throughout the image. Ten, small, yellow circles overlaid at various points across the image indicate the positions of the ten stars surveyed in this study.\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1829&#038;h=2000&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1829w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=274&#038;h=300&#038;fit=crop&#038;crop=faces%2Cfocalpoint 274w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=768&#038;h=840&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=936&#038;h=1024&#038;fit=crop&#038;crop=faces%2Cfocalpoint 936w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1405&#038;h=1536&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1405w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=366&#038;h=400&#038;fit=crop&#038;crop=faces%2Cfocalpoint 366w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=549&#038;h=600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 549w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=823&#038;h=900&#038;fit=crop&#038;crop=faces%2Cfocalpoint 823w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JC439JQCXEY252WM2K1QF6Q6-2K.jpg?w=1097&#038;h=1200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1097w\" sizes=\"auto, (max-width: 1829px) 100vw, 1829px\"><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">This is a James Webb Space Telescope image of NGC 346, a massive star cluster in the Small Magellanic Cloud, a dwarf galaxy that is one of the Milky Way\u2019s nearest neighbors. With its relative lack of elements heavier than hydrogen and helium, the NGC 346 cluster serves as a nearby proxy for studying stellar environments with similar conditions in the early, distant universe. Ten, small, yellow circles overlaid on the image indicate the positions of the ten stars surveyed in this study.<\/div>\n<div class=\"hds-credits\">NASA, ESA, CSA, STScI, Olivia C. Jones (UK ATC), Guido De Marchi (ESTEC), Margaret Meixner (USRA)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h2 class=\"wp-block-heading\">A Different Environment in Early Times<\/h2>\n<p>In the early universe, stars formed from mostly hydrogen and helium, and very few heavier elements such as carbon and iron, which came later through supernova explosions.<\/p>\n<p>\u201cCurrent models predict that with so few heavier elements, the disks around stars have a short lifetime, so short in fact that planets cannot grow big,\u201d said the Webb study\u2019s co-investigator Elena Sabbi, chief scientist for Gemini Observatory at the National Science Foundation\u2019s NOIRLab in Tucson. \u201cBut Hubble did see those planets, so what if the models were not correct and disks could live longer?\u201d<\/p>\n<p>To test this idea, scientists trained Webb on the Small Magellanic Cloud, a dwarf galaxy that is one of the Milky Way\u2019s nearest neighbors. In particular, they examined the massive, star-forming cluster NGC 346, which also has a relative lack of heavier elements. The cluster served as a nearby proxy for studying stellar environments with similar conditions in the early, distant universe.<\/p>\n<p>Hubble observations of NGC 346 from the mid 2000s revealed many stars about 20 to 30 million years old that seemed to still have planet-forming disks around them. This went against the conventional belief that such disks would dissipate after 2 or 3 million years.<\/p>\n<p>\u201cThe Hubble findings were controversial, going against not only empirical evidence in our galaxy but also against the current models,\u201d said De Marchi. \u201cThis was intriguing, but without a way to obtain <a href=\"https:\/\/webbtelescope.org\/glossary.html#h3-CK-b6199c5e-9065-4803-891c-6f17deada9a6\" target=\"_blank\" rel=\"noreferrer noopener\">spectra<\/a> of those stars, we could not really establish whether we were witnessing genuine accretion and the presence of disks, or just some artificial effects.\u201d<\/p>\n<p>Now, thanks to Webb\u2019s sensitivity and resolution, scientists have the first-ever spectra of forming, Sun-like stars and their immediate environments in a nearby galaxy.<\/p>\n<p>\u201cWe see that these stars are indeed surrounded by disks and are still in the process of gobbling material, even at the relatively old age of 20 or 30 million years,\u201d said De Marchi. \u201cThis also implies that planets have more time to form and grow around these stars than in nearby star-forming regions in our own galaxy.\u201d<\/p>\n<h2 class=\"wp-block-heading\">Image B: Protoplanetary Disks in NGC 346 Spectra (NIRSpec)<\/h2>\n<div class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-wide\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=1920&#038;h=1080&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" width=\"1920\" height=\"1080\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=1920&#038;h=1080&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"Graphic titled Star in NGC 346, Molecular Hydrogen in Protoplanetary Disk, NIRSpec Microshutter Array Spectroscopy showing brightness of 2.02- to 2.37-micron light of a star and its environment (plotted in yellow) and a star\u2019s environment only (plotted in pink) on an xy graph of brightness versus wavelength in microns. Two wavelength bands, ranging from 2.05 to 2.07 and 2.16 to 2.18, are highlighted in red and labeled Hot Atomic Helium, He. A band from 2.11 to 2.13 in blue is labeled Cold Molecular Hydrogen, H 2. The spectrum of the star plus environment (yellow) has prominent peaks at 2.06 and 2.17 microns (He), and at 2.12 microns (H). The spectrum of the star\u2019s environment only (pink) also has peaks at 2.06 and 2.17 microns (He), but not at 2.12 (H). The two spectra are offset vertically for readability. An inset shows them plotted with the same vertical alignment: the helium peaks on the star plus environment spectrum are slightly taller than those of the environment only.\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=1920&#038;h=1080&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1920w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=300&#038;h=169&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=768&#038;h=432&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=1024&#038;h=576&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=1536&#038;h=864&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=400&#038;h=225&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=600&#038;h=338&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=900&#038;h=506&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2024\/webb-STScI-01JBCNRXJDAT3CJ208E54PQ45B-2K.jpg?w=1200&#038;h=675&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w\" sizes=\"auto, (max-width: 1920px) 100vw, 1920px\"><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">This graph shows, on the bottom left in yellow, a spectrum of one of the 10 target stars in this study (as well as accompanying light from the immediate background environment). Spectral fingerprints of hot atomic helium, cold molecular hydrogen, and hot atomic hydrogen are highlighted. On the top left in magenta is a spectrum slightly offset from the star that includes only light from the background environment. This second spectrum lacks a spectral line of cold molecular hydrogen.  <br \/>On the right is the comparison of the top and bottom lines. This comparison shows a large peak in the cold molecular hydrogen coming from the star but not its nebular environment. Also, atomic hydrogen shows a larger peak from the star. This indicates the presence of a protoplanetary disk immediately surrounding the star. The data was taken with the microshutter array on the James Webb Space Telescope\u2019s NIRSpec (Near-Infrared Spectrometer) instrument.<\/div>\n<div class=\"hds-credits\">Illustration: NASA, ESA, CSA, Joseph Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h2 class=\"wp-block-heading\">A New Way of Thinking<\/h2>\n<p>This finding refutes previous theoretical predictions that when there are very few heavier elements in the gas around the disk, the star would very quickly blow away the disk. So the disk\u2019s life would be very short, even less than a million years. But if a disk doesn\u2019t stay around the star long enough for the dust grains to stick together and pebbles to form and become the core of a planet, how can planets form?<\/p>\n<p>The researchers explained that there could be two distinct mechanisms, or even a combination, for planet-forming disks to persist in environments scarce in heavier elements.<\/p>\n<p>First, to be able to blow away the disk, the star applies radiation pressure. For this pressure to be effective, elements heavier than hydrogen and helium would have to reside in the gas. But the massive star cluster NGC 346 only has about ten percent of the heavier elements that are present in the chemical composition of our Sun. Perhaps it simply takes longer for a star in this cluster to disperse its disk.<\/p>\n<p>The second possibility is that, for a Sun-like star to form when there are few heavier elements, it would have to start from a larger cloud of gas. A bigger gas cloud will produce a bigger disk. So there is more mass in the disk and therefore it would take longer to blow the disk away, even if the radiation pressure were working in the same way.<\/p>\n<p>\u201cWith more matter around the stars, the accretion lasts for a longer time,\u201d said Sabbi. \u201cThe disks take ten times longer to disappear. This has implications for how you form a planet, and the type of system architecture that you can have in these different environments. This is so exciting.\u201d<\/p>\n<p>The science team\u2019s paper appears in the Dec. 16 issue of The Astrophysical Journal.<\/p>\n<h2 class=\"wp-block-heading\">Image C: NGC 346: Hubble and Webb Observations<\/h2>\n<div class=\" hds-module hds-module-full wp-block-nasa-blocks-image-before-after\">\n<div>\n        Image Before\/After\n    <\/div>\n<\/div>\n<p><em>The James Webb Space Telescope is the world\u2019s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).<\/em><\/p>\n<p><em>The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA\u2019s Goddard Space Flight Center in Greenbelt manages the telescope and mission operations. Lockheed Martin Space, based in Denver also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.<\/em><\/p>\n<h2 class=\"wp-block-heading\">Downloads<\/h2>\n<p><strong>Right click any image to save it or open a larger version<\/strong> in a new tab\/window via the browser\u2019s popup menu.<\/p>\n<p><strong><a href=\"https:\/\/webbtelescope.org\/contents\/news-releases\/2024\/news-2024-135#section-id-2\" target=\"_blank\" rel=\"noreferrer noopener\">View\/Download all image products at all resolutions<\/a><\/strong> for this article from the Space Telescope Science Institute.<\/p>\n<p><strong>View\/Download the science paper<\/strong>\u00a0from the <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/ad7a63\" target=\"_blank\" rel=\"noreferrer noopener\">The Astrophysical Journal<\/a>.<\/p>\n<h2 class=\"wp-block-heading\">Media Contacts<\/h2>\n<p><strong>Laura\u00a0Betz<\/strong>\u00a0\u2013\u00a0<a href=\"mailto:laura.e.betz@nasa.gov\">laura.e.betz@nasa.gov<\/a><br \/>NASA\u2019s <a href=\"http:\/\/www.nasa.gov\/goddard\" target=\"_blank\" rel=\"noreferrer noopener\">Goddard Space Flight Center<\/a>, Greenbelt, Md.<\/p>\n<p><strong>Ann Jenkins<\/strong> \u2013 <a href=\"mailto:jenkins@stsci.edu\">jenkins@stsci.edu<\/a>, <strong>Christine Pulliam<\/strong> \u2013 <a href=\"mailto:cpulliam@stsci.edu\">cpulliam@stsci.edu<\/a><br \/><a href=\"https:\/\/www.stsci.edu\/\" target=\"_blank\" rel=\"noreferrer noopener\">Space Telescope Science Institute<\/a>, Baltimore, Md.<\/p>\n<h2 class=\"wp-block-heading\">Related Information<\/h2>\n<p><strong>Past releases on NGC 346:<\/strong> Webb <a href=\"https:\/\/www.nasa.gov\/universe\/nasas-webb-uncovers-star-formation-in-clusters-dusty-ribbons\/\">NIRCam image<\/a> and <a href=\"https:\/\/www.nasa.gov\/general\/nasas-webb-captures-an-ethereal-view-of-ngc-346\/\">MIRI image<\/a><\/p>\n<p><strong>Article:<\/strong> Highlighting other <a href=\"https:\/\/webbtelescope.org\/contents\/articles\/webbs-star-formation-discoveries\" target=\"_blank\" rel=\"noreferrer noopener\">Webb Star Formation Discoveries<\/a><\/p>\n<p><strong>Simulation Video:<\/strong> <a href=\"https:\/\/svs.gsfc.nasa.gov\/10662\/\" target=\"_blank\" rel=\"noreferrer noopener\">Planetary Systems and Origins of Life<\/a><\/p>\n<p><strong>Animation Video:<\/strong> <a href=\"https:\/\/webbtelescope.org\/contents\/media\/videos\/01G6X2C9R0TPVCHXSRBCEVNW03\" target=\"_blank\" rel=\"noreferrer noopener\">Exploring star and planet formation<\/a> (English), and in <a href=\"https:\/\/webbtelescope.org\/contents\/media\/videos\/01H6SK6NZ8SZVPXM93ERH2RGGW\" target=\"_blank\" rel=\"noreferrer noopener\">Spanish<\/a><\/p>\n<p><a href=\"https:\/\/www.astropix.org\/search?q=ngc+346\" target=\"_blank\" rel=\"noreferrer noopener\">More Images of NGC 346 on AstroPix<\/a><\/p>\n<p><strong><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/latestnews\/\" rel=\"noopener\">More Webb News<\/a><\/strong><\/p>\n<p><strong><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/multimedia\/images\/\" rel=\"noopener\">More Webb Images<\/a><\/strong><\/p>\n<p><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/science-overview\/\" rel=\"noopener\"><strong>Webb Science Themes<\/strong><\/a><\/p>\n<p><strong><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/\" rel=\"noopener\">Webb Mission Page<\/a><\/strong> <\/p>\n<h2 class=\"wp-block-heading\">Related For Kids<\/h2>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/planet-what-is\/en\/\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>What is a planet?<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/james-webb-space-telescope\/en\/\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>What is the Webb Telescope?<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>SpacePlace for Kids<\/strong><\/a><\/p>\n<h2 class=\"wp-block-heading\">En Espa\u00f1ol<\/h2>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/galaxy\/sp\/\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>\u00bfQu\u00e9 es un planeta?<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/ciencia.nasa.gov\/\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>Ciencia de la NASA<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/www.nasa.gov\/es\/\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>NASA en espa\u00f1ol\u00a0<\/strong><\/a><\/p>\n<p><a href=\"https:\/\/spaceplace.nasa.gov\/sp\/\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>Space Place\u00a0para ni\u00f1os<\/strong><\/a><\/p>\n<div class=\"hds-topic-cards nasa-gb-align-full maxw-full width-full padding-y-6 padding-x-3 color-mode-dark hds-module hds-module-full wp-block-nasa-blocks-topic-cards\">\n<div class=\"grid-container grid-container-block-lg padding-x-0\">\n<div class=\"grid-row flex-align-center margin-bottom-3\">\n<div class=\"desktop:grid-col-8 margin-bottom-2 desktop:margin-bottom-0\">\n<div class=\"label color-carbon-60 margin-bottom-2\">Keep Exploring<\/div>\n<h2 class=\"heading-36 line-height-sm\">Related Topics<\/h2>\n<\/div>\n<\/div>\n<div class=\"grid-row grid-gap-2 hds-topic-cards-wrapper\">\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/james-webb-space-telescope\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<h3 class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>James Webb Space Telescope<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewbox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg><br \/>\n\t\t\t\t\t\t\t<\/h3>\n<p class=\"margin-bottom-0 margin-top-2 color-carbon-20-important\">Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the\u2026<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1536\" height=\"890\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" block_context=\"nasa-block\" srcset=\"https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp 3600w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=300,174 300w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=768,445 768w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1024,593 1024w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1536,890 1536w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=2048,1186 2048w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=400,232 400w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=600,348 600w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=900,521 900w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1200,695 1200w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=2000,1158 2000w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\"><\/figure>\n<\/div>\n<p><\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/universe\/stars\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<p class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Stars<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewbox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1536\" height=\"864\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" block_context=\"nasa-block\" srcset=\"https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp 1920w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=300,169 300w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=768,432 768w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=1024,576 1024w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=1536,864 1536w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=400,225 400w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=600,338 600w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=900,506 900w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp?resize=1200,675 1200w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\"><\/figure>\n<\/div>\n<p><\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/universe\/galaxies\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<p class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Galaxies<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewbox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"938\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp?w=1200\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" block_context=\"nasa-block\" srcset=\"https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp 1200w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp?resize=300,235 300w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp?resize=768,600 768w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp?resize=1024,800 1024w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp?resize=400,313 400w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp?resize=600,469 600w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp?resize=900,704 900w\" sizes=\"auto, (max-width: 1200px) 100vw, 1200px\"><\/figure>\n<\/div>\n<p><\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/universe\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<p class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Universe<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewbox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img loading=\"lazy\" decoding=\"async\" width=\"1536\" height=\"1514\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" block_context=\"nasa-block\" srcset=\"https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg 3941w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=300,296 300w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=768,757 768w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=1024,1009 1024w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=1536,1514 1536w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=2048,2019 2048w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=50,50 50w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=100,100 100w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=400,394 400w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=600,591 600w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=900,887 900w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=1200,1183 1200w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/09\/ngc5068-1-flat-final.jpg?resize=2000,1972 2000w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\"><\/figure>\n<\/div>\n<p><\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\n<div class=\"nasa-gb-align-full width-full maxw-full padding-x-3 padding-y-0 article_a hds-module hds-module-full wp-block-nasa-blocks-credits-and-details\">\n<section class=\"padding-x-0 padding-top-5 padding-bottom-2 desktop:padding-top-7 desktop:padding-bottom-9\">\n<div class=\"grid-row grid-container maxw-widescreen padding-0\">\n<div class=\"grid-col-12 desktop:grid-col-2 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div class=\"padding-top-3 border-top-1px border-color-carbon-black\">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-14\">Share<\/h2>\n<\/div>\n<div class=\"padding-bottom-2\">\n<ul class=\"social-icons social-icons-round\">\n<li class=\"social-icon social-icon-x\">\n\t\t\t\t\t\t\t<a href=\"https:\/\/x.com\/intent\/tweet?via=NASA&#038;text=NASA%E2%80%99s%20Webb%20Finds%20Planet-Forming%20Disks%20Lived%20Longer%20in%20Early%20Universe&#038;url=https%3A%2F%2Fscience.nasa.gov%2Fmissions%2Fwebb%2Fnasas-webb-finds-planet-forming-disks-lived-longer-in-early-universe%2F\" aria-label=\"Share on X.\"><br \/>\n\t\t\t\t\t\t\t\t<svg width=\"1200\" height=\"1227\" viewbox=\"0 0 1200 1227\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><path d=\"M714.163 519.284L1160.89 0H1055.03L667.137 450.887L357.328 0H0L468.492 681.821L0 1226.37H105.866L515.491 750.218L842.672 1226.37H1200L714.137 519.284H714.163ZM569.165 687.828L521.697 619.934L144.011 79.6944H306.615L611.412 515.685L658.88 583.579L1055.08 1150.3H892.476L569.165 687.854V687.828Z\" fill=\"white\"><\/path><\/svg><br \/>\n\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t<\/li>\n<li class=\"social-icon social-icon-facebook\">\n\t\t\t\t\t\t\t<a href=\"https:\/\/www.facebook.com\/sharer.php?u=https%3A%2F%2Fscience.nasa.gov%2Fmissions%2Fwebb%2Fnasas-webb-finds-planet-forming-disks-lived-longer-in-early-universe%2F\" aria-label=\"Share on Facebook.\" rel=\"noopener\"><br \/>\n\t\t\t\t\t\t\t\t<svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewbox=\"0 0 24 24\" aria-hidden=\"true\"><path d=\"M9 8h-3v4h3v12h5v-12h3.642l.358-4h-4v-1.667c0-.955.192-1.333 1.115-1.333h2.885v-5h-3.808c-3.596 0-5.192 1.583-5.192 4.615v3.385z\"><\/path><\/svg><br \/>\n\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t<\/li>\n<li class=\"social-icon social-icon-linkedin\">\n\t\t\t\t\t\t\t<a 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345zm71 0c0-228-188-416-416-416V132c285 0 520 235 520 520z\"><\/path><circle cx=\"219\" cy=\"581\" r=\"71\"><\/circle><\/svg><br \/>\n\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"grid-col-12 desktop:grid-col-5 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div class=\"padding-top-3 border-top-1px border-color-carbon-black\">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-14\">Details<\/h2>\n<\/div>\n<div class=\"grid-row margin-bottom-3\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Last Updated<\/div>\n<\/div>\n<div class=\"grid-col-8\">Dec 15, 2024<\/div>\n<\/div>\n<div class=\"grid-row margin-bottom-3\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Editor<\/div>\n<\/div>\n<div class=\"grid-col-8\">Marty McCoy<\/div>\n<\/div>\n<div class=\"grid-row margin-bottom-3\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Contact<\/div>\n<\/div>\n<div class=\"grid-col-8\">\n<div class=\"margin-bottom-3\">\n<div>Laura Betz<\/div>\n<div><a href=\"mailto:laura.e.betz@nasa.gov\">laura.e.betz@nasa.gov<\/a><\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"grid-col-12 desktop:grid-col-5 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div class=\"padding-top-3 border-top-1px border-color-carbon-black \">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-14\">Related Terms<\/h2>\n<\/div>\n<ul class=\"article-tags\">\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/astrophysics\/\" rel=\"noopener\">Astrophysics<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/galaxies\/\" rel=\"noopener\">Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/science-research\/astrophysics\/galaxies-stars-black-holes\/\" rel=\"noopener\">Galaxies, Stars, &#038; Black Holes<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/www.nasa.gov\/goddard\/\">Goddard Space Flight Center<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/mission\/webb\" rel=\"noopener\">James Webb Space Telescope (JWST)<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/\" rel=\"noopener\">Science &#038; Research<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/stars\/\" rel=\"noopener\">Stars<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/\" rel=\"noopener\">The Universe<\/a><\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<p class=\"wpematico_credit\"><small>Powered by <a href=\"http:\/\/www.wpematico.com\" target=\"_blank\">WPeMatico<\/a><\/small><\/p>\n<p><a  href=\"https:\/\/science.nasa.gov\/missions\/webb\/nasas-webb-finds-planet-forming-disks-lived-longer-in-early-universe\/\"  target=\"_blank\" rel=\"noopener\">Get The Details&#8230;<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>NASA\u2019s James Webb Space Telescope just solved a conundrum by proving a controversial finding made with the agency\u2019s Hubble Space Telescope more than 20 years ago. In 2003, Hubble provided evidence of a massive planet around a very old star, almost as old as the universe. 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