{"id":14936,"date":"2026-01-26T12:02:02","date_gmt":"2026-01-26T16:02:02","guid":{"rendered":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/nasa-reveals-new-details-about-dark-matters-influence-on-universe\/"},"modified":"2026-01-26T12:02:02","modified_gmt":"2026-01-26T16:02:02","slug":"nasa-reveals-new-details-about-dark-matters-influence-on-universe","status":"publish","type":"post","link":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/nasa-reveals-new-details-about-dark-matters-influence-on-universe\/","title":{"rendered":"NASA Reveals New Details About Dark Matter\u2019s Influence on Universe"},"content":{"rendered":"<h2 style=\"text-align: center;\">NASA Reveals New Details About Dark Matter\u2019s Influence on Universe<\/h2>\n<p><!-- no image --><\/p>\n<div class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\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:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png\"><img fetchpriority=\"high\" decoding=\"async\" width=\"1839\" height=\"2048\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?w=1839\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"\" block_context=\"nasa-block\" loading=\"eager\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png 5285w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=269,300 269w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=768,855 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=920,1024 920w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=1379,1536 1379w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=1839,2048 1839w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=359,400 359w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=539,600 539w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=808,900 808w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=1078,1200 1078w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/1-pia26702.png?resize=1796,2000 1796w\" sizes=\"auto, (max-width: 1839px) 100vw, 1839px\"><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Containing nearly 800,000 galaxies, this image from NASA\u2019s James Webb Space Telescope is overlaid with a map of dark matter, represented in blue. Researchers used Webb data to find the invisible substance via its gravitational influence on regular matter.<\/div>\n<div class=\"hds-credits\">NASA\/STScI\/J. DePasquale\/A. Pagan<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p><em>With the Webb telescope\u2019s unprecedented sensitivity, scientists are learning more about dark matter\u2019s influence on stars, galaxies, and even planets like Earth.<\/em><\/p>\n<p>Scientists using data from NASA\u2019s James Webb Space Telescope have made one of the most detailed, high-resolution maps of dark matter ever produced. It shows how the invisible, ghostly material overlaps and intertwines with \u201cregular\u201d matter, the stuff that makes up stars, galaxies, and everything we can see.<\/p>\n<p>Published Monday, Jan. 26, in Nature Astronomy, the map builds on previous research to provide additional confirmation and new details about how dark matter has shaped the universe on the largest scales \u2014 galaxy clusters millions of light-years across \u2014 that ultimately give rise to galaxies, stars, and planets like Earth.<\/p>\n<p>\u201cThis is the largest dark matter map we\u2019ve made with <a href=\"https:\/\/science.nasa.gov\/mission\/webb\/\" rel=\"noopener\">Webb<\/a>, and it\u2019s twice as sharp as any dark matter map made by other observatories,\u201d said Diana Scognamiglio, lead author of the paper and an astrophysicist at NASA\u2019s Jet Propulsion Laboratory in Southern California. \u201cPreviously, we were looking at a blurry picture of dark matter. Now we\u2019re seeing the invisible scaffolding of the universe in stunning detail, thanks to Webb\u2019s incredible resolution.\u201d<\/p>\n<div class=\"hds-image-carousel grid-container grid-container-block padding-top-4 padding-bottom-4 hds-module hds-module-full alignfull wp-block-nasa-blocks-image-carousel\">\n<div class=\"hds-carousel-wrapper\">\n<div class=\"image-carousel-slider margin-0\" data-client-id=\"carousel-69778ff866d3f\" data-variation=\"carousel\" data-autoplay=\"\" data-autoplay-speed=\"2000\" data-play-pause=\"\" data-transition-type=\"slide\" data-progress=\"\" data-progress-labels=\"\" data-start-label=\"Start\" data-end-label=\"End\" data-labels-initialized=\"true\">\n<div class=\"display-block width-full\" data-label=\"\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"1024\" height=\"576\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?w=1024\" class=\"attachment-large size-large\" alt=\"\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg 4000w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=300,169 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=768,432 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=1024,576 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=1536,864 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=2048,1152 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=400,225 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=600,338 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=900,506 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=1200,675 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1a-pia26703-new.jpg?resize=2000,1125 2000w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\"><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Created using data from NASA\u2019s Webb telescope in 2026 (right) and from the Hubble Space Telescope in 2007 (left), these images show the presence of dark matter in the same region of sky. Webb\u2019s higher resolution is providing new insights into how this invisible component influences the distribution of ordinary matter in the universe.<\/div>\n<div class=\"hds-credits\">NASA\/STScI\/A. Pagan<\/div>\n<\/figcaption><\/div>\n<\/p><\/div>\n<\/figure><\/div>\n<div class=\"display-block width-full\" data-label=\"\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"1024\" height=\"576\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?w=1024\" class=\"attachment-large size-large\" alt=\"\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg 4000w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=300,169 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=768,432 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=1024,576 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=1536,864 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=2048,1152 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=400,225 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=600,338 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=900,506 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=1200,675 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1b-pia26703-new.jpg?resize=2000,1125 2000w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\"><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Dense regions of dark matter are connected by lower-density filaments, forming a weblike structure known as the cosmic web. This pattern appears more clearly in the Webb data than in the earlier Hubble image. Ordinary matter, including galaxies, tends to trace this same underlying structure shaped by dark matter.<\/div>\n<div class=\"hds-credits\">NASA\/STScI\/A. Pagan<\/div>\n<\/figcaption><\/div>\n<\/p><\/div>\n<\/figure><\/div>\n<div class=\"display-block width-full\" data-label=\"\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"1024\" height=\"576\" src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?w=1024\" class=\"attachment-large size-large\" alt=\"\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg 4000w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=300,169 300w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=768,432 768w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=1024,576 1024w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=1536,864 1536w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=2048,1152 2048w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=400,225 400w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=600,338 600w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=900,506 900w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=1200,675 1200w, https:\/\/www.nasa.gov\/wp-content\/uploads\/2026\/01\/e1c-pia26703-new.jpg?resize=2000,1125 2000w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\"><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Some dark matter structures appear smaller in the Webb data because they are coming into sharper focus. Webb\u2019s higher resolution also makes it possible to better confine the size and location of the dark matter clusters in the lower left of the image.<\/div>\n<div class=\"hds-credits\">NASA\/STScI\/A. Pagan<\/div>\n<\/figcaption><\/div>\n<\/p><\/div>\n<\/figure><\/div>\n<\/p><\/div>\n<div class=\"hds-carousel-nav display-flex margin-left-auto margin-right-0\" data-carousel-id=\"image-carousel-slider-carousel-69778ff866d3f\">\n\t\t\t\t<button class=\"hds-carousel-nav-arrow hds-carousel-arrow-prev\"><br \/>\n\t\t\t\t\t<svg version=\"1.1\" x=\"0px\" y=\"0px\" width=\"9px\" height=\"9px\" viewbox=\"0 0 9 9\"><path class=\"st0\" d=\"M3.5,4.5l3.7-3.6L6.3,0L1.8,4.5L6.3,9l0.9-0.9L3.5,4.5z\"><\/path><\/svg><br \/>\n\t\t\t\t<\/button><br \/>\n\t\t\t\t\t\t\t<button class=\"hds-carousel-nav-arrow hds-carousel-arrow-next margin-right-0\"><br \/>\n\t\t\t\t\t<svg version=\"1.1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" x=\"0px\" y=\"0px\" width=\"9px\" height=\"9px\" viewbox=\"0 0 9 9\"><path class=\"st0\" d=\"M5.5,4.5L1.8,8.1L2.7,9l4.5-4.5L2.7,0L1.8,0.9L5.5,4.5z\"><\/path><\/svg><br \/>\n\t\t\t\t<\/button>\n\t\t\t<\/div>\n<\/p><\/div>\n<\/p><\/div>\n<p>Dark matter doesn\u2019t emit, reflect, absorb, or even block light, and it passes through regular matter like a ghost. But it does interact with the universe through gravity, something the map shows with a new level of clarity. Evidence for this interaction lies in the degree of overlap between dark matter and regular matter. According to the paper\u2019s authors, Webb\u2019s observations confirm that this close alignment can\u2019t be a coincidence but, rather, is due to dark matter\u2019s gravity pulling regular matter toward it throughout cosmic history.<\/p>\n<p>\u201cWherever we see a big cluster of thousands of galaxies, we also see an equally massive amount of dark matter in the same place. And when we see a thin string of regular matter connecting two of those clusters, we see a string of dark matter as well,\u201d said Richard Massey, an astrophysicist at Durham University in the United Kingdom and a coauthor of the new study. \u201cIt\u2019s not just that they have the same shapes. This map shows us that dark matter and regular matter have always been in the same place. They grew up together.\u201d<\/p>\n<h3 class=\"wp-block-heading\"><strong>Closer look<\/strong><\/h3>\n<p>Found in the constellation Sextans, the area covered by the new map is a section of sky about 2.5 times larger than the full Moon. A global community of scientists have observed this region with at least 15 ground- and space-based telescopes for the Cosmic Evolution Survey (COSMOS). Their goal: to precisely measure the location of regular matter here and then compare it to the location of dark matter. The first dark matter map of the area was made in 2007 using data from NASA\u2019s <a href=\"https:\/\/science.nasa.gov\/mission\/hubble\/\" rel=\"noopener\">Hubble Space Telescope<\/a>, a project led by Massey and JPL astrophysicist Jason Rhodes, a coauthor of the paper.<\/p>\n<p>Webb peered at this region for a total of about 255 hours and identified nearly 800,000 galaxies, some of which were detected for the first time. Scognamiglio and her colleagues then looked for dark matter by observing how its mass curves space itself, which in turn bends the light traveling to Earth from distant galaxies. When observed by researchers, it\u2019s as if the light of those galaxies has passed through a warped windowpane.<\/p>\n<p>The Webb map contains about 10 times more galaxies than maps of the area made by ground-based observatories and twice as many as Hubble\u2019s. It reveals new clumps of dark matter and captures a higher-resolution view of the areas previously seen by Hubble.<\/p>\n<p><a>To refine measurements of the distance to many galaxies for the map, the team used Webb\u2019s Mid-Infrared Instrument (<\/a><a href=\"https:\/\/www.jpl.nasa.gov\/missions\/mid-infrared-instrument-miri\/\" rel=\"noopener\">MIRI<\/a>), designed and managed through launch by JPL, along with other space- and ground-based telescopes. The wavelengths that MIRI detects also make it adept at detecting galaxies obscured by cosmic dust clouds.<\/p>\n<h3 class=\"wp-block-heading\"><strong>Why it matters<\/strong><\/h3>\n<p>When the universe began, regular matter and dark matter were probably sparsely distributed. Scientists think dark matter began to clump together first and that those dark matter clumps then pulled together regular matter, creating regions with enough material for stars and galaxies to begin to form.<\/p>\n<p>In this way, dark matter determined the large-scale distribution of galaxies in the universe. And by prompting galaxy and star formation to begin earlier than they would have otherwise, dark matter\u2019s influence also played a role in creating the conditions for planets to eventually form. That\u2019s because the first generations of stars were responsible for turning hydrogen and helium \u2014 which made up the vast majority of atoms in the early universe \u2014 into the rich array of elements that now compose planets like Earth. In other words, dark matter provided more time for complex planets to form.<\/p>\n<p>\u201cThis map provides stronger evidence that without dark matter, we might not have the elements in our galaxy that allowed life to appear,\u201d said Rhodes. \u201cDark matter is not something we encounter in our everyday life on Earth, or even in our solar system, but it has definitely influenced us.\u201d<\/p>\n<p>Scognamiglio and some of her coauthors will also map dark matter with NASA\u2019s upcoming <a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/\" rel=\"noopener\">Nancy Grace Roman Space Telescope<\/a> over an area 4,400 times bigger than the COSMOS region. Roman\u2019s primary science goals include learning more about dark matter\u2019s fundamental properties and how they may or may not have changed over cosmic history. But Roman\u2019s maps won\u2019t beat Webb\u2019s spatial resolution. More detailed looks at dark matter will be possible only with a next-generation telescope like the Habitable Worlds Observatory, NASA\u2019s next astrophysics flagship concept.<\/p>\n<h3 class=\"wp-block-heading\"><strong>More about Webb<\/strong><\/h3>\n<p>The James Webb Space Telescope 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).<\/p>\n<p>To learn more about Webb, visit:<\/p>\n<p><a href=\"https:\/\/science.nasa.gov\/mission\/webb\/\" rel=\"noopener\"><strong>https:\/\/science.nasa.gov\/webb<\/strong><\/a><\/p>\n<h3 class=\"wp-block-heading\"><strong>Media Contacts<\/strong><\/h3>\n<p>Calla Cofield \/ Ian O\u2019Neill<br \/>Jet Propulsion Laboratory, Pasadena, Calif.<br \/>626-808-2469 \/ 818-354-2649<br \/>calla.e.cofield@jpl.nasa.gov \/ ian.j.oneill@jpl.nasa.gov<\/p>\n<p>2026-002<\/p>\n<div class=\"nasa-gb-align-full width-full maxw-full padding-x-3 padding-y-0 hds-module hds-module-full alignfull wp-block-nasa-blocks-related-articles\">\n<section class=\"hds-related-articles padding-x-0 padding-y-3 desktop:padding-top-7 desktop:padding-bottom-9\">\n<div class=\"w-100 grid-row grid-container maxw-widescreen padding-0 text-align-left\">\n<div class=\"margin-bottom-4\">\n<h2 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\/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t3 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/learning-resources\/science-activation\/nasas-universe-of-learning-unveils-fresh-facilitator-guides-inspired-by-community-feedback\/\" class=\"color-carbon-black\" rel=\"noopener\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" loading=\"lazy\" alt=\"\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/cds\/learn\/science-activation-stories\/2026\/UOL_Program_Guides_Webpage_TimothyRhueII.png\"><\/figure>\n<\/p><\/div>\n<\/p><\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">3 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA\u2019s Universe of Learning Unveils Fresh Facilitator Guides Inspired by Community Feedback<\/h3>\n<\/div>\n<p class=\"p-md color-carbon-60\">The goal of NASA\u2019s Universe of Learning (UoL) is to connect the public to the\u2026<\/p>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewbox=\"0 0 16 16\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"><\/path><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"><\/path><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t5 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/missions\/webb\/nasa-webb-finds-young-sun-like-star-forging-spewing-common-crystals\/\" class=\"color-carbon-black\" rel=\"noopener\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" loading=\"lazy\" alt=\"\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2026\/01\/STScI-01KESWN3G28KZCQPZ2GHHDKAC3.png\"><\/figure>\n<\/p><\/div>\n<\/p><\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">5 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA Webb Finds Young Sun-Like Star Forging, Spewing Common Crystals<\/h3>\n<\/div>\n<p class=\"p-md color-carbon-60\">Astronomers have long sought evidence to explain why comets at the outskirts of our own\u2026<\/p>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewbox=\"0 0 16 16\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"><\/path><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"><\/path><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t5 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p><\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<\/p><\/div>\n<\/section><\/div>\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 alignfull 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\">Discover More Topics From NASA<\/h2>\n<\/p><\/div>\n<\/p><\/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<\/p><\/div>\n<\/p><\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" loading=\"lazy\" alt=\"\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp\"><\/figure>\n<\/p><\/div>\n<p>\t\t\t<\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/mission\/roman-space-telescope\/dark-matter\/\" 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>Dark Matter<\/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\">Scientists first suspected dark matter\u2019s existence over 80 years ago when Swiss-American astronomer Fritz Zwicky observed that galaxies in the\u2026<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" loading=\"lazy\" alt=\"\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/10\/darkmatter.jpg\"><\/figure>\n<\/p><\/div>\n<p>\t\t\t<\/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<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>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><br \/>\n\t\t\t\t\t\t\t<\/h3>\n<p class=\"margin-bottom-0 margin-top-2 color-carbon-20-important\">Astronomers estimate that the universe could contain up to one septillion stars \u2013 that\u2019s a one followed by 24 zeros.\u2026<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" loading=\"lazy\" alt=\"\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/may102022-x1pt5flare-171-131-304-jpg.webp\"><\/figure>\n<\/p><\/div>\n<p>\t\t\t<\/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<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>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><br \/>\n\t\t\t\t\t\t\t<\/h3>\n<p class=\"margin-bottom-0 margin-top-2 color-carbon-20-important\">Galaxies consist of stars, planets, and vast clouds of gas and dust, all bound together by gravity. The largest contain\u2026<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" loading=\"lazy\" alt=\"\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/spiral-galaxy-jpg.webp\"><\/figure>\n<\/p><\/div>\n<p>\t\t\t<\/a>\n\t\t\t\t<\/div>\n<\/p><\/div>\n<\/p><\/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:\/\/www.nasa.gov\/missions\/webb\/nasa-reveals-new-details-about-dark-matters-influence-on-universe\/\"  target=\"_blank\" rel=\"noopener\">Get The Details&#8230;<\/a><br \/>\nNaomi Hartono  <\/p>\n","protected":false},"excerpt":{"rendered":"<p>With the Webb telescope\u2019s unprecedented sensitivity, scientists are learning more about dark matter\u2019s influence on stars, galaxies, and even planets like Earth. Scientists using data from NASA\u2019s James Webb Space Telescope have made one of the most detailed, high-resolution maps of dark matter ever produced. 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