{"id":12883,"date":"2025-01-13T18:02:28","date_gmt":"2025-01-13T22:02:28","guid":{"rendered":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/webb-watches-carbon-rich-dust-shells-form-expand-in-star-system\/"},"modified":"2025-01-13T18:02:28","modified_gmt":"2025-01-13T22:02:28","slug":"webb-watches-carbon-rich-dust-shells-form-expand-in-star-system","status":"publish","type":"post","link":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/webb-watches-carbon-rich-dust-shells-form-expand-in-star-system\/","title":{"rendered":"Webb Watches Carbon-Rich Dust Shells Form, Expand in Star System"},"content":{"rendered":"<h2 style=\"text-align: center;\">Webb Watches Carbon-Rich Dust Shells Form, Expand in Star System<\/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 width-full border-bottom-1px 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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\">6 Min Read<\/div>\n<h1 class=\"heading-41 line-height-md color-spacesuit-white-important\">\n\t\t\t\t\t\t\t\tWebb Watches Carbon-Rich Dust Shells Form, Expand in Star System\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 loading=\"lazy\" decoding=\"async\" width=\"400\" height=\"400\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAKG1DSKTAJ2EKCDE6XBN9-1K.jpg?w=400&#038;h=400&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"A portion of Webb\u2019s 2023 observation of Wolf-Rayet 140. A bright white hexagon is toward the bottom left-center. This is the two stars. Blue diffraction spikes point diagonally toward 8, 11, and 1 o\u2019clock. Surrounding the central light are a series of regularly spaced rings. A segment of each of the rings at around 2 o\u2019clock appears brighter. These bright patches form a line that travels to the upper right. A few blue background dots are on the black background of space.\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAKG1DSKTAJ2EKCDE6XBN9-1K.jpg?w=400&#038;h=400&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAKG1DSKTAJ2EKCDE6XBN9-1K.jpg?w=150&#038;h=150&#038;fit=crop&#038;crop=faces%2Cfocalpoint 150w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAKG1DSKTAJ2EKCDE6XBN9-1K.jpg?w=300&#038;h=300&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAKG1DSKTAJ2EKCDE6XBN9-1K.jpg?w=50&#038;h=50&#038;fit=crop&#038;crop=faces%2Cfocalpoint 50w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAKG1DSKTAJ2EKCDE6XBN9-1K.jpg?w=100&#038;h=100&#038;fit=crop&#038;crop=faces%2Cfocalpoint 100w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAKG1DSKTAJ2EKCDE6XBN9-1K.jpg?w=200&#038;h=200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 200w\" sizes=\"auto, (max-width: 400px) 100vw, 400px\"><\/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>A portion of Webb\u2019s 2023 observation of Wolf-Rayet 140.<\/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>Image: NASA, ESA, CSA, STScI; Science: Emma Lieb (University of Denver), Ryan Lau (NSF NOIRLab), Jennifer Hoffman (University of Denver)<\/span>\n\t\t\t\t\t<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>Astronomers have long tried to track down how elements like carbon, which is essential for life, become widely distributed across the universe. Now, NASA\u2019s James Webb Space Telescope has examined one ongoing source of carbon-rich dust in our own Milky Way galaxy in greater detail: Wolf-Rayet 140, a system of two massive stars that follow a tight, elongated orbit.<\/p>\n<p>As they swing past one another (within the central white dot in the Webb images), the stellar winds from each star slam together, the material compresses, and carbon-rich dust forms. Webb\u2019s latest observations show 17 dust shells shining in mid-infrared light that are expanding at regular intervals into the surrounding space.<\/p>\n<h2 class=\"wp-block-heading\">Image A: Compare Observations of Wolf-Rayet 140 (MIRI Images)<\/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\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=400&#038;h=400&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" width=\"400\" height=\"400\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=400&#038;h=400&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"A three-part graphic. The left and center images show two observations of Wolf-Rayet 140, from July 2022 at left and from September 2023 at center. Both show a bright white point of light surrounded by 17 regularly spaced, hazy dust shells at the bottom, right, and upper right. The panels each have an outline of a square overlaid toward the top right, which has a brighter white outline of a triangle. At left, the triangle points up and is labeled a. At right, the triangle points down and is labeled b. The third panel at right shows a magnified version of the areas outlined in the left and center panels. There are two labels. At top left, a, and at bottom right, b. It is very obvious that the arced orange shells do not perfectly match in the middle where they are spliced together. The arcs at left appear lower, and the arcs at right all appear higher. Each arc lines up for about half its width.\" block_context=\"nasa-block\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=400&#038;h=400&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=150&#038;h=150&#038;fit=crop&#038;crop=faces%2Cfocalpoint 150w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=300&#038;h=300&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=50&#038;h=50&#038;fit=crop&#038;crop=faces%2Cfocalpoint 50w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=100&#038;h=100&#038;fit=crop&#038;crop=faces%2Cfocalpoint 100w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/webb\/science\/2025\/webb-STScI-01JFGAWXXNPAEQHBG1QM637NGH-2K.jpg?w=200&#038;h=200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 200w\" sizes=\"auto, (max-width: 400px) 100vw, 400px\"><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">Two mid-infrared images from NASA\u2019s James Webb Space Telescope of Wolf-Rayet 140 show carbon-rich dust moving in space. At right, the two triangles from the main images are matched up to show how much difference 14 months makes: The dust is racing away from the central stars at almost 1% the speed of light. These stars are 5,000 light-years away in our own Milky Way galaxy.<\/div>\n<div class=\"hds-credits\">Image: NASA, ESA, CSA, STScI; Science: Emma Lieb (University of Denver), Ryan Lau (NSF NOIRLab), Jennifer Hoffman (University of Denver)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p>\u201cThe telescope not only confirmed that these dust shells are real, its data also showed that the dust shells are moving outward at consistent velocities, revealing visible changes over incredibly short periods of time,\u201d said Emma Lieb, the lead author of the new paper and a doctoral student at the University of Denver in Colorado.<\/p>\n<p>Every shell is racing away from the stars at more than 1,600 miles per second (2,600 kilometers per second), almost 1% the speed of light. \u201cWe are used to thinking about events in space taking place slowly, over millions or billions of years,\u201d added Jennifer Hoffman, a co-author and a professor at the University of Denver. \u201cIn this system, the observatory is showing that the dust shells are expanding from one year to the next.\u201d<\/p>\n<p>Like clockwork, the stars\u2019 winds generate dust for several months every eight years, as the pair make their closest approach during a wide, elongated orbit. Webb also shows how dust formation varies \u2014 look for the darker region at top left in both images.<\/p>\n<h2 class=\"wp-block-heading\">Video A: Fade Between 2022 and 2023 Observations of Wolf-Rayet 140<\/h2>\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:\/\/assets.science.nasa.gov\/content\/dam\/science\/missions\/webb\/science\/2025\/webb-wr140.gif?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\/content\/dam\/science\/missions\/webb\/science\/2025\/webb-wr140.gif?w=1920&#038;h=1080&#038;fit=clip&#038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"The video alternates between two James Webb Space Telescope images of the two-star system Wolf-Rayet 140, the first taken in 2022 and the second in 2023.  Both show a bright white point of light surrounded by 17 regularly spaced, hazy dust shells at the bottom, right, and upper right. There is noticeably less color in the upper left. The central point, where the two stars are located, has a rough hexagon shape.  By alternating between them, it\u2019s clear that the dust shells are moving outward, becoming wider.\" block_context=\"nasa-block\"><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">This video alternates between two mid-infrared light observations from NASA\u2019s James Webb Space Telescope of Wolf-Rayet 140. Over only 14 months, Webb showed the dust in the system has expanded. This two-star system has sent out more than 17 shells of dust over 130 years.<\/div>\n<div class=\"hds-credits\">Video: NASA, ESA, CSA, STScI.; Science: Emma Lieb (University of Denver), Ryan Lau (NSF NOIRLab), Jennifer Hoffman (University of Denver)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<h2 class=\"wp-block-heading\">Video B: Stars\u2019 Orbits in Wolf-Rayet 140 (Visualization)<\/h2>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube\">\n<div class=\"wp-block-embed__wrapper\">\n<\/div><figcaption class=\"wp-element-caption\">When the two massive stars in Wolf-Rayet 140 swing past one another, their winds collide, material compresses, and carbon-rich dust forms. The stronger winds of the hotter star in the Wolf-Rayet system blow behind its slightly cooler (but still hot) companion. The stars create dust for several months in every eight-year orbit.<br \/><strong>Video: NASA, ESA, CSA, Joseph Olmsted (STScI).<\/strong><\/figcaption><\/figure>\n<p>The telescope\u2019s mid-infrared images detected shells that have persisted for more than 130 years. (Older shells have dissipated enough that they are now too dim to detect.) The researchers speculate that the stars will ultimately generate tens of thousands of dust shells over hundreds of thousands of years.<\/p>\n<p>\u201cMid-infrared observations are absolutely crucial for this analysis, since the dust in this system is fairly cool. Near-infrared and visible light would only show the shells that are closest to the star,\u201d explained Ryan Lau, a co-author and astronomer at NSF NOIRLab in Tuscon, Arizona, who led the <a href=\"https:\/\/webbtelescope.org\/contents\/early-highlights\/webb-reveals-shells-of-dust-surrounding-brilliant-binary-star-system.html\" target=\"_blank\" rel=\"noreferrer noopener\">initial research<\/a> about this system. \u201cWith these incredible new details, the telescope is also allowing us to study exactly when the stars are forming dust \u2014 almost to the day.\u201d<\/p>\n<p>The dust\u2019s distribution isn\u2019t uniform. Though this isn\u2019t obvious at first glance, zooming in on the shells in Webb\u2019s images reveals that some of the dust has \u201cpiled up,\u201d forming amorphous, delicate clouds that are as large as our entire solar system. Many other individual dust particles float freely. Every speck is as small as one-hundredth the width of a human hair. Clumpy or not, all of the dust moves at the same speed and is carbon rich.<\/p>\n<h2 class=\"wp-block-heading\"><strong>The Future of This System<\/strong><\/h2>\n<p>What will happen to these stars over millions or billions of years, after they are finished \u201cspraying\u201d their surroundings with dust? The <a href=\"https:\/\/webbtelescope.org\/glossary.html#h3-CK-dfa07506-1b7d-4be1-957e-e5ae4759e2cc\" target=\"_blank\" rel=\"noreferrer noopener\">Wolf-Rayet star<\/a> in this system is 10 times more massive than the Sun and nearing the end of its life. In its final \u201cact,\u201d this star will either explode as a <a href=\"https:\/\/webbtelescope.org\/glossary.html#h3-CK-9aebc019-bab1-4f81-a85d-9656033065ae\" target=\"_blank\" rel=\"noreferrer noopener\">supernova<\/a> \u2014 possibly blasting away some or all of the dust shells \u2014 or collapse into a <a href=\"https:\/\/webbtelescope.org\/glossary.html#h3-CK-8ca8fa7b-0187-4f84-995a-564896cc9717\" target=\"_blank\" rel=\"noreferrer noopener\">black hole<\/a>, which would leave the dust shells intact.<\/p>\n<p>Though no one can predict with any certainty what will happen, researchers are rooting for the black hole scenario. \u201cA major question in astronomy is, where does all the dust in the universe come from?\u201d Lau said. \u201cIf carbon-rich dust like this survives, it could help us begin to answer that question.\u201d<\/p>\n<p>\u201cWe know carbon is necessary for the formation of rocky planets and solar systems like ours,\u201d Hoffman added. \u201cIt\u2019s exciting to get a glimpse into how binary star systems not only create carbon-rich dust, but also propel it into our galactic neighborhood.\u201d<\/p>\n<p>These results have been published in the\u00a0<a href=\"https:\/\/doi.org\/10.3847\/2041-8213\/ad9aa9\" target=\"_blank\" rel=\"noreferrer noopener\">Astrophysical Journal Letters<\/a><strong> <\/strong>and were presented in a press conference at the 245th meeting of the American Astronomical Society in National Harbor, Maryland.<\/p>\n<p><em>The James Webb Space Telescope is the world\u2019s premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe 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 the Canadian Space Agency.<\/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\/2025\/news-2025-103#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 research results<\/strong> from the\u00a0<a href=\"https:\/\/doi.org\/10.3847\/2041-8213\/ad9aa9\" target=\"_blank\" rel=\"noreferrer noopener\">Astrophysical Journal Letters<\/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>Claire Blome<\/strong> \u2013 <a href=\"mailto:cblome@stsci.edu\">cblome@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<p><strong>Science<\/strong> \u2013 Emma Lieb (University of Denver)<\/p>\n<h2 class=\"wp-block-heading\">Related Information<\/h2>\n<p><strong>Webb Blog:<\/strong> <a href=\"https:\/\/blogs.nasa.gov\/webb\/2022\/10\/12\/webb-reveals-shells-of-dust-surrounding-brilliant-binary-star-system\/\" target=\"_blank\" rel=\"noreferrer noopener\">Learn more about WR 140<\/a><\/p>\n<p><strong>Infographic:<\/strong> <a href=\"https:\/\/webbtelescope.org\/contents\/media\/images\/01FEGX8A3Z6QCZW7RCD1EZ6F96\" target=\"_blank\" rel=\"noreferrer noopener\">Choose your path: Destiny of Dust<\/a><\/p>\n<p><strong>SVS Graphic:<\/strong> <a href=\"https:\/\/svs.gsfc.nasa.gov\/13873\/\" target=\"_blank\" rel=\"noreferrer noopener\">Periodic Table of the Elements: Origins of the Elements<\/a><\/p>\n<p><strong><a href=\"https:\/\/nasa3d.arc.nasa.gov\/detail\/WR-140\" target=\"_blank\" rel=\"noreferrer noopener\">3D Resource for WR140<\/a><\/strong><\/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\/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:\/\/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\/astrophysics\/focus-areas\/how-do-stars-form-and-evolve\/stories\/\" 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 Stories<\/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=\"1280\" height=\"1141\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?w=1280\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" block_context=\"nasa-block\" srcset=\"https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp 1280w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?resize=300,267 300w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?resize=768,685 768w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?resize=1024,913 1024w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?resize=400,357 400w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?resize=600,535 600w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?resize=900,802 900w, https:\/\/smd-cms.nasa.gov\/wp-content\/uploads\/2023\/04\/hubble-ngc3603-opo1022a-jpg.webp?resize=1200,1070 1200w\" sizes=\"auto, (max-width: 1280px) 100vw, 1280px\"><\/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\" 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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=Webb%20Watches%20Carbon-Rich%20Dust%20Shells%20Form%2C%20Expand%20in%20Star%20System&#038;url=https%3A%2F%2Fscience.nasa.gov%2Fmissions%2Fwebb%2Fwebb-watches-carbon-rich-dust-shells-form-expand-in-star-system%2F\" aria-label=\"Share on 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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\/category\/universe\/stars\/binary-stars\/\" rel=\"noopener\">Binary Stars<\/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\/category\/universe\/nebulae\/\" rel=\"noopener\">Nebulae<\/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\/category\/universe\/galaxies\/milky-way\/\" rel=\"noopener\">The Milky Way<\/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\/webb-watches-carbon-rich-dust-shells-form-expand-in-star-system\/\"  target=\"_blank\" rel=\"noopener\">Get The Details&#8230;<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Astronomers have long tried to track down how elements like carbon, which is essential for life, become widely distributed across the universe. 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