{"id":147147,"date":"2025-11-22T13:47:22","date_gmt":"2025-11-22T13:47:22","guid":{"rendered":"https:\/\/www.newsbeep.com\/il\/147147\/"},"modified":"2025-11-22T13:47:22","modified_gmt":"2025-11-22T13:47:22","slug":"this-dying-star-is-forming-a-strange-spider-structure-and-webb-is-giving-scientists-a-brand-new-view","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/il\/147147\/","title":{"rendered":"This dying star is forming a strange spider structure, and Webb is giving scientists a brand new view"},"content":{"rendered":"<p>This incredible picture of cosmic chaos shows a dying star ejecting shells of material outwards into space.<\/p>\n<p>The extended lobes and twisted knots of gas and dust have earned the object, NGC 6537, the nickname Red Spider Nebula.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"800\" src=\"https:\/\/www.newsbeep.com\/il\/wp-content\/uploads\/2025\/11\/NGC-6072-webb-social.jpg\" alt=\"James Webb Space Telescope view of planetary nebula NGC 6072. Credit: NASA, ESA, CSA, STScI\" class=\"wp-image-174115\"\/>Credit: NASA, ESA, CSA, STScI<\/p>\n<p>And the James Webb Space telescope is revealing the secrets of the Red Spider like never before.<\/p>\n<p>The dying throes of a star like our own<\/p>\n<p>The Red Spider Nebula is a type of cosmic cloud known as a <a href=\"https:\/\/www.skyatnightmagazine.com\/space-science\/planetary-nebula\" rel=\"nofollow noopener\" target=\"_blank\">planetary nebula<\/a>.<\/p>\n<p>These amazing objects give us a future glimpse of how our our Sun might end its life, as planetary nebulae are the final stages of a Sun-like star.<\/p>\n<p>Having exhausted much of its fuel, the star balloons into a cool red giant, then casts its outer layers into space.<\/p>\n<p>This exposes the star&#8217;s white hot core, and ultraviolet light from the dense stellar remnant lights up the cast-off material, causing it to glow.<\/p>\n<p>Many planetary nebulae appear like rounded, puffed-out objects, which is why they are known as &#8216;planetary&#8217;, even though they don&#8217;t have anything to do with planets.<\/p>\n<p>The Red Spider Nebula, however, looks anything but spherical. Its long, spindly structure and central &#8216;body&#8217; is what&#8217;s earned it the &#8216;spider&#8217; nickname.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"800\" src=\"https:\/\/www.newsbeep.com\/il\/wp-content\/uploads\/2025\/11\/james-webb-space-telescope-red-spider-nebula.jpg\" alt=\"James Webb Space Telescope image of NGC 6537, the Red Spider Nebula. Credit: ESA\/Webb, NASA &amp; CSA, J. H. Kastner (Rochester Institute of Technology)\" class=\"wp-image-178790\"\/>James Webb Space Telescope image of NGC 6537, the Red Spider Nebula. Credit: ESA\/Webb, NASA &amp; CSA, J. H. Kastner (Rochester Institute of Technology)<br \/>\nExploring the Red Spider<\/p>\n<p>The James Webb Space Telescope used its Near-InfraRed Camera\u00a0(NIRCam) instrument to give astronomers a new view of the Red Spider Nebula.<\/p>\n<p>Because Webb views the cosmos in <a href=\"https:\/\/www.skyatnightmagazine.com\/space-science\/infrared-astronomy\" rel=\"nofollow noopener\" target=\"_blank\">infrared<\/a>, it can reveal objects that aren&#8217;t normally visible with the human eye.<\/p>\n<p>In the case of the Red Spider Nebula, the James Webb Space Telescope has given astronomers a view of never-before-seen details in the cloud, against a backdrop of thousands of stars.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"1203\" src=\"https:\/\/www.newsbeep.com\/il\/wp-content\/uploads\/2025\/11\/webb-red-spider-nebula.jpg\" alt=\"James Webb Space Telescope image of NGC 6537, the Red Spider Nebula. Credit: ESA\/Webb, NASA &amp; CSA, J. H. Kastner (Rochester Institute of Technology)\" class=\"wp-image-178791\"\/>James Webb Space Telescope image of NGC 6537, the Red Spider Nebula. Credit: ESA\/Webb, NASA &amp; CSA, J. H. Kastner (Rochester Institute of Technology)<\/p>\n<p>We can clearly see the central star of the Red Spider Nebula glowing in infrared, much brighter than the dusty gas that surrounds it.<\/p>\n<p>In optical images, for example those captured by the Hubble Space Telescope, the star appears faint and blue.<\/p>\n<p>Webb has also revealed a shroud of hot dust around the central star.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"668\" src=\"https:\/\/www.newsbeep.com\/il\/wp-content\/uploads\/2025\/11\/hubble-red-spider-nebula.jpg\" alt=\"Hubble Space Telescope image of the Red Spider Nebula. Credit: ESA &amp; Garrelt Mellema (Leiden University, the Netherlands)\" class=\"wp-image-178793\"\/>Hubble Space Telescope image of the Red Spider Nebula. Credit: ESA &amp; Garrelt Mellema (Leiden University, the Netherlands)<br \/>\nA companion for the spider star?<\/p>\n<p>Although we can only see a single star at the heart of the Red Spider Nebula, astronomers say it may have a hidden companion.<\/p>\n<p>They say that might explain why the nebula has such a unique shape, as a second star would explain its narrow waist and wide outflows.<\/p>\n<p>A similar hourglass shape is seen in other planetary nebulae like the <a href=\"https:\/\/www.skyatnightmagazine.com\/news\/webb-butterfly-nebula\" rel=\"nofollow noopener\" target=\"_blank\">Butterfly Nebula, which\u00a0Webb also observed<\/a>.<\/p>\n<p>Webb reveals the full extent of the Red Spider Nebula&#8217;s outstretched lobes, forming the \u2018legs\u2019 of the spider.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"800\" src=\"https:\/\/www.newsbeep.com\/il\/wp-content\/uploads\/2025\/11\/jwst-butterfly-nebula.jpg\" alt=\"Image of the Butterfly Nebula using data from the James Webb Space Telescope and the Atacama Large Millimeter\/submillimeter Array. Credit: ESA\/Webb, NASA &amp; CSA, M. Matsuura, ALMA (ESO\/NAOJ\/NRAO), N. Hirano, M. Zamani (ESA\/Webb)\" class=\"wp-image-175262\"\/>Image of the Butterfly Nebula using data from the James Webb Space Telescope and the Atacama Large Millimeter\/submillimeter Array. Credit: ESA\/Webb, NASA &amp; CSA, M. Matsuura, ALMA (ESO\/NAOJ\/NRAO), N. Hirano, M. Zamani (ESA\/Webb)<\/p>\n<p>The lobes, seen in blue, are traced by light emitted from H2\u00a0molecules.<\/p>\n<p>These lobes are bubble-like structures, each stretching about three lightyears across.<\/p>\n<p>Gas flowing from the centre of the nebula has inflated the bubbles over thousands of years.<\/p>\n<p>Webb&#8217;s view of the Red Spider Nebula shows more gas jetting out from the nebula\u2019s centre.<\/p>\n<p>The purple \u2018S\u2019 shape at the heart of the nebula follows light from ionised iron atoms.<\/p>\n<p>This marks where a jet is shooting outwards from near the central star and smashing into cast-off material, creating the twisted, rippling structure seen here.<\/p>\n","protected":false},"excerpt":{"rendered":"This incredible picture of cosmic chaos shows a dying star ejecting shells of material outwards into space. 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