{"id":656951,"date":"2026-10-25T20:32:13","date_gmt":"2026-10-25T20:32:13","guid":{"rendered":"https:\/\/www.newsbeep.com\/il\/656951\/"},"modified":"2026-10-25T20:32:13","modified_gmt":"2026-10-25T20:32:13","slug":"webb-reveals-the-brilliant-chaos-of-two-merging-galaxies","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/il\/656951\/","title":{"rendered":"Webb reveals the brilliant chaos of two merging galaxies"},"content":{"rendered":"<p>Arp 220 is one of the brightest infrared galaxies in the nearby universe, with intense star formation fueled by a collision that began 700 million years ago.<\/p>\n<p class=\"wp-block-paragraph\">From a distance, Arp 220 looks like a single galaxy with a brilliant center and enormous clouds of glowing material spreading into space.\u00a0<\/p>\n<p class=\"wp-block-paragraph\">But the <a href=\"https:\/\/science.nasa.gov\/mission\/webb\/\" target=\"_blank\" rel=\"noreferrer noopener nofollow\">James Webb Space Telescope<\/a> has revealed something far more complicated.<\/p>\n<p class=\"wp-block-paragraph\">The object is actually two spiral galaxies in the process of merging, creating one of the brightest infrared galaxies in the nearby universe.<\/p>\n<p class=\"wp-block-paragraph\">Located roughly 250 million light-years from Earth, Arp 220 offers astronomers a remarkable opportunity to study what happens when galaxies collide, gas clouds compress, and new stars begin forming at extraordinary rates.<\/p>\n<p>A collision 700 million years in the making<\/p>\n<p class=\"wp-block-paragraph\">The story of Arp 220 began about 700 million years ago, when two spiral galaxies started colliding.<\/p>\n<p class=\"wp-block-paragraph\">Their enormous gravitational forces pulled at each other\u2019s stars, gas, and dust, gradually transforming both galaxies.<\/p>\n<p class=\"wp-block-paragraph\">Unlike a collision between solid objects, a <a href=\"https:\/\/www.earth.com\/space\/powerful-gamma-ray-burst-grb-230906a-erupts-from-wreckage-of-colliding-galaxies\/\" rel=\"nofollow noopener\" target=\"_blank\">galactic merger<\/a> unfolds over hundreds of millions of years.\u00a0<\/p>\n<p class=\"wp-block-paragraph\">Individual stars are so widely separated that direct collisions between them are extremely unlikely.<\/p>\n<p class=\"wp-block-paragraph\">Instead, gravity reshapes the galaxies, changing the paths of stars and drawing enormous quantities of gas toward their centers.<\/p>\n<p class=\"wp-block-paragraph\">In Arp 220, that process triggered an intense period of star formation. The merger has become a natural laboratory for understanding how galaxies grow and change.<\/p>\n<p class=\"wp-block-paragraph\">Although the two galaxies appear to form a single object in Webb\u2019s image, their original cores remain distinguishable.<\/p>\n<p class=\"wp-block-paragraph\">Earlier <a href=\"https:\/\/esahubble.org\/images\/heic0810bf\/\" target=\"_blank\" rel=\"noreferrer noopener nofollow\">observations<\/a> by NASA\u2019s Hubble Space Telescope revealed that these centers are separated by approximately 1,200 light-years. Each contains a rotating ring where stars are forming.<\/p>\n<p>A galaxy brighter than a trillion suns<\/p>\n<p class=\"wp-block-paragraph\">Arp 220 belongs to a rare category known as ultraluminous infrared galaxies. These objects release enormous amounts of energy, much of it at infrared wavelengths.<\/p>\n<p class=\"wp-block-paragraph\">According to <a href=\"https:\/\/www.nasa.gov\/\" target=\"_blank\" rel=\"noreferrer noopener nofollow\">NASA<\/a>, Arp 220 shines with the luminosity of more than one trillion suns. By comparison, the Milky Way has a total luminosity of roughly 10 billion suns.<\/p>\n<p class=\"wp-block-paragraph\">Much of Arp 220\u2019s extraordinary infrared brightness comes from dust absorbing energy produced by intense activity within the merging galaxies and radiating that energy at longer wavelengths.<\/p>\n<p class=\"wp-block-paragraph\">The region surrounding the galactic centers is especially remarkable.<\/p>\n<p class=\"wp-block-paragraph\">Approximately 200 massive star clusters occupy a dusty area measuring just 5,000 light-years across. That is only about five percent of the Milky Way\u2019s diameter.<\/p>\n<p class=\"wp-block-paragraph\">Yet this relatively small region contains roughly as much gas as the entire <a href=\"https:\/\/www.earth.com\/space\/milky-way-devoured-a-massive-dwarf-galaxy-12-3-billion-years-ago\/\" rel=\"nofollow noopener\" target=\"_blank\">Milky Way<\/a>.<\/p>\n<p>Webb reveals the hidden structure<\/p>\n<p class=\"wp-block-paragraph\">Dust presents a major challenge when astronomers study galaxies. Thick clouds can block visible light, concealing stars and other structures.<\/p>\n<p class=\"wp-block-paragraph\">Infrared observations help researchers investigate regions that would otherwise remain difficult to see.<\/p>\n<p class=\"wp-block-paragraph\">For this image, Webb combined observations from its Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI).<\/p>\n<p class=\"wp-block-paragraph\">Together, these instruments reveal different aspects of Arp 220, including its bright central regions and the material extending outward from the merger.<\/p>\n<p class=\"wp-block-paragraph\">The brilliant spikes radiating from the center are especially noticeable. They are diffraction spikes, an optical effect produced when intense light interacts with the telescope\u2019s structure.<\/p>\n<p class=\"wp-block-paragraph\">The reddish-orange streams and filaments trace material associated with the galaxies, including carbon-rich organic molecules.<\/p>\n<p class=\"wp-block-paragraph\">Meanwhile, faint blue structures near the outskirts reveal tidal tails, streams of material pulled away by the gravitational forces of the merger.<\/p>\n<p class=\"wp-block-paragraph\">These features help astronomers reconstruct how the two <a href=\"https:\/\/www.earth.com\/space\/ghost-town-galaxies-hold-big-secrets-about-the-early-universe\/\" rel=\"nofollow noopener\" target=\"_blank\">galaxies<\/a> have interacted over time.<\/p>\n<p>The remains of exploding stars<\/p>\n<p class=\"wp-block-paragraph\">The intense star formation in Arp 220 also means that massive stars can reach the ends of their lives in a relatively short astronomical time.<\/p>\n<p class=\"wp-block-paragraph\">Some explode as supernovae, releasing tremendous energy and scattering newly formed elements into surrounding space.<\/p>\n<p class=\"wp-block-paragraph\">Radio telescope observations have identified approximately 100 supernova remnants within a region less than 500 light-years across.<\/p>\n<p class=\"wp-block-paragraph\">That concentration provides further evidence of the extraordinary stellar activity occurring near the galactic centers.<\/p>\n<p class=\"wp-block-paragraph\">Supernovae also influence their surroundings. Their expanding shock waves can heat gas, redistribute material, and affect the formation of subsequent generations of stars.<\/p>\n<p class=\"wp-block-paragraph\">In a crowded environment like Arp 220, these processes take place alongside the gravitational forces driving the merger.<\/p>\n<p>Why astronomers study merging galaxies<\/p>\n<p class=\"wp-block-paragraph\"><a href=\"https:\/\/www.earth.com\/space\/webb-captures-a-galaxy-collision-with-a-radiant-smile\/\" rel=\"nofollow noopener\" target=\"_blank\">Galactic mergers<\/a> are an important part of cosmic evolution.\u00a0<\/p>\n<p class=\"wp-block-paragraph\">Over billions of years, interactions between galaxies can alter their shapes, change their star formation rates, and influence the growth of the supermassive black holes at their centers.<\/p>\n<p class=\"wp-block-paragraph\">Arp 220 is particularly valuable because it is relatively nearby by cosmic standards.<\/p>\n<p class=\"wp-block-paragraph\">Its distance of 250 million light-years places it in the constellation Serpens, the Serpent. It is the closest known ultraluminous infrared galaxy.<\/p>\n<p class=\"wp-block-paragraph\">Its name comes from astronomer Halton Arp\u2019s Atlas of Peculiar Galaxies, a catalog of unusual-looking galaxies and interacting systems.<\/p>\n<p class=\"wp-block-paragraph\">The object appears as entry number 220, reflecting its distinctive structure and history.<\/p>\n<p class=\"wp-block-paragraph\">By comparing observations from Webb, Hubble, and radio telescopes, scientists can investigate different layers of this complex system.<\/p>\n<p class=\"wp-block-paragraph\">Each wavelength reveals information that the others cannot, helping researchers build a more complete picture of the collision.<\/p>\n<p>A glimpse into the future of galaxies<\/p>\n<p class=\"wp-block-paragraph\">The image of Arp 220 captures a transformation that is still unfolding.<\/p>\n<p class=\"wp-block-paragraph\">Two galaxies that once existed separately are gradually becoming one, while their combined gas supplies fuel intense star formation.<\/p>\n<p class=\"wp-block-paragraph\">Over time, that activity will change as the available gas is consumed, dispersed, or redistributed.<\/p>\n<p class=\"wp-block-paragraph\">Our own Milky Way has also experienced galactic interactions throughout its history, and encounters between galaxies continue to shape the <a href=\"https:\/\/www.earth.com\/space\/universes-expansion-rate-hubble-tension-puzzles-astronomers\/\" rel=\"nofollow noopener\" target=\"_blank\">universe<\/a> today.<\/p>\n<p class=\"wp-block-paragraph\">Arp 220 shows just how dramatic those changes can become.<\/p>\n<p class=\"wp-block-paragraph\">What appears in Webb\u2019s image as a single brilliant object is actually the result of hundreds of millions of years of gravitational interaction, stellar birth, and destruction.<\/p>\n<p class=\"wp-block-paragraph\">Image Credit: NASA\/ESA\/CSA\/STScI<\/p>\n<p class=\"wp-block-paragraph\">\u2014\u2013<\/p>\n<p class=\"wp-block-paragraph\">Like what you read? <a href=\"https:\/\/www.earth.com\/subscribe\/\" rel=\"nofollow noopener\" target=\"_blank\">Subscribe to our newsletter<\/a> for engaging articles, exclusive content, and the latest updates.\u00a0<\/p>\n<p class=\"wp-block-paragraph\">Check us out on <a href=\"https:\/\/www.earth.com\/earthsnap\/\" rel=\"nofollow noopener\" target=\"_blank\">EarthSnap<\/a>, a free app brought to you by <a href=\"https:\/\/www.earth.com\/author\/eralls\/\" rel=\"nofollow noopener\" target=\"_blank\">Eric Ralls<\/a> and Earth.com.<\/p>\n<p class=\"wp-block-paragraph\">\u2014\u2013<\/p>\n","protected":false},"excerpt":{"rendered":"Arp 220 is one of the brightest infrared galaxies in the nearby universe, with intense star formation fueled&hellip;\n","protected":false},"author":2,"featured_media":656952,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[85,46,141,145],"class_list":["post-656951","post","type-post","status-publish","format-standard","has-post-thumbnail","category-space","tag-il","tag-israel","tag-science","tag-space"],"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/posts\/656951","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/comments?post=656951"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/posts\/656951\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/media\/656952"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/media?parent=656951"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/categories?post=656951"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/tags?post=656951"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}