{"id":625965,"date":"2026-04-24T17:19:10","date_gmt":"2026-04-24T17:19:10","guid":{"rendered":"https:\/\/www.newsbeep.com\/ca\/625965\/"},"modified":"2026-04-24T17:19:10","modified_gmt":"2026-04-24T17:19:10","slug":"sombrero-galaxy-the-universes-dusty-brimmed-hat-revealed-like-never-before","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/ca\/625965\/","title":{"rendered":"Sombrero Galaxy: The Universe\u2019s Dusty Brimmed Hat Revealed Like Never Before"},"content":{"rendered":"<p>                    <a href=\"https:\/\/noirlab.edu\/public\/news\/archive\/program\/ctio\/\" rel=\"nofollow noopener\" target=\"_blank\"><br \/>\n                        <img decoding=\"async\" class=\"program-logo\" src=\"https:\/\/www.newsbeep.com\/ca\/wp-content\/uploads\/2026\/01\/logo127.png\" alt=\"Cerro Tololo Inter-American Observatory\"\/><br \/>\n                    <\/a><\/p>\n<p>\n                    noirlab2612 \u2014 Photo Release\n                <\/p>\n<p>    <img decoding=\"async\" src=\"https:\/\/www.newsbeep.com\/ca\/wp-content\/uploads\/2026\/01\/logo248.png\" alt=\"DECam - Blanco\" class=\"w-100 mb-20\"\/><\/p>\n<p>Dark Energy Camera spies the faint glowing features of Messier 104, known as the Sombrero Galaxy<\/p>\n<p class=\"date\">24 April 2026<\/p>\n<p class=\"text_intro pr_first\">Messier 104, nicknamed the Sombrero Galaxy, is a popular target for amateur observing and astronomical research. Its recognizable extended halo, as well as a faint stellar stream, are captured in exquisite detail in this image from the Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation V\u00edctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of NSF NOIRLab.<\/p>\n<p>The <a href=\"https:\/\/en.wikipedia.org\/wiki\/Sombrero_Galaxy\" rel=\"nofollow noopener\" target=\"_blank\">Sombrero galaxy (Messier 104)<\/a> is a galactic masterpiece that captivates scientists and astronomy enthusiasts alike. Its intricate system of <a href=\"https:\/\/en.wikipedia.org\/wiki\/Globular_cluster\" rel=\"nofollow noopener\" target=\"_blank\">globular star clusters<\/a> lends insight into stellar populations, and astronomers are intrigued by the supermassive black hole <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/1996ApJ...473L..91K\/abstract\" rel=\"nofollow noopener\" target=\"_blank\">at its center<\/a>. Its distinctive visual features and relative brightness make it a favorite among amateur astronomers. The fascinating story of its discovery, involving three esteemed astronomers, has earned it a spot on one of the most important lists of deep sky objects. Today, it stands as one of the most iconic galaxies in the night sky.<\/p>\n<p>Messier 104 resides approximately 30 million light-years from Earth in the constellation Virgo (see <a href=\"https:\/\/noirlab.edu\/public\/images\/vir\/\" rel=\"nofollow noopener\" target=\"_blank\">finder chart<\/a>). Spanning an impressive 50,000 light-years across, it is among the largest objects of the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Virgo_Cluster\" rel=\"nofollow noopener\" target=\"_blank\">Virgo Galaxy Cluster<\/a>. Despite its grandeur, it appears relatively dim in the night sky \u2014 just below the threshold of naked-eye visibility, though it can be observed with a small telescope or binoculars.<\/p>\n<p>This image was captured with the 570-megapixel Department of Energy-fabricated Dark Energy Camera (<a href=\"https:\/\/noirlab.edu\/public\/programs\/ctio\/victor-blanco-4m-telescope\/decam\/\" rel=\"nofollow noopener\" target=\"_blank\">DECam<\/a>) mounted on the U.S. National Science Foundation <a href=\"https:\/\/noirlab.edu\/public\/programs\/ctio\/victor-blanco-4m-telescope\/\" rel=\"nofollow noopener\" target=\"_blank\">V\u00edctor M. Blanco 4-meter Telescope<\/a> at Cerro Tololo Inter-American Observatory (<a href=\"https:\/\/noirlab.edu\/public\/programs\/ctio\/\" rel=\"nofollow noopener\" target=\"_blank\">CTIO<\/a>) in Chile, a Program of NSF NOIRLab.<\/p>\n<p>The incredible resolution of DECam reveals the Sombrero Galaxy\u2019s <a href=\"https:\/\/noirlab.edu\/public\/images\/noirlab2612a\/zoomable\/\" rel=\"nofollow noopener\" target=\"_blank\">striking features<\/a>. At its core is an intensely bright nucleus, which is surrounded by a swarm of around 2000 <a href=\"https:\/\/en.wikipedia.org\/wiki\/Globular_cluster\" rel=\"nofollow noopener\" target=\"_blank\">globular star clusters<\/a>. A thin, dark band of cold dust and hydrogen gas traces the perimeter of the disk, where most of the galaxy\u2019s star formation takes place. The moniker \u201cSombrero Galaxy\u201d comes from its striking resemblance to a sombrero, with its pronounced central bulge and dark dust trail that resemble the lofty crown and expansive brim of the traditional Mexican hat.<\/p>\n<p>Also visible in this image is the galaxy\u2019s enormous glowing halo, which appears to stretch over three times the width of the Sombrero itself. This may be the first time the halo has been captured with this level of detail and at this large a scale. DECam\u2019s incredible sensitivity also captured a sweeping stellar stream extending from the south side of the galaxy. The halo and the stellar stream are populated with stars that have been torn from their home galaxies, hinting at a past galactic merger between the Sombrero and a smaller satellite galaxy.<\/p>\n<p>The story of Messier 104\u2019s discovery is intertwined with the endeavors of several prominent astronomers. It was initially spotted by the French astronomer and comet hunter <a href=\"https:\/\/en.wikipedia.org\/wiki\/Pierre_M%C3%A9chain\" rel=\"nofollow noopener\" target=\"_blank\">Pierre M\u00e9chain<\/a> in 1781 when he was an associate of the renowned comet hunter <a href=\"https:\/\/en.wikipedia.org\/wiki\/Charles_Messier\" rel=\"nofollow noopener\" target=\"_blank\">Charles Messier<\/a>. At that time, Messier was compiling a list of non-cometary celestial objects, now famously known as the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_object\" rel=\"nofollow noopener\" target=\"_blank\">Messier Catalogue<\/a>, to aid other astronomers in distinguishing these objects from passing comets.<\/p>\n<p>Interestingly, Messier 104 did not find its place in the original publication of Messier&#8217;s list. However, it was later discovered that Messier added it by hand to his personal copy. Independently, in 1784, the well-known astronomer <a href=\"https:\/\/en.wikipedia.org\/wiki\/William_Herschel\" rel=\"nofollow noopener\" target=\"_blank\">William Herschel<\/a> also stumbled upon this remarkable galaxy and designated it as H I.43.<\/p>\n<p>It wasn\u2019t until French astronomer <a href=\"https:\/\/en.wikipedia.org\/wiki\/Camille_Flammarion\" rel=\"nofollow noopener\" target=\"_blank\">Camille Flammarion&#8217;s<\/a> subsequent confirmation that these two independent discoveries were the same object that Messier 104 officially earned its place in the Messier Catalogue in 1921. Thus, through the collaborative efforts of these astronomers across different eras, the Sombrero Galaxy has become a celebrated addition to our knowledge of deep sky objects.<\/p>\n<p>Its alluring visual characteristics, coupled with its accessibility to amateur equipment, contribute to Messier 104\u2019s popularity among stargazers. Amateur astronomers often enjoy observing and photographing the Sombrero Galaxy, making it a prime target for citizen science projects and public outreach efforts. It is an excellent subject for sharing the wonders of the Universe with the public and fostering engagement with astronomy and science.<\/p>\n<p>More information<\/p>\n<p>The Dark Energy Camera (<a href=\"https:\/\/noirlab.edu\/public\/programs\/ctio\/victor-blanco-4m-telescope\/decam\/\" rel=\"nofollow noopener\" target=\"_blank\">DECam<\/a>) was designed specifically for the Dark Energy Survey (<a href=\"https:\/\/www.darkenergysurvey.org\/\" rel=\"nofollow noopener\" target=\"_blank\">DES<\/a>). It was funded by the U.S. Department of Energy (DOE) and was built and tested at DOE&#8217;s Fermilab. To provide new insights into the accelerating expansion of our Universe, the DECam records the motions and distances of galaxies in the distant past. While the full DES study ended in 2019, the camera continues to provide new insights to astronomers and astrophysicists.<\/p>\n<p><a href=\"https:\/\/noirlab.edu\/\" rel=\"nofollow noopener\" target=\"_blank\">NSF NOIRLab<\/a>, the U.S. National Science Foundation center for ground-based optical-infrared astronomy, operates the <a href=\"https:\/\/www.noirlab.edu\/public\/programs\/gemini-observatory\/\" rel=\"nofollow noopener\" target=\"_blank\">International Gemini Observatory<\/a> (a facility of <a href=\"https:\/\/www.nsf.gov\/\" rel=\"nofollow noopener\" target=\"_blank\">NSF<\/a>, <a href=\"http:\/\/www.nrc-cnrc.gc.ca\/eng\/solutions\/facilities\/gemini.html\" rel=\"nofollow noopener\" target=\"_blank\">NRC\u2013Canada<\/a>, <a href=\"http:\/\/www.conicyt.cl\/astronomia\/oficina-gemini-chile\/\" rel=\"nofollow noopener\" target=\"_blank\">ANID\u2013Chile<\/a>, <a href=\"https:\/\/www.gov.br\/mcti\/pt-br\" rel=\"nofollow noopener\" target=\"_blank\">MCTIC\u2013Brazil<\/a>, <a href=\"http:\/\/www.geminiargentina.mincyt.gob.ar\/\" rel=\"nofollow noopener\" target=\"_blank\">MINCyT\u2013Argentina<\/a>, and <a href=\"http:\/\/kgmt.kasi.re.kr\/kgmtscience\" rel=\"nofollow noopener\" target=\"_blank\">KASI\u2013Republic of Korea<\/a>), NSF Kitt Peak National Observatory (<a href=\"https:\/\/www.noirlab.edu\/public\/programs\/kitt-peak-national-observatory\/\" rel=\"nofollow noopener\" target=\"_blank\">KPNO<\/a>), NSF Cerro Tololo Inter-American Observatory (<a href=\"https:\/\/www.noirlab.edu\/public\/programs\/ctio\/\" rel=\"nofollow noopener\" target=\"_blank\">CTIO<\/a>), the Community Science and Data Center (<a href=\"https:\/\/www.noirlab.edu\/public\/programs\/csdc\/\" rel=\"nofollow noopener\" target=\"_blank\">CSDC<\/a>), and NSF\u2013DOE <a href=\"https:\/\/www.noirlab.edu\/public\/programs\/vera-c-rubin-observatory\/\" rel=\"nofollow noopener\" target=\"_blank\">Vera C. Rubin Observatory<\/a> (in cooperation with <a href=\"https:\/\/www.energy.gov\/science\/office-science\" rel=\"nofollow noopener\" target=\"_blank\">DOE<\/a>\u2019s <a href=\"https:\/\/www6.slac.stanford.edu\/\" rel=\"nofollow noopener\" target=\"_blank\">SLAC<\/a> National Accelerator Laboratory). It is managed by the Association of Universities for Research in Astronomy (<a href=\"https:\/\/www.aura-astronomy.org\/\" rel=\"nofollow noopener\" target=\"_blank\">AURA<\/a>) under a cooperative agreement with <a href=\"https:\/\/www.nsf.gov\/\" rel=\"nofollow noopener\" target=\"_blank\">NSF<\/a> and is headquartered in Tucson, Arizona.\u00a0<\/p>\n<p>The scientific community is honored to have the opportunity to conduct astronomical research on I\u2019oligam Du\u2019ag (Kitt Peak) in Arizona, on Maunakea in Hawai\u2018i, and on Cerro Tololo and Cerro Pach\u00f3n in Chile. We recognize and acknowledge the very significant cultural role and reverence of I\u2019oligam Du\u2019ag (Kitt Peak) to the Tohono O\u2019odham Nation, and Maunakea to the Kanaka Maoli (Native Hawaiians) community.<\/p>\n<p>    Contacts<\/p>\n<p>\n        Josie Fenske<br \/>Public Information Officer<br \/>NSF NOIRLab<br \/>Email: <a href=\"https:\/\/noirlab.edu\/public\/news\/noirlab2612\/mailto:josie.fenske@noirlab.edu\" rel=\"nofollow noopener\" target=\"_blank\">josie.fenske@noirlab.edu<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"noirlab2612 \u2014 Photo Release Dark Energy Camera spies the faint glowing features of Messier 104, known as the&hellip;\n","protected":false},"author":2,"featured_media":625966,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7],"tags":[49,48,66],"class_list":["post-625965","post","type-post","status-publish","format-standard","has-post-thumbnail","category-science","tag-ca","tag-canada","tag-science"],"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/625965","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/comments?post=625965"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/625965\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media\/625966"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media?parent=625965"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/categories?post=625965"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/tags?post=625965"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}