{"id":5630,"date":"2025-04-09T10:38:07","date_gmt":"2025-04-09T10:38:07","guid":{"rendered":"https:\/\/www.europesays.com\/uk\/5630\/"},"modified":"2025-04-09T10:38:07","modified_gmt":"2025-04-09T10:38:07","slug":"methane-detected-in-the-atmosphere-of-the-nearest-t-dwarf","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/uk\/5630\/","title":{"rendered":"Methane detected in the atmosphere of the nearest T dwarf"},"content":{"rendered":"<p>            <img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.europesays.com\/uk\/wp-content\/uploads\/2025\/04\/methane-detected-in-th.jpg\" alt=\"Methane detected in the atmosphere of the nearest T dwarf\" title=\"Images of the position of WISE1810 on 21 July 2024 from GTC\/EMIR in the J, H and Ks bands. The object is marked with a red circle. The field of view of each image is 45\u2032\u2032\u00d745\u2032\u2032. North is up and East left. Credit: arXiv (2025). DOI: 10.48550\/arxiv.2503.22289\" width=\"800\" height=\"388\"\/><\/p>\n<p>                Images of the position of WISE1810 on 21 July 2024 from GTC\/EMIR in the J, H and Ks bands. The object is marked with a red circle. The field of view of each image is 45\u2032\u2032\u00d745\u2032\u2032. North is up and East left. Credit: arXiv (2025). DOI: 10.48550\/arxiv.2503.22289<\/p>\n<p>Using the 10.4-m Gran Telescopio Canarias (GTC), European astronomers have detected methane in the atmosphere of WISEA J181006.18\u2212101000.5\u2014the closest T dwarf to Earth. The finding was reported in a research paper <a href=\"https:\/\/arxiv.org\/abs\/2503.22289\" target=\"_blank\" rel=\"noopener\">published<\/a> March 28 on the arXiv pre-print server.<\/p>\n<p>Brown dwarfs are intermediate objects between planets and stars. Astronomers generally agree that they are substellar objects occupying the mass range between 13 and 80 Jupiter masses. One subclass of <a href=\"https:\/\/phys.org\/tags\/brown+dwarfs\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">brown dwarfs<\/a> (with effective temperatures between 500 and 1,500 K) is known as T dwarfs, and represents the coolest and least luminous substellar objects so far detected.<\/p>\n<p>Studies of T dwarfs could help astronomers better understand objects near the disputed planet\/star boundary, for instance, giant exoplanets. However, although many brown dwarfs have been detected to date, T dwarfs are not so common, as only about 400 such objects have been identified.<\/p>\n<p>WISEA J181006.18\u2212101000.5, or WISE1810 for short, is a metal-poor T dwarf at a distance of just 29 light years from the Earth. It has a radius of about 0.65 Jupiter radii and is some 17 times more massive than Jupiter. The effective temperature of WISE1810 is estimated to be within the range of 800\u20131,300 K.<\/p>\n<p>Previous low-resolution near-infrared and mid-infrared observations of WISE1810 have suggested that it has a significantly chemically modified atmosphere dominated by hydrogen and water vapor. However, no evidence of <a href=\"https:\/\/phys.org\/tags\/methane\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">methane<\/a> has been found, which is a defining characteristic molecule of the T-dwarf type.<\/p>\n<p>This has changed with the recent publication of a new study conducted by a team of astronomers led by Jerry Zhang of the University of La Laguna, Spain. They obtained new near-infrared photometry of WISE1810 with GTC&#8217;s Espectrografo Multiobjeto Infra-Rojo (EMIR), which resulted in clear detection of methane in the atmosphere of this T dwarf.<\/p>\n<p>The detection of methane further supports the classification of WISE1810 as T-type instead of L-type, which was suggested by some studies. The researchers add that no evidence of carbon monoxide and potassium has been found in the atmosphere of this object.<\/p>\n<p>Based on the collected data, the carbon abundance for WISE1810 was estimated to be -1.5 dex, which inferred a metallicity at a level of -1.7 dex. The effective temperature of the T dwarf was constrained to be about 1,000 K.<\/p>\n<p>The authors of the paper explain that the low metallicity of WISE1810 probably accounts majorly for the non-detection of atomic potassium but a <a href=\"https:\/\/phys.org\/tags\/lower+temperature\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">lower temperature<\/a> could also boost this effect.<\/p>\n<p>The study also found that WISE1810 has a heliocentric velocity of -83 km\/s. This finding indicates that the object is more likely associated with the Milky Way&#8217;s thick disk rather than the halo, despite its very low metallicity.<\/p>\n<p><strong>More information:<\/strong><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tJerry Jun-Yan Zhang et al, Detection of Methane in the Closest Extreme Metal-poor T Dwarf WISEA J181006.18-101000.5, arXiv (2025). <a data-doi=\"1\" href=\"https:\/\/dx.doi.org\/10.48550\/arxiv.2503.22289\" target=\"_blank\" rel=\"noopener\">DOI: 10.48550\/arxiv.2503.22289<\/a><\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t\t<strong>Journal information:<\/strong><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a href=\"https:\/\/phys.org\/journals\/arxiv\/\" target=\"_blank\" rel=\"noopener\">arXiv<\/a><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"icon_open\" href=\"http:\/\/arxiv.org\/\" target=\"_blank\" rel=\"nofollow noopener\"><\/p>\n<p>\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/p>\n<p class=\"article-main__note mt-4\">\n\t\t\t\t\t\t\t\t\t\t\t\t  \u00a9 2025 Science X Network\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t<strong>Citation<\/strong>:<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tMethane detected in the atmosphere of the nearest T dwarf (2025, April 7)<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tretrieved 9 April 2025<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tfrom https:\/\/phys.org\/news\/2025-04-methane-atmosphere-nearest-dwarf.html\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no<br \/>\n\t\t\t\t\t\t\t\t\t\t\t part may be reproduced without the written permission. The content is provided for information purposes only.\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n","protected":false},"excerpt":{"rendered":"Images of the position of WISE1810 on 21 July 2024 from GTC\/EMIR in the J, H and Ks&hellip;\n","protected":false},"author":2,"featured_media":5631,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[75,76,74,71,70,72,53,73,16,15],"class_list":{"0":"post-5630","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-science","8":"tag-materials","9":"tag-nanotech","10":"tag-physics","11":"tag-physics-news","12":"tag-science","13":"tag-science-news","14":"tag-technology","15":"tag-technology-news","16":"tag-uk","17":"tag-united-kingdom"},"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@uk\/114307576976769136","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/5630","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/comments?post=5630"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/5630\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media\/5631"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media?parent=5630"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/categories?post=5630"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/tags?post=5630"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}