{"id":791445,"date":"2024-11-24T07:50:00","date_gmt":"2024-11-24T12:50:00","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=791445"},"modified":"2024-11-24T07:50:00","modified_gmt":"2024-11-24T12:50:00","slug":"is-this-a-volcanic-exoplanet-hints-are-in-its-atmosphere","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=791445","title":{"rendered":"Is this a volcanic exoplanet? Hints are in its atmosphere"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<figure id=\"attachment_493461\" aria-describedby=\"caption-attachment-493461\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><figcaption id=\"caption-attachment-493461\" class=\"wp-caption-text\">Artist\u2019s concept of L 98-59 d, a super-Earth world 35 light-years away. Now, new results from NASA\u2019s Webb Space Telescope suggest it might be an active volcanic exoplanet with a sulfur-rich atmosphere. Image via NASA.<\/figcaption><\/figure>\n<ul>\n<li><strong>L 98-59 d is a super-Earth exoplanet,<\/strong> discovered in 2019. It\u2019s 35 light-years away and about 1.5 times the size of Earth.<\/li>\n<li><strong>The Webb space telescope observed the planet<\/strong> again recently, looking for evidence of an atmosphere.<\/li>\n<li><strong>It found the planet has a sulfur-rich atmosphere<\/strong>, the new results suggest. Astronomers said it might be an active volcanic world, with volcanoes reminiscent of those on Jupiter\u2019s volcanic moon Io.<\/li>\n<\/ul>\n<p>The 2025 EarthSky Lunar Calendar is now available! A unique and beautiful poster-sized calendar. Makes a great gift. Get yours today!<\/p>\n<h3>Is this a volcanic exoplanet?<\/h3>\n<p>Volcanoes are common in our solar system. Earth, Mars and Venus all have them. Even some moons do, for example, Jupiter\u2019s moon Io. But what about distant exoplanets around other stars? On November 11, 2024, researchers at The Open University in the U.K. said they\u2019ve found possible evidence for a sulfur-rich atmosphere on a planet 35 light-years away. The planet is labeled L 98-59 d. It\u2019s about 1.5 times the size of Earth. The researchers tentatively detected the gases sulfur dioxide (SO2) and hydrogen sulfide (H2S) in its atmosphere. If confirmed, it would indicate the surface is likely molten or volcanic. Exoplanet L 98-59 d would also be the smallest of the distant planets known so far that have confirmed atmospheres.<\/p>\n<p>The researchers used NASA\u2019s Webb Space Telescope to make the discovery.<\/p>\n<p>Researcher Agnibha Banerjee at The Open University wrote about the new findings in The Conversation on November 11, 2024.<\/p>\n<p>The researchers published their peer-reviewed findings in <em>The Astrophysical Letters<\/em> on October 30, 2024.<\/p>\n<h3>Meet L 98-59 d<\/h3>\n<p>L 98-59 d is a rocky planet, like Earth, and about 1.5 times the size of Earth. This puts it in the category of super-Earth. It orbits an M-type star \u2013 or red dwarf \u2013 35 light-years from Earth. NASA\u2019s Transiting Exoplanet Survey Satellite (TESS) space telescope discovered it in 2019. <\/p>\n<p>TESS used the transit method to detect the planet. That\u2019s when a planet transits \u2013 passes in front of \u2013 its star, as seen from Earth. L 98-59 d orbits close to its star, completing an orbit in only 7.5 days.<\/p>\n<blockquote class=\"twitter-tweet\" data-width=\"500\" data-dnt=\"true\">\n<p lang=\"en\" dir=\"ltr\">&#8220;Researchers, including academics from The Open University (OU) have discovered a possible sulphur-rich atmosphere of exoplanet L 98-59 d, signalling possible volcanoes on its surface.&#8221;<\/p>\n<p>Read more on <a rel=\"nofollow\" href=\"https:\/\/twitter.com\/hashtag\/OUNews?src=hash&amp;ref_src=twsrc%5Etfw\">#OUNews<\/a>! <a rel=\"nofollow\" href=\"https:\/\/t.co\/SlLf4gYxvP\">pic.twitter.com\/SlLf4gYxvP<\/a><\/p>\n<p>\u2014 Faculty of STEM, The Open University (@OU_STEM) <a rel=\"nofollow\" href=\"https:\/\/twitter.com\/OU_STEM\/status\/1852650664955887683?ref_src=twsrc%5Etfw\">November 2, 2024<\/a><\/p>\n<\/blockquote>\n<h3>A volcanic exoplanet with a sulfur-rich atmosphere?<\/h3>\n<p>Banerjee and colleagues used NASA\u2019s Webb Space Telescope to observe one transit of the planet. As the planet passed in front of the star, Webb tried to detect an atmosphere. It did so by analyzing the transmission spectrum of the planet. That is where some light is absorbed by the atmosphere and some is transmitted through it. In the spectrum, the dark lines and dim bands of light correspond to atoms and molecules in the planet\u2019s atmosphere. And, indeed, the analysis showed evidence of a possible atmosphere, more specifically an atmosphere filled with sulfur dioxide and hydrogen sulfide. The paper stated:<\/p>\n<blockquote>\n<p>The atmospheric spectrum indicates the possible presence of the sulfur-bearing species H2S and SO2, which could hint at active volcanism on this planet if verified by future observations.<\/p>\n<\/blockquote>\n<p>What does that mean?<\/p>\n<figure id=\"attachment_493477\" aria-describedby=\"caption-attachment-493477\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/earthsky.org\/upl\/2024\/11\/Io-moon-volcanoes-June-28-1997.jpg\" alt=\"Planet-like body with mottled surface of various bright colors, on black background. A small bluish plume shape is at the top.\" width=\"800\" height=\"578\" class=\"size-full wp-image-493477\" srcset=\"https:\/\/earthsky.org\/upl\/2024\/11\/Io-moon-volcanoes-June-28-1997.jpg 800w, https:\/\/earthsky.org\/upl\/2024\/11\/Io-moon-volcanoes-June-28-1997-300x217.jpg 300w, https:\/\/earthsky.org\/upl\/2024\/11\/Io-moon-volcanoes-June-28-1997-768x555.jpg 768w\" sizes=\"auto, (max-width: 800px) 100vw, 800px\"\/><figcaption id=\"caption-attachment-493477\" class=\"wp-caption-text\">View larger. | L 98-59 d\u2019s volcanoes are likely more similar to those on Jupiter\u2019s moon Io than those on Earth. NASA\u2019s Galileo spacecraft obtained this image on June 28, 1997. Here, an active volcano erupts on the moon\u2019s limb at the top. Image via NASA\/JPL\/ University of Arizona.<\/figcaption><\/figure>\n<h3>A volcanic world, but not like Earth<\/h3>\n<p>The discovery of those two gases suggests L 98-59 d is likely a volcanic or molten world. However, it would be unlike any of the planets in our solar system that have volcanoes. Earth, of course, has many active volcanoes. In addition, there is growing evidence that Venus\u2019 volcanoes are still active as well. And there are huge volcanoes on Mars, although they have been dead or dormant for millions to billions of years. But Earth\u2019s atmosphere is dominated by nitrogen, while the atmospheres of Venus and Mars are mostly carbon dioxide.<\/p>\n<h3>An Io-like world?<\/h3>\n<p>So, this means the volcanic processes on L 98-59 d are likely quite different. In fact, they might be more similar to Jupiter\u2019s moon Io, which is the most volcanically active body in our solar system. On Io, tidal heating drives volcanism. Jupiter\u2019s immense gravity pulls and squeezes Io, heating it on the inside.<\/p>\n<p>As a result, Io\u2019s insides are constantly melting and spewing out through volcanoes. This may be similar to L 98-59 d, because it orbits so close to its star.<\/p>\n<p>If L 98-59 d is truly volcanically active, and in a way not seen on rocky planets in our own solar system, that would be exciting for planetary scientists. It would be a chance to get a glimpse of volcanic processes not seen on planets before. As the paper noted:<\/p>\n<blockquote>\n<p>The rocky planets in the solar system all have different atmospheric compositions, and the study of such atmospheres in exoplanetary systems could unlock a rich diversity of unexplored chemistries.<\/p>\n<\/blockquote>\n<p>Bottom line: L 98-59 d, a super-Earth 35 light-years away, may be a volcanic exoplanet. NASA\u2019s Webb space telescope has detected a possible sulfur-rich atmosphere.<\/p>\n<p>Source: Atmospheric Retrievals Suggest the Presence of a Secondary Atmosphere and Possible Sulfur Species on L98-59 d from JWST Nirspec G395H Transmission Spectroscopy<\/p>\n<p>Via The Conversation<\/p>\n<p>Read more:<\/p>\n<p>Is there a volcanic exomoon orbiting this giant exoplanet?<\/p>\n<p>Wow! New volcano on Jupiter\u2019s moon Io<\/p>\n<p>Active Venus volcanoes revealed again in Magellan data<\/p>\n<p><span class=\"cp-load-after-post\"\/><\/div>\n<div>\n<div class=\"post-author\">\n<h4>Paul Scott Anderson<\/h4>\n<p>                    View Articles\n                  <\/p><\/div>\n<div class=\"post-tags\">\n<h6 data-udy-fe=\"text_7c58270d\">About the Author:<\/h6>\n<p>Paul Scott Anderson has had a passion for space exploration that began when he was a child when he watched Carl Sagan\u2019s Cosmos. He studied English, writing, art and computer\/publication design in high school and college. He later started his blog The Meridiani Journal in 2005, which was later renamed Planetaria. He also later started the blog Fermi Paradoxica, about the search for life elsewhere in the universe.&#13;<br \/>\n&#13;<br \/>\nWhile interested in all aspects of space exploration, his primary passion is planetary science and SETI. In 2011, he started writing about space on a freelance basis with Universe Today. He has also written for SpaceFlight Insider and AmericaSpace and has also been published in The Mars Quarterly. He also did some supplementary writing for the iOS app Exoplanet.&#13;<br \/>\n&#13;<br \/>\nHe has been writing for EarthSky since 2018, and also assists with proofing and social media.<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<p><script async src=\"https:\/\/platform.twitter.com\/widgets.js\" charset=\"utf-8\"><\/script><br \/>\n<br \/><br \/>\n<br \/><a href=\"https:\/\/earthsky.org\/space\/volcanic-exoplanet-l-98-59-d-super-earth-exoplanets-volcanoes\/?rand=772280\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Artist\u2019s concept of L 98-59 d, a super-Earth world 35 light-years away. Now, new results from NASA\u2019s Webb Space Telescope suggest it might be an active volcanic exoplanet with a&hellip; <\/p>\n","protected":false},"author":1,"featured_media":791446,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[46],"tags":[],"class_list":["post-791445","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-earth-sky"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/791445","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=791445"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/791445\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/791446"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=791445"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=791445"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=791445"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}