{"id":785721,"date":"2024-07-13T12:01:59","date_gmt":"2024-07-13T17:01:59","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=785721"},"modified":"2024-07-13T12:01:59","modified_gmt":"2024-07-13T17:01:59","slug":"exoplanet-could-be-an-enormous-version-of-europa","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=785721","title":{"rendered":"Exoplanet Could be an Enormous Version of Europa"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<p>Certain exoplanets pique scientists\u2019 interest more than others. Some of the most interesting are those that lie in the habitable zone of their stars. However, not all of those planets would be similar to Earth \u2013 in fact, finding a planet about the size of Earth is already stretching the limits of most exoplanet-hunting telescopes. So the scientific community rejoiced when researchers at the Universit\u00e9 de Montr\u00e9al announced they found an exoplanet in the size range of the Earth. However, it appears to be almost entirely covered in water, making it more similar to a giant version of Europa, the ice-covered moon of Jupiter.\u00a0<\/p>\n<p><span id=\"more-167735\"\/><\/p>\n<p>There\u2019s a lot to unpack in the press release describing the discovery. The exoplanet they studied is known as LHS 1140b. It\u2019s located 48 light-years away in the constellation Cetus, making it one of the closest known exoplanets in its star\u2019s habitable zone.<\/p>\n<p>That star, LHS 1140, is only about 20% the size of our Sun, and the energy it puts out is smaller. LHS 1140b is one of two potential exoplanets orbiting it, but until now, scientists have debated whether it was a \u201cmini-Neptune\u201d or a \u201csuper-Earth.\u201d If it were a \u201cmini-Neptune,\u201d it would be surrounded by hydrogen gas, but the researchers did not find that.<\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\">\n<p>\n<span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" title=\"LHS 1140b - A Habitable Super-Earth 39 Light Years Away?\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/4PVGe2GNbYc?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe><\/span>\n<\/p><figcaption class=\"wp-element-caption\">LHS 1140b has long been a center of attention for astronomers \u2013 as Anton Petrov describes here.<br \/>Credit \u2013 Anton Petrov YouTube Channel<\/figcaption><\/figure>\n<p>They used \u201cdirector\u2019s discretionary time,\u201d which means observational time directly assigned by the project\u2019s director of the James Webb Space Telescope (JWST). They combined it with data collected from TESS, Spitzer, and Hubble. After looking closely at LHS 1140 b\u2019s atmosphere, they saw something familiar\u2014nitrogen. This was interesting for a few reasons. First, it ruled out the possibility of LHS 1140b being a \u201cmini-Neptune,\u201d as the hydrogen-rich atmosphere would have been very distinct in the data.\u00a0<\/p>\n<p>Second, it is now officially the first known temperate exoplanet to have a \u201csecondary\u201d atmosphere \u2013 i.e., one created after the planet\u2019s formation. Nitrogen does not naturally form part of a planet\u2019s atmosphere at the outset and must be developed later through chemical processes. So far, no exoplanets in their star\u2019s habitable zones have been observed with this gas in their atmosphere, though it had long been theorized since our own planet\u2019s atmosphere is so rich in it.<\/p>\n<p>But even more intriguingly, with the possibility that it was a \u201cmini-Neptune\u201d eliminated, it seemed LHS 1140b became a good candidate for a \u201csuper-Earth\u201d \u2013 about 1.7 times larger than our home planet and 5.6 times its mass. However, the researchers also noticed the planet was much less dense than expected, indicating that about 10-20% of that mass could be water rather than rock.<\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\">\n<p>\n<span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" title=\"The Future of Exoplanet Research\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/6b377MO20uE?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe><\/span>\n<\/p><figcaption class=\"wp-element-caption\">Fraser discusses how we JWST to find exoplanets.<\/figcaption><\/figure>\n<p>Having that much water could lead to several different outcomes. First, there is the possibility of LHS 1140b being a \u201cHycean world,\u201d which would be entirely covered by a liquid-water ocean. This seems unlikely, as the star\u2019s energy output doesn\u2019t provide enough energy to keep an entire planet-sized ocean warm enough not to freeze.<\/p>\n<p>This leads to the second possibility\u2014a \u201csnowball\u201d world where a thick layer of snow covers the rocky interior. This is still possible, but it requires weather patterns that might be hard to discern remotely, even with JWST.<\/p>\n<p>So that leaves a final possibility\u2014an ice world, where thick sheets of ice cover the entirety of the planet\u2019s surface. We already know of one such world a lot closer to home\u2014Europa. It is completely covered in ice, though intriguingly, it also has a liquid ocean underneath those ice sheets. The researchers think there is a good chance a similar subsurface ocean could exist on LHS 1140b as well.<\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\">\n<p>\n<span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" title=\"Is There Hope For TRAPPIST-1 Planets with James Webb?\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/mtx72I1r3T4?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe><\/span>\n<\/p><figcaption class=\"wp-element-caption\">Fraser discusses how to research exoplanet atmospheres with JWST.<\/figcaption><\/figure>\n<p>That would make it the first known exoplanet to have confirmed liquid water. However, the data suggested another intriguing possibility \u2013 it could be a snowball planet with a \u201cbull\u2019s eye ocean\u201d at the point where the star\u2019s heat is strongest on it. This ocean could be around 4,000 km across, about half the size of the Atlantic Ocean on Earth. Models suggest that the water temperature in the ocean could even reach 20 C, a comfortable room temperature, though a bit cold to swim in.\u00a0<\/p>\n<p>However, none of these details have been confirmed yet, and doing so will require\u2014you guessed it\u2014more observational time. In particular, the researchers are interested in whether there is carbon dioxide in LHS 1140b\u2019s atmosphere. A greenhouse gas could make it more likely that the planet\u2019s overall temperature would be warm enough to make it a Hycean world rather than a snowball with one isolated ocean.\u00a0<\/p>\n<p>Observing carbon dioxide in an exoplanet as far away as LHS 1140 could take years of intermittent observational time on JWST. While LHS 1140b is now definitively one of the most promising candidates for finding liquid water on a planet\u2019s surface \u2013 and therefore be a prime candidate for finding life on an exoplanet \u2013 continued observation of that kind would have to compete with all the other worthy use cases for JWST\u2019s time.\u00a0<\/p>\n<p>For now, the researchers hope to receive more observational time, even if it isn\u2019t enough to confirm the presence of carbon dioxide. However, eventually, there will be more and stronger planet-hunting telescopes than even the JWST. Someday, there will be enough observational time on at least one of them to confirm whether or not LHS 1140b does indeed have a liquid ocean. That day might be one of the most monumental in the history of the study of exoplanets\u2014and maybe for humanity itself.<\/p>\n<p>Learn More:<br \/>Universit\u00e9 de Montr\u00e9al \u2013 Astronomers Find Surprising Ice World in the Habitable Zone with Webb Data<br \/>Cadieux et al. \u2013 Transmission Spectroscopy of the Habitable Zone Exoplanet LHS 1140 b with JWST\/NIRISS<br \/>UT \u2013 Is This The Exoplanet Where Life Will First Be Found?<br \/>UT \u2013 A New Venus-Sized World Found in the Habitable Zone of its Star<\/p>\n<p>Lead Image:<br \/>Illustration of exoplanet LHS 1140 b, including a \u201cbulls-eye ocean\u201d.<br \/>Credit \u2013 B. Gougeon \/ UdeM<\/p>\n<div class=\"sharedaddy sd-block sd-like jetpack-likes-widget-wrapper jetpack-likes-widget-unloaded\" id=\"like-post-wrapper-24000880-167735-6692aff1a9ac7\" data-src=\"https:\/\/widgets.wp.com\/likes\/?ver=13.2#blog_id=24000880&amp;post_id=167735&amp;origin=www.universetoday.com&amp;obj_id=24000880-167735-6692aff1a9ac7&amp;n=1\" data-name=\"like-post-frame-24000880-167735-6692aff1a9ac7\" data-title=\"Like or Reblog\">\n<h3 class=\"sd-title\">Like this:<\/h3>\n<p><span class=\"button\"><span>Like<\/span><\/span> <span class=\"loading\">Loading&#8230;<\/span><\/p>\n<p><span class=\"sd-text-color\"\/><\/div>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"https:\/\/www.universetoday.com\/167735\/exoplanet-could-be-an-enormous-version-of-europa\/?rand=772204\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Certain exoplanets pique scientists\u2019 interest more than others. Some of the most interesting are those that lie in the habitable zone of their stars. However, not all of those planets&hellip; <\/p>\n","protected":false},"author":1,"featured_media":785722,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[13],"tags":[],"class_list":["post-785721","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-genaero"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/785721","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=785721"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/785721\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/785722"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=785721"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=785721"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=785721"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}