{"id":24032,"date":"2024-05-19T17:12:46","date_gmt":"2024-05-19T09:12:46","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/astronomers-find-an-earth-sized-exoplanet-around-a-tiny-star-and-a-large-but-ultra-light-exoplanet-around-a-sun-like-star\/"},"modified":"2024-05-19T17:12:46","modified_gmt":"2024-05-19T09:12:46","slug":"astronomers-find-an-earth-sized-exoplanet-around-a-tiny-star-and-a-large-but-ultra-light-exoplanet-around-a-sun-like-star","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/astronomers-find-an-earth-sized-exoplanet-around-a-tiny-star-and-a-large-but-ultra-light-exoplanet-around-a-sun-like-star\/","title":{"rendered":"Astronomers find an Earth-sized exoplanet around a tiny star and a large, but ultra-light exoplanet around a Sun-like star"},"content":{"rendered":"<p>Astronomers from the Search for Planets Eclipsing Ultra-cool Stars (SPECULOOS) project found an Earth-sized exoplanet orbiting an ultracool dwarf star about 55 light-years away. The team concluded that the exoplanet, called SPECULOOS-3b, likely has a rocky surface and no atmosphere.<\/p>\n<p>The SPECULOOS project is a network of six robotic telescopes, four in the Southern Hemisphere and two in the Northern Hemisphere, that aims to search for exoplanets around 1,600 nearby ultracool dwarf stars.<\/p>\n<p>Moreover, some of the project\u2019s scientists are part of an international collaboration that found a giant, but ultra-light exoplanet called WASP-193b. The exoplanet is about 1.5 times the size of Jupiter but has a mass only about one-seventh that of Jupiter. The planet is so light that the teams compare its density with that of cotton candy.<\/p>\n<\/p>\n<p>An Earth-sized exoplanet around a tiny star<\/p>\n<p>The SPECULOOS project first studied SPECULOOS-3b\u2019s star in 2019 and 2021. While the observations from 2021 showed signs of a planet, the results were inconclusive as the signal was distorted by noise caused by bad weather on the day of observation. When <em>Artemis<\/em>, the SPECULOOS Northern Observatory\u2019s telescope in Tenerife, Spain, observed the star in July 2022, the observations showed a clear signature of an exoplanet.<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" aria-describedby=\"caption-attachment-99999\" class=\"size-full wp-image-99999\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/SPECULOOS-3_NASA-scaled.jpg\" alt=\"\" width=\"2560\" height=\"1440\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/SPECULOOS-3_NASA-scaled.jpg 2560w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/SPECULOOS-3_NASA-350x197.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/SPECULOOS-3_NASA-622x350.jpg 622w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/SPECULOOS-3_NASA-768x432.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/SPECULOOS-3_NASA-1920x1080.jpg 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/SPECULOOS-3_NASA-1170x658.jpg 1170w\" sizes=\"(max-width: 2560px) 100vw, 2560px\"><\/p>\n<p id=\"caption-attachment-99999\" class=\"wp-caption-text\">Artist\u2019s impression of SPECULOOS-3b orbiting it\u2019s flaring, ultracool brown dwarf star. (Credit: NASA\/JPL-Caltech)<\/p>\n<p>When an exoplanet transits its star, which means it passes in front of its star from Earth\u2019s perspective, the star appears slightly dimmer. Astronomers study how the star\u2019s light changes during these transits to infer the exoplanet\u2019s properties.<\/p>\n<h4 class=\"widget-title penci-border-arrow\">See Also<\/h4>\n<ul>\n<li>Astronomy &amp; Planetary Science<\/li>\n<li>Space Science Section<\/li>\n<li>Click here to join L2<\/li>\n<\/ul>\n<p>\u201cWhile there were structures in the 2021 data that didn\u2019t look convincing, the 2022 Artemis data really got our attention,\u201d said Artem Burdanov of the Massachusetts Institute of Technology (MIT), who manages the SPECULOOS Northern Observatory. \u201cWe started to analyze one clear transit-like signal in the Artemis data, quickly decided to launch a campaign around this star, and then things just started lining up.\u201d<\/p>\n<p>Space Shuttle models<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>Aerospace &amp; Defense<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>NASA mission patches<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>\n<p>     (adsbygoogle = window.adsbygoogle || []).push({});<\/p>\n<p>With the new observations, the scientists could measure the size of SPECULOOS-3b and its star. They found that the star was similar in size to Jupiter or about one-tenth the size of the Sun. By measuring how much the star dimmed during transits, the team concluded that SPECULOOS-3b must be about the same size as the Earth.<\/p>\n<p>Additionally, the team found that the exoplanet orbits its star in about 17 hours, at a very close distance. \u201cWe believe that the planet rotates synchronously, so that the same side, called the day side, always faces the star, just like the Moon does for the Earth. On the other hand, the night side hand, would be locked in endless darkness,\u201d said study lead Micha\u00ebl Gillon of the University of Li\u00e8ge in Belgium.<\/p>\n<p><iframe id=\"twitter-widget-1\" scrolling=\"no\" frameborder=\"0\" allowtransparency=\"true\" allowfullscreen=\"true\" class=\"\" style=\"position: static; visibility: visible; width: 0px; height: 0px; display: block; flex-grow: 1;\" title=\"X Post\" src=\"https:\/\/platform.twitter.com\/embed\/Tweet.html?creatorScreenName=NASASpaceflight&amp;dnt=true&amp;embedId=twitter-widget-1&amp;features=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%3D%3D&amp;frame=false&amp;hideCard=false&amp;hideThread=false&amp;id=1790685564779339985&amp;lang=en&amp;origin=https%3A%2F%2Fwww.nasaspaceflight.com%2F2024%2F05%2Fspeculoos-3b-and-wasp-193b%2F&amp;sessionId=a1bbcbbd3018f3b8b3dce4f9cd0badb7fee06a53&amp;siteScreenName=NASASpaceflight&amp;theme=light&amp;widgetsVersion=6a3ad42b224df%3A1778106238597&amp;width=550px\" data-gtm-yt-inspected-13=\"true\" data-gtm-yt-inspected-20=\"true\" data-tweet-id=\"1790685564779339985\"><\/iframe><\/p>\n<blockquote class=\"twitter-tweet\" data-width=\"550\" data-dnt=\"true\" data-twitter-extracted-i1783494460008515577=\"true\">\n<p lang=\"en\" dir=\"ltr\">Astronomer Micha\u00ebl Gillon and the #SPECULOOS team discovered a new Earth-sized exoplanet around SPECULOOS-3, an &#8220;ultracool dwarf&#8221; star as small as Jupiter, twice as cold as our Sun, and located  55 light-years from Earth.&nbsp;#ULi\u00e8ge @NatureAstronomy @NASA https:\/\/t.co\/2bQGJNhBmz pic.twitter.com\/K0l9RBpbD6<\/p>\n<p>\u2014 Universit\u00e9 de Li\u00e8ge (@UniversiteLiege) May 15, 2024<\/p>\n<\/blockquote>\n<p>Even though the ultracool dwarf star is 1,000 times dimmer than the sun and about twice as cold, NASA\u2019s Transiting Exoplanet Survey Satellite (TESS) revealed it is very active. This, combined with the short distance between SPECULOOS-3b and its star, means that the exoplanet is continuously bombarded with radiation, about 16 times more than the Earth receives from the sun. The astronomers believe this radiation has likely stripped any atmosphere away, leaving a bare rocky surface.<\/p>\n<p>The team believes that SPECULOOS-3b is a great target for future studies by the joint NASA, European Space Agency, and Canadian Space Agency James Webb Space Telescope (JWST). The lack of atmosphere would allow Webb to study the exoplanet\u2019s surface and its geological history. A brighter surface would reveal recent geological activity, as older surfaces become darker from erosion by meteoroid impacts or other influences from space.<\/p>\n<p>\u201cSPECULOOS-3b is the first planet for which we can consider moving toward constraining surface properties of planets beyond the solar system,\u201d&nbsp;says co-author Julien de Wit of MIT. \u201cWith this world, we could basically start doing exoplanetary geology. How cool is that?\u201d<\/p>\n<p>Gillon et al.\u2019s results were published in the journal <em>Nature Astronomy<\/em> on May 15.<\/p>\n<p>A large, but ultra-light exoplanet around a Sun-like star<\/p>\n<p>WASP-193b orbits a Sun-like star about 1,200 light years from Earth, completing one orbit every 6.25 days. By analyzing how much of the star\u2019s light was blocked during transits, the scientists concluded that the planet is substantially bigger than Jupiter, with a radius about 1.5 times larger.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-100000\" class=\"size-full wp-image-100000\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/MIT-PuffPlanet-01-press.jpg\" alt=\"\" width=\"1920\" height=\"1920\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/MIT-PuffPlanet-01-press.jpg 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/MIT-PuffPlanet-01-press-350x350.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/MIT-PuffPlanet-01-press-768x768.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/MIT-PuffPlanet-01-press-1170x1170.jpg 1170w\" sizes=\"(max-width: 1920px) 100vw, 1920px\"><\/p>\n<p id=\"caption-attachment-100000\" class=\"wp-caption-text\">Artist\u2019s impression of puffy Jupiter WASP-193b orbiting it\u2019s Sun-like star. (Credit: K. Ivanov)<\/p>\n<p>The exoplanet was originally detected and studied by the Wide Angle Search for Planets (WASP) project. The team used additional observations, among which observations by one of SPECULOOS telescopes and TESS, to study WASP-193b in more detail.<\/p>\n<p>\u201cTypically, big planets are pretty easy to detect because they are usually massive, and lead to a big pull on their star,\u201d said de Wit. \u201cBut what was tricky about this planet was, even though it\u2019s big \u2014 huge \u2014 its mass and density are so low that it was actually very difficult to detect with just the radial velocity technique. It was an interesting twist.\u201d<\/p>\n<p>Using the radial velocity technique, astronomers analyze how the star\u2019s spectrum is distorted by mass pulling on the star. In this technique, a larger mass, or planet, distorts the spectrum more. \u201c[WASP-193b] is so very light that it took four years to gather data and show that there is a mass signal, but it\u2019s really, really tiny,\u201d said lead author Khalid Barkaoui of the University of Li\u00e8ge and MIT.<\/p>\n<p>With the exoplanet\u2019s mass determined as 14 percent that of Jupiter, the team was able to calculate WASP-193b\u2019s density at 0.059 grams per cubic centimeter, which is a lot lower than Jupiter\u2019s density of about 1.33 grams per cubic centimeter and Earth\u2019s of 5.51 grams per cubic centimeter. This makes the planet an extreme example of a class of large and light exoplanets astronomers call puffy Jupiters.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-100001\" class=\"size-full wp-image-100001\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/wasp-193b.jpg\" alt=\"\" width=\"2530\" height=\"1129\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/wasp-193b.jpg 2530w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/wasp-193b-350x156.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/wasp-193b-630x281.jpg 630w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/wasp-193b-768x343.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/wasp-193b-1920x857.jpg 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/05\/wasp-193b-1170x522.jpg 1170w\" sizes=\"(max-width: 2530px) 100vw, 2530px\"><\/p>\n<p id=\"caption-attachment-100001\" class=\"wp-caption-text\">Comparison of various planets, including Jupiter and WASP-193b. (Credit: Barkaoui et al.)<\/p>\n<p>\u201cWASP-193b is the second least dense planet discovered to date, after Kepler-51d, which is much smaller,\u201d explains Barkaoui. \u201cIts extremely low density makes it a real anomaly among the more than five thousand exoplanets discovered to date. This extremely low density cannot be reproduced by standard models of irradiated gas giants, even under the unrealistic assumption of a coreless structure.\u201d<\/p>\n<p>The scientists looked for reasons the exoplanet\u2019s density was so low but came away empty-handed, as none of the standard models could adequately explain the observed density. Instead, the team determined how future studies could provide answers, and concluded that only a single transit observation by Webb could provide a lot more insights into the unique planet.<\/p>\n<p>\u201cThe bigger a planet\u2019s atmosphere, the more light can go through,\u201d said de Wit. \u201cSo it\u2019s clear that this planet is one of the best targets we have for studying atmospheric effects. It will be a Rosetta Stone to try and resolve the mystery of puffy Jupiters.\u201d<\/p>\n<p>Barkaoui et al.\u2019s results were published in the journal <em>Nature Astronomy<\/em> on May 14.<\/p>\n<p><em>(Lead image: artist\u2019s impressions of SPECULOOS-3b (left) and WASP-193b. Credit: L. Garcia (left), K. Ivanov (right))<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Astronomers from the Search for Planets Eclipsing Ultra-cool Stars (SPECULOOS) project found an Earth-sized exoplanet orbiting an ultracool dwarf star about 55 light-years away. The team concluded that the exoplanet, called SPECULOOS-3b, likely has a rocky surface and no atmosphere. The SPECULOOS project is a network of six robotic telescopes, four in the Southern Hemisphere [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[559,8285,8286,8287,8288],"class_list":["post-24032","post","type-post","status-publish","format-standard","hentry","category-news","tag-exoplanets","tag-speculoos-3","tag-speculoos-3b","tag-wasp-193","tag-wasp-193b"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24032"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=24032"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24032\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=24032"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=24032"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=24032"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}