{"id":791958,"date":"2024-12-12T07:09:03","date_gmt":"2024-12-12T12:09:03","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=791958"},"modified":"2024-12-12T07:09:03","modified_gmt":"2024-12-12T12:09:03","slug":"astronomers-map-giant-starspots-on-distant-xx-trianguli","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=791958","title":{"rendered":"Astronomers map giant starspots on distant XX Trianguli"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<figure id=\"attachment_495016\" aria-describedby=\"caption-attachment-495016\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><figcaption id=\"caption-attachment-495016\" class=\"wp-caption-text\">A visualization of starspots on the red giant star XX Trianguli. The size of the sun is shown on the left for comparison. Image via HUN-REN RCAES\/ Zs. Kov\u00e1ri, MOME\/ \u00c1. Radv\u00e1nyi, AIP\/ K. Strassmeier.<\/figcaption><\/figure>\n<li><strong>Astronomers mapped starspots on the red giant star XX Trianguli<\/strong> using Doppler imaging over 16 years. <\/li>\n<li><strong>Some of these distant starspots are big,<\/strong> bigger than our entire sun!<\/li>\n<li><strong>XX Trianguli\u2019s starspot activity is chaotic and non-periodic<\/strong>, in contrast to our sun\u2019s regular 11-year cycle of activity.<\/li>\n<h3>XX Trianguli as \u2018the most spotted star in the sky\u2019<\/h3>\n<p>If you follow EarthSky\u2019s daily sun news, you know an active sun has many sunspots, or temporary dark spots on its surface. Our sun is a star, so it\u2019s no surprise that distant stars have dark spots, too. Astronomers call them starspots. On December 4, 2024, astronomers at Konkoly Thege Mikl\u00f3s Astronomical Institute in Hungary said they\u2019ve mapped starspots on a star called XX Trianguli. They found this star has enormous spots, bigger than our entire sun! But, unlike our sun \u2013 which waxes and wanes in activity over an 11-year cycle \u2013 XX Trianguli appears to lack a regular cycle of producing spots.<\/p>\n<p>The researchers published their study in the peer-reviewed journal <em>Nature Communications<\/em> on December 4, 2024. <\/p>\n<p>XX Trianguli is located in the direction of our northern constellation Triangulum. It\u2019s about 642 light-years away. And this star is about the same mass as our sun. But the star is about 10 times bigger than our sun, because its outer layers have expanded outward. <\/p>\n<p>In other words, XX Trianguli is a red giant, near the end of its evolutionary lifetime. Zsolt Kov\u00e1ri, at the Konkoly Observatory in Hungary, explained:<\/p>\n<blockquote>\n<p>The large-amplitude variations in the brightness of the red giant XX Trianguli have been observed before, so it was also known that the variations were caused by dark spots, coming in and out view as the star rotates around its axis in 24 days. These spots are even larger than the entire surface of our sun, which is why XX Trianguli has been dubbed \u2018the most spotted star in the sky.\u2019<\/p>\n<\/blockquote>\n<h3>The sun\u2019s a pretty stable star<\/h3>\n<p>The creation and maintenance of our sun\u2019s magnetic field is thanks to what scientists call a solar dynamo. The movement of charged particles inside the sun, and the sun\u2019s rotation, are the main drivers of this dynamo.<\/p>\n<p>Characteristics of the sun\u2019s magnetic field, in turn, drive the 11-year sun cycle of activity. Each cycle sees an increase, then a decrease, in sun surface phenomena such as solar flares and sunspots. Throughout 2024, our sun has been extremely active. Experts at NASA believe it reached the peak of the current sunspot cycle this fall.<\/p>\n<h3>XX Trianguli\u2019s starspots show it\u2019s a chaotic star<\/h3>\n<p>In contrast, the distant star XX Trianguli doesn\u2019t have a regular sunspot cycle. In fact, the astronomers said its dynamo is <\/p>\n<blockquote>\n<p>\u2026 Non-periodic, most likely chaotic in nature.<\/p>\n<\/blockquote>\n<p>Kov\u00e1ri commented:<\/p>\n<blockquote>\n<p>The solar dynamo shows a cyclic behavior in the number and distribution of sunspots that repeats every 11 years on average, known as the butterfly diagram. However, XX Trianguli is a red giant star about 10 times larger than the sun and its internal structure differs significantly from the sun\u2019s, which is a main sequence dwarf. We found no evidence of similar cycles for XX Trianguli.<\/p>\n<p>By studying stellar dynamos, we can also get closer to understanding the solar dynamo. Moreover, dynamo operation is not only responsible for the magnetic features on the sun or other spotted stars, but also the Earth\u2019s magnetic field is created by a similar mechanism, which, on the other hand, happens to protect our technical civilization from harmful solar storms. <\/p>\n<p>Our goal is to be able to observe the manifestations of the dynamo mechanism in as many stars with different characteristics as possible, since by knowing the similarities and differences, we will ultimately better understand the processes that shape our own environment.<\/p>\n<\/blockquote>\n<p><iframe loading=\"lazy\" title=\"16 years of XX Trianguli\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/T0VGzGRBOqY?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><br \/><em>This video about the starspots on XX Trianguli is from Konkoly Observatory in Hungary.<\/em> <\/p>\n<h3>Mapping starspots on a distant star<\/h3>\n<p>From 2006 to 2022, scientists observed XX Trianguli using the STELLA robotic telescopes in Tenerife, Spain. This twin telescope system, operated remotely, is designed to monitor activity on the surface of stars. <\/p>\n<p>Overall, the researchers collected over 2,000 XX Trianguli spectra (measurements of the star\u2019s component colors) over 16 years. Then, they used the spectra to reconstruct 99 images of the star\u2019s surface, using a technique called Doppler imaging.<\/p>\n<figure id=\"attachment_495015\" aria-describedby=\"caption-attachment-495015\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/earthsky.org\/upl\/2024\/12\/Stella-robotic-observatory.jpeg\" alt=\"Two telescopes on a mountaintop, in the same building. On either side of them are curved roof covers that can be drawn in to shelter the observatory.\" width=\"800\" height=\"600\" class=\"size-full wp-image-495015\" srcset=\"https:\/\/earthsky.org\/upl\/2024\/12\/Stella-robotic-observatory.jpeg 800w, https:\/\/earthsky.org\/upl\/2024\/12\/Stella-robotic-observatory-300x225.jpeg 300w, https:\/\/earthsky.org\/upl\/2024\/12\/Stella-robotic-observatory-768x576.jpeg 768w\" sizes=\"auto, (max-width: 800px) 100vw, 800px\"\/><figcaption id=\"caption-attachment-495015\" class=\"wp-caption-text\">The STELLA Robotic Observatory in Tenerife, Spain. Image via Michael Weber\/ Wikimedia Commons (CC BY-SA 2.0 DE).<\/figcaption><\/figure>\n<h3>Doppler imaging<\/h3>\n<p>Doppler imaging is a method for visualizing the surface of bright stars. Basically, using specialized equipment, astronomers break up a star\u2019s light into its component colors. This observing technique is spectroscopy. Within this rainbow \u2013 or the spectrum \u2013 are dark spectral lines. Elements on the star\u2019s surface, like sodium and calcium, create these lines by absorbing light at specific wavelengths. As the star rotates, wavelengths of light from different surface regions shift slightly from their expected positions (a phenomenon called the Doppler effect). With this in mind, astronomers use advanced calculations to interpret those shifts to produce a surface map of the star. <\/p>\n<p>Kov\u00e1ri said the observations of this spotted star will continue and might reveal future details about the star\u2019s dynamo operation.<\/p>\n<figure id=\"attachment_495017\" aria-describedby=\"caption-attachment-495017\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/earthsky.org\/upl\/2024\/12\/XX-Trianguli-99-maps.png\" alt=\"A compilation of 99 individual maps showing starspots. Each map is in an orange rectangle with dark patches indicating the sunspots.\" width=\"650\" height=\"767\" class=\"size-full wp-image-495017\" srcset=\"https:\/\/earthsky.org\/upl\/2024\/12\/XX-Trianguli-99-maps.png 650w, https:\/\/earthsky.org\/upl\/2024\/12\/XX-Trianguli-99-maps-254x300.png 254w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\"\/><figcaption id=\"caption-attachment-495017\" class=\"wp-caption-text\">Mercator projections of the starspots on XX Trianguli, obtained using Doppler imaging. In all, scientists created 99 maps over 16 years. Image via Strassmeier, K. G., et al.\/ Nature Communications (CC BY-NC-ND 4.0).<\/figcaption><\/figure>\n<p>Bottom line: Astronomers have mapped starspots over a 16-year period on a star named XX Trianguli using advanced Doppler imaging techniques.<\/p>\n<p>Source: Long-term Doppler imaging of the star XX Trianguli indicates chaotic non-periodic dynamo<\/p>\n<p>Via Konkoly Observatory <\/p>\n<p>Read more: Polaris, the North Star, has spots on its surface<\/p>\n<p><span class=\"cp-load-after-post\"\/><\/div>\n<div>\n<div class=\"post-author\">\n<h4>Shireen Gonzaga<\/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>Shireen Gonzaga is a freelance writer who enjoys writing about natural history. She is also a technical editor at an astronomical observatory where she works on documentation for astronomers.<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"https:\/\/earthsky.org\/space\/astronomers-map-starspots-xx-trianguli\/?rand=772280\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>A visualization of starspots on the red giant star XX Trianguli. The size of the sun is shown on the left for comparison. Image via HUN-REN RCAES\/ Zs. Kov\u00e1ri, MOME\/&hellip; <\/p>\n","protected":false},"author":1,"featured_media":791959,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[46],"tags":[],"class_list":["post-791958","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\/791958","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=791958"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/791958\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/791959"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=791958"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=791958"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=791958"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}