{"id":11198,"date":"2024-06-12T18:00:18","date_gmt":"2024-06-12T22:00:18","guid":{"rendered":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/coming-in-hot-nasas-chandra-checks-habitability-of-exoplanets\/"},"modified":"2024-06-12T18:00:18","modified_gmt":"2024-06-12T22:00:18","slug":"coming-in-hot-nasas-chandra-checks-habitability-of-exoplanets","status":"publish","type":"post","link":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/coming-in-hot-nasas-chandra-checks-habitability-of-exoplanets\/","title":{"rendered":"Coming in Hot \u2014 NASA\u2019s Chandra Checks Habitability of Exoplanets"},"content":{"rendered":"<h2 style=\"text-align: center;\">Coming in Hot \u2014 NASA\u2019s Chandra Checks Habitability of Exoplanets<\/h2>\n<p><!-- no image --><\/p>\n<div class=\"width-full maxw-full margin-left-auto margin-right-auto hds-media-align-inline hds-module wp-block-nasa-blocks-video\">\n<div class=\"hds-cover-wrapper width-full maxw-full flex-column\">\n<div class=\"hds-video-container width-full embed-container\"><video title=\"exoplanets-890e3c\" class=\"video-js video-player vjs-fluid width-full\" data-setup='{\"controls\":true,\"preload\":\"auto\",\"plugins\":{\"mux\":{\"debug\":false,\"data\":{\"env_key\":\"91nns8oppqdfqc44lgo4b1gni\",\"player_name\":\"www.nasa.gov Player\",\"video_name\":\"exoplanets-890e3c\"}}}}' preload=\"none\"><source src=\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2024\/06\/exoplanets-890e3c.mp4\" type=\"video\/mp4\"><p class=\"vjs-no-js\">To view this video please enable JavaScript, and consider upgrading to a web browser that<br \/>\n\t\t\t\t\t<a href=\"https:\/\/videojs.com\/html5-video-support\/\" target=\"_blank\" rel=\"noopener\">supports HTML5 video<\/a><\/p>\n<p><\/source><\/video><\/div>\n<\/div>\n<div class=\"hds-media-caption hds-caption padding-y-2\">\n<div class=\"hds-credits\">\n<div>Movie: Cal Poly Pomona\/B. Binder; Illustration: NASA\/CXC\/M.Weiss<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>This graphic shows a three-dimensional map of stars near the Sun. These stars are close enough that they could be prime targets for direct imaging searches for planets using future telescopes. The blue haloes represent stars that have been observed with NASA\u2019s Chandra X-ray Observatory and ESA\u2019s XMM-Newton. The yellow star at the center of this diagram represents the position of the Sun. The concentric rings show distances of 5, 10, and 15 parsecs (one parsec is equivalent to roughly 3.2 light-years).<\/p>\n<p>Astronomers are using these X-ray data to determine how habitable exoplanets may be based on whether they receive lethal radiation from the stars they orbit, as described in\u00a0<a href=\"https:\/\/chandra.cfa.harvard.edu\/press\/24_releases\/press_061224.html\" rel=\"noopener\">our latest press release<\/a>. This type of research will help guide observations with the next generation of telescopes aiming to make the first images of planets like Earth.<\/p>\n<p>Researchers examined stars that are close enough to Earth that telescopes set to begin operating in the next decade or two \u2014 including the Habitable Worlds Observatory in space and Extremely Large Telescopes on the ground \u2014 could take images of planets in the stars\u2019 so-called habitable zones. This term defines orbits where the planets could have liquid water on their surfaces.<\/p>\n<p>There are several factors influencing what could make a planet suitable for life as we know it. One of those factors is the amount of harmful X-rays and ultraviolet light they receive, which can damage or even strip away the planet\u2019s atmosphere.<\/p>\n<p>Based on X-ray observations of some of these stars using data from Chandra and XMM-Newton, the research team examined which stars could have hospitable conditions on orbiting planets for life to form and prosper. They studied how bright the stars are in X-rays, how energetic the X-rays are, and how much and how quickly they change in X-ray output, for example, due to flares. Brighter and more energetic X-rays can cause more damage to the atmospheres of orbiting planets.<\/p>\n<p>The researchers used almost 10 days of Chandra observations and about 26 days of XMM observations, available in archives, to examine the X-ray behavior of 57 nearby stars, some of them with known planets. Most of these are giant planets like Jupiter, Saturn or Neptune, while only a handful of planets or planet candidates could be less than about twice as massive as Earth.<\/p>\n<p>These results were presented at the 244th meeting of the American Astronomical Society meeting in Madison, Wisconsin, by Breanna Binder (California State Polytechnic University in Pomona).<\/p>\n<p>NASA\u2019s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory\u2019s Chandra X-ray Center controls science from Cambridge, Massachusetts and flight operations from Burlington, Massachusetts.<\/p>\n<p><a href=\"https:\/\/chandra.harvard.edu\/photo\/2024\/exoplanets\/\" rel=\"noopener\">Read more from NASA\u2019s Chandra X-ray Observatory.<\/a><\/p>\n<p>For more Chandra images, multimedia and related materials, visit:<\/p>\n<p class=\"has-text-align-center\"><a href=\"https:\/\/www.nasa.gov\/mission\/chandra-x-ray-observatory\/\">https:\/\/www.nasa.gov\/mission\/chandra-x-ray-observatory\/<\/a><\/p>\n<p><strong>Visual Description:<\/strong><\/p>\n<p>This video shows a three-dimensional map of stars near the Sun on the left side of our screen and a dramatic illustration of a star with a planet orbiting around it on the right side.<\/p>\n<p>The star map on the left shows many circular dots of different colors floating within an illustrated three-sided box. Each wall of the box is constructed in a grid pattern, with straight lines running horizontally and vertically like chicken wire. Dots that are colored blue represent stars that have been observed with NASA\u2019s Chandra and ESA\u2019s XMM-Newton.<\/p>\n<p>Suspended in the box, at about the halfway point, is a series of three concentric circles surrounding a central dot that indicates the placement of our Sun. The circles represent distances of 5, 10, and 15 parsecs. One parsec is equivalent to roughly 3.2 light-years.<\/p>\n<p>In the animation, the dot filled, chicken wire box spins around slowly, first on its X axis and then on its Y axis, providing a three-dimensional exploration of the plotted stars.<\/p>\n<h2 class=\"wp-block-heading\">News Media Contact<\/h2>\n<p>Megan Watzke<br \/>Chandra X-ray Center<br \/>Cambridge, Mass.<br \/>617-496-7998<\/p>\n<p>Jonathan Deal<br \/>Marshall Space Flight Center<br \/>Huntsville, Ala.<br \/>256-544-0034<\/p>\n<p class=\"wpematico_credit\"><small>Powered by <a href=\"http:\/\/www.wpematico.com\" target=\"_blank\" rel=\"noopener\">WPeMatico<\/a><\/small><\/p>\n<p><a href=\"https:\/\/www.nasa.gov\/missions\/chandra\/coming-in-hot-nasas-chandra-checks-habitability-of-exoplanets\/\" target=\"_blank\" rel=\"noopener\">Get The Details&#8230;<\/a><br \/>\nLee Mohon  <\/p>\n","protected":false},"excerpt":{"rendered":"<p>This graphic shows a three-dimensional map of stars near the Sun. These stars are close enough that they could be prime targets for direct imaging searches for planets using future telescopes. The blue haloes represent stars that have been observed with NASA\u2019s Chandra X-ray Observatory and ESA\u2019s XMM-Newton. 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