{"id":197356,"date":"2017-06-07T17:52:44","date_gmt":"2017-06-07T21:52:44","guid":{"rendered":"http:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/astronomers-find-planet-hotter-than-most-stars-astronomy-now-online\/"},"modified":"2017-06-07T17:52:44","modified_gmt":"2017-06-07T21:52:44","slug":"astronomers-find-planet-hotter-than-most-stars-astronomy-now-online","status":"publish","type":"post","link":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/astronomy\/astronomers-find-planet-hotter-than-most-stars-astronomy-now-online\/","title":{"rendered":"Astronomers find planet hotter than most stars &#8211; Astronomy Now Online"},"content":{"rendered":"<p><p>This artists concept  shows planet KELT-9b orbiting its host star, KELT-9. It is the  hottest gas giant planet discovered so far. Credit:  NASA\/JPL-Caltech  <\/p>\n<p>    A newly discovered Jupiter-like world is so hot, its being    vaporized by its own star.  <\/p>\n<p>    With a dayside temperature of more than 7,800 degrees    Fahrenheit (4,600 Kelvin), KELT-9b is a planet that is hotter    than most stars. But its blue A-type star, called KELT-9, is    even hotter  in fact, it is probably unraveling the planet    through evaporation.  <\/p>\n<p>    This is the hottest gas giant planet that has ever been    discovered, said Scott Gaudi, astronomy professor at The Ohio    State University in Columbus, who led a study on the topic. He    worked on this study while on sabbatical at NASAs Jet    Propulsion Laboratory, Pasadena, California. The unusual planet    is described in the journal Nature and at a presentation at the    American Astronomical Society summer meeting this week in    Austin, Texas.  <\/p>\n<p>    KELT-9b is 2.8 times more massive than Jupiter, but only half    as dense. Scientists would expect the planet to have a smaller    radius, but the extreme radiation from its host star has caused    the planets atmosphere to puff up like a balloon.  <\/p>\n<p>    Because the planet is tidally locked to its star  as the moon    is to Earth  one side of the planet is always facing toward    the star, and one side is in perpetual darkness. Molecules such    as water, carbon dioxide and methane cant form on the dayside    because it is bombarded by too much ultraviolet radiation. The    properties of the nightside are still mysterious  molecules    may be able to form there, but probably only temporarily.  <\/p>\n<p>    Its a planet by any of the typical definitions of mass, but    its atmosphere is almost certainly unlike any other planet    weve ever seen just because of the temperature of its    dayside, Gaudi said.  <\/p>\n<p>    The KELT-9 star is only 300 million years old, which is young    in star time. It is more than twice as large, and nearly twice    as hot, as our Sun. Given that the planets atmosphere is    constantly blasted with high levels of ultraviolet radiation,    the planet may even be shedding a tail of evaporated planetary    material like a comet.  <\/p>\n<p>    KELT-9 radiates so much ultraviolet radiation that it may    completely evaporate the planet, said Keivan StasSun, a    professor of physics and astronomy at Vanderbilt University,    Nashville, Tennessee, who directed the study with Gaudi.  <\/p>\n<p>    But this scenario assumes the star doesnt grow to engulf the    planet first.  <\/p>\n<p>    KELT-9 will swell to become a red giant star in a few hundred    million years, said Stassun. The long-term prospects for    life, or real estate for that matter, on KELT-9b are not    looking good.  <\/p>\n<p>    The planet is also unusual in that it orbits perpendicular to    the spin axis of the star. That would be analogous to the    planet orbiting perpendicular to the plane of our solar system.    One year on this planet is less than two days.  <\/p>\n<p>    KELT-9b is nowhere close to habitable, but Gaudi said theres a    good reason to study worlds that are unlivable in the extreme.  <\/p>\n<p>    As has been highlighted by the recent discoveries from the    MEarth collaboration, the planet around Proxima Centauri, and    the astonishing system discovered around TRAPPIST-1, the    astronomical community is clearly focused on finding Earth-like    planets around small, cooler stars like our Sun. They are easy    targets and theres a lot that can be learned about potentially    habitable planets orbiting very low-mass stars in general. On    the other hand, because KELT-9bs host star is bigger and    hotter than the Sun, it complements those efforts and provides    a kind of touchstone for understanding how planetary systems    form around hot, massive stars, Gaudi said.  <\/p>\n<p>    The KELT-9b planet was found using one of the two telescopes    called KELT, or Kilodegree Extremely Little Telescope. In late    May and early June 2016, astronomers using the KELT-North    telescope at Winer Observatory in Arizona noticed a tiny drop    in the stars brightness  only about half of one percent     which indicated that a planet may have passed in front of the    star. The brightness dipped once every 1.5 days, which means    the planet completes a yearly circuit around its star every    1.5 days.  <\/p>\n<p>    Subsequent observations confirmed the signal to be due to a    planet, and revealed it to be what astronomers call a hot    Jupiter  the kind of planet the KELT telescopes are designed    to spot.  <\/p>\n<p>    Astronomers at Ohio State, Lehigh University in Bethlehem,    Pennsylvania, and Vanderbilt jointly operate two KELTs (one    each in the northern and southern hemispheres) to fill a large    gap in the available technologies for finding exoplanets. Other    telescopes are designed to look at very faint stars in much    smaller sections of the sky, and at very high resolution. The    KELTs, in contrast, look at millions of very bright stars at    once, over broad sections of sky, and at low resolution.  <\/p>\n<p>    This discovery is a testament to the discovery power of small    telescopes, and the ability of citizen scientists to directly    contribute to cutting-edge scientific research, said Joshua    Pepper, astronomer and assistant professor of physics at Lehigh    University in Bethlehem, Pennsylvania, who built the two KELT    telescopes.  <\/p>\n<p>    The astronomers hope to take a closer look at KELT-9b with    other telescopes  including NASAs Spitzer and Hubble space    telescopes, and eventually the James Webb Space Telescope,    which is scheduled to launch in 2018. Observations with Hubble    would enable them to see if the planet really does have a    cometary tail, and allow them to determine how much longer that    planet will survive its current hellish condition.  <\/p>\n<p>    Thanks to this planets star-like heat, it is an exceptional    target to observe at all wavelengths, from ultraviolet to    infrared, in both transit and eclipse. Such observations will    allow us to get as complete a view of its atmosphere as is    possible for a planet outside our solar system, said Knicole    Colon, paper co-author who was based at NASA Ames Research    Center in Californias Silicon Valley during the time of this    study.  <\/p>\n<p><!-- Auto Generated --><\/p>\n<p>Visit link: <\/p>\n<p><a target=\"_blank\" rel=\"nofollow\" href=\"https:\/\/astronomynow.com\/2017\/06\/07\/astronomers-find-planet-hotter-than-most-stars\/\" title=\"Astronomers find planet hotter than most stars - Astronomy Now Online\">Astronomers find planet hotter than most stars - Astronomy Now Online<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p> This artists concept shows planet KELT-9b orbiting its host star, KELT-9. It is the hottest gas giant planet discovered so far <a href=\"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/astronomy\/astronomers-find-planet-hotter-than-most-stars-astronomy-now-online\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":3,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[257798],"tags":[],"class_list":["post-197356","post","type-post","status-publish","format-standard","hentry","category-astronomy"],"_links":{"self":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/posts\/197356"}],"collection":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/comments?post=197356"}],"version-history":[{"count":0,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/posts\/197356\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/media?parent=197356"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/categories?post=197356"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/tags?post=197356"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}