{"id":39519,"date":"2011-09-18T15:46:23","date_gmt":"2011-09-18T15:46:23","guid":{"rendered":"http:\/\/euvolution.com\/futurist-transhuman-news-blog\/a-planet-with-two-suns-is-found\/"},"modified":"2011-09-18T15:46:23","modified_gmt":"2011-09-18T15:46:23","slug":"a-planet-with-two-suns-is-found","status":"publish","type":"post","link":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/astronomy\/a-planet-with-two-suns-is-found.php","title":{"rendered":"A Planet With Two Suns is Found"},"content":{"rendered":"<div><a href=\"http:\/\/euvolution.com\/futurist-transhuman-news-blog\/wp-content\/plugins\/wp-o-matic\/cache\/72eef_ucsb091611.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/euvolution.com\/futurist-transhuman-news-blog\/wp-content\/plugins\/wp-o-matic\/cache\/72eef_ucsb091611.jpg\" alt=\"\" width=\"487\" height=\"365\" style=\"padding-left:10px; padding-right: 10px;\"><\/a><p>Schematic of the planet with two suns. Click for larger. Credit: Avi Shporer and team \/ University of California Santa Barbara<\/p><\/div><p>&nbsp;<\/p><p>Ah this is very cool to think about even beyond Star wars.<\/p><p>By the way, I was out looking for the supernova this morning (thwarted by clouds) but was treated to the Moon and the star Sheratan, a bright bluish star only about 5 degrees away.&nbsp; If you happen out tomorrow about 6 a.m. your time have a look.&nbsp; Tomorrow, it should be clear enough here to also see the star Lorenzin Alpha ARI. Alpha ARI is a bit brighter than Sheratan and a bit yellower. The three should make for a nice pairing.<\/p><p>Back to the two suns, below is a fun snippit from <a href=\"http:\/\/www.ia.ucsb.edu\/pa\/display.aspx?pkey=2561\">the press release from the University of California Santa Barbara <\/a>and clicking the &ldquo;more&rdquo; link at the bottom will get you the entire press release or you can just click the link.<\/p><blockquote><p>The planet&rsquo;s orbital period is 229 days, while the stellar binary has a 41-day orbit. Although the planet&rsquo;s orbital period is close to that of Venus in our solar system, it is not an Earth-like, terrestrial planet. Its radius and mass are similar to those of Saturn, making it a gas giant planet. The two stars are both smaller than the Sun. The bigger of the two, the primary, measures 69 percent of the Sun&rsquo;s mass and 65 percent of its radius. The smaller star, the secondary, is considerably smaller, with 20 percent of the Sun&rsquo;s mass and 23 percent of its radius. In fact, the secondary star is the smallest low-mass star to have its mass and radius measured at such high precision.<\/p><\/blockquote><p><span><\/span><\/p><p>UC Santa Barbara astrophysicist Avi Shporer is part of the NASA team that has found the first known planet with two &ldquo;suns,&rdquo; an idea popularized by the 1977 movie &ldquo;Star Wars.&rdquo; The discovery is published this week in the journal Science.<\/p><p>In the iconic scene from &ldquo;Star Wars,&rdquo; Luke Skywalker gazes into the distance as two suns set on the horizon. This type of planet is called a circumbinary planet, meaning it orbits a binary star system, as opposed to a single star like our Sun. Circumbinary planets have been pursued by astronomers for decades. Although some scientists have claimed to detect such a planet in the past, none of those claims have been widely accepted by the scientific community.<\/p><p>The Science article reports the first clear detection of a circumbinary planet. The system is called Kepler-16, and it is the 16th planetary system discovered by NASA&rsquo;s Kepler space telescope. It is located approximately 220 light-years from our Sun, near the constellation Cygnus, in the Milky Way galaxy.<\/p><p>&ldquo;It is the combination of the unprecedented precision and the continuous observations from space that allowed the detection of Kepler-16,&rdquo; said Shporer, who is also a researcher with the UCSB-affiliated Las Cumbres Observatory Global Telescope Network (LCOGT) based in Goleta.<\/p><p>At first, the system was identified as an eclipsing binary star, a system of two stars orbiting each other and showing eclipses once every orbital period. Excitement within the Kepler team grew when the scientists were able to identify transits &mdash; small, shallow eclipses induced by a small body such as a planet as it eclipses its parent stars. Further analysis confirmed that these transits are indeed induced by a planet in an orbit around both stars.<\/p><p>&ldquo;This system is so fascinating since it is viewed edge-on, and all three bodies &mdash; the two stars and the planet &mdash; are all eclipsing each other,&rdquo; said Laurance Doyle of the Search for Extraterrestrial Intelligence (SETI) Institute, lead author of the Science paper.<\/p><p>Kepler is a NASA discovery-class mission designed to look for Earth-like planets orbiting Sun-like stars in their habitable zone. Kepler is looking for these planets by continuously monitoring the light intensity of over 150,000 stars simultaneously. Kepler&rsquo;s high sensitivity makes it capable of detecting the minute decrease in a star&rsquo;s light caused by a small planet crossing the line of sight to the star, thereby momentarily blocking a small fraction of the light coming from the star.<\/p><p>&ldquo;The transits and mutual eclipses enable a detailed characterization of the system, including the mass and radius of all objects and their orbits,&rdquo; said Shporer.<\/p><p>The depth of an eclipse gives a sense of the size of the eclipsing body. In the case of Kepler-16, the exact timing of the eclipses is affected by the gravitational pull of the planet. Although the planet&rsquo;s mass is small relative to the two stars, it is able to slightly affect their orbit, making the stellar eclipses occur earlier or later, by up to a minute, compared to a constant period model. As for the planetary transits, analysis of Kepler&rsquo;s measurements is challenging because the timing of the transits deviates significantly from a constant period model, since each transit occurs at a different orbital phase of the inner star.<\/p><p>The planet&rsquo;s orbital period is 229 days, while the stellar binary has a 41-day orbit. Although the planet&rsquo;s orbital period is close to that of Venus in our solar system, it is not an Earth-like, terrestrial planet. Its radius and mass are similar to those of Saturn, making it a gas giant planet. The two stars are both smaller than the Sun. The bigger of the two, the primary, measures 69 percent of the Sun&rsquo;s mass and 65 percent of its radius. The smaller star, the secondary, is considerably smaller, with 20 percent of the Sun&rsquo;s mass and 23 percent of its radius. In fact, the secondary star is the smallest low-mass star to have its mass and radius measured at such high precision.<\/p><p>Ground-based observations are an important part of the Kepler project. &ldquo;At LCOGT, we are using our telescopes as part of the large effort carried out by U.S. astronomers and others, to follow-up and accurately characterize the detections made by Kepler,&rdquo; said Tim Brown, scientific director of LCOGT and an adjunct professor of physics at UCSB. Brown is an important member of the Kepler team.<\/p><p>The Kepler-16 discovery is one of a series of discoveries made by Kepler since its launch in March 2009. Shporer said the most interesting ones are probably yet to come as Kepler continues to monitor the stars.<\/p>","protected":false},"excerpt":{"rendered":"<p>Schematic of the planet with two suns. Click for larger. Credit: Avi Shporer and team \/ University of California Santa Barbara&nbsp;Ah this is very cool to think about even beyond Star wars.By the way, I was out looking for the &hellip; <a href=\"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/astronomy\/a-planet-with-two-suns-is-found.php\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"limit_modified_date":"","last_modified_date":"","_lmt_disableupdate":"","_lmt_disable":"","footnotes":""},"categories":[21],"tags":[],"class_list":["post-39519","post","type-post","status-publish","format-standard","hentry","category-astronomy"],"modified_by":null,"_links":{"self":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts\/39519"}],"collection":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/comments?post=39519"}],"version-history":[{"count":0,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts\/39519\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/media?parent=39519"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/categories?post=39519"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/tags?post=39519"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}