{"id":39938,"date":"2013-01-07T21:46:43","date_gmt":"2013-01-07T13:46:43","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/nasa-kepler-closing-in-on-earths-analogue\/"},"modified":"2013-01-07T21:46:43","modified_gmt":"2013-01-07T13:46:43","slug":"nasa-kepler-closing-in-on-earths-analogue","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/nasa-kepler-closing-in-on-earths-analogue\/","title":{"rendered":"NASA Kepler closing in on \u201cEarth\u2019s Analogue\u201d"},"content":{"rendered":"<p>The continuing success of NASA\u2019s Kepler mission was highlighted on Monday, following the discovery of 461 new planet candidates \u2013 four of which are less than twice the size of Earth and orbit in their sun\u2019s habitable zone. Scientists believe it\u2019s just a matter of \u201cwhen\u201d a twin of our own planet is found by the spacecraft.\n<\/p>\n<p>\nKepler\u2019s Mission:<\/p>\n<p>The Kepler spacecraft \u2013 a telescope designed to search for Earth-like terrestrial planets in the Cygnus and Lyra constellations \u2013 was launched on a Delta II launch vehicle from Cape Canaveral Air Force Station back in March, 2009.<\/p>\n<p>Kepler was inserted into an Earth-trailing heliocentric orbit \u2013 a solar orbit that trails the Earth by an increase of one week per year. As such, Kepler completes one revolution of the sun every 372.5 days (~53 weeks) \u2013 one week longer than that of Earth\u2019s heliocentric orbit.<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" class=\"alignleft size-full wp-image-27628\" title=\"Kepler Space Telescope\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2013\/01\/A317.jpg\" alt=\"Kepler Space Telescope\" width=\"320\" height=\"273\">Dedicated to the detection and study of extra-solar terrestrial planets that orbit their parent stars inside the habitable zone, the Kepler mission is the first in proposed series of missions that will study the characteristics of Earth-like extra-solar planets.<\/p>\n<p>The habitable zone \u2013 or an area where water can exist in its three forms (most importantly in a liquid state) \u2013 is the main area of interest for Kepler and its science team, with Kepler\u2019s main objective to determine whether rocky planets are a common natural formation.<\/p>\n<p>Unlike previous observations conducted by orbital and ground-base telescopes, Kepler looks at a swath of the sky roughly equivalent to the size of one\u2019s hand if held at arm\u2019s length.<\/p>\n<p>This area of observation yields approximately 156,000 stars for Kepler\u2019s science team to monitor for any trace of the tell-tale \u201cdimming\u201d effect caused when a planetary body passes in front of its parent star \u2013 a detection method known as the transit method of discovery.<\/p>\n<p>Aerospace industry analysis<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>Rocket building kits<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>Spaceflight history books<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>It didn\u2019t take long for Kepler to prove itself as a pivotal component of NASA\u2019s desire to understand extra-solar system dynamics and planet frequency in star systems in our \u201clocal\u201d part of the Milky Way Galaxy.<\/p>\n<h4 class=\"widget-title penci-border-arrow\">See Also<\/h4>\n<ul>\n<li>Robotic Mission Forum<\/li>\n<li>L2 Future Spacecraft<\/li>\n<li>Click here to Join L2<\/li>\n<\/ul>\n<p>Within the first 43-days of observation, scientific data from Kepler, combined with follow up observations from ground-based telescopes, confirmed the discovery of five new exoplanets \u2013 including the now well-known Kepler-7b.<\/p>\n<p>Following this formal announcement, the next significant Kepler data release occurred on June 15, 2010 when it was revealed that Kepler\u2019s data had identified 706 stars \u201cfrom its first data set (that) have exoplanet candidates with sizes from as small as that of the Earth to larger than that of Jupiter.<\/p>\n<p>The June 15 \u2013 \u201cCharacteristics of Kepler Planetary Candidates Based on the First Data Set: The Majority are Found to be Neptune-Size and Smaller\u201d \u2013 report only released information on 306 of these exoplanet system candidates. Data on the remaining 400 stars was released in February 2011.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignleft size-full wp-image-27629\" title=\"Exoplanet find\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2013\/01\/A68.jpg\" alt=\"Exoplanet find\" width=\"326\" height=\"245\">On August 26, 2010 Kepler scientists announced another unprecedented discovery \u2013 the confirmation of two new exoplanets orbiting the same star as discovered via the transit method of detection.<\/p>\n<p>As NASA reported, the tell-tale transit signatures of two planets were seen in the data beamed back from Kepler.<\/p>\n<p>The two planets, orbiting a star dubbed Kepler-9 located approximately 2,300 light years from Earth, have been designated Kepler-9b and 9c and were discovered over a seven month observational period.<\/p>\n<p>The transit method of detection, which measures the \u201cdimming\u201d of a star\u2019s apparent light as an exoplanet passes between the star and Earth (Kepler in this case), is used in addition to planetary discovery to determine the size of any confirmed exoplanets by measuring the amount of \u201cdimming\u201d during transit.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignleft size-full wp-image-27630\" title=\"Kepler Discovery\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2013\/01\/Z312.jpg\" alt=\"Kepler Discovery\" width=\"347\" height=\"255\">Kepler has kept up the pace since, with the end of 2012 showing the space telescope has helped to provide confirmation of 817 planets around 642 stars \u2013 with 2,320 Kepler planetary candidates awaiting confirmation.<\/p>\n<p>Now, kicking off 2013 \u2013 with the mission extended past its original three year plan \u2013 Kepler\u2019s team announced the discovery of 461 new planet candidates, with four of the potential new planets are less than twice the size of Earth and orbit in their sun\u2019s habitable zone.<\/p>\n<p>Based on observations conducted from May 2009 to March 2011, the findings show a steady increase in the number of smaller-size planet candidates and the number of stars with more than one candidate.<\/p>\n<p>\u201cThere is no better way to kickoff the start of the Kepler extended mission than to discover more possible outposts on the frontier of potentially life bearing worlds,\u201d said Christopher Burke, Kepler scientist at the SETI Institute, who is leading the analysis.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignleft size-medium wp-image-27631\" title=\"Kepler's search area\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2013\/01\/Z6-350x274.jpg\" alt=\"Kepler's search area\" width=\"350\" height=\"274\">Since the last Kepler catalog was released in February 2012, the number of candidates discovered in the Kepler data has increased by 20 percent and now totals 2,740 potential planets orbiting 2,036 stars. The most dramatic increases are seen in the number of Earth-size and super Earth-size candidates discovered, which grew by 43 and 21 percent respectively.<\/p>\n<p>The new data increases the number of stars discovered to have more than one planet candidate from 365 to 467. Today, 43 percent of Kepler\u2019s planet candidates are observed to have neighbor planets.<\/p>\n<p>\u201cThe large number of multi-candidate systems being found by Kepler implies that a substantial fraction of exoplanets reside in flat multi-planet systems,\u201d said Jack Lissauer, planetary scientist at NASA\u2019s Ames Research Center. \u201cThis is consistent with what we know about our own planetary neighborhood.\u201d<\/p>\n<p>Scientists believe they are on track to find a planet that mirrors Earth, with the only question being \u201cwhen\u201d.<\/p>\n<p>\u201cThe analysis of increasingly longer time periods of Kepler data uncovers smaller planets in longer period orbits \u2013 orbital periods similar to Earth\u2019s,\u201d said Steve Howell, Kepler mission project scientist at Ames. \u201cIt is no longer a question of will we find a true Earth analogue, but a question of when.\u201d<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignleft size-medium wp-image-27632\" title=\"William Borucki\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2013\/01\/Z9-350x227.jpg\" alt=\"William Borucki\" width=\"350\" height=\"227\">Marking the success of the mission so far, Monday also saw the announcement by the National Academy of Sciences that William Borucki, science principal investigator for NASA\u2019s Kepler mission at Ames Research Center is the recipient of the 2013 Henry Draper Medal.<\/p>\n<p>Borucki is honored for his founding concept and visionary leadership during the development of Kepler, which uses transit photometry to determine the frequency and kinds of planets around other stars.<\/p>\n<p>\u201cThis is a commendable recognition for Bill Borucki and the Kepler mission,\u201d said John Grunsfeld, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. \u201cIt is well deserved and a tribute both to Bill\u2019s dedication and persistence and the fantastic and exciting results from Kepler.\u201d<\/p>\n<p>(Images via NASA).<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The continuing success of NASA\u2019s Kepler mission was highlighted on Monday, following the discovery of 461 new planet candidates \u2013 four of which are less than twice the size of Earth and orbit in their sun\u2019s habitable zone. Scientists believe it\u2019s just a matter of \u201cwhen\u201d a twin of our own planet is found by [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":30311,"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":[2826],"class_list":["post-39938","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news","tag-kepler"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/39938"}],"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=39938"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/39938\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media\/30311"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=39938"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=39938"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=39938"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}