{"id":8766,"date":"2016-05-10T07:32:46","date_gmt":"2016-05-10T07:32:46","guid":{"rendered":"http:\/\/revoscience.com\/en\/?p=8766"},"modified":"2016-05-10T07:32:46","modified_gmt":"2016-05-10T07:32:46","slug":"flying-observatory-detects-atomic-oxygen-in-martian-atmosphere","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/flying-observatory-detects-atomic-oxygen-in-martian-atmosphere\/","title":{"rendered":"Flying Observatory Detects Atomic Oxygen in Martian Atmosphere"},"content":{"rendered":"<figure id=\"attachment_8767\" aria-describedby=\"caption-attachment-8767\" style=\"width: 300px\" class=\"wp-caption alignright\"><a href=\"http:\/\/revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-8767\" src=\"http:\/\/revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0-300x298.jpg\" alt=\"SOFIA\/GREAT spectrum of oxygen [O I] superimposed on an image of Mars from the MAVEN mission. The amount of atomic oxygen computed from this SOFIA data is about half the amount expected. Credits: SOFIA\/GREAT spectrum: NASA\/DLR\/USRA\/DSI\/MPIfR\/GREAT Consortium\/ MPIfS\/Rezac et al. 2015. Mars image: NASA\/MAVEN (Mars Atmosphere and Volatile Evolution Mission)\" width=\"300\" height=\"298\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0-300x298.jpg 300w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0-150x150.jpg 150w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg 320w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/a><figcaption id=\"caption-attachment-8767\" class=\"wp-caption-text\">SOFIA\/GREAT spectrum of oxygen [O I] superimposed on an image of Mars from the MAVEN mission. The amount of atomic oxygen computed from this SOFIA data is about half the amount expected.<br \/>Credits: SOFIA\/GREAT spectrum: NASA\/DLR\/USRA\/DSI\/MPIfR\/GREAT Consortium\/ MPIfS\/Rezac et al. 2015. Mars image: NASA\/MAVEN (Mars Atmosphere and Volatile Evolution Mission)<\/figcaption><\/figure>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\">An instrument onboard the Stratospheric Observatory for Infrared Astronomy (SOFIA) detected atomic oxygen in the atmosphere of Mars for the first time since the last observation\u00a040 years ago. These atoms were found in the upper layers of the Martian atmosphere known as the mesosphere.\u00a0<\/span><\/p>\n<div class=\"dnd-atom-wrapper type-image context-side_image\" style=\"font-weight: normal; color: rgb(0, 0, 0); text-align: justify;\">\n<div class=\"dnd-drop-wrapper\"><\/div>\n<div class=\"dnd-legend-wrapper\">\n<div class=\"link\"><span style=\"color: #000000;\">Atomic oxygen affects how other gases escape Mars and therefore has a significant impact on the planet\u2019s atmosphere. Scientists detected only about half the amount of oxygen expected, which may be due to variations in the Martian atmosphere. Scientists will continue to use SOFIA to study these variations to help better understand the atmosphere of the Red Planet.<\/span><\/div>\n<\/div>\n<\/div>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\">&#8220;Atomic oxygen in the Martian atmosphere is notoriously difficult to measure,&#8221;\u00a0said Pamela Marcum, SOFIA project scientist. &#8220;To observe the far-infrared wavelengths needed to detect atomic oxygen, researchers must be above the majority of Earth\u2019s atmosphere and use highly sensitive instruments, in this case a spectrometer. SOFIA provides both capabilities.&#8221;<\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\">The Viking and Mariner missions of the 1970s made the last measurements of atomic oxygen in the Martian atmosphere. These more recent observations were possible thanks to SOFIA\u2019s airborne location, flying between 37,000-45,000 feet, above most of the infrared-blocking moisture in Earth\u2019s atmosphere. The advanced detectors on one of the observatory\u2019s instruments, the German Receiver for Astronomy at Terahertz Frequencies (GREAT), enabled astronomers to distinguish the oxygen in the Martian atmosphere from oxygen in Earth\u2019s atmosphere. Researchers presented their findings in a paper published in the journal\u00a0<em>Astronomy and Astrophysics<\/em>\u00a0in 2015.<\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\">SOFIA is a Boeing 747SP jetliner modified to carry a 100-inch diameter telescope. It is a joint project of NASA and the German Aerospace Center. NASA\u2019s Ames Research Center in Moffett Field, California, manages the SOFIA program, science and mission operations in cooperation with the Universities Space Research Association headquartered in Columbia, Maryland, and the German SOFIA Institute (DSI) at the University of Stuttgart. The aircraft is based at NASA\u2019s Armstrong Flight Research Center&#8217;s hangar 703 in Palmdale, California.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>The advanced detectors on one of the observatory\u2019s instruments, the German Receiver for Astronomy at Terahertz Frequencies (GREAT), enabled astronomers to distinguish the oxygen in the Martian atmosphere from oxygen in Earth\u2019s atmosphere.<\/p>\n","protected":false},"author":6,"featured_media":8767,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[20],"tags":[],"class_list":["post-8766","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-space-news"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0-150x150.jpg",150,150,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0-300x298.jpg",300,298,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",65,65,false],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",320,318,false],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",96,96,false],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/05\/marsgreat_0.jpg",150,149,false]},"author_info":{"info":["Amrita Tuladhar"]},"category_info":"<a href=\"https:\/\/www.revoscience.com\/en\/category\/news\/space-news\/\" rel=\"category tag\">Space\/ AstroPhysics<\/a>","tag_info":"Space\/ AstroPhysics","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/8766","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/6"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=8766"}],"version-history":[{"count":0,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/8766\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/8767"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=8766"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=8766"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=8766"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}