{"id":208447,"date":"2017-02-16T18:00:13","date_gmt":"2017-02-16T23:00:13","guid":{"rendered":"http:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/uncategorized\/potential-landing-sites-for-mars-2020-narrowed-down-to-three-spaceflight-insider.php"},"modified":"2017-02-16T18:00:13","modified_gmt":"2017-02-16T23:00:13","slug":"potential-landing-sites-for-mars-2020-narrowed-down-to-three-spaceflight-insider","status":"publish","type":"post","link":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/space-flight\/potential-landing-sites-for-mars-2020-narrowed-down-to-three-spaceflight-insider.php","title":{"rendered":"Potential Landing Sites for Mars 2020 Narrowed Down to Three &#8211; SpaceFlight Insider"},"content":{"rendered":"<p><p>      Paul Knightly    <\/p>\n<p>      February 16th, 2017    <\/p>\n<p>      Three potential landing sites for NASAs Mars 2020 rover.      Image Credit: NASA    <\/p>\n<p>    The number of potential landing sites for the Mars 2020    rover has been narrowed    down to three, from a list of eight, following a conference of    scientists last week. The top three landing sites    that were selected were in Northeast Syrtis Major,    Jezero Crater, and the Columbia Hills in Gusev Crater. The    landing sites in the Columbia Hills and Syrtis Major    display evidence of geothermal and mineral hot springs that    could have been conducive to hosting primitive life, and Jerezo    Crater shows evidence that it was once a lake of liquid    water.  <\/p>\n<p>      This image lies in the middle of a candidate landing site in      the Northeast part of Syrtis Major, a huge shield      volcano, and near the Northwest rim of Isidis      Planitia, a giant impact basin. Image & Caption      Credit: NASA \/ JPL-CALTECH \/ MSSS \/ JHU-APL    <\/p>\n<p>    Northeast Syrtis Major was once influenced by volcanic    activity that warmed underground sources of water ice that    reached the surface as mineral hot springs. These hot springs    could have hosted microbial life similar to organisms that have    been found in similar environments on Earth. The area also    displays layered terrain that holds a record of the    interactions between water and minerals throughout early    Martian history.  <\/p>\n<p>      On ancient Mars, water-carved channels and transported      sediments to form fans and deltas within lake basins.      Examination of spectral data acquired from orbit shows that      some of these sediments have minerals that indicate chemical      alteration by water. Here in Jezero Crater delta, sediments      contain clays and carbonates. The image combines information      from two instruments on NASAs Mars Reconnaissance Orbiter:      the Compact Reconnaissance Imaging Spectrometer for Mars and      the Context Camera. (Reference: Ehlmann et al.      2008.) Image & Caption Credit: NASA \/ JPL-CALTECH \/ MSSS      \/ JHU-APL    <\/p>\n<p>    Jezero Crater is an example of the on-again\/off-again nature of    liquid water on Mars. There is evidence that the crater was    filled and drained of water on at least two different occasions    around 3.5 billion years ago. Channels can be seen leading into    and out of the crater, and there is spectral evidence that    suggests clay minerals were formed and deposited as sediment in    the lake. These clay minerals are similar to the sediments    being examined by the Curiosityrover in Gale    Crater and could have played host to microbial life.  <\/p>\n<p>      This approximate true-color image taken by the Mars      Exploration Rover Spirit shows a rock outcrop dubbed      Longhorn, and behind it, the sweeping plains of Gusev      Crater. On the horizon, the rim of Gusev Crater is clearly      visible. The view is to the south of the rovers current      position. The image consists of four frames taken by the      750-, 530- and 430-nanometer filters of Spirits      panoramic camera on sol 210 (August 5, 2004). Image &      Caption Credit: NASA \/ JPL-CALTECH \/ MSSS \/ JHU-APL    <\/p>\n<p>    The Columbia Hills were famously explored by the Mars    Exploration Rover (MER) Spirit between 20032010 where    it discovered evidence the area once hosted a hot spring with    liquid water similar in composition to hot springs found on    Earth. If selected as the final landing site, the Mars 2020    rover would further inspect hot spring sediments to investigate    their potential to host life. Mars 2020 will also revisit an    outcrop that was visited by Spirit which in a recent    analysis by scientists was thought to resemble a fossilized mat    of microbial organisms that have been found in similar hot    spring sediments on Earth. This particular outcrop represents    the strongest evidence for fossilized life to have been found    on the Martian surface to date.  <\/p>\n<p>    The Mars 2020 rover is designed to    address several key scientific objectives and the effectiveness    of the potential landing sites to meet those objectives    factored into the selection of the final three landing sites.    Those objectives are the following:  <\/p>\n<p>    Additionally, the Mars 2020 landing site must also meet the    following criteria:  <\/p>\n<p>    The three finalist landing sites were selected from an original    list of 8 which also included Eberswalde Crater, Holden Crater,    Mawrth Vallis, Nili Fossae, and Southwest    Melas Chasma. The rover is currently under development    and is similar in construction and function to    Curiosity and is targeted to launch during the summer    of 2020 and landing on Mars in early 2021.  <\/p>\n<\/p>\n<p>    Tagged: Mars Mars 2020 NASA The Range  <\/p>\n<p>      Paul is currently a graduate student in Space and Planetary      Sciences at the University of Akransas in Fayetteville. He      grew up in the Kansas City area and developed an interest in      space at a young age at the start of the twin Mars      Exploration Rover missions in 2003. He began his studies in      aerospace engineering before switching over to geology at      Wichita State University where he earned a Bachelor of      Science in 2013. After working as an environmental geologist      for a civil engineering firm, he began his graduate studies      in 2016 and is actively working towards a PhD that will focus      on the surficial processes of Mars. He also participated in a      2-week simluation at The Mars Society's Mars Desert Research      Station in 2014 and remains involved in analogue mission      studies today. Paul has been interested in science outreach      and communication over the years which in the past included      maintaining a personal blog on space exploration from high      school through his undergraduate career and in recent years      he has given talks at schools and other organizations over      the topics of geology and space. He is excited to bring his      experience as a geologist and scientist to the Spaceflight      Insider team writing primarily on space science topics.    <\/p>\n<p><!-- Auto Generated --><\/p>\n<p>Read more from the original source:<\/p>\n<p><a target=\"_blank\" href=\"http:\/\/www.spaceflightinsider.com\/missions\/solar-system\/mars-2020-three-potential-landing-sites\/\" title=\"Potential Landing Sites for Mars 2020 Narrowed Down to Three - SpaceFlight Insider\">Potential Landing Sites for Mars 2020 Narrowed Down to Three - SpaceFlight Insider<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p> Paul Knightly February 16th, 2017 Three potential landing sites for NASAs Mars 2020 rover. Image Credit: NASA The number of potential landing sites for the Mars 2020 rover has been narrowed down to three, from a list of eight, following a conference of scientists last week. The top three landing sites that were selected were in Northeast Syrtis Major, Jezero Crater, and the Columbia Hills in Gusev Crater.  <a href=\"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/space-flight\/potential-landing-sites-for-mars-2020-narrowed-down-to-three-spaceflight-insider.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":[18],"tags":[],"class_list":["post-208447","post","type-post","status-publish","format-standard","hentry","category-space-flight"],"modified_by":null,"_links":{"self":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts\/208447"}],"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=208447"}],"version-history":[{"count":0,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts\/208447\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/media?parent=208447"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/categories?post=208447"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/tags?post=208447"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}