{"id":24898,"date":"2021-08-08T21:56:06","date_gmt":"2021-08-08T13:56:06","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/perseverances-first-sample-collection-fails-new-science-points-to-subsurface-martian-clay-lakes\/"},"modified":"2021-08-08T21:56:06","modified_gmt":"2021-08-08T13:56:06","slug":"perseverances-first-sample-collection-fails-new-science-points-to-subsurface-martian-clay-lakes","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/perseverances-first-sample-collection-fails-new-science-points-to-subsurface-martian-clay-lakes\/","title":{"rendered":"Perseverance\u2019s first sample collection fails, new science points to subsurface Martian clay lakes"},"content":{"rendered":"<p>NASA\u2019s Perseverance Mars rover recently attempted its first-ever sample collection of the Martian surface on August 6. However, data shows that while the rover\u2019s drill successfully drilled into the surface, no regolith was collected in the sample tube.<\/p>\n<p>Meanwhile, as Perseverance was preparing for the sample collection event, a team of researchers using ESA\u2019s Mars Express orbiter found evidence that previously thought of lakes of water underneath Mars\u2019 south pole might actually be made of clay.<\/p>\n<\/p>\n<p><b>Perseverance\u2019s sample collection failure<\/b><\/p>\n<p>On August 6, Perseverance\u2019s 2-meter robotic arm lowered to the Martian surface, where a drill located at the end of the arm began carving into the local rock.<\/p>\n<p>Inside the bit used to drill into the surface was a small, hollow titanium cylinder container. This container aimed to collect the dust, sand, rock, and other regolith displaced by the drill. Once the drilling was complete, the tube should have been filled with surface material the size of a piece of chalk. <\/p>\n<p>This entire process is called sample collection and is a crucial part of Perseverance\u2019s mission as well as two follow-on NASA and ESA Sample Return flights slated for launch in 2026.<\/p>\n<p>However, the August 6 drilling event data shows that the sample collection tube did not collect any surface material.&nbsp;<\/p>\n<p>NASA educational resources<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>Space Shuttle models<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>Technology News<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({});<br \/>\n<iframe id=\"twitter-widget-1\" scrolling=\"no\" frameborder=\"0\" allowtransparency=\"true\" allowfullscreen=\"true\" class=\"\" style=\"position: absolute; visibility: hidden; width: 0px; height: 0px; display: block; flex-grow: 1;\" title=\"X Post\" src=\"https:\/\/platform.twitter.com\/embed\/Tweet.html?creatorScreenName=haygenwarren&amp;dnt=true&amp;embedId=twitter-widget-1&amp;features=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%3D%3D&amp;frame=false&amp;hideCard=false&amp;hideThread=false&amp;id=1423773624054341638&amp;lang=en&amp;origin=https%3A%2F%2Fwww.nasaspaceflight.com%2F2021%2F08%2Fmars-sample-collection-clay-lakes%2F&amp;sessionId=834e9214a40b587518f79881d638b9009ebbdbca&amp;siteScreenName=NASASpaceflight&amp;theme=light&amp;widgetsVersion=6a3ad42b224df%3A1778106238597&amp;width=550px\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\" data-tweet-id=\"1423773624054341638\"><\/iframe><\/p>\n<blockquote class=\"twitter-tweet\" data-width=\"550\" data-dnt=\"true\" data-twitter-extracted-i1783496815420650217=\"true\">\n<p lang=\"en\" dir=\"ltr\">#SamplingMars is one of my most complicated tasks. Early pics and data show a successful drill hole, but no sample in the tube\u2013something we\u2019ve never seen in testing on Earth. Mars keeps surprising us. We\u2019re working through this new challenge. More to come. https:\/\/t.co\/XyXBssvKe6 pic.twitter.com\/VTNvMA2jqN<\/p>\n<p>\u2014 NASA&#8217;s Perseverance Mars Rover (@NASAPersevere) August 6, 2021<\/p>\n<\/blockquote>\n<p>Mission operators, reviewing the data returned, found that the coring bit and the sample tube were in the correct positions for the sample collection. Further data showed that Perseverance successfully performed the post-drilling operations as intended and that the tube was processed correctly.<\/p>\n<\/p>\n<h4 class=\"widget-title penci-border-arrow\">See Also<\/h4>\n<ul>\n<li>Mars 2020 Updates<\/li>\n<li>Mars Rover Section<\/li>\n<li>Future Vehicles Section<\/li>\n<li>Click here to Join L2<\/li>\n<\/ul>\n<p>Yet after the entire drilling process was complete, measurements indicated the tube did not have any surface material inside of it.<\/p>\n<p>\u201cThe sampling process is autonomous from beginning to end. One of the steps that occur after placing a probe into the collection tube is to measure the volume of the sample,\u201d said Jessica Samuels, surface mission manager for Perseverance at NASA\u2019s Jet Propulsion Laboratory (JPL).&nbsp;<\/p>\n<p>\u201cThe probe did not encounter the expected resistance that would be there if a sample were inside the tube.&nbsp;The initial thinking is that the empty tube is more likely a result of the rock target not reacting the way we expected during coring, and less likely a hardware issue with the Sampling and Caching System.\u201d&nbsp;<\/p>\n<p>An immediate course of action is to use the WATSON (Wide Angle Topographic Sensor for Operations and eNgineering) camera to investigate the drill hole. WATSON is located at the end of the 2-meter robotic arm, allowing it to observe the hole from various angles at close range.&nbsp;<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" aria-describedby=\"caption-attachment-79539\" class=\"wp-image-79539\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/PIA24795a-1-350x213.png\" alt=\"\" width=\"767\" height=\"467\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/PIA24795a-1-350x213.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/PIA24795a-1-575x350.png 575w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/PIA24795a-1-180x110.png 180w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/PIA24795a-1-768x467.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/PIA24795a-1-1170x712.png 1170w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/PIA24795a-1.png 1297w\" sizes=\"(max-width: 767px) 100vw, 767px\"><\/p>\n<p id=\"caption-attachment-79539\" class=\"wp-caption-text\">This image, taken by one of Perseverance\u2019s Front Hazard Avoidance Cameras, shows the hole drilled by the rover. (Credit: NASA\/JPL-Caltech)<\/p>\n<p>Perseverance\u2019s teams will use the data from the August 6 event and WATSON\u2019s observations throughout the coming days to correct the issue ahead of future sampling attempts.&nbsp;<\/p>\n<p>\u201cOver the next few days, the team will be spending more time analyzing the data we have and also acquiring some additional diagnostic data to support understanding the root cause for the empty tube,\u201d said Trosper.<\/p>\n<p>Part of Perseverance\u2019s mission is to leave sample containers at specific locations along its route so that a future Sample Fetch Rover, to be launched in 2026 for a three year cruise to Mars under the current plan, can retrieve them and bring the samples back to a co-launched Mars Ascent Vehicle that will take them into Martian orbit for rendezvous with an ESA-built Earth Return Orbiter for the trip back to Earth.<\/p>\n<p><b>Martian clay lakes<\/b><\/p>\n<p>Deeper under the Martian surface then Perseverance\u2019s sample collection activities, a group of researchers led by Roberto Orosei of Italy\u2019s Istituto Nazionale di Astrofisica announced in 2018 evidence of subsurface water lakes below the ice cap at Mars\u2019 south pole.<\/p>\n<p>Using ESA\u2019s Mars Express orbiter, bright radar signals were seen through the rock and ice of the Martian south polar ice cap, signals that could be interpreted as liquid water.<\/p>\n<p>As with every scientific observation, scientists began searching for ways to see whether these lakes were what they appeared to be or if there were in fact something different.<\/p>\n<p><iframe id=\"twitter-widget-2\" scrolling=\"no\" frameborder=\"0\" allowtransparency=\"true\" allowfullscreen=\"true\" class=\"\" style=\"position: absolute; visibility: hidden; width: 0px; height: 0px; display: block; flex-grow: 1;\" title=\"X Post\" src=\"https:\/\/platform.twitter.com\/embed\/Tweet.html?creatorScreenName=haygenwarren&amp;dnt=true&amp;embedId=twitter-widget-2&amp;features=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%3D%3D&amp;frame=false&amp;hideCard=false&amp;hideThread=false&amp;id=1420759439078948869&amp;lang=en&amp;origin=https%3A%2F%2Fwww.nasaspaceflight.com%2F2021%2F08%2Fmars-sample-collection-clay-lakes%2F&amp;sessionId=834e9214a40b587518f79881d638b9009ebbdbca&amp;siteScreenName=NASASpaceflight&amp;theme=light&amp;widgetsVersion=6a3ad42b224df%3A1778106238597&amp;width=550px\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\" data-tweet-id=\"1420759439078948869\"><\/iframe><\/p>\n<blockquote class=\"twitter-tweet\" data-width=\"550\" data-dnt=\"true\" data-twitter-extracted-i1783496815420650217=\"true\">\n<p lang=\"en\" dir=\"ltr\">Clays, not water, may be the source of \u201clakes\u201d detected on Mars, according to a new study. It\u2019s one of three in the last month in which scientists took a closer look at radar data peering under the ice of the Martian south pole. https:\/\/t.co\/mI85NFjnBE pic.twitter.com\/VYbU7ulzVB<\/p>\n<p>\u2014 NASA JPL (@NASAJPL) July 29, 2021<\/p>\n<\/blockquote>\n<p>In three recently published studies from various teams, new data suggests that the lakes aren\u2019t made of liquid water, but rather from clay instead.&nbsp;<\/p>\n<p>All three of the studies used the same data from the 2018 study led by Orosei. The Mars Express\u2019 Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) instrument collected the data\/evidence used.&nbsp;<\/p>\n<p>MARSIS bounces radio waves off Mars\u2019 surface and atmosphere and then listens for the radio waves that travel back to it, called \u201cechoes.\u201d MARSIS then analyzes these echoes.<\/p>\n<p>Jeffrey Plaut of JPL and Aditya Khuller of Arizona State University analyzed 15 years of MARSIS data, looking through approximately 44,000 radar echoes.<\/p>\n<p>The result was dozens of bright spots, just like the ones in the 2018 Orosei et al. study, in Mars\u2019 southern polar ice cap. However, the new research, recently published in the journal Geophysical Research Letters, suggests that liquid water physically cannot exist in these \u201clakes.\u201d<\/p>\n<p>In their paper, Plaut and Khuller observe that the signals from the bright spots are too close to the surface where it would be too cold for water to remain liquid, even when mixed with perchlorates which lower water molecules\u2019 natural freezing point.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-79542\" class=\"wp-image-79542\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/E1-bright_radar_reflections-302x350.png\" alt=\"\" width=\"459\" height=\"532\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/E1-bright_radar_reflections-302x350.png 302w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/E1-bright_radar_reflections-768x891.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/E1-bright_radar_reflections.png 1155w\" sizes=\"(max-width: 459px) 100vw, 459px\"><\/p>\n<p id=\"caption-attachment-79542\" class=\"wp-caption-text\">This image of Mars\u2019 south pole ice cap shows were the bright radar spots were seen in the MARSIS data. (Credit: ESA\/NASA\/JPL-Caltech)<\/p>\n<p>Furthermore, Carver Bierson of Arizona State University et al., in their review, showed that materials such as clays, metal-bearing minerals, and saline ice could cause the reflective signals shown in the MARSIS data. Bierson et al.\u2019s results are also published in the journal Geophysical Research Letters.<\/p>\n<p>Furthering Bierson et al.\u2019s research in his paper,&nbsp;Issac Smith of York University in Toronto,&nbsp;took&nbsp;their research and \u2014 remembering that a group of clays, called smectites, were common all over Mars\u2019 surface \u2014&nbsp;started measuring smectite properties.<\/p>\n<p>In the lab, Smith et al. took samples of smectite and measured how radar signals interacted with them by putting the samples into cylinders designed to measure radar signals.&nbsp;<\/p>\n<p>Smith et al. then cooled the smectite with liquid nitrogen, freezing them to minus 50\u00b0C \u2014 a temperature close to what it would experience at the Martian south pole.<\/p>\n<p>After numerous tests, Smith et al. compared their results to the MARSIS data and found that smectite\u2019s response in the lab almost perfectly matched the signals seen in the MARSIS data.&nbsp;<\/p>\n<p>Knowing this, Smith et al. checked for clays surrounding the bright radar spots in the MARSIS observations using NASA\u2019s Mars Reconnaissance Orbiter\u2019s Compact Reconnaissance Imaging Spectrometer (CRISM) instrument.&nbsp;<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-79544\" class=\"wp-image-79544\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/115392main_spolarcap_summer-350x256.jpeg\" alt=\"\" width=\"752\" height=\"550\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/115392main_spolarcap_summer-350x256.jpeg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/115392main_spolarcap_summer-479x350.jpeg 479w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/115392main_spolarcap_summer-768x561.jpeg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2021\/08\/115392main_spolarcap_summer.jpeg 845w\" sizes=\"(max-width: 752px) 100vw, 752px\"><\/p>\n<p id=\"caption-attachment-79544\" class=\"wp-caption-text\">The southern polar ice cap of Mars imaged by Mars Global Surveyor in 2000 during Martian summer. Smith et al. used MRO to search for smectite in this area. (Credit: NASA\/JPL\/MSSS)<\/p>\n<p>While CRISM can\u2019t see directly through the ice where these \u201clakes\u201d are, it can search the surface and surrounding areas for certain minerals. To this end, CRISM searched the Martian south pole and surrounding areas for smectites. <\/p>\n<p>And it found them&nbsp;at the south pole in the areas surrounding the bright radar spots seen in the MARSIS data. <\/p>\n<p>Researchers caution that the only way to confirm what the bright radar spots found in the MARSIS data really are is to land at the south pole; however, collective new research highly suggests these previously-thought-of-lakes are made of clay.<\/p>\n<p>Mars Express is in its 18th year of operation, having launched on June 2, 2003 on a Soyuz-FG\/Fregat rocket from Kazakhstan and entered Martian orbit on December 25 that same year. The orbiter is currently in an approved mission extension period that lasts until December 31, 2022.<\/p>\n<p><em>(Lead image: NASA\u2019s Perseverance rover studies a Mars rock outcrop. Credit: NASA\/JPL-Caltech)<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>NASA\u2019s Perseverance Mars rover recently attempted its first-ever sample collection of the Martian surface on August 6. However, data shows that while the rover\u2019s drill successfully drilled into the surface, no regolith was collected in the sample tube. Meanwhile, as Perseverance was preparing for the sample collection event, a team of researchers using ESA\u2019s Mars [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"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":[246,367,2272,190,1633],"class_list":["post-24898","post","type-post","status-publish","format-standard","hentry","category-news","tag-esa","tag-mars","tag-mars-express","tag-nasa","tag-perseverance"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24898"}],"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=24898"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/24898\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=24898"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=24898"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=24898"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}