{"id":194,"date":"2026-03-17T11:07:57","date_gmt":"2026-03-17T10:07:57","guid":{"rendered":"https:\/\/geops.geol.u-psud.fr\/etp\/?p=194"},"modified":"2026-03-17T11:09:00","modified_gmt":"2026-03-17T10:09:00","slug":"exomars-tgo-and-rosalind-franklin","status":"publish","type":"post","link":"https:\/\/geops.geol.u-psud.fr\/etp\/en\/2026\/03\/17\/exomars-tgo-and-rosalind-franklin\/","title":{"rendered":"ExoMars TGO and Rosalind Franklin"},"content":{"rendered":"<p><b>Funding:<\/b> CNES, INSU<\/p>\n<p><b>Principal investigators:<\/b> B. Bultel, F. Schmidt, F. Costard<\/p>\n<p><b>GEOPS staff involved:<\/b> B. Bultel, F. Schmidt, F. Costard, F. Andrieu, A. Cornillon<\/p>\n<p><b>Partners:<\/b> V. Ciarletti (LATMOS), A.C. Vandaele, I. Thomas (BIRA \u2013 Belgium)<\/p>\n<p>&nbsp;<\/p>\n<p><strong><img decoding=\"async\" class=\"aligncenter size-full wp-image-143\" src=\"https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover.jpg\" alt=\"\" width=\"1000\" height=\"562\" srcset=\"https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover-200x112.jpg 200w, https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover-300x169.jpg 300w, https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover-400x225.jpg 400w, https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover-600x337.jpg 600w, https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover-768x432.jpg 768w, https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover-800x450.jpg 800w, https:\/\/geops.geol.u-psud.fr\/etp\/wp-content\/uploads\/sites\/4\/2025\/12\/ExoMars_Rosalind_Franklin_rover.jpg 1000w\" sizes=\"(max-width: 1000px) 100vw, 1000px\" \/><\/strong><\/p>\n<p>&nbsp;<\/p>\n<p><strong>\u00a0<\/strong><\/p>\n<p>The ESA\u2019s ExoMars mission comprises two components: the Trace Gas Orbiter (TGO) and the Rosalind Franklin rover.<br \/>\nOur team is involved in these missions. Fr\u00e9d\u00e9ric Schmidt has been selected by the ESA as a Guest Scientist for the ExoMars TGO. He works primarily with the NOMAD and ACS instruments. Fran\u00e7ois Costard is the Principal Investigator (PI) for the WISDOM radar on Rosalind Franklin. Benjamin Bultel is a member of the Rosalind Franklin Rover Science Operations Working Group (RSOWG). He takes part in mission simulation exercises and analyses of terrestrial sample analogues to prepare for the rover\u2019s mission.<br \/>\nThe Rosalind Franklin rover aims to determine the habitability of Mars. Our team is involved in preparing for the mission as well as in understanding the geological context of the landing site. We provide analogue environments in the laboratory\u2019s cold chamber as well as sampling campaigns of analogue rocks.<br \/>\nThe ExoMars TGO research project focuses on the Martian surface and, in particular, on the deposits of volatiles (mainly CO\u2082 and H\u2082O) present in the polar regions (up to 40\u00b0 latitude). Seasonal deposits have been proposed as a source\/sink of minor chemical species on Mars. They are also involved in Mars\u2019 major climate cycle and are therefore essential for understanding the current climate. Furthermore, the study of volatiles is crucial for calibrating climate models in order to study the past climate. Quantitative spectroscopy from ExoMars.TGO using the NOMAD and ACS instruments in nadir-pointing mode allows us to provide significant new insights into the microphysics of the ice surface.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Funding: CNES, INSU Principal investigators: B. Bultel, F. Schmidt, F.  [&#8230;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[22,24,26,28],"tags":[],"class_list":["post-194","post","type-post","status-publish","format-standard","hentry","category-datation-equipements-en","category-mars-planetes-primitif-en","category-processus-planetaire-en","category-volcanisme-actif-en"],"_links":{"self":[{"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/posts\/194","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/comments?post=194"}],"version-history":[{"count":3,"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/posts\/194\/revisions"}],"predecessor-version":[{"id":197,"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/posts\/194\/revisions\/197"}],"wp:attachment":[{"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/media?parent=194"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/categories?post=194"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/geops.geol.u-psud.fr\/etp\/wp-json\/wp\/v2\/tags?post=194"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}