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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004415naa a2200589 4500
001oai:DiVA.org:ri-72569
003SwePub
008240411s2024 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:ri:diva-725692 URI
024a https://doi.org/10.1038/s41598-024-57458-42 DOI
040 a (SwePub)ri
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Zorzano, Maria-Pazu Centro de Astrobiología, Spain4 aut
2451 0a Present-day thermal and water activity environment of the Mars Sample Return collection
264 1b Nature Research,c 2024
338 a electronic2 rdacarrier
500 a M.-P.Z. was supported by Grant PID2019-104205GB-C21 funded by MCIN/AEI/10.13039/501100011033 and by Grant PID2022-140180OB-C21 funded by MCIN/AEI/10.13039/501100011033/FEDER, UE., UE. G. M wants to acknowledge JPL funding from USRA Contract Number 1638782. C.D.K.H was supported by Canadian Space Agency Mars 2020 Participating Scientist Grant CSA CGCPU 20EXPMARS. S.S. acknowledges funding from the Swedish National Space Agency (Contracts 2021-00092 and 137/19). V.D. thanks the FRS-FNRS for support. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). K.C.B. was funded by NASA Mars 2020 Grant 80NSSC20K0235. J.M.F. was supported by the Spanish Agency for Research, Contract PID2022-142750OB-I00. E.M.H. acknowledges funding from NASA RSS PS 80NSSC20K0239. A.D.C. was funded by NASA Mars 2020 Returned Sample Science Participating Scientist Program Grant 80NSSC20K0237. V.D. thanks the FRS-FNRS and PDR 35284099 for support
520 a The Mars Sample Return mission intends to retrieve a sealed collection of rocks, regolith, and atmosphere sampled from Jezero Crater, Mars, by the NASA Perseverance rover mission. For all life-related research, it is necessary to evaluate water availability in the samples and on Mars. Within the first Martian year, Perseverance has acquired an estimated total mass of 355 g of rocks and regolith, and 38 μmoles of Martian atmospheric gas. Using in-situ observations acquired by the Perseverance rover, we show that the present-day environmental conditions at Jezero allow for the hydration of sulfates, chlorides, and perchlorates and the occasional formation of frost as well as a diurnal atmospheric-surface water exchange of 0.5–10 g water per m2 (assuming a well-mixed atmosphere). At night, when the temperature drops below 190 K, the surface water activity can exceed 0.5, the lowest limit for cell reproduction. During the day, when the temperature is above the cell replication limit of 245 K, water activity is less than 0.02. The environmental conditions at the surface of Jezero Crater, where these samples were acquired, are incompatible with the cell replication limits currently known on Earth. 
650 7a TEKNIK OCH TEKNOLOGIERx Maskinteknik0 (SwePub)2032 hsv//swe
650 7a ENGINEERING AND TECHNOLOGYx Mechanical Engineering0 (SwePub)2032 hsv//eng
653 a Environment
653 a Habitability
653 a Jezero
653 a Mars sample return
653 a Temperature
653 a Water activity
653 a chloride
653 a perchlorate
653 a sulfate
653 a surface water
653 a water
653 a article
653 a astronomy
653 a atmosphere
653 a cell division
653 a hydration
653 a night
653 a nonhuman
653 a regolith
653 a rock
653 a water availability
700a Siljeström, Sandrau RISE,Metodik, textil och medicinteknik4 aut0 (Swepub:ri)SandraSi@ri.se
700a Martínez-Frías, Jesusu Instituto de Geociencias, Spain4 aut
710a Centro de Astrobiología, Spainb Metodik, textil och medicinteknik4 org
773t Scientific Reportsd : Nature Researchg 14:1q 14:1x 2045-2322
856u https://doi.org/10.1038/s41598-024-57458-4y Fulltext
856u https://ri.diva-portal.org/smash/get/diva2:1850903/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:ri:diva-72569
8564 8u https://doi.org/10.1038/s41598-024-57458-4

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