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DOI10.1029/2018GL081402
Crater Statistics on the Dark-Toned, Mafic Floor Unit in Jezero Crater, Mars
Shahrzad, Stephanie1; Kinch, Kjartan M.2; Goudge, Timothy A.3; Fassett, Caleb I.4; Needham, Debra H.4; Quantin-Nataf, Cathy5; Knudsen, Cecillie P.2
2019-03-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2019
卷号46期号:5页码:2408-2416
文章类型Article
语种英语
国家Denmark; USA; France
英文摘要

Jezero crater is a similar to 45-km impact crater on the margin of Isidis basin on Mars. Jezero is the landing site for NASA's Mars 2020 rover mission. The crater hosts a paleolake, and fluvio-lacustrine deposits formed in this lake remain accessible to exploration. A dark-toned deposit on the crater floor overlies light-toned carbonate-bearing deposits and has been interpreted as a lava flow. We determined the average thickness of this deposit at the margins to be similar to 13.00.8 m. We analyzed the statistics of impact craters superposed on this deposit and estimated its model age as 2.60.5Ga in the Hartmann system, placing it most likely in the Early Amazonian. The error estimate here includes an estimate of the uncertainty associated with the crater counts. Acquisition, caching, and eventual return of a sample from this unit could provide an important calibration point for Mars crater chronology.


Plain Language Summary Jezero crater is a large impact crater on Mars with a diameter of about 45 km. In the Martian deep past this crater hosted a long-lived lake. On 19 November NASA announced that Jezero crater will be the landing site for the coming Mars 2020 mission. On top of sediments on the central crater floor is a distinctive deposit of dark rocks that possibly originated as a lava flow after the lake had dried out. We studied the statistics of small impact craters on this dark deposit. Such impact crater statistic is widely used as a tool for dating Martian terrains. We report a derived model age of 2.60.2 Ga for these rocks. One central goal of the Mars 2020 mission is to select and store a cache of rock samples that will be returned to Earth by a later mission for study in terrestrial laboratories. If this dark deposit is indeed lava, a sample could be dated in terrestrial laboratories. Together with our crater statistics reported here, this could provide a crucial tie-point for recalibration of the crater count dating system for Mars, which now relies on extrapolation from samples collected on the Moon.


英文关键词Jezero crater crater counting Mars 2020 Mars age
领域气候变化
收录类别SCI-E
WOS记录号WOS:000462612900010
WOS关键词IMPACT BASINS ; SYSTEM
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/181600
专题气候变化
作者单位1.Univ Copenhagen, Dept Geosci & Nat Resource Management, Copenhagen, Denmark;
2.Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark;
3.Univ Texas Austin, Jackson Sch Geosci, Austin, TX 78712 USA;
4.NASA, Marshall Space Flight Ctr, Huntsville, AL USA;
5.Univ Claude Bernard, Univ Lyon, Lab Geol Lyon, Terre,Planetes,Environm, Villeurbanne, France
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Shahrzad, Stephanie,Kinch, Kjartan M.,Goudge, Timothy A.,et al. Crater Statistics on the Dark-Toned, Mafic Floor Unit in Jezero Crater, Mars[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(5):2408-2416.
APA Shahrzad, Stephanie.,Kinch, Kjartan M..,Goudge, Timothy A..,Fassett, Caleb I..,Needham, Debra H..,...&Knudsen, Cecillie P..(2019).Crater Statistics on the Dark-Toned, Mafic Floor Unit in Jezero Crater, Mars.GEOPHYSICAL RESEARCH LETTERS,46(5),2408-2416.
MLA Shahrzad, Stephanie,et al."Crater Statistics on the Dark-Toned, Mafic Floor Unit in Jezero Crater, Mars".GEOPHYSICAL RESEARCH LETTERS 46.5(2019):2408-2416.
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