Evidence from Opportunity's Microscopic Imager for Water on Meridiani Planum

Author:

Herkenhoff K. E.12345,Squyres S. W.12345,Arvidson R.12345,Bass D. S.12345,Bell J. F.12345,Bertelsen P.12345,Ehlmann B. L.12345,Farrand W.12345,Gaddis L.12345,Greeley R.12345,Grotzinger J.12345,Hayes A. G.12345,Hviid S. F.12345,Johnson J. R.12345,Jolliff B.12345,Kinch K. M.12345,Knoll A. H.12345,Madsen M. B.12345,Maki J. N.12345,McLennan S. M.12345,McSween H. Y.12345,Ming D. W.12345,Rice J. W.12345,Richter L.12345,Sims M.12345,Smith P. H.12345,Soderblom L. A.12345,Spanovich N.12345,Sullivan R.12345,Thompson S.12345,Wdowiak T.12345,Weitz C.12345,Whelley P.12345

Affiliation:

1. U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA.

2. Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA.

3. Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA.

4. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

5. Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics and Geophysics, University of Copenhagen, Denmark.

Abstract

The Microscopic Imager on the Opportunity rover analyzed textures of soils and rocks at Meridiani Planum at a scale of 31 micrometers per pixel. The uppermost millimeter of some soils is weakly cemented, whereas other soils show little evidence of cohesion. Rock outcrops are laminated on a millimeter scale; image mosaics of cross-stratification suggest that some sediments were deposited by flowing water. Vugs in some outcrop faces are probably molds formed by dissolution of relatively soluble minerals during diagenesis. Microscopic images support the hypothesis that hematite-rich spherules observed in outcrops and soils also formed diagenetically as concretions.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference28 articles.

1. On the wave age dependence of wind stress over pure wind seas

2. K. E. Herkenhoff et al., J. Geophys. Res.108, 8065 10.1029/2003JE002076 (2003).

3. Textures of the Soils and Rocks at Gusev Crater from Spirit's Microscopic Imager

4. A martian solar day has a mean period of 24 hours 39 min 35.244 s and is referred to as a sol to distinguish this from a ∼3% shorter solar day on Earth.

5. The Opportunity Rover's Athena Science Investigation at Meridiani Planum, Mars

Cited by 131 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Gravity aspects for Mars;Icarus;2023-12

2. Sands on Meridiani Planum, Mars;Journal of Geophysical Research: Planets;2023-10

3. Hydrocarbons on Mars;International Journal of Astrobiology;2023-09-21

4. Modern water at low latitudes on Mars: Potential evidence from dune surfaces;Science Advances;2023-04-28

5. Recent Aqueous Activity on Mars Evidenced by Transverse Aeolian Ridges in the Zhurong Exploration Region of Utopia Planitia;Geophysical Research Letters;2023-03-28

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3