The Possible Aqueous Origins of Manganese Alteration Minerals in the Máaz Formation of Jezero Crater.

IF 2.3 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Astrobiology Pub Date : 2026-10-01 Epub Date: 2026-06-29 DOI:10.1177/15311074261461401
Kimberly P Sinclair, Benton C Clark, Michael W M Jones, David C Catling, William T Elam, Yang Liu
{"title":"The Possible Aqueous Origins of Manganese Alteration Minerals in the Máaz Formation of Jezero Crater.","authors":"Kimberly P Sinclair, Benton C Clark, Michael W M Jones, David C Catling, William T Elam, Yang Liu","doi":"10.1177/15311074261461401","DOIUrl":null,"url":null,"abstract":"<p><p>Home to a lake around 4 billion years ago, Jezero Crater is a unique location to study the interplay between igneous processes and aqueous alteration on ancient Mars. The Máaz formation, rich in basaltic rock, is the highest stratigraphic unit on the crater floor and hosts a diversity of alteration phases that indicate multiple aqueous episodes affected the crater floor rocks. Using data from the Planetary Instrument for X-ray Lithochemistry aboard the Perseverance rover, we investigated manganese enrichments across the crater floor. We report on multiple distinct types of Mn-rich materials. The first, in the Guillaumes abrasion low in the Máaz formation, has been tentatively identified as the rare mineral despujolsite (Ca<sub>3</sub>Mn<sup>4+</sup>(SO<sub>4</sub>)<sub>2</sub>(OH)<sub>6</sub>·3H<sub>2</sub>O), which forms on Earth in hydrothermal and lacustrine deposits. In the Alfalfa abrasion patch, high in the Máaz formation, we find Mn-enriched magnetite spatially associated with a Ca-dominant sulfate that may contain minor Mn, which suggests a history of serpentinization followed by exposure to oxidizing acidic fluids. These findings underscore the complexity of aqueous alteration over the course of Jezero history. Future sample return missions could refine mineralogical interpretations and provide more information to improve our understanding of aqueous conditions and habitability in the crater.</p>","PeriodicalId":8645,"journal":{"name":"Astrobiology","volume":" ","pages":"794-810"},"PeriodicalIF":2.3000,"publicationDate":"2026-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrobiology","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1177/15311074261461401","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2026/6/29 0:00:00","PubModel":"Epub","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

Home to a lake around 4 billion years ago, Jezero Crater is a unique location to study the interplay between igneous processes and aqueous alteration on ancient Mars. The Máaz formation, rich in basaltic rock, is the highest stratigraphic unit on the crater floor and hosts a diversity of alteration phases that indicate multiple aqueous episodes affected the crater floor rocks. Using data from the Planetary Instrument for X-ray Lithochemistry aboard the Perseverance rover, we investigated manganese enrichments across the crater floor. We report on multiple distinct types of Mn-rich materials. The first, in the Guillaumes abrasion low in the Máaz formation, has been tentatively identified as the rare mineral despujolsite (Ca3Mn4+(SO4)2(OH)6·3H2O), which forms on Earth in hydrothermal and lacustrine deposits. In the Alfalfa abrasion patch, high in the Máaz formation, we find Mn-enriched magnetite spatially associated with a Ca-dominant sulfate that may contain minor Mn, which suggests a history of serpentinization followed by exposure to oxidizing acidic fluids. These findings underscore the complexity of aqueous alteration over the course of Jezero history. Future sample return missions could refine mineralogical interpretations and provide more information to improve our understanding of aqueous conditions and habitability in the crater.

耶泽罗陨石坑Máaz地层中锰蚀变矿物的可能水源
大约40亿年前,耶泽罗陨石坑是一个湖泊的所在地,是研究古代火星上火成岩过程和水蚀变之间相互作用的独特地点。Máaz组富含玄武质岩石,是火山口底部最高的地层单元,其蚀变阶段的多样性表明火山口底部岩石受到多次含水事件的影响。利用毅力号探测器上的x射线岩石化学行星仪器的数据,我们研究了陨石坑底部的锰富集情况。我们报告了多种不同类型的富锰材料。第一种是在Máaz组的Guillaumes磨损层中,初步确定为稀有矿物despujolsite (Ca3Mn4+(SO4)2(OH)6·3H2O),形成于地球上的热液和湖相矿床。在高Máaz地层的苜蓿磨蚀斑中,我们发现富锰磁铁矿在空间上与可能含有少量锰的以钙为主的硫酸盐相关,这表明蛇纹岩化的历史随后暴露于氧化酸性流体中。这些发现强调了耶泽罗历史过程中含水变化的复杂性。未来的样品返回任务可以完善矿物学解释,并提供更多信息,以提高我们对陨石坑的水条件和可居住性的理解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
Astrobiology
Astrobiology 生物-地球科学综合
CiteScore
7.70
自引率
11.90%
发文量
100
审稿时长
3 months
期刊介绍: Astrobiology is the most-cited peer-reviewed journal dedicated to the understanding of life''s origin, evolution, and distribution in the universe, with a focus on new findings and discoveries from interplanetary exploration and laboratory research. Astrobiology coverage includes: Astrophysics; Astropaleontology; Astroplanets; Bioastronomy; Cosmochemistry; Ecogenomics; Exobiology; Extremophiles; Geomicrobiology; Gravitational biology; Life detection technology; Meteoritics; Planetary geoscience; Planetary protection; Prebiotic chemistry; Space exploration technology; Terraforming
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信
小红书