Mars in the late Noachian : evolution of a habitable surface environment

Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2008. This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections. Includes bibliographical references. Th...

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Main Author: Johnson, Sarah Stewart
Other Authors: Maria T. Zuber., Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.
Format: Thesis
Language:English
Published: Massachusetts Institute of Technology 2008
Subjects:
Online Access:http://hdl.handle.net/1721.1/45605
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spelling ftmit:oai:dspace.mit.edu:1721.1/45605 2023-06-11T04:15:59+02:00 Mars in the late Noachian : evolution of a habitable surface environment Johnson, Sarah Stewart Maria T. Zuber. Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences. zma --- 2008 240 p. application/pdf http://hdl.handle.net/1721.1/45605 eng eng Massachusetts Institute of Technology http://hdl.handle.net/1721.1/45605 318645666 M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 Earth Atmospheric and Planetary Sciences Thesis 2008 ftmit 2023-05-29T08:34:48Z Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2008. This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections. Includes bibliographical references. This dissertation addresses whether simple life forms might have existed on Mars during the late Noachian epoch, and whether those life forms, or their traces, can be detected today. It begins by analyzing the ancient Martian climate in light of new evidence that sulfur chemistry played a prominent role in the planet's early evolution. It finds that sulfur-induced greenhouse warming could have periodically heated the planet enough to support liquid water, thereby creating warm, wet, clement conditions. Moreover, it finds that those warming pulses, while short-lived over geologic time, may have persisted for hundreds of years. If sulfur helped create environmental conditions capable of hosting life, however, it also created conditions that were adverse to sustaining it. In particular, dissipation of sulfur volatiles cooled the climate, and sulfur rainout contributed to the acidity of Martian surface waters. The dissertation therefore proceeds to analyze the potential for persistence and detection of life in terrestrial environments with Mars-like characteristics. It first investigates the potential for detecting ancient life by searching for lipid biomarkers in sulfur-rich acid salt lakes, concluding that a variety of biomarkers may be more resistant to decay than previously believed. It then analyzes soil samples from permafrost, discovering the oldest independently authenticated viable organisms ever found, and positing low-level metabolic activity and DNA repair as a survival mechanism in ancient cells. Finally, the dissertation uses deep sequencing to examine prokaryotic diversity in a terrestrial Mars-like river characterized by low pH and high concentrations of iron and sulfur, with results considered in ... Thesis permafrost DSpace@MIT (Massachusetts Institute of Technology)
institution Open Polar
collection DSpace@MIT (Massachusetts Institute of Technology)
op_collection_id ftmit
language English
topic Earth
Atmospheric
and Planetary Sciences
spellingShingle Earth
Atmospheric
and Planetary Sciences
Johnson, Sarah Stewart
Mars in the late Noachian : evolution of a habitable surface environment
topic_facet Earth
Atmospheric
and Planetary Sciences
description Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2008. This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections. Includes bibliographical references. This dissertation addresses whether simple life forms might have existed on Mars during the late Noachian epoch, and whether those life forms, or their traces, can be detected today. It begins by analyzing the ancient Martian climate in light of new evidence that sulfur chemistry played a prominent role in the planet's early evolution. It finds that sulfur-induced greenhouse warming could have periodically heated the planet enough to support liquid water, thereby creating warm, wet, clement conditions. Moreover, it finds that those warming pulses, while short-lived over geologic time, may have persisted for hundreds of years. If sulfur helped create environmental conditions capable of hosting life, however, it also created conditions that were adverse to sustaining it. In particular, dissipation of sulfur volatiles cooled the climate, and sulfur rainout contributed to the acidity of Martian surface waters. The dissertation therefore proceeds to analyze the potential for persistence and detection of life in terrestrial environments with Mars-like characteristics. It first investigates the potential for detecting ancient life by searching for lipid biomarkers in sulfur-rich acid salt lakes, concluding that a variety of biomarkers may be more resistant to decay than previously believed. It then analyzes soil samples from permafrost, discovering the oldest independently authenticated viable organisms ever found, and positing low-level metabolic activity and DNA repair as a survival mechanism in ancient cells. Finally, the dissertation uses deep sequencing to examine prokaryotic diversity in a terrestrial Mars-like river characterized by low pH and high concentrations of iron and sulfur, with results considered in ...
author2 Maria T. Zuber.
Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.
format Thesis
author Johnson, Sarah Stewart
author_facet Johnson, Sarah Stewart
author_sort Johnson, Sarah Stewart
title Mars in the late Noachian : evolution of a habitable surface environment
title_short Mars in the late Noachian : evolution of a habitable surface environment
title_full Mars in the late Noachian : evolution of a habitable surface environment
title_fullStr Mars in the late Noachian : evolution of a habitable surface environment
title_full_unstemmed Mars in the late Noachian : evolution of a habitable surface environment
title_sort mars in the late noachian : evolution of a habitable surface environment
publisher Massachusetts Institute of Technology
publishDate 2008
url http://hdl.handle.net/1721.1/45605
op_coverage zma ---
genre permafrost
genre_facet permafrost
op_relation http://hdl.handle.net/1721.1/45605
318645666
op_rights M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.
http://dspace.mit.edu/handle/1721.1/7582
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