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...
Main Author: | |
---|---|
Other Authors: | , |
Format: | Thesis |
Language: | English |
Published: |
Massachusetts Institute of Technology
2008
|
Subjects: | |
Online Access: | http://hdl.handle.net/1721.1/45605 |
id |
ftmit:oai:dspace.mit.edu:1721.1/45605 |
---|---|
record_format |
openpolar |
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 |
_version_ |
1768373286621675520 |