Title Information
Title
Sulfates in Valles Marineris as Indicators of the Aqueous Evolution of Mars
Name: Personal
Name Part
Roach, Leah H.
Role
Role Term: Text
creator
Origin Information
Copyright Date (keyDate="yes", encoding="w3cdtf")
2009
Physical Description
Extent
xxiii, 273 p.
digitalOrigin
born digital
Note
Thesis (Ph.D.) -- Brown University (2009)
Name: Personal
Name Part
Mustard, John
Role
Role Term: Text
director
Name: Personal
Name Part
Head, James
Role
Role Term: Text
reader
Name: Personal
Name Part
Huang, Yongsong
Role
Role Term: Text
reader
Name: Personal
Name Part
Wyatt, Michael
Role
Role Term: Text
reader
Name: Personal
Name Part
Weitz, Cathy
Role
Role Term: Text
reader
Name: Corporate
Name Part
Brown University. Geological Sciences
Role
Role Term: Text
sponsor
Genre (aat)
theses
Abstract
Sulfates are important secondary minerals produced from the evaporation of fluids involved in the aqueous alteration of Mars' primary lithology [Tosca et al. 2005]. Sulfates are potentially good tracers of past environment, and the presence, abundance, and formation processes of sulfates on the surface can all characterize how much water was available. The Valles Marineris canyon system contains many large sulfate deposits. A recent mineralogic model posits that Mars had three eras of alteration mineral formation as the planet cooled and water was increasing unavailable ? Phyllosian, Theiikian, and Siderikian [Bibring et al. 2005]. These eras of phyllosilicate, sulfate, and anhydrous iron oxide formation were hypothesized based on OMEGA (Observatoire pour la Mineralogie, l'Eau, les Glaces et l'Activite) spectral data. This thesis uses higher resolution spectral and imaging data from the Mars Reconnaissance Orbiter, and especially the CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) instrument to test that model. The theses is broken into three topics: (1) the stability of sulfates to alteration under current Martian conditions and how much sulfate hydration state reflects recent periods of high obliquity; (2) the stratigraphic relationship of sulfates and ferric oxides in Valles Marineris and the possible low temperature diagenetic process that formed them; and (3) detailed local and regional stratigraphy of sulfates and other alteration minerals in Valles Marineris. This mapping in Ius Chasma showed phyllosilicate alteration of the Noachian basement predated sulfate deposition. Alteration minerals in Valles Marineris range from other precipitated at low pH (jarosite) to intermediate pH (poorly crystalline hydrated silicate ? liekly a sulfate/smectite mixture) to high pH (smectites). These phases are found in adjacent outcrops, indicating water was available in isolated areas and that Mars retains its early geochemical history. Additionally, the thesis presents mapping of all sulfate deposits in Valles Marineris detected with OMEGA and CRISM spectral data. Terrestrial and martian sulfate deposits are compared to see what these sulfates can tell us about the aqueous evolution of Mars.
Subject (Local)
Topic
Mars
Subject (Local)
Topic
spectroscopy
Subject (Local)
Topic
aqueous geochemistry
Subject (FAST) (authorityURI="http://id.worldcat.org/fast", valueURI="http://id.worldcat.org/fast/1716036")
Topic
Sulfates
Subject (FAST) (authorityURI="http://id.worldcat.org/fast", valueURI="http://id.worldcat.org/fast/1129108")
Topic
Spectrum analysis
Subject (FAST) (authorityURI="http://id.worldcat.org/fast", valueURI="http://id.worldcat.org/fast/1243063")
Geographic
Mars (Planet)
Record Information
Record Content Source (marcorg)
RPB
Record Creation Date (encoding="iso8601")
20091218
Language
Language Term: Code (ISO639-2B)
eng
Language Term: Text
English
Identifier: DOI
10.7301/Z0FX77QC
Access Condition: rights statement (href="http://rightsstatements.org/vocab/InC/1.0/")
In Copyright
Access Condition: restriction on access
Collection is open for research.
Type of Resource (primo)
dissertations