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  5. CONSTRAINING MARTIAN SEDIMENTATION VIA ANALYSIS OF STRATAL PACKAGING, INTRACRATER LAYERED DEPOSITS, ARABIA TERRA, MARS
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CONSTRAINING MARTIAN SEDIMENTATION VIA ANALYSIS OF STRATAL PACKAGING, INTRACRATER LAYERED DEPOSITS, ARABIA TERRA, MARS

Date Issued
May 1, 2011
Author(s)
Cadieux, Sarah Beth
Advisor(s)
Linda C. Kah
Additional Advisor(s)
Christopher Fedo
Devon Burr
Permanent URI
https://trace.tennessee.edu/handle/20.500.14382/45132
Abstract

Craters within Arabia Terra, Mars, contain hundreds of meters of layered strata


showing systematic alternation between slope- and cliff-forming units, suggesting either

rhythmic deposition of distinct lithologies or lithologies that experienced differential

cementation. Hypothesized origins of these intercrater layered deposits include

lacustrine, aeolian, volcanic airfall, and impact surge deposition. On Earth, rhythmically

deposited strata can be examined in terms of stratal packaging, wherein the interplay of

tectonics, sediment deposition, and change in base level results in predictable patterns

with respect to changes in the amount of space available for sediment accumulation.

Fundamental differences between tectonic regimes of Earth and Mars demand that

packaging of layered strata primarily reflects changes in sediment influx and base level.

Analysis of stratal packaging may therefore help us understand the relative roles of these

parameters, and provide crucial constraint on martian depositional models.

Rhythmic stratal patterns in Becquerel Crater (7°W 22°N) have been attributed to

astronomical forcing of regional climate. A clear depositional model, however, has yet to

be presented. Here, we reanalyze strata of Becquerel Crater and compare results with

two additional crater successions. Results indicate that, by contrast with Becquerel

Crater, strata within Danielson Crater (7°W 8°N) and an unnamed crater (Crater X;

1.2°W 9°N) do not record hierarchical packaging readily attributable to astronomical

effects, and suggest that regional climate forcing may not be readily applied as a

paradigm for all intracrater deposition. Similarities in depositional style in these three

craters, however, may be linked by a model for sediment accumulation—with potential

links to regional climate—wherein episodic melting of ground ice raised local base level,

stabilized aeolian sedimentation, and resulted in differential cementation of accumulated

strata.

Subjects

Mars

Sedimentology

Stratigraphy

Arabia Terra

Layering

Disciplines
Geology
Physical Processes
Sedimentology
Degree
Master of Science
Major
Geology
Embargo Date
December 1, 2011
File(s)
Thumbnail Image
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0-CadieuxSarahMay2011thesisAttachments.xlsx

Size

116.31 KB

Format

Microsoft Excel XML

Checksum (MD5)

535246e48c7ee6be719fad323b044a2a

Thumbnail Image
Name

CadieuxSarahMay2011thesis.pdf

Size

38.62 MB

Format

Adobe PDF

Checksum (MD5)

1c2cf9ca28e96b595a81b65148f64ae5


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