Evidence for plunging river plume deposits in the Pahrump Hills member of the Murray formation, Gale crater, Mars
File(s)Stack_et_al-2018-Sedimentology.pdf (4.84 MB)
Accepted version
Author(s)
Type
Journal Article
Abstract
Recent robotic missions to Mars have offered new insights into the extent, diversity and habitability of the Martian sedimentary rock record. Since the Curiosity rover landed in Gale crater in August 2012, the Mars Science Laboratory Science Team has explored the origins and habitability of ancient fluvial, deltaic, lacustrine and aeolian deposits preserved within the crater. This study describes the sedimentology of a ca 13 m thick succession named the Pahrump Hills member of the Murray formation, the first thick fine‐grained deposit discovered in situ on Mars. This work evaluates the depositional processes responsible for its formation and reconstructs its palaeoenvironmental setting. The Pahrump Hills succession can be sub‐divided into four distinct sedimentary facies: (i) thinly laminated mudstone; (ii) low‐angle cross‐stratified mudstone; (iii) cross‐stratified sandstone; and (iv) thickly laminated mudstone–sandstone. The very fine grain size of the mudstone facies and abundant millimetre‐scale and sub‐millimetre‐scale laminations exhibiting quasi‐uniform thickness throughout the Pahrump Hills succession are most consistent with lacustrine deposition. Low‐angle geometric discordances in the mudstone facies are interpreted as ‘scour and drape’ structures and suggest the action of currents, such as those associated with hyperpycnal river‐generated plumes plunging into a lake. Observation of an overall upward coarsening in grain size and thickening of laminae throughout the Pahrump Hills succession is consistent with deposition from basinward progradation of a fluvial‐deltaic system derived from the northern crater rim into the Gale crater lake. Palaeohydraulic modelling constrains the salinity of the ancient lake in Gale crater: assuming river sediment concentrations typical of floods on Earth, plunging river plumes and sedimentary structures like those observed at Pahrump Hills would have required lake densities near freshwater to form. The depositional model for the Pahrump Hills member presented here implies the presence of an ancient sustained, habitable freshwater lake in Gale crater for at least ca 103 to 107 Earth years.
Date Issued
2019-08-01
Date Acceptance
2018-11-01
Citation
Sedimentology, 2019, 65 (5), pp.1768-1802
ISSN
0037-0746
Publisher
Wiley
Start Page
1768
End Page
1802
Journal / Book Title
Sedimentology
Volume
65
Issue
5
Copyright Statement
© 2019 Owner. This is the accepted version of the following article: Stack, K. M., Grotzinger, J. P., Lamb, M. P., Gupta, S. , Rubin, D. M., Kah, L. C., Edgar, L. A., Fey, D. M., Hurowitz, J. A., McBride, M. , Rivera‐Hernández, F. , Sumner, D. Y., Van Beek, J. K., Williams, R. M. and Aileen Yingst, R. (2019), Evidence for plunging river plume deposits in the Pahrump Hills member of the Murray formation, Gale crater, Mars. Sedimentology. doi:10.1111/sed.12558, which has been published in final form at https://doi.org/10.1111/sed.12558.
Sponsor
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Grant Number
ST/J005169/1
ST/N000579/1
Subjects
Science & Technology
Physical Sciences
Geology
Curiosity rover
Gale crater
lacustrine
Mars
Mars Science Laboratory
sedimentology
stratigraphy
SCIENCE LABORATORY MISSION
GRAINED SEDIMENTARY-ROCKS
TURBIDITY CURRENTS
JEZERO CRATER
HYPERPYCNAL FLOWS
CLAY-MINERALS
CYCLIC STEPS
EVOLUTION
DELTA
RESERVOIR
0403 Geology
Geology
Publication Status
Published
Date Publish Online
2019-02-18