HR: 1340h
AN: P13D-1560 [Abstracts]
TI: The extent of phyllosilicates in the northern highlands around Mawrth Vallis: CRISM observations of Western Arabia Terra
AU: * Noe Dobrea, E Z
EM: edobrea@msss.com
AF: Jet Propulsion Laboratories, Mail Stop 183-501
4800 Oak Grove Drv, Pasadena, CA 91109, United States
AU: Bishop, J L
EM: jbishop@arc.nasa.gov
AF: SETI Institute/NASA ARC, 515 N Whisman Rd, Mountain View, CA 94043, United States
AU: McKeown, N
EM: nmckeown@emerald.ucsc.edu
AF: UC Santa Cruz, 1156 High Street, Santa Cruz, CA 95060, United States
AU: Mustard, J F
EM: John_Mustard@brown.edu
AF: Dept. of Geological Sciences
Brown University, 324 Brook St, Providence, RI 02906, United States
AU: Ehlmann, B L
EM: bethany_ehlmann@brown.edu
AF: Dept. of Geological Sciences
Brown University, 324 Brook St, Providence, RI 02906, United States
AU: Murchie, S L
EM: Scott.Murchie@jhuapl.edu
AF: Applied Physics Laboratory, 11100 John Hopkins Rd, Laurel, MD 20723, United States
AU: Bibring, J
EM: bibring@ias.u-psud.fr
AF: IAS
Univerisity of Paris, 98 B, Boulevard Arago, Paris, 75014, France
AU: Poulet, F
EM: francois.poulet@ias.u-psud.fr
AF: IAS
Univerisity of Paris, 98 B, Boulevard Arago, Paris, 75014, France
AU: Malaret, E
EM: malaret@ACTGATE.COM
AF: Applied Coherent Technology, Inc., 112 Elden St., Herndon, VA 20170, United States
AU: Hash, C
EM: hash@actgate.com
AF: Applied Coherent Technology, Inc., 112 Elden St., Herndon, VA 20170, United States
AU: TEAM, C
EM: scott.murchie@jhuapl.edu
AB:
The largest spatial exposure of phyllosilicates on the surface of Mars occurs on the highland plains around
Mawrth Vallis. It extends for about 300 kilometers southward from the edge of the dichotomy boundary, covering
an area of over 200 x 300 km (e.g., Poulet et al 2005; Noe Dobrea and Michalski 2006; Loizeau et al 2007) over an
elevation range of ~2000 m. At least two different types of phyllosilicates (Fe/Mg smectites, and Al smectites),
presenting complex spatial and stratigraphic relationships, have been identified in OMEGA data. Stratigraphically,
the phyllosilicate-bearing units appear exposed from under a darker, indurated, and more heavily cratered unit,
suggesting that it has recently been exhumed (Michalski and Noe Dobrea, 2007) from under an overlying unit. It
is unclear, however, whether the clay-bearing units extend into the southern highlands and into the northern
lowlands.
In this investigation, we use both OMEGA spectral cubes (~1 km/pixel) and CRISM multispectral data sampled at
256 pixels per degree and map projected into 5-degree tiles (~230 m/pixel) to further constrain the extent of
phyllosilicates in the Mawrth Vallis region. We find a good correlation between the spatial distribution of
phyllosilicates as detected by CRISM and OMEGA, where coverage overlaps. We identify additional small,
localized phyllosilicate exposures in CRISM tiles in places up to 100 km farther than the boundaries previously
identified with OMEGA. These exposures are found around craters to the south, in interior deposits of a crater to
the east, and in association with hummocks in the lowlands to the north. Additional phyllosilicate signatures are
observed in darker materials at the base of the escarpment that constitutes the dichotomy boundary in this area.
The exposures show spatial variability of the 2.2- and 2.3-μ m absorptions, suggesting complex spatial and
stratigraphic relationships similar to those previously observed in the largest exposures. The identification of
phyllosilicate exposures in the southern highlands may suggest that the clay-bearing unit observed around
Mawrth Vallis is in fact an exposure of a much more extensive clay unit that may underlie at least part of the
southern highlands. Additionally, the identification of phyllosilicates in some of the hummocks of the northern
lowlands suggests that these hummocks may be erosional remnants of a formerly more extensive unit, leading
to the possibility that the dichotomy boundary has erosionally regressed.
DE: 3672 Planetary mineralogy and petrology (5410)
DE: 5464 Remote sensing
DE: 5470 Surface materials and properties
DE: 6225 Mars
SC: Planetary Sciences [P]
MN: 2007 Fall Meeting