Geologic and spectral mapping of etched terrain deposits in northern Meridiani Planum
نویسندگان
چکیده
[1] A 1 km vertical section of etched terrain and hematite-bearing plains materials and nearby cratered terrain surfaces was mapped in the northern portion of Meridiani Planum using MOC, THEMIS, MOLA, and OMEGA data. The oldest materials are the cratered plains, which have 0.4 to 2.5 mm spectral reflectance dominated by a mix of low and high calcium pyroxenes. Etched plains materials overlie this unit and are exposed within a 120 km NW-SE trending valley to the south of the cratered plains. Lower etched plains materials exhibit a kieserite signature on a plateau-forming horizon and polyhydrated sulfate signatures on the main valley floor. The upper etched plains unit exhibits signatures consistent with hydrated iron oxides and is covered by what is interpreted to be a relatively thin layer of basaltic sand and hematitic concretions (the hematite-bearing plains unit). The youngest unit consists of ejecta deposits from a cluster of six craters that mantle the eastern portion of the study area. The thick section of etched plains materials ( 900 m) with exposures of hydrated sulfates and hydrated iron oxides implies that measurements made by the Opportunity rover (located 390 km to the southwest of the study area) are at the top of an extensive section of layered sedimentary materials formed in and/or altered in an aqueous environment and exposed by aeolian erosion.
منابع مشابه
Geomorphic and Spectral Mapping of Northern Meridiani Planum
Introduction: Mars Orbiter Camera (MOC), Mars Orbiter Laser Altimeter (MOLA), Thermal Emission Imaging System (THEMIS), and Mars Express Observatoire pour la Minéralogie, l’Eau, les Glaces et l’Activité (OMEGA) data were compiled and coregistered for analysis of a several hundred meter vertical section of plains, etched, and cratered units in the northern portion of Meridiani Planum. Five units...
متن کاملFormation of jarosite-bearing deposits through aqueous oxidation of pyrite at Meridiani Planum, Mars
[1] The discovery of sulfate-rich layered deposits with hematite spherules at the landing site of the Opportunity rover is consistent with mineral deposition in an aqueous environment. We evaluate conditions responsible for the formation of a jarosite-goethite-gypsum assemblage with speciation calculations. The results show that the assemblage could have precipitated from acidic solutions forme...
متن کاملLithologic Unit Mapping Based on Omega/mars Express Data
This paper develops a procedure for mapping Martian lithologic units, using the OMEGA/Mars Express data. The procedure consists of correcting Martian atmospheric absorptions based on an empirical transmission function method, noise-free principle components analysis based on a minimum noise fraction (MNF) method, lithologic unit delineation, and spectral matching of the units to spectral librar...
متن کاملStructure of Polygonal Impact Craters at Meridiani Planum, Mars, and a Model Relating Target Structure to Crater Shape
Introduction: Among the classic field-and laboratory studies of crater structure, a handful have mentioned the influence of fracture networks upon crater shapes [1,2,3] and few later investigations have addressed the problem directly (see [4] for a recent study and thorough review). A polygonal simple crater is thought to result when the excavation flow exploits planes-of-weakness in the target...
متن کاملGeologic mapping of ejecta deposits in Oppia Quadrangle, Asteroid (4) Vesta
Oppia Quadrangle Av-10 (288–360 E, ±22 ) is a junction of key geologic features that preserve a rough history of Asteroid (4) Vesta and serves as a case study of using geologic mapping to define a relative geologic timescale. Clear filter images, stereo-derived topography, slope maps, and multispectral color-ratio images from the Framing Camera on NASA’s Dawn spacecraft served as basemaps to cr...
متن کامل