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Soils of Eagle Crater and Meridiani Planum at the Opportunity Rover Landing Site
L. A. Soderblom, R. C. Anderson, R. E. Arvidson, J. F. Bell III, N. A. Cabrol, W. Calvin, P. R. Christensen, B. C. Clark, T. Economou, B. L. Ehlmann, W. H. Farrand, D. Fike, R. Gellert, T. D. Glotch, M. P. Golombek, R. Greeley, J. P. Grotzinger, K. E. Herkenhoff, D. J. Jerolmack, J. R. Johnson, B. Jolliff, G. Klingelhöfer, A. H. Knoll, Z. A. Learner, R. Li, M. C. Malin, S. M. McLennan, H. Y. McSween, D. W. Ming, R. V. Morris, J. W. Rice Jr., L. Richter, R. Rieder, D. Rodionov, C. Schröder, F. P. Seelos IV, J. M. Soderblom, S. W. Squyres, R. Sullivan, W. A. Watters, C. M. Weitz, M. B. Wyatt, A. Yen and J. Zipfel
New Series, Vol. 306, No. 5702, Opportunity at Meridiani Planum (Dec. 3, 2004), pp. 1715-1726
Published by: American Association for the Advancement of Science
Stable URL: http://www.jstor.org/stable/3839765
Page Count: 12
You can always find the topics here!Topics: Impact craters, Basaltic soils, Outcrops, Hematite, Soil composition, Basalt, Sedimentary soils, Waves, Sand, Soil erosion
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The soils at the Opportunity site are fine-grained basaltic sands mixed with dust and sulfate-rich outcrop debris. Hematite is concentrated in spherules eroded from the strata. Ongoing saltation exhumes the spherules and their fragments, concentrating them at the surface. Spherules emerge from soils coated, perhaps from subsurface cementation, by salts. Two types of vesicular clasts may represent basaltic sand sources. Eolian ripples, armored by well-sorted hematite-rich grains, pervade Meridiani Planum. The thickness of the soil on the plain is estimated to be about a meter. The flatness and thin cover suggest that the plain may represent the original sedimentary surface.
Science © 2004 American Association for the Advancement of Science