Pancam Multispectral Imaging Results from the Spirit Rover at Gusev Crater

J. F. Bell(Ames Research Center), S. W. Squyres(Ames Research Center), R. E. Arvidson(Ames Research Center), H. M. Arneson(Ames Research Center), D. Bass(Ames Research Center), D. L. Blaney(Ames Research Center), Nathalie A. Cabrol(Ames Research Center), W. M. Calvin(Ames Research Center), Jack D. Farmer(Ames Research Center), W. H. Farrand(Ames Research Center), W. Goetz(Ames Research Center), M. P. Golombek(Ames Research Center), J. A. Grant(Ames Research Center), R. Greeley(Ames Research Center), E. A. Guinness(Ames Research Center), Alexander G. Hayes(Ames Research Center), M. Y. H. Hubbard(Ames Research Center), K. E. Herkenhoff(Ames Research Center), M. J. Johnson(Ames Research Center), J. R. Johnson(Ames Research Center), J. Joseph(Ames Research Center), K. M. Kinch(Ames Research Center), M. T. Lemmon(Ames Research Center), R. Li(Ames Research Center), M. B. Madsen(Ames Research Center), J. N. Maki(Ames Research Center), M. C. Malin(Ames Research Center), Elaina McCartney(Ames Research Center), S. M. McLennan(Ames Research Center), H. Y. McSween(Ames Research Center), D. W. Ming(Ames Research Center), J. E. Moersch(Ames Research Center), R. V. Morris(Ames Research Center), E. Z. Noe Dobrea(Ames Research Center), T. J. Parker(Ames Research Center), J. Proton(Ames Research Center), J. W. Rice(Ames Research Center), F. P. Seelos(Ames Research Center), J. M. Soderblom(Ames Research Center), L. A. Soderblom(Ames Research Center), Jascha Sohl‐Dickstein(Ames Research Center), R. Sullivan(Ames Research Center), M. J. Wolff(Ames Research Center), Aimei Wang(Ames Research Center)
Science
August 5, 2004
Cited by 159Open Access
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Abstract

Panoramic Camera images at Gusev crater reveal a rock-strewn surface interspersed with high- to moderate-albedo fine-grained deposits occurring in part as drifts or in small circular swales or hollows. Optically thick coatings of fine-grained ferric iron-rich dust dominate most bright soil and rock surfaces. Spectra of some darker rock surfaces and rock regions exposed by brushing or grinding show near-infrared spectral signatures consistent with the presence of mafic silicates such as pyroxene or olivine. Atmospheric observations show a steady decline in dust opacity during the mission, and astronomical observations captured solar transits by the martian moons, Phobos and Deimos, as well as a view of Earth from the martian surface.


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