Phobos and Deimos
Observations by the Imager for Mars Pathfinder of Phobos and Deimos were used to produce low resolution spectra of the satellites [Thomas et al., 1999; Murchie et al., 1999]. HiRISE has been used to image them, in colour with high spatial resolution, to reveal inhomogeneities in material properties on on the surface. Preliminary colour maps of one face of each object have been produced showing remarkable structure on their surfaces. We are currently using digital terrain models of Phobos from DLR in Germany to try to model the Stickney impact and investigate its grooves and ejecta.
Pieters, C.M., S. Murchie, N. Thomas, and D. Britt, (2014), Composition of surface materials on the moons of Mars, Planetary and Space Science, accepted, 19 February 2014, doi: 10.1016/j.pss.2014.02.008.
Thomas, N., R. Stelter, A. Ivanov, N.T. Bridges, K.E. Herkenhoff, and A.S. McEwen, (2010), Spectral heterogeneity on Phobos and Deimos: HiRISE observations and comparisons to Mars Pathfinder results, Planetary and Space Science, 59, 1281-1292, doi:10.1016/j.pss.2010.04.018.
Thomas, N. Britt, D.T., Herkenhoff, K.E., Murchie, S.L., Keller, H.U., and Smith, P.H. (1998) Observations of Phobos, Deimos, and bright stars with the Imager for Mars Pathfinder. J. Geophys. Res., 104, 9055-9068.
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