| Article ID | Journal | Published Year | Pages | File Type | 
|---|---|---|---|---|
| 10705269 | Planetary and Space Science | 2011 | 12 Pages | 
Abstract
												The spectral gradients at optical wavelengths observed for both Phobos and Deimos are quantitatively in good agreement with those found by unresolved photometric observations made by the Imager for Mars Pathfinder (IMP; Thomas et al., JGR, 104, 9055-9068, 1999). The spectral gradients of the blue and red units on Phobos bracket the results from IMP.
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											Authors
												N. Thomas, R. Stelter, A. Ivanov, N.T. Bridges, K.E. Herkenhoff, A.S. McEwen, 
											