Interpretation of the surface brightness of Phobos.
Analysis of disk resolved images of Phobos obtained by the Phobos 2 spacecraft allows us to study the surface scattering law and albedo variations.  From low phase angle images we find variations in local geometric albedo approximately 10%, with a correlation length approximately 1km.  The scattering law is reasonably well matched by the recent proposed LPI (Lumme et al. 1990a)  model, which allows us to deduce a small scale (approximately 1 mm) surface roughness (approximately 0.5), defined here as the rms. tangent of the local surface normal relative to the mean surface normal in the Duxbury (1991) model of Phobos.  This value is very close to what has been found for Mercury and the Moon.
Peltoniemi
J I
JI
Observatory and Astrophysics Laboratory, University of Helsinki, Finland.
Lumme
K
K
Irvine
W M
WM
D001256:Astronomy / Q000379:methods; D004735:Energy Transfer; D005118:Extraterrestrial Environment; D008027:Light; D018535:Mars; D008433:Mathematics; D008962:Models, Theoretical; D012542:Scattering, Radiation; D012987:Soil; D018531:Spacecraft
D012987:Soil