Insights into the origins of Phobos and Deimos based on a spectral comparison with small bodies and Martian materials

Open Access

Table C.1

Spectral slope in the VIS (0.7–0.9 µm) and NIR (1.5–2.2 µm) wavelength range for radiance factor and SSA spectra of Deimos (Fraeman et al. 2012, 2014).

Deimos spectra	α	VIS slope (0.7–0.9 µm)	NIR slope (1.5–2.2 µm)
Raw I/F	22°	10.7 %.(100 nm)⁻¹	2.9 %.(100 nm)⁻¹
Corrected I/F	30°	9.8 %.(100 nm)⁻¹	2.7 %.(100 nm)⁻¹
Single-scattering albedo	–	10.8 %.(100 nm)⁻¹	2.8 %.(100 nm)⁻¹

Notes. The phase angle α of observations is not indicated for the singlescattering albedo spectrum as it is independent of the geometry of observation by definition.

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