Phobos as a D-type captured asteroid, spectral modeling from 0.25 to 4.0 μm

• Published in: The Astrophysical Journal
• Main Authors: Pajola M., Lazzarin M., Dalle Ore C. M., Cruikshank D. P., Roush T. L., Magrin S., Bertini I., La Forgia F., Barbieri C.
• Other Authors: Pajola, M., Lazzarin, M., Dalle Ore, C. M., Cruikshank, D. P., Roush, T. L., Magrin, S., Bertini, I., La Forgia, F., Barbieri, C.
• Format: Article in Journal/Newspaper
• Language: English
• Published: 2013
• Subjects: planets and satellites: individual (Phobos); planets and satellites: surface; techniques: imaging spectroscopy; Tagish; Tagish Lake
• Online Access: http://hdl.handle.net/11367/88372; https://doi.org/10.1088/0004-637X/777/2/127; http://iopscience.iop.org/0004-637X/777/2/127/pdf/0004-637X_777_2_127.pdf

This paper describes the spectral modeling of the surface of Phobos in the wavelength range between 0.25 and 4.0 μm. We use complementary data to cover this spectral range: the OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System on board the ESA Rosetta spacecraft) reflectance spectru...