
Abstract We find a clear diversity in the 3 μm and 10 μm features of three Cybele asteroids: (107) Camilla, (121) Hermione, and (65) Cybele. (121) Hermione exhibits a “check-like” 3 μm feature, which may be attributed to OH-dominated minerals and (107) Camilla shows a rounded “bowl” like feature closer to that of (65) Cybele, which may be attributed to H 2 O-dominated minerals. The 10 μm features of these three asteroids are also different from each other.
SPEX, SURFACE, Infrared observations, BELT, ICE, Astronomy & Astrophysics, Asteroids, Surfaces, SPECTROGRAPH, WATER, ORGANICS, Spectroscopy, SPITZER-SPACE-TELESCOPE
SPEX, SURFACE, Infrared observations, BELT, ICE, Astronomy & Astrophysics, Asteroids, Surfaces, SPECTROGRAPH, WATER, ORGANICS, Spectroscopy, SPITZER-SPACE-TELESCOPE
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