Asteroids (65) Cybele, (107) Camilla and (121) Hermione: Infrared spectral diversity among the Cybeles

Bibcode
2012Icar..221..453H
DOI
10.1016/j.icarus.2012.07.013
Hargrove, Kelsey D.; Kelley, Michael S.; Campins, Humberto; Licandro, J.; Emery, Josh
Bibliographical reference

Icarus, Volume 221, Issue 1, p. 453-455.

Advertised on:
9
2012
Journal
ICARUS
Number of authors
5
IAC number of authors
1
Citations
13
Refereed citations
12
Description
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 H2O-dominated minerals. The 10 μm features of these three asteroids are also different from each other.
Related projects
Project Image
Minor Bodies of the Solar System
This project studies the physical and compositional properties of the so-called minor bodies of the Solar System, that includes asteroids, icy objects, and comets. Of special interest are the trans-neptunian objects (TNOs), including those considered the most distant objects detected so far (Extreme-TNOs or ETNOs); the comets and the comet-asteroid
Julia de
León Cruz
In progress
Type
Refereed
Exoplanetary Systems & Solar System (SEYSS)

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