107 Camilla is one of the biggest main belt asteroids. It orbits within the Cybele Group, beyond most of the main belt asteroids. It has a very dark surface and is made of carbonate. It was found by N. R. Pogson on November 17, 1868, and named after Camilla, Queen of the Volsci in Roman mythology.
Moon (S/2001 (107) I)[change | change source]
References[change | change source]
- J. Torppa; et al. (2003). "Shapes and rotational properties of thirty asteroids from photometric data" (PDF). Icarus. 164: 346.
- "IAUC 7599". Archived from the original on 2006-05-01. Retrieved 2007-12-24.
- 107 Camilla and S/2001 (107) 1, F. Marchis Archived 2010-01-17 at WebCite
- F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185: 39.
- Assuming a similar density to the primary.
- "Supplemental IRAS Minor Planet Survey". Archived from the original on 2010-01-17. Retrieved 2007-12-24.CS1 maint: BOT: original-url status unknown (link)
- Axis ratios (rounded to nearest 5 km) based on lightcurve analysis of Torppa et al. (2003), however taking IRAS mean diameter is inconsistent with the maximum value of the short axis obtained in Marchis et al. (2006). Hence, presumably IRAS measurements were taken of a large face. Therefore, anchoring absolute size by reuqiring the shortest axis to be no larger than the maximum allowed by Marchis et al. (2006).
- Error estimate derived from consideration of and given errors in a and P. See propagation of uncertainty.
- "PDS spectral class data". Archived from the original on 2010-01-17. Retrieved 2007-12-24.CS1 maint: BOT: original-url status unknown (link)