107 Camilla

outer main-belt asteroid

References change

  1. 1.0 1.1 1.2 J. Torppa; et al. (2003). "Shapes and rotational properties of thirty asteroids from photometric data" (PDF). Icarus. 164 (2): 346. doi:10.1016/S0019-1035(03)00146-5. S2CID 119609765. Archived from the original (PDF) on 2015-11-06. Retrieved 2007-12-24.
  2. 2.0 2.1 2.2 "IAUC 7599". Archived from the original on 2006-05-01. Retrieved 2007-12-24.
  3. 3.0 3.1 3.2 3.3 3.4 107 Camilla and S/2001 (107) 1, F. Marchis Archived 2007-07-24 at the Wayback Machine
  4. 4.0 4.1 4.2 4.3 F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185 (1): 39–63. Bibcode:2006Icar..185...39M. doi:10.1016/j.icarus.2006.06.001. PMC 2600456. PMID 19081813.
  5. Assuming a similar density to the primary.
  6. 6.0 6.1 6.2 "Supplemental IRAS Minor Planet Survey". Archived from the original on 2010-01-17. Retrieved 2007-12-24.{{cite web}}: CS1 maint: bot: original URL status unknown (link)
  7. 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).
  8. Error estimate derived from consideration of   and given errors in a and P. See propagation of uncertainty.
  9. "PDS spectral class data". Archived from the original on 2010-01-17. Retrieved 2007-12-24.{{cite web}}: CS1 maint: bot: original URL status unknown (link)

Other websites change