107 Camilla

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  1. ^ Lutz D. Schmadel, Dictionary of Minor Planets Names, p.25.
  2. ^ Morrison, D.; Chapman, C. R. (March 1976), "Radiometric diameters for an additional 22 asteroids", Astrophysical Journal 204: 934–939, Bibcode:2008mgm..conf.2594S, doi:10.1142/9789812834300_0469. 
  3. ^ a b c J. Torppa et al. (2003). "Shapes and rotational properties of thirty asteroids from photometric data" (PDF). Icarus 164 (2): 346. Bibcode:2003Icar..164..346T. doi:10.1016/S0019-1035(03)00146-5. 
  4. ^ a b c IAUC 7599
  5. ^ a b c d e 107 Camilla and S/2001 (107) 1, F. Marchis
  6. ^ a b c d 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. 
  7. ^ Assuming a similar density to the primary.
  8. ^ Yeomans, Donald K., "107 Camilla", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), retrieved 2013-03-25. 
  9. ^ a b c Jim Baer (2008). "Recent Asteroid Mass Determinations". Personal Website. Retrieved 2008-12-05. 
  10. ^ a b c Supplemental IRAS Minor Planet Survey
  11. ^ 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 requiring the shortest axis to be no larger than the maximum allowed by Marchis et al. (2006).
  12. ^ Error estimate derived from consideration of M \propto a^3/P^2 and given errors in a and P. See propagation of uncertainty.
  13. ^ PDS spectral class data
  14. ^ "AstDys (107) Camilla Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2010-06-28. 

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