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Asteroid mass determination: (1) Ceres

Published online by Cambridge University Press:  25 May 2016

M. Carpino  and
Z. Knežević
M. Carpino
Affiliation:
Osservatorio astronomico di Brera, Milano
Z. Knežević
Affiliation:
Astronomska opservatorija, Beograd

Extract

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Recent improvements of observational accuracy, stellar catalogues and efficiency of the procedures for searching for asteroid close encounters (Kuzmanoski and Knežević, 1993) gave rise to an increased interest in the problem of determination of asteroid masses (Bowell et al., 1995).

Type
Part IV - Asteroids: Theory and Ephemerides
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 203 - 206
Copyright
Copyright © Kluwer 1996 

References

Bowell, E., Muinonen, K. and Wasserman, L.H. (1995) Asteroid mass determination from multiple asteroid-asteroid encounters, Proceedings of Mariehamn, in press Google Scholar
Goffin, E. (1991) The orbit of 203 Pompeja and the mass of Ceres, Astron. Astrophys. 249, 563–568 Google Scholar
Kuzmanoski, M. and Knežević, Z. (1993) Close encounters with large asteroids in the next 50 years, Icarus 103, 93–103 CrossRefGoogle Scholar
Kuzmanoski, M. and Knežević, Z. (1994) Asteroid close encounters and mutual perturbations, Planet. Space Sci. 42, 297–299 CrossRefGoogle Scholar
Standish, E. M., Newhall, X X, Williams, J. G. and Folkner, W. M. (1995) JPL Planetary and Lunar Ephemerides, DE403/LE403, JPL IOM 314.10-127 .CrossRefGoogle Scholar
Williams, G.V. (1992) The mass of (1) Ceres from perturbations on (348) May, in Harris, A.E. and Bowell, E. eds., Asteroids, Comets, Meteors 1991, Lunar and Planetary Institute, Houston, Texas, 641–643 Google Scholar