Abstract
The expansion of the external gravitational potential of solid, irregular bodies of non-near spherical shape in terms of Spheroidal Harmonics is introduced as a way to minimize the divergence region, or Brillouin sphere, associated with the use of the more usual Spherical Harmonics. A method for the numerical evaluation of the spheroidal Stokes coefficients is proposed.
The support of the Italian Space Agency (ASI) is gratefully acknowledged.
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Casotto, S. (2002). On the Expansion of the External Gravitational Potential in Spheroidal Harmonics. In: Celletti, A., Ferraz-Mello, S., Henrard, J. (eds) Modern Celestial Mechanics: From Theory to Applications. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-2304-6_23
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DOI: https://doi.org/10.1007/978-94-017-2304-6_23
Publisher Name: Springer, Dordrecht
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