4.7 Article

ON THE GRAVITATIONAL FIELDS OF MACLAURIN SPHEROID MODELS OF ROTATING FLUID PLANETS

Journal

ASTROPHYSICAL JOURNAL
Volume 764, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/764/1/67

Keywords

gravitation; hydrodynamics; planets and satellites: general; planets and satellites: interiors

Funding

  1. UK NERC
  2. STFC
  3. Leverhulme
  4. National Science Foundation [NSF AST-0909206]
  5. Natural Environment Research Council [NE/G003548/1] Funding Source: researchfish
  6. Direct For Mathematical & Physical Scien
  7. Division Of Astronomical Sciences [0909206] Funding Source: National Science Foundation
  8. NERC [NE/G003548/1] Funding Source: UKRI

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Hubbard recently derived an important iterative equation for calculating the gravitational coefficients of a Maclaurin spheroid that does not require an expansion in a small distortion parameter. We show that this iterative equation, which is based on an incomplete solution of the Poisson equation, diverges when the distortion parameter is not sufficiently small. We derive a new iterative equation that is based on a complete solution of the Poisson equation and, hence, always converges when calculating the gravitational coefficients of a Maclaurin spheroid.

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