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Carl Friedrich Gauss
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Gauss shifted significant focus toward celestial mechanics following the discovery of the dwarf planet Ceres/) in 1801. Astronomers struggled to predict Ceres's/) orbit due to insufficient observational data. Gauss developed the method of least squares to fit the observed points to a parabolic path, successfully recalculating the true [orbi…
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Oblate Spheroid
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The mathematical description of the Earth's flattening was central to early geophysical theory. Sir Isaac Newton, in his Principia, mathematically demonstrated that the Earth, being a rotating fluid mass, must be an oblate spheroid, predicting a polar flattening of approximately $1/230$ [Citation Needed: Principia, Book III, Proposition 19].
Later, Carl Friedrich Gauss, while developing methods for orbital determination, impl…