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Representation of the gravitational potential of a level ellipsoid by a simple layer

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Abstract

A closed-form expression is obtained for the density of a simple layer, equipotential to an oblate level ellipsoid of revolution in an outer space. The potential of any level spheroid of positive mass with the inward direction of the attracting force on its surface can be represented in this way. A family of density functions defined within the whole volume of a level ellipsoid of revolution is found. Several density examples are considered.

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Data sharing not applicable to this article as no datasets were generated or analyzed during the current study.

References

  • Antonov, V.A., Timoshkova, E.I., Kholshevnikov, K.V.: Introduction to the Theory of Newtonian Potential. Nauka, Moscow (1988) (in Russian)

  • Hofmann-Wellenhof, B., Moritz, H.: Physical Geodesy. Springer (2006)

  • Kholshevnikov, K.V., Milanov, D.V., Shaidulin, V.S.: The Laplace series of ellipsoidal figures of revolution. Vestnik St. Petersb. Univ. Math. 50, 406–413 (2017). https://doi.org/10.3103/S1063454117040112

    Article  MATH  Google Scholar 

  • Kholshevnikov, K.V., Milanov, D.V., Shaidulin, V.S.: Laplace series for the level ellipsoid of revolution. Celest. Mech. Dyn. Astr. 130, 64 (2018). https://doi.org/10.1007/s10569-018-9851-7

    Article  ADS  MathSciNet  MATH  Google Scholar 

  • Kondratiev, B.P.: Theory of Potential, and Figures of Equilibrium. Inst. Kosm. Res., Moscow (2003) (in Russian)

  • Korn, G.A., Korn, T.M.: Mathematical Handbook for Scientists and Engineers: Definitions, Theorems, and Formulas for Reference and Review. McGraw-Hill (1968)

  • Pizzetti, P.: Principii Della Teoria Meccanica Della Figura dei Pianeti. E. Spoerri, Pisa (1913)

    MATH  Google Scholar 

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Acknowledgements

The author will be forever grateful to Professor Konstantin V. Kholshevnikov (1939–2021), who pointed him the direction of this research and gave a lot of invaluable advices. The author also thanks Professor Luis Floría for the careful review of the article and numerous useful remarks.

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Correspondence to D. V. Milanov.

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Appendix

Appendix

The function \(H(\varepsilon )\) defined by (19) decreases on the interval [0, 1]. Let us express the dependence of H on \(\varepsilon \) explicitly and make sure that its derivative is negative,

$$\begin{aligned}&H(\varepsilon ) = \frac{1}{\varepsilon ^5} \left( 3(2\varepsilon ^4 - 15\varepsilon ^2 + 9)\sqrt{1 - \varepsilon ^2}\arcsin \varepsilon - \right. \left. 8\varepsilon ^5 + 18\varepsilon ^3 - 9\varepsilon \right) , \\&\begin{aligned} H'(\varepsilon )&= \frac{3}{\varepsilon ^6} \left( 3(4\varepsilon ^2 - 5)\sqrt{1 - \varepsilon ^2}\arcsin \varepsilon + 2\varepsilon ^5 - 17\varepsilon ^3 + 15\varepsilon \right) \\ {}&= \frac{3\sqrt{1-\varepsilon ^2}}{\varepsilon ^7} \left( (15 - 2\varepsilon ^2)\sqrt{1-\varepsilon ^2} - 3(5 - 4\varepsilon ^2)\frac{\arcsin \varepsilon }{\varepsilon }\right) . \end{aligned} \end{aligned}$$

Let us expand the square root and the arcsine into series up to the fourth degree of \(\varepsilon ^2\):

$$\begin{aligned} \begin{aligned}&(15 - 2\varepsilon ^2)\sqrt{1-\varepsilon ^2} - 3(5 - 4\varepsilon ^2)\frac{\arcsin \varepsilon }{\varepsilon } \\&\quad < (15 - 2\varepsilon ^2)\left( 1 - \frac{\varepsilon ^2}{2} - \frac{\varepsilon ^4}{8} - \frac{\varepsilon ^6}{16} - \frac{5\varepsilon ^8}{128}\right) - 3(5 - 4\varepsilon ^2)\left( 1 + \frac{\varepsilon ^2}{6} + \frac{3\varepsilon ^4}{40} + \frac{5\varepsilon ^6}{112} + \frac{35\varepsilon ^8}{1152}\right) \\&\quad =\varepsilon ^6\left( \frac{85}{192}\varepsilon ^2 - \frac{8}{21}\varepsilon - \frac{16}{35}\right) . \end{aligned} \end{aligned}$$

The maximum of the quadratic trinomial in the last expression is attained at \(\varepsilon =1\) and equals \(-2657/6720\).

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Milanov, D.V. Representation of the gravitational potential of a level ellipsoid by a simple layer. Celest Mech Dyn Astron 134, 26 (2022). https://doi.org/10.1007/s10569-022-10086-4

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