Geodesic
A sequence adapted from the movement of the center of mass of two planets in solar system
Communications in Mathematics, Tome 26 (2018) no. 2, pp. 147-152 Cet article a éte moissonné depuis la source Czech Digital Mathematics Library

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In this paper we derive a sequence from a movement of center of~mass of arbitrary two planets in some solar system, where the planets circle on concentric circles in a same plane. A trajectory of center of mass of the planets is discussed. A sequence of points on the trajectory is chosen. Distances of the points to the origin are calculated and a distribution function of a sequence of the distances is found.
In this paper we derive a sequence from a movement of center of~mass of arbitrary two planets in some solar system, where the planets circle on concentric circles in a same plane. A trajectory of center of mass of the planets is discussed. A sequence of points on the trajectory is chosen. Distances of the points to the origin are calculated and a distribution function of a sequence of the distances is found.
Classification : 11K31, 70F05
Keywords: distribution function; g-discrepancy; sequence of points; center of mass; trajectory of two planets; solar system 
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Fialová, Jana. A sequence adapted from the movement of the center of mass of two planets in solar system. Communications in Mathematics, Tome 26 (2018) no. 2, pp. 147-152. http://geodesic.mathdoc.fr/item/COMIM_2018_26_2_a5/

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