The ephemeris program GLE200

J. Schastok; H. Gleixner; M. Soffel; H. Ruder; M. Schneider

doi:10.1016/0010-4655(89)90041-6

The ephemeris program GLE200

J. Schastok, H. Gleixner, M. Soffel, H. Ruder, M. Schneider

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Abstract

The program GLE2000 solves the equations of motion for the pointmasses of planets, Earth, Moon and Sun in the first post-Newtonian approximation by numerical integration. Considered are also: the action of five minor planets, the dynamics of extended bodies and tidal friction. The program is able to reproduce the internationally accepted reference ephemeris DE200 to a high precision.

Original language	English
Pages (from-to)	167-170
Number of pages	4
Journal	Computer Physics Communications
Volume	54
Issue number	1
DOIs	https://doi.org/10.1016/0010-4655(89)90041-6
State	Published - Apr 1989

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title = "The ephemeris program GLE200",

abstract = "The program GLE2000 solves the equations of motion for the pointmasses of planets, Earth, Moon and Sun in the first post-Newtonian approximation by numerical integration. Considered are also: the action of five minor planets, the dynamics of extended bodies and tidal friction. The program is able to reproduce the internationally accepted reference ephemeris DE200 to a high precision.",

author = "J. Schastok and H. Gleixner and M. Soffel and H. Ruder and M. Schneider",

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T1 - The ephemeris program GLE200

AU - Schastok, J.

AU - Gleixner, H.

AU - Soffel, M.

AU - Ruder, H.

AU - Schneider, M.

PY - 1989/4

Y1 - 1989/4

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AB - The program GLE2000 solves the equations of motion for the pointmasses of planets, Earth, Moon and Sun in the first post-Newtonian approximation by numerical integration. Considered are also: the action of five minor planets, the dynamics of extended bodies and tidal friction. The program is able to reproduce the internationally accepted reference ephemeris DE200 to a high precision.

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DO - 10.1016/0010-4655(89)90041-6

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SN - 0010-4655

VL - 54

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JO - Computer Physics Communications

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The ephemeris program GLE200

Abstract

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