Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mvsfa..33...68v&link_type=abstract
Moskovskii Universitet, Vestnik, Seriia 3 - Fizika, Astronomiia (ISSN 0579-9392), vol. 33, no. 2, Mar.-Apr. 1992, p. 68-73. In R
Astronomy and Astrophysics
Astronomy
Circular Orbits, Galactic Rotation, Gravitation Theory, Relativistic Theory, Solar System, Celestial Mechanics, Orbit Perturbation, Orbital Elements, Planetary Orbits
Scientific paper
It is noted that noninertial effects caused by the motion of the solar system together with nearby stars of the Local Group around the Galactic center are not considered in the standard post-Newtonian examination of gravitational effects in the solar system. The noninertial problem is considered here assuming that the solar system moves as a whole in a circular orbit around the center of the Galaxy according to Newton's law. Based on this, corrections are calculated to the post-Newtonian trajectories of the planets around the sun, and the corresponding observational manifestations are examined.
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