Simulating the Precession of Venus

ORAL

Abstract

The orbit of Venus precesses at a total rate of 204 arc seconds per century. The gravitational forces from the other 7 planets produce a rate of 1075'' according to Newtonian gravity. In 1908, Walter Ritz published a modified law of gravity. We will use his theory to simulate the precession of Venus and demonstrate that his theory gives the correct amount.

Authors

  • Pradeep Ojha

    Weatherford College

  • Zhenrong Zhang

    The Cyclotron Institute at Texas A&M University, SF Austin State Univ, Texas A&M University, University of Texas at Arlington, Weatherford College, Texas A&M University/Baylor University/Princeton University, Baylor University/Texas A&M University, Texas A&M University/Baylor University, Baylor University

  • Zhenrong Zhang

    The Cyclotron Institute at Texas A&M University, SF Austin State Univ, Texas A&M University, University of Texas at Arlington, Weatherford College, Texas A&M University/Baylor University/Princeton University, Baylor University/Texas A&M University, Texas A&M University/Baylor University, Baylor University

  • James Espinosa

    Weatherford College