Ephemeris theories JPL DE, INPOP and EPM

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Abstract

This paper provides an overview and description of three leading sources of planetary ephemerides: the ephemerides from the Jet Propulsion Laboratory (JPL) and their developed ephemeris theory DE; the ephemerides from the Institute of Celestial Mechanics and Ephemeris Calculation (IMCCE) and their developed theory INPOP; and the ephemeris theory EPM developed at the Institute of Applied Astronomy of the Russian Academy of Sciences (IAA RAS). The methods and observational data sets used in constructing each of the theories are described. A comparison of the ephemerides computed within these theories is made using examples from future space missions. It is shown that the differences in computed positions do not exhibit systematic characteristics and represent rather random discrepancies caused by variations in dynamic models and the observational data taken into account. The overall conclusion from the comparison of the ephemerides is that none of the considered options (JPL DE, EPM, and INPOP) has an advantage in terms of accuracy. All three options are equally valid, and any of the three ephemeris options can be used in practice.

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About the authors

I. A. Moiseev

Lomonosov Moscow State University

Author for correspondence.
Email: lxyniti@gmail.com

Department of Celestial Mechanics, Astrometry and Gravimetry, Faculty of Physics

Russian Federation, Moscow

N. V. Emelyanov

Lomonosov Moscow State University, Sternberg Astronomical Institute

Email: emelia@sai.msu.ru
Russian Federation, Moscow

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