Estimations of changes of the Sun's mass and the gravitation constant from the modern observations of planets and spacecraft
E.V. Pitjeva, N.P. Pitjev

TL;DR
This study analyzes over 635,000 observations from 1961-2010 to estimate potential changes in the Sun's mass and the gravitational constant, finding a slight decrease in the gravitational constant over time.
Contribution
It provides new estimates of the Sun's mass change and gravitational constant variation using extensive observational data and ephemerides analysis in post-Newtonian approximation.
Findings
Estimated decrease in heliocentric gravitational constant at (-5.0 ± 4.1)×10^{-14} per year.
Derived bounds for the change in G/G as between -4.2×10^{-14} and +7.5×10^{-14} per year.
Detected positive secular changes in planetary semi-major axes consistent with a decreasing gravitational constant.
Abstract
More than 635 000 positional observations (mostly radiotechnical) of planets and spacecraft (1961-2010), have been used for estimating possible changes of the gravitation constant, the solar mass, and semi-major axes of planets, as well as the value of the astronomical unit, related to them. The analysis of the observations has been performed on the basis of the EPM2010 ephemerides of IAA RAS in post-newtonian approximation. The obtained results indicate on decrease in the heliocentric gravitation constant per year at the level The positive secular changes of semi-major axes have been obtained simultaneously for the planets Mercury, Venus, Mars, Jupiter, Saturn, as expected if the geliocentric gravitation constant is decreasing in century wise. The change of the mass of the Sun due to the solar…
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