Determination of the geocentric gravitational constant from laser ranging on near-earth satellites

Details Determination of the geocentric gravitational constant from laser ranging on near-earth satellites Determination of the geocentric gravitational constant from laser ranging on near-earth satellites

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978georl...5.1031l&link_type=abstract

Geophysical Research Letters, vol. 5, Dec. 1978, p. 1031-1034.

Physics

4

Earth Gravitation, Geocentric Coordinates, Gravitational Constant, Laser Range Finders, Satellite Observation, Interplanetary Spacecraft, Lageos (Satellite), Lunar Rangefinding, Mechanical Measurement, Satellite Orbits

Scientific paper

Laser range observations taken on the near-earth satellites of Lageos (a = 1.92 e.r.), Starlette (a = 1.15 e.r.), BE-C (a = 1.18 e.r.), and Geos-3 (a = 1.13 e.r.) have been combined to determine an improved value of the geocentric gravitational constant (GM). The value of GM is 398600.61 cu km/sec per sec, based upon a speed of light, c, of 299792.5 km/sec. Using the IAG-adopted value of c equalling 299792.458 km/sec scales GM to 398600.44 cu km/sec per sec. The uncertainty in this value is assessed to be plus or minus 0.02 cu km/sec per sec. Determinations of GM from the data taken on these four satellites individually show variations of only .04 cu km/sec per sec from the combined result. The Lageos information dominated the combined solution, and gave the most consistent results in its data subset solutions. The value obtained for GM from near-earth laser ranging compares quite favorably with the most recent results of the lunar laser and interplanetary experiments.

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