|
Detailed Reference Information |
Lerch, F.J., Laubscher, R.E., Klosko, S.M., Smith, D.E., Kolenkiewicz, R., Putney, B.H., Marsh, J.G. and Brownd, J.E. (1978). Determination of the geocentric gravitational constant from laser ranging on near-earth satellites. Geophysical Research Letters 5: doi: 10.1029/GL005i012p01031. issn: 0094-8276. |
|
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 km 3/sec2, 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 km km 3/sec2. The uncertainty in this value is assessed to be ¿.02 km3/sec2. Determinations of GM from the data taken on these four satellites individually show variations of only .04 km 3/sec2 from the combined results. 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. |
|
|
|
BACKGROUND DATA FILES |
|
|
Abstract |
|
|
|
|
|
Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
|
|
|