Abstract
The error in calculating the gravitational constant using the differential equation of motion is estimated. It is shown that a preliminary calculation of the oscillation period of a torsion balance using the standard value of the gravitational constant G 0 and the oscillation period when the spherical attracting masses are fixed at the nearer of the two positions produces a reduction in the error in calculating G in each combination of positions.
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REFERENCES
O. V. Karagioz and V. P. Izmailov, Izmerit. Tekh., No. 10, 3 (1996).
O. V. Karagioz, V. P. Izmailov, N. I. Agafonov, et al., Izv. Akad. Nauk SSSR Ser. Fiz. Zemli, No. 5, 106 (1976).
O. V. Karagioz, V. P. Izmailov, and M. A. Kudryavitskii, Izmerit. Tekh., No. 12, 3 (1998).
N. I. Kolosnitsyn, Metrolog., No. 11, 3 (1990).
M. S. Urmaev, Orbital Methods of Space Geodesy [in Russian], Nedra, Moscow (1981).
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Izmailov, V.P., Kudryavitskii, M.A. & Karagioz, O.V. Increasing the Accuracy of the Oscillation Period of Torsion Balances for Calculations of the Gravitational Constant. Measurement Techniques 45, 1–6 (2002). https://doi.org/10.1023/A:1015199212536
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DOI: https://doi.org/10.1023/A:1015199212536