Hostname: page-component-77c89778f8-gvh9x Total loading time: 0 Render date: 2024-07-21T00:40:40.307Z Has data issue: false hasContentIssue false
  • English
  • Français

Determination of the Mass of Jupiter from Observations of 10 Hygiea During 1932–1969

Published online by Cambridge University Press:  14 August 2015

N. S. Chernykh
N. S. Chernykh*
Affiliation:
Crimean Astrophysical Observatory, Crimea, U.S.S.R.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An attempt has been made to derive the mass of Jupiter from modern observations of the minor planet 10 Hygiea. The calculations have been made using computer programmes prepared at the Institute for Theoretical Astronomy. From 250 observations 1932 to 1967 we obtained the reciprocal mass 1047.345±0.040 (rms error). After excluding some less reliable observations and allowing for the elliptic aberration terms we obtained 1047.326±0.033. By means of a more sophisticated computer programme and utilizing 100 additional observations, some of them made in 1969, we obtained the value 1047.324±0.023. Our results are compared with recent determinations by other investigators.

Type
Part III/Motions of the Short-Period Comets
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972 , pp. 233 - 238
Copyright
Copyright © Reidel 1972 

References

Bec, A.: 1969, Astron. Astrophys. 2, 381.Google Scholar
Belyaev, N. A.: 1967, Byull. Inst. Teor. Astron. 10, 696.Google Scholar
Clemence, G. M.: 1949, Proc. Am. Phil. Soc. 93, 7.Google Scholar
de Sitter, W.: 1938, Bull. Astron. Inst. Neth. 8, 307.Google Scholar
Fiala, A. D.: 1969, Bull. Am. Astron. Soc. 1, 342.Google Scholar
Herget, P.: 1968, Astron. J. 73, 737.CrossRefGoogle Scholar
Hill, G. W.: 1873, Collected Mathematical Works , Vol. I.Google Scholar
Kazimirchak-Polonskaya, E. I.: 1967, Trudy Inst. Teor. Astron. 12.Google Scholar
Khanina, F. B.: 1965, Byull. Inst. Teor. Astron. 10, 424.Google Scholar
Klepczynski, W. J.: 1967, Astron. J. 72, 808.CrossRefGoogle Scholar
Klepczynski, W. J.: 1969, Astron. J. 74, 774.CrossRefGoogle Scholar
Kulikov, D. K. and Subbotina, N. S.: 1963, in Problemy Dvizheniya Iskusstvennykh Nebesnykh Tel , Moscow.Google Scholar
Newcomb, S.: 1895, Astron. Pap. Washington 5, part 5.Google Scholar
O'Handley, D. A.: 1968, Astron. J. 73, 529.Google Scholar
Orel'skaya, V. I.: 1962, Byull. Inst. Teor. Astron. 8, 660.Google Scholar
Zielenbach, J. W.: 1969, Astron. J. 74, 567.CrossRefGoogle Scholar