Artigo Revisado por pares

The Mass of Jupiter from the Motion of (76) Freia

1971; Institute of Physics; Volume: 76; Linguagem: Inglês

10.1086/111204

ISSN

1538-3881

Autores

W. J. Klepczyński, P. M. Janiczek, A. D. Fiala,

Tópico(s)

Astro and Planetary Science

Resumo

In Hill's 1873 list of minor planets of the Hecuba group suitable for determination of the mass of Jupiter, (76) Freia has the largest coefficient for the long-period term in longitude. Observations consisted of 15 photographic plates taken at Heidelberg Observatory (1912-1933) and remeasured at the U. S. Naval Observatory, several plates remeasured at Lowell and Goethe Link Observatories, and 79 plates taken at the Naval Observatory (1947-1971). In addition, 43 visual observations taken at Berlin, Vienna, and Leipxig Observatories ( ) were reduced to the same catalogue system as the photo- graphic observations. Variational equations were integrated for the differential correction process. The derived reciprocal mass of Jupiter is 1047.366+0.007 (m.e.).

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