Masses of the Trojan Groups of Jupiter


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Resumo

The possibility of obtaining dynamical estimates of the total masses in the two Trojan asteroid groups of Jupiter is investigated. The compact Greek (L4) and Trojan (L5) groups contain several tens of thousands of asteroids near the stable Lagrange points moving in a 1: 1 resonance with the orbital motion of Jupiter. The dynamical mass estimates

\(\begin{array}{*{20}{c}}
{{M_{L4}} = (8.63 \pm 0.51) \times {{10}^{ - 6}}{M_ \oplus },} \\
{{M_{L5}} = (5.46 \pm 0.54) \times {{10}^{ - 6}}{M_ \oplus }}
\end{array}\)
have been obtained by processing more than 800 thousand observations of planets and spacecraft using the new EPM2019 version of planetary ephemerides created at IAA RAS.

Sobre autores

E. Pitjeva

Institute of Applied Astronomy

Autor responsável pela correspondência
Email: evp@iaaras.ru
Rússia, nab. Kutuzova 10, St. Petersburg, 191187

N. Pitjev

Institute of Applied Astronomy; St. Petersburg State University

Email: evp@iaaras.ru
Rússia, nab. Kutuzova 10, St. Petersburg, 191187; Universitetski pr. 28, St. Petersburg, 198504

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Declaração de direitos autorais © Pleiades Publishing, Inc., 2019