Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004pabei..22...45s&link_type=abstract
Progress in Astronomy (ISSN 1000-8349), Vol. 22, No. 1, p. 45 - 56 (2004)
Astronomy and Astrophysics
Astronomy
Celestial Mechanics, Uranian Satellites, Review, Planets And Satellites
Scientific paper
The data of the satellites acquired by spacecraft-centered radio and optical observations during the Voyager 2 encountering Uranus provide the first reliable estimation of the masses of all five major satellites. Contemporary quantitative theories on the motion of the Uranian satellites have been promoted. Laskar (1986) developed the first relatively complete (semi-) analytical theory (GUST86) with its high accuracy being confirmed by some authors. After that, the contributions of the refinement on the theory should be mentioned Malhotra (1989), Lazzaro (1987, 1991), investigated the effect of the near-resonance on the secular motion of the satellites; Taylor (1998), re-determined the masses of the five major satellites by the theoretical fitting into observations through numerical integration; Christou and Murray (1997) applied a second order Laplace-Lagrange theory to the satellite system. A general survey of how the quantitative theories of motion for the Uranian satellites was set up and developed is presented in the paper.
Liu Jian-Rong
Qiao Rong-Chuan
Shen Kai-Xian
No associations
LandOfFree
Study and development of contemporary (quantitative) theories on the motion of the Uranian major satellites does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Study and development of contemporary (quantitative) theories on the motion of the Uranian major satellites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Study and development of contemporary (quantitative) theories on the motion of the Uranian major satellites will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1028542