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Science 4 August 1989: Vol. 245. no. 4917, pp. 500 - 504 DOI: 10.1126/science.245.4917.500
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Articles
Neptune's Story
P. GOLDREICH 1,
N. MURRAY 1,
P. Y. LONGARETTI 1, and
D. BANFIELD 1
1 California Institute of Technology, Pasadena, CA 91125.
It is conjectured that Triton was captured from a heliocentric orbit as the result of a collision with what was then one of Neptune's regular satellites. The immediate post-capture orbit was highly eccentric with a semimajor axis a 103RN and a periapse distance rp that oscillated periodically above a minimum value of about 5RN. Dissipation due to tides raised by Neptune in Triton caused Triton's orbit to evolve to its present state in 109 years. For much of this time Triton was almost entirely molten. While its orbit was evolving, Triton cannibalized most of the regular satellites of Neptune and also perturbed Nereid, thus accounting for that satellite's highly eccentric and inclined orbit. The only regular satellites of Neptune that survived were those that formed well within 5RN and they move on inclined orbits as the result of chaotic perturbations forced by Triton. Neptune's arcs are confined around the corotation resonances of one of these inner satellites. The widths and lengths of the arcs imply that the satellite's radius is at least 30/(sin i)2/3 kilometers for i 1, where i is the angle of inclination.
Submitted on May 16, 1989
Accepted on July 3, 1989
THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
- Triton, Pluto, and the Origin of the Solar System.
- J. I. Lunine and J. I. Lunine (1993)
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- The Impact Cratering Record on Triton.
- R. G. Strom, R. G. Strom, S. K. Croft, and J. M. Boyce (1990)
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250, 437-439
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- The Voyager 2 Encounter with the Neptunian System.
- E. C. Stone, E. C. Stone, and E. D. Miner (1989)
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246, 1417-1421
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- Voyager 2 at Neptune: Imaging Science Results.
- B. A. Smith, B. A. Smith, L. A. Soderblom, D. Banfield, c. Barnet, A. T. Basilevsky, R. F. Beebe, K. Bollinger, J. M. Boyce, A. Brahic, et al. (1989)
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246, 1422-1449
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