Conservation of the Tisserand parameter at close encounters of interplanetary objects with Jupiter-Reference-Cited by-同舟云学术

Conservation of the Tisserand parameter at close encounters of interplanetary objects with Jupiter

Published:1995 Issue:1-3 Volume:68 Page:71-94
ISSN:0167-9295
Container-title:Earth, Moon, and Planets
language:en
Short-container-title:Earth Moon Planet

Author:

Carusi A.,Kres�k ?.,Valsecchi G. B.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00671499.pdf

Reference14 articles.

1. A. Carusi and F. Pozzi: 1978a. A new method for close encounter computation, Moon and Planets19, 65?70.

2. A. Carusi and F. Pozzi: 1978b. Planetary close encounters between Jupiter and about 3000 fictitious minor bodies, Moon and Planets19, 71?87.

3. A. Carusi, ?. Kres�k and G.B. Valsecchi: 1981. Perturbations by Jupiter of a chain of objects moving in the orbit of Comet Oterma, Astron. Astrophys.99, 262?269.

4. A. Carusi, ?. Kres�k and G.B. Valsecchi: 1982. Orbital patterns of interplanetary objects at close encounters with Jupiter, Bull. Astron. Inst. Czechosl.33, 141?150.

5. E. Everhart: 1976. The evolution of comet orbits, inThe Study of Comets (B. Donn, M. Mumma, W. Jackson, M. A'Hearn and R. Harrington eds.), NASA SP-393, pp. 445?461.

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