A note to comet ejection process from the Uranus-Neptune region

Details A note to comet ejection process from the Uranus-Neptune region A note to comet ejection process from the Uranus-Neptune region

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992coska..22..209n&link_type=abstract

Contributions of the Astronomical Observatory Skalnate Pleso, vol. 22, p. 209-214.

Astronomy and Astrophysics

Astronomy

2

Comets, Cosmogony, Celestial Mechanics

Scientific paper

A simple energy balance of comet ejection from the Uranus-Neptune region is discussed. If we assume that the orbits of Uranus and Neptune remain stable during the ejection process, the necessary energy loss of perturbing planets needs a compensation. Planetary perturbations leading to short-period orbits of a part of comets are suggested as an explanation. Considerations about the total energy conservation become more important if a high mass of Oort cloud is supposed.

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