Verification of some hypotheses for unknown planets through an analysis of the interorbital minimum comet-planet distances

Details Verification of some hypotheses for unknown planets through an analysis of the interorbital minimum comet-planet distances Verification of some hypotheses for unknown planets through an analysis of the interorbital minimum comet-planet distances

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kfnt...13d..56g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 13, p. 56

Physics

Comets, Planetary Orbits, Orbital Elements, Pluto (Planet), Celestial Mechanics, Distance, Hypotheses

Scientific paper

An analysis is made of the minimal inter-orbital comet-planet distances for 613 long-period comets and three hypothetic planets. The existence of transplutonian planets is suggested. Special analysis of the distribution of n(rho) with respect to Pluto displays a remarkable maximum at small values of rho. In the case of the first planet, for rho less than 0.009 a.u., the observed frequency of comet appearance is approximately 13.5 times that of theoretical one. A similar excess is obtained for the second (rho less than 0.1873 a.u.) and the third (rho less than 0.2 a.u.) planet.

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