Motion of the fast exoplanets |
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Authors: | Valery A. Kotov |
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Affiliation: | 1.Crimean Astrophysical Observatory,Nauchny,Russia |
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Abstract: | It is shown that a number of superfast, with periods (< 2) d, exoplanets revolve around parent stars with periods, near-commensurate with (P_{E}) and/or (2 P_{E} / pi), where the exoplanet resonance timescale (P_{E}=9603(85)) s agrees fairly well with the period (P_{0}= 9600.606(12)) s of the so-called “cosmic oscillation” (the probability that the two timescales would coincide by chance is near (3 times10^{-4}); the (P_{0}) period was discovered first in the Sun, and later on—in other objects of Cosmos). True nature of the exoplanet (P_{0}) resonance is unknown. |
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