Motion of the fast exoplanets

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.