On homogeneous statistical distributions exoplanets for their dynamic parameters

TL;DR

This paper derives homogeneous statistical distributions for exoplanet orbital and physical parameters, considering orbital resonances and wavelet analysis, challenging the necessity of including finer effects in distribution modeling.

Contribution

It introduces a new approach to modeling exoplanet distributions that accounts for orbital resonances without requiring complex wavelet-based effects.

Findings

Homogeneous distributions for exoplanet parameters are established.

Inclusion of wavelet effects is deemed unnecessary for accurate distribution modeling.

Orbital resonances are incorporated into the statistical framework.

Abstract

Correct distributions of extrasolar systems for their orbital parameters (semi-major axes, period, eccentricity) and physical characteristics (mass, spectral type of parent star) are received. Orbital resonances in extrasolar systems are considered. It is shown, that the account of more thin effects, including with use of wavelet methods, in obviously incorrectly reduced distributions it is not justified, to what the homogeneous statistical distributions for dynamic parameters of exoplanets, received in the present work, testify.