Gravitational quantization of exoplanet orbits in HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186

TL;DR

This paper applies the global polytropic model to analyze and predict exoplanet orbits in five systems, comparing computed and observed planetary distances to validate the model's effectiveness.

Contribution

It introduces the application of the global polytropic model to multiple exoplanet systems for orbit prediction and validation.

Findings

Computed planetary distances closely match observed data

Model successfully predicts additional potential orbits

Provides a new approach for exoplanet orbit analysis

Abstract

The so-called "global polytropic model" is applied to the numerical study of the exoplanet systems HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186. We compare computed distances of planets from their host stars with corresponding observations and discuss some further orbit predictions made by the model.