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

2015/06/21 by V. S. Geroyannis, Geroyannis, Vassilis S.
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #Stellar, planetary, and galactic studies

paper · pdf · doi:10.48550/arxiv.1506.06344

openalex publication_date 2015/06/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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.

Citations

• Gravitational quantization of exoplanet orbits in 55 Cnc, \υ\n And, Kepler-11, Kepler-20, and Kepler-90

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