Gravitational quantization of exoplanet orbits in HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186
Geroyannis et al
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.
Wednesday, July 22, 2015
The Global Polytropic Model Applied to Exoplanet Orbits
Posted by Will Baird at 8:00 AM
Labels: HD 10180, kepler-102, kepler-186, kepler-32, kepler-33, orbital mechanics
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