A global polytropic model for the solar system - Planetary distances and masses resulting from the complex Lane-Emden differential equation

Details A global polytropic model for the solar system - Planetary distances and masses resulting from the complex Lane-Emden differential equation A global polytropic model for the solar system - Planetary distances and masses resulting from the complex Lane-Emden differential equation

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993em%26p...61..131g&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 61, no. 2, p. 131-139.

Statistics

Computation

2

Astronomical Models, Celestial Mechanics, Polytropic Processes, Solar System, Computational Astrophysics, Jupiter (Planet), Mass Distribution, Probability Theory, Sun

Scientific paper

A global polytropic nonrotating model is developed to study the
planetary nebula in a state of pure hydrostatic equilibrium. Polytropic
shells with negative Re are identified using mathematical methods.

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