Sunqm-3s7: Predict Mass Density R-Distribution for Gas/ice Planets Based on {N,n} QM Probability Distribution

Authors: Yi Cao

Using the same method developed in paper SunQM-3s6, the (close to the true) mass density r-distribution for gas/ice planets has been estimated based on {N,n} QM probability distribution. Based on this calculation (as well as on other scientists’ calculation), the center core mass density for Jupiter, Saturn, Uranus, Neptune, and the undiscovered {3,2} planet (if it does formed) are estimated to be: ~ 26000 kg/m^3, ~ 23000 kg/m^3, ~ 16500 kg/m^3, ~ 17000 kg/m^3, and ~ 16000 kg/m^3 respectively. The results from this paper (as well as from papers of SunQM-3s6 and SunQM-3s8) strongly suggest that all planets and stars were formed and evolved under planet's (or star's) QM.

Comments: 11 Pages.

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Submission history

[v1] 2018-12-17 13:57:38

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