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Title:
Isotopes Tell Origin and Operation of the Sun
Authors:
Manuel, O.; Kamat, Sumeet A.; Mozina, Michael
Publication:
eprint arXiv:astro-ph/0510001
Publication Date:
09/2005
Origin:
ARXIV
Comment:
20 pages, 16 figures with 2 running difference images from SOHO and TRACE, and one Table of puzzling observations since 1957 that unmasked the Iron Sun. First Crisis in Cosmology Conference, Moncao, Portugal, 23-25 June 2005
Bibliographic Code:
2005astro.ph.10001M

Abstract

The Iron Sun formed on the collapsed core of a supernova and now acts as a magnetic plasma diffuser, as did the precursor star, separating ions by mass. This process covers the solar surface with lightweight elements and with lighter isotopes of each element. Running difference images expose rigid, iron-rich structures below the fluid photosphere made of lightweight elements. The energy source for the Sun and ordinary stars seems to be neutron-emission and neutron-decay, with partial fusion of the decay product, rather than simple fusion of hydrogen into helium or heavier elements. Neutron-emission from the solar core and neutron-decay generate about sixty five percent of solar luminosity and H-fusion generates about thirty-five percent. The upward flow of H ions maintains mass-separation in the Sun. Only about one percent of this neutron decay product survives its upward journey to depart as solar-wind hydrogen.
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