Solar Abundance of Elements from Neutron-Capture Cross Sections

Details Solar Abundance of Elements from Neutron-Capture Cross Sections Solar Abundance of Elements from Neutron-Capture Cross Sections

2004-12-19

arxiv.org/abs/astro-ph/0412502v1

Astronomy and Astrophysics

Astrophysics

2 pages with 4 figures, submitted for oral presentation in the Genesis Mission Special Session, 36th Lunar and Planetary Scien

Scientific paper

Excess lightweight products of slow neutron capture in the photosphere, over the mass range of 25 to 207 amu, confirm the solar mass separation recorded by excess lightweight isotopes in the solar wind, over the mass range of 3 to 136 amu [Solar Abundance of the Elements, Meteoritics, volume 18, 1983, pages 209 to 222]. Both measurements show that major elements inside the Sun are Fe, O, Ni, Si and S, like those in rocky planets.

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