The solar mercury abundance

Details The solar mercury abundance The solar mercury abundance

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...123..279w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 123, no. 2, July 1983, p. 279-282.

Physics

10

Abundance, Mercury Isotopes, Solar Physics, Absorption Cross Sections, Neutron Cross Sections, Nuclear Fusion

Scientific paper

The solar mercury abundance was determined through s-process systematics in order to obtain the Maxwellian averaged capture cross sections of mercury isotopes in C1 carbonaceous chondrites. The activation tests were carried out at 25 keV to study the neutron cross-sections of three Hg isotopes. The Hg-202 cross section led to an estimate of the solar Hg abundance of within 0.04 of 0.24 x 1 millionth of the Si abundance. The r-process was found to produce about 23 percent of the Hg-202 abundance.

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