Using Nickel Features in the Spectra of Olivine-dominated A- and S(I)-type Asteroids to Determine the Oxidation State of the Solar Nebula

Details Using Nickel Features in the Spectra of Olivine-dominated A- and S(I)-type Asteroids to Determine the Oxidation State of the Solar Nebula Using Nickel Features in the Spectra of Olivine-dominated A- and S(I)-type Asteroids to Determine the Oxidation State of the Solar Nebula

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998lpi....29.1370g&link_type=article

29th Annual Lunar and Planetary Science Conference, March 16-20, 1998, Houston, TX, abstract no. 1370.

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