The bulk composition of the eucrite parent asteroid and its bearing on planetary evolution

Details The bulk composition of the eucrite parent asteroid and its bearing on planetary evolution The bulk composition of the eucrite parent asteroid and its bearing on planetary evolution

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980znata..35..204d&link_type=abstract

Zeitschrift für Naturforschung, Teil a, vol. 35 a, Feb. 1980, p. 204-216.

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Moore County Meteorite, Serra De Mage Meteorite, Binda Meteorite, Malvern Meteorite, Molteno Meteorite, Le Teilleul Meteorite, Kapoeta Meteorite, Zmenj Meteorite, Yamato 1 Meteorite, Parent Bodies, Frankfort Meteorite, Asteroids, Eucrites, Composition, Planets, Data, Evolution, Volatile Elements, Meteorites, Howardites, Diogonites, Silicon, Major Elements, Scandium, Trace Elements, Chlorine, Barium, Anomalies, Classification, Rare Earth Elements, Chemistry, Moon, Comparisons, Yamato Meteorites, Antarctic Me

Scientific paper

The purpose of the paper is to calculate the bulk composition of the eucrite parent asteroid. Analytical data on the chemistry of howardites are examined, and a second iteration of the mixing computation is studied. It is shown that howardites fit well into a binary mixing diagram for both their major and trace element compositions. In the mixing diagram, computed from the elemental compositions of howardites, it is found that a certain composition (PR) contains all refractory incompatible elements in quasi-C1 abundances. It is also found that the bulk composition of EPA is almost chondritic, with a considerable depletion of volatile and moderately volatile elements.

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