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Title: Experimental partitioning studies near the Fe-FeS eutectic, with an emphasis on elements important to iron meteorite chronologies (Pb, Ag, Pd, and Tl)

Journal Article · · Geochimica et Cosmochimica Acta; (United States)
 [1];  [2];  [3]
  1. NASA Johnson Space Center, Houston, TX (United States)
  2. Woods Hole Oceanographic Institution, MA (United States)
  3. Los Alamos National Lab., NM (United States)

Partition coefficients (D) for metal/sulfide liquid, troilite/sulfide liquid, and schreibersite/sulfide liquid have been experimentally determined for Ag, Au, Mo, Ni, Pb, Pd, and Tl. With these partition coefficients, it should be possible to better understand the [sup 107]Pd-[sup 107]Ag and [sup 205]Tl-[sup 205]Pb systems of iron meteorites. In general, the schreibersite/metal and troilite/metal partition coefficients for compatible' elements are quite similar to those inferred from natural assemblages. In contrast, these same partition coefficients for incompatible' elements often do not even qualitatively agree with analyses of iron meteorites. The authors suggest that analyses of incompatible elements in iron meteorites may sometimes be dominated by minor/trace phases. Identification of such phases may allow refinement of the initial isotopic composition of Pb in the early solar system. If the trace impurity model is correct, it may also be possible to reconcile iron meteorite cooling rates inferred from silver isotopic systematics with those deduced from metallography. 36 refs., 2 figs., 6 tabs.

OSTI ID:
6736188
Journal Information:
Geochimica et Cosmochimica Acta; (United States), Vol. 57:2; ISSN 0016-7037
Country of Publication:
United States
Language:
English