John M. Bird
Cornell University
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Featured researches published by John M. Bird.
Earth and Planetary Science Letters | 1975
John M. Bird; Maura S. Weathers
Abstract Josephinite is a terrestrial iron-nickel alloy with an intergrown magnesium silicate, and arsenide and sulphide phases, and andradite garnet; several specimens have been found to contain elemental silicon and CaO · 2“FeO”. Josephinite is not awaruite, an iron-nickel mineral formed by serpentinization of ultramafic rocks. Because of its geologic setting and unique mineralogy we propose that josephinite might have originated in the region of the coremantle boundary, was transported via a deep-mantle “plume” and diatreme mechanism into lithosphere mantle that has been emplaced in the Klamaths by ophiolite obduction. Regardless of such a hypothesis, we report here the discovery of terrestrial silicon occurring with josephinite, which seems to preclude a lithosphere environment of origin for josephinite.
The Journal of Geology | 1985
Cyrena Anne Goodrich; John M. Bird
Two types of metallic iron were identified in a collection of samples from the Tertiary iron-bearing basalts of Uivfaq, Disko Island, Greenland. High-carbon iron has 2.9-4.0 wt % carbon and eutectic textures of iron and cohenite (
Science | 1984
Jon S. Gold; William A. Bassett; Maura S. Weathers; John M. Bird
Tectonics | 1996
Ann E. Blythe; John M. Bird; Gomaa I. Omar
Fe_{3}C
Tectonics | 1993
Karl R. Wirth; John M. Bird; Ann E. Blythe; David J. Harding; Matthew T. Heizler
The Journal of Geology | 1977
John M. Bird; Maura S. Weathers
) similar to those of commercial white cast iron. It occurs in approximately spherical bodies, up to 15 mm in diameter, that appear to have been immiscible metallic liquids within basaltic magma. Low-carbon samples have ~1.8-2.0 wt % carbon and textures similar to those of commercial hypereutectoid steel. They occur principally as large (up to 22 tons) cumulate masses. Both types of metal could have crystallized at low pressure from iron-carbon liquids of their present bulk carbon contents. Fe, Ni, Co, Cu, and P oxides in basaltic magma were reduced by carbon derived principally from assimilated Cretaceous-Tertiary sediments. Niand Ni/Cu ratios of the metal are similar to those of terrestrial basalts. The magma contained excess carbon (graphite), so the metal formed as an immiscible C-saturated liquid (represented by the high-carbon samples). Carbon geobarometry indicates that reduction took place at pressures less than ~400 bars (1.2 km). Separation of the metal from excess carbon caused decarburization of most of the high-carbon metal to form low-carbon metal. The decarburization reaction,
Geology | 1992
Karl R. Wirth; John M. Bird
Geology | 1983
John S. Dickey; William A. Bassett; John M. Bird; Maura S. Weathers
C(in metal) + O_{2} = CO or CO_{2}
Earth and Planetary Science Letters | 1978
P. Bochsler; Anton Stettler; John M. Bird; Maura S. Weathers
Remote Sensing of Environment | 1989
David J. Harding; Karl R. Wirth; John M. Bird
, is exothermic and produced enough heat locally to raise the temperature of the low-carbon metal to at least its melting point (~1390 C). P and some Fe were also oxidized and removed from the metal as FeO and