1970
DOI: 10.1016/0016-7037(70)90063-3
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Olivine and pyroxene in the Orgueil meteorite

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Cited by 36 publications
(19 citation statements)
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“…Reid et al (1970) and Fuchs et al (1973) concluded that these forsterite grains represent condensates from the solar nebula (Grossman and Olsen, 1974;Olsen and Grossman, 1978;Steele, 1986bSteele, , 1989Weinbruch et al, 1993Weinbruch et al, , 2000Klerner, 2001) and that melt inclusions in them are also direct condensates (Fuchs et al, 1973;Yoneda and Grossman, 1995). Melt condensates may form when the equilibrium condensation temperatures of mineral assemblages exceed their solidus temperatures.…”
Section: Formation Models Of Refractory Forsteritementioning
confidence: 96%
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“…Reid et al (1970) and Fuchs et al (1973) concluded that these forsterite grains represent condensates from the solar nebula (Grossman and Olsen, 1974;Olsen and Grossman, 1978;Steele, 1986bSteele, , 1989Weinbruch et al, 1993Weinbruch et al, , 2000Klerner, 2001) and that melt inclusions in them are also direct condensates (Fuchs et al, 1973;Yoneda and Grossman, 1995). Melt condensates may form when the equilibrium condensation temperatures of mineral assemblages exceed their solidus temperatures.…”
Section: Formation Models Of Refractory Forsteritementioning
confidence: 96%
“…Such forsterites should have ϳ0.2 mol% fayalite and MnO and NiO contents in the ppm range (Palme and Fegley, 1990). Reid et al (1970) and Fuchs et al (1973) were the first to describe isolated FeO-poor, refractory forsterite grains from carbonaceous chondrites (e.g., Fig. 1A).…”
Section: Formation Models Of Refractory Forsteritementioning
confidence: 99%
“…Refractory forsterite is proposed to have formed as a nebular condensate or as a product of crystallization within Fe-poor chondrules (Reid et al, 1970;Fuchs et al, 1973;Grossman and Olsen, 1974;Olsen and Grossman, 1978;Richardson and McSween, 1978;Steele, 1986b;Jones, 1992;Weinbruch et al, 1993Weinbruch et al, , 2000Jones et al, 2000Jones et al, , 2004Pack et al, 2004Pack et al, , 2005Jones and Carey, 2006). If refractory forsterite is a nebular condensate, its oxygen-isotope composition should represent equilibrium with nebular values at that time or location.…”
Section: Origin Of Isolated Forsteritementioning
confidence: 98%
“…3. Composition ranges of olivine (Fa) in grains from nine Wild 2 particles, compared with those for chondritic IDPs (Zolensky and Barrett 1994) and primitive chondrite matrix olivine (Greshake 1997;Brearley 1993;Reid et al 1970;Kerridge and MacDougal 1976;Krot et al 1995;Fuchs et al 1973;Nagahara 1984;Matsunami et al 1990). Vertical scale is number of analyses normalized to a total of 1. diffraction (SXRD) or selected area electron diffraction (SAED) patterns reveal low-calcium pyroxenes to be orthoenstatite, requiring slow cooling, but in the majority of cases we have only EDX analyses and are not certain whether we have ortho-or clinopyroxene.…”
Section: Wild 2 Olivine and Low-calcium Pyroxenementioning
confidence: 99%