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Fig. 5 | Earth, Planets and Space

Fig. 5

From: The layered structure model for winonaite parent asteroid implicated by textural and mineralogical diversity

Fig. 5

Mineral composition of silicate phases in winonaites. a Fa versus Fs (mol %) in olivine and orthopyroxene, respectively (modified from Folco et al. 2006); composition of pyroxene (b) and plagioclase (c) in the studied meteorites (the literature data were taken from Goodrich et al. 2011). The two-pyroxene thermometer boundaries were taken from Lindsley and Andersen (1983)

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