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Fig. 2 | Progress in Earth and Planetary Science

Fig. 2

From: Major element composition of an Early Enriched Reservoir: constraints from 142Nd/144Nd isotope systematics in the early Earth and high-pressure melting experiments of a primitive peridotite

Fig. 2

Calculated melt fraction as a function of the formation age of the EER. Bold and dashed lines show melt fractions for the case of X = 0.3 and 1, respectively. The blue bar indicates the maximum formation age of the EER. EER Early Enriched Reservoir (low-Sm/Nd reservoir which can compensate for the 142Nd/144Nd difference between ASE and chondrites)

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