Abstract
The content of short-living radioactive elements in the silicate part of the proto-planetary cloud matter is sufficient, in the inner part of even small proto-planetary bodies with a radius of about 50 km, to provide a temperature higher than the melting temperature of iron.
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Anfilogov, V.N., Khachay, Y.V. (2015). Conclusions. In: Some Aspects of the Formation of the Solar System. SpringerBriefs in Earth Sciences. Springer, Cham. https://doi.org/10.1007/978-3-319-17831-8_8
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DOI: https://doi.org/10.1007/978-3-319-17831-8_8
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