Conference Abstracts
The early history of the earth
Suid-Afrikaanse Tydskrif vir Natuurwetenskap en Tegnologie | Vol 7, No 1 | a898 |
DOI: https://doi.org/10.4102/satnt.v7i1.898
| © 1988 C. P. Snyman
| This work is licensed under CC Attribution 4.0
Submitted: 17 March 1988 | Published: 17 March 1988
Submitted: 17 March 1988 | Published: 17 March 1988
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C. P. Snyman,, South AfricaFull Text:
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In view of the principle of actualism the early history of the earth must be explained on the basis of present-day natural phenomena and the basic Laws of Nature. The study of the solar system leads to the conclusion that the planets were formed as by-products when the sun developed from a rotating cloud of cosmic gas and dust. The protoplanets or planetesimals could have accreted as a result of mutual collisions, during which they could have become partly molten so that they could differentiate into a crust, a mantle and a core on the basis of differences in density.
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