Stellar Evolution And Its Relations to Geological Time

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T. Sterry Hunt, in a lecture on " The Chemistry of the Primeval Earth, " delivered at the Eoyal Institution (May 31, 1867), put forward, apparently quite independently, opinions on dissocia- tion similar to those of Brodie. In this lecture he says : " I considered the chemistry of nebulae, sun, and stars in the combined light of spectroscopic analysis and Deville's researches on dissociation, and con- cluded with the generalisation that the breaking-up of compounds, or dissociation of elements,... by intense heat is a principle of universal application, so that we may suppose that all the elements which make up the sun, or our planet, would, when so intensely heated as to be in the gaseous condition which all matter is capable of assuming, remain uncombined, that is to say, would exist together in the state of chemical elements, whose further dissociation in stellar or nebulous masses may even give us evidence of matter still more elemental than that revealed ifi the experiments of the laboratory, where we can only conjecture the compound nature of many of the so- called elementary substances.

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