Stellar Evolution And Its Relations to Geological Time
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In our eReader you can find the full English version of the book. Read Stellar Evolution And Its Relations to Geological Time Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book 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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To quickly assess the difficulty of the text, read a short excerpt:
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.
What to read after Stellar Evolution And Its Relations to Geological Time?
You can find similar books in the "Read Also" column, or choose other free books by James Croll to read onlineMoreLess
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