 ... with a meteorite glowing in a denser one also given off by itself when more highly heated. Further, it has been seen that the nebula spectrum was exactly reproduced in the comets of 1866 and 1867, when away from the sun. As the collision of meteorites...  Proceedings of the Royal Society of London - Page 127by Royal Society (Great Britain) - 1888Full view - About this book
 | Sir Norman Lockyer - 1888 - 668 pages
...gently in a very tenuous atmosphere given off by itself as is the spectrum of a comet near the sun by a meteorite glowing in a denser one also given off...explanation of the phenomena in one case, it must, faute Je mieux, be accepted for the other. The well-known constituents of meteorites, especially olivine,... | |
 | Royal Society (Great Britain) - 1888 - 586 pages
...with the other three lines. The lines at 500 and 495 and F have been seen in the glow of the Dhurmsala meteorite when heated, but the origin of 495 has not...de mieux, be accepted for the other. The well-known constituents of meteorites, especially olivine, fully explain all the spectroscopic phenomena presented... | |
 | 1888 - 868 pages
...gently in a very tenuous atmosphere given off by itself as is the spectrum of a comet near the sun by a meteorite glowing in a denser one also given off...explanation of the phenomena in one case, it must, fault de mieujc, be accepted for the other. The well-known constituents of meteorites, especially olivine,... | |
 | 1888 - 478 pages
...long to yield up the secret of its origin. " The result of this comparison," Mr. Lockyer remarks, " is that the nebula spectrum is as closely associated...also given off by itself when more highly heated." The fundamental nebular line — that at wave-length 500 — is the chief constituent of the light... | |
 | 1888 - 464 pages
...before long to yield up the secret of its origin. "The result of this comparison," Mr. Lockyer remarks, "is that the nebula spectrum is as closely associated...also given off by itself when more highly heated." I The fundamental nebular line — that at wave-length 500 — is the chief constituent of the light... | |
 | Sir Norman Lockyer - 1888 - 674 pages
...gently in a very tenuous atmosphere given off by itself as is the spectrum of a comet near the sun by a meteorite glowing in a denser one also given off...in the comets of 1866 and 1867, when away from the san. As the collision of meteorites is accepted for the explanation of the phenomena in one case, it... | |
 | Sir Norman Lockyer - 1888 - 900 pages
...gently in a very tenuous atmosphere given off by itself as is the spectrum of a comet near the sun by a meteorite glowing in a denser one also given off by itself when more highly he.Ued. Further, it has been seen that the nebula spectrum was exactly reproduced in the comets of... | |
 | John Thornton (M.A.) - 1890 - 372 pages
...gently in a very luminous atmosphere given off by itself as is the spectrum of a comet near the sun by a meteorite glowing in a denser one ; also given off...nebula spectrum was exactly reproduced in the comets of 1 866 and 1867 when away from the sun. As the collision of meteorites is accepted for the explanation... | |
 | John Thornton (M.A.) - 1893 - 378 pages
...gently in a very luminous atmosphere given off by itself as is the spectrum of a comet near the sun by a meteorite glowing in a denser one ; also given off...explanation of the phenomena in one case it must, /aute de mieax, be accepted for the other. The well-known constituents of meteorites, especially olivine,... | |
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