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. FIG.

17. Long and short lines of Strontium and Calcium.

18. Arrangement of electric lamp for demonstrating the existence of long and short lines

19. Plan and section of cup used with salts

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20. Aluminium cup placed in the spark-stand as in use 21. Method of observing the spectra of solutions

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22. Examination of the spectra of solution by blowing the solute into the

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racteristic absorption of some bodies

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23. Diagram illustrating the various kinds of absorption, and the cha

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24. Absorption of different thicknesses of the colouring matter of litmus. 69 25. Arrangement for observing the absorption spectra of metallic vapours 70 26. Arrangement for observing the absorption spectra of the metals driven into vapour by the oxhyydrogen flame.

27. Reduced copy of Becquerel's photograph of the complete solar spectrum taken in 1842

28. Wave-length solar spectrum showing the lines (from L to R) the positions of which have been determined by Mascart.

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29. The H-lines in the blue end of the solar spectrum, from a photograph by the author

30. Dr. Miller's arrangements for photographing spectra

31. Dr. Miller's diagrams of the ultra-violet spectra of some of the elements in air

32. Copies of Dr. Miller's maps of the ultra-violet spectrum of platinum in various gases showing the length of the solar and ultra-violet spectrum

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33. Slit allowing five photographs to be taken on the same plate by using

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STUDIES IN

SPECTRUM ANALYSIS.

CHAPTER I.

WAVES.

§ 1. Preliminary.

THE work of the true man of Science is a perpetual striving after a better and closer knowledge of the planet on which his lot is cast, and of the universe in the vastness of which that planet is lost. The only way of doing this effectually, is to proceed as gradually, and therefore as surely as possible, along the dim untrodden ground lying beyond the known. Such is scientific work. There is no magic, no fetish in it. There is no special class of men to whom it is given to become more familiar with the beauties and secrets of nature than another. Each of us by his own work and thought, if he so choose, may enlarge the circle of his own knowledge at least, and thus make the universe. more and more beautiful, to himself at all events, if not to others.

Futher, it now and then happens in the history of the human race upon this planet, that one particular generation gathers a rich harvest of this better and closer knowledge, this advancement generally coming from an exceeding small germ of thought.

Several such instances suggest themselves. How once a Dutchman experimenting with two spectacle-glasses produced the Telescope; and how the field of the known and the knowable has been enlarged by the invention of that wonderful instrument. How once Sir Isaac Newton was in a garden and saw an apple fall; and how the germ of thought which was started in his mind by that simple incident fructified into the theory of Universal Gravitation. Each step of this kind has more firmly knit the universe together, has welded it into a more and more perfect whole, and has enhanced the marvellous beauty of its structure.

Future times will say that either this, or perhaps the next, generation, is as favoured a one as that which saw the invention of the telescope or the immortal discovery of Newton for as by the invention of the telescope the universe was almost infinitely extended; as from Newton's discovery we learned that like energies were acting in like manner everywhere; so in our time does the Spectroscope show us that like matter is acting in like manner everywhere; so that if matter and energy be not identical, then these two, namely, matter and energy, may be termed the foundation stones of the universe in which we dwell.

The newer the science the more wary must be the

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