Michelson A.A. The relative Motion of the Earth and the Ether. // American Journal of Science.—Fourth Series, Vol. III, No. 18.—June, 1897.

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THE

AMERICAN

JOURNAL OF SCIENCE.

Editor: EDWARD S. DANA.

ASSOCIATE EDITORS

Profsssors GEO. L. GOODALE, JOHN TROWBRIDGE,

H. P. BOWDITCH and W. G. FARLOW, of Cambridge,

Professors O. C. MARSH, A. E. YERRILL and H. S. WILLIAMS, of New Haven,

Professor GEORGE F. BARKER, of Philadelphia, Professor H. A. ROWLAND, of Baltimore,

Mr. J. S. DILLER, of Washington.

FOURTH SERIES.

VOL. III—[WHOLE NUMBER, CLIII.]

Nos. 13-18.

JANUARY TO JUNE, 1897.

WITH SEVEN PLATES.

NEW HAVEN, CONNECTICUT. 1897.

Art. LI.—The relative Motion of the Earth and the Ether; by Albert A. Michelson.

To account for the phenomenon of aberration Fresnel supposes the luminiferous ether at rest, the earth moving through this medium without communicating any perceptible part of its motion. On this theory it has been shown* that it should be possible to detect a difference of the velocity of light in two directions at right angles. As no such difference was observed, it would seem to follow that Fresnel’s hypothesis is incorrect.

Another theory is that of Stokes, in which the aberration is accounted for if the relative velocity of the earth and the ether have a potential. This requirement, however, is inconsistent with the results of the experiment just cited, which indicates that at the earth’s surface the relative motion is zero.

In the hope of detecting a relative motion corresponding to a difference of level, the following experiment was undertaken.

I take this opportunity of gratefully acknowledging the faithful and efficient services rendered in the execution of this work by Professor S. W. Stratton and Mr. C. R. Mann.

l.

Light from the source s, a calcium light or an electric arc lamp, separated into two pencils at a plane-parallel glass plate,

o, lightly silvered. The two pencils were reflected by double mirrors along the paths oabcoe, and ocbaoe, respectively. The two paths being equal, interference fringes could be observed with the aid of the telescope at e. Fig. 2 shows details of the corner at c: pq are plane-parallel glass disks, cemented to the

*This Journal, November, 1887.



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