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A.A Michelson - Motion of the Earth and Ether.
477

little in the definition of each, the measurements may be made with very considerable precision.[1]

The observations were taken in the morning, at noon, evening and night; no special care being taken as to the exact hour. The results are summed up in the table containing the observations taken and reduced by Mr. Mann, as follows:—

The micrometer was set on one spot, then on the central fringe, then on the other spot, giving three readings of the micrometer. The first reading was subtracted from the third, giving the distance between the spots in divisions of the micrometer head. The second reading was subtracted from the third, giving the distance of the central fringe from the lower in divisions of the micrometer head. This last remainder was divided by the first, giving the distance n of the central fringe from the lower spot in fractions of the distance between the spots regarded as unity.

Each reading was reduced this way and the mean of ten taken as the result for any given time. The weights p were calculated as usual from the formula: .

Date.

6 A.M.

12 Noon.

6 P.M.

11 P.M.

n

p

pn

n

p

pn

n

p

pn

n

p

pn

March 11

.500
67
33.50
.515
40
20.60
.503
12
6.03
.480
20
9.60
.513
38
19.49
.506
10
5.06
.490
32
15.68

March 13

.495
11
5.44
.530
33
17.49

March 16

.507
55
27.88
.490
50
24.95
.492
13
6.40
.479
60
28.74
.509
120
61.08
.491
45
22.09
.488
40
49.52
.487
22
10.71

March 17

.490
40
19.60
.504
80
40.32
.500
35
17.50
.488
105
51.24
.488
50
24.40
.502
60
30.12
.498
30
14.94
.496
100
49.60

March 18

.501
80
40.08
.492
80
39.36
.493
40
19.72
.498
25
12.45
.507
50
25.35
.488
25
12.20
.498
35
17.43

Sums.

461
231.47
438
220.28
205
101.37
399
195.45

Means

.502 ± .002

.503 ± .003

.494 ± .002

.490 ± .002


12 Noon - 11 P. M. = .013

1 fringe = .250       maximum displacement fringe.

The conclusion from these results is that if there is any displacement of the fringes it is less than one-twentieth of a fringe.

If we consider the times occupied by the two pencils in completing

  1. On account of the inequality of the angles of incidence and reflection there will be a slight difference between the real and apparent positions of the double image. This difference will be altogether too minute to produce any appreciable error. Again, this difference in direction produces a difference in the length of the two paths—which is however of the second order and can also be neglected.