Transactions of the American Philosophical Society
Transactions of the American Philosophical Society
American Philosophical Society
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Mr. Ellicott's observation appears worthy of the utmost confidence and he says that the exte- rior contact is within the limits of half a second. By the European observations it will be seen, that the time employed by the diameter of Mercury in the egress « 3' 02", 1 and ac- cording to Mr. Ellicott's observations =» 3' 05", 5 which proves that both contacts were well observed: taking the mean, the un- certainty appears to be 1" 7 and, all circumstances considered, the error of longitude can sca...rcely equal 6" of time. From the new tables of Mr. Lalande. k 9 m ■ Conjunction in the ecliptic. . • . . . . 1 04 36 0S tnie longitude from the mean equinox. . . 46 54 17 3 g 't Helioncentric latitude. S. 5 47 470 0's aberration t .-—19" 80.; nutation «— 12" 6 g 'a aberration iri longitude, s-f. 6 85 ; aberration in latitude — — - 3 28 0's horary motion. -*~ 144 926 and g relative geocentric horary motion in the interval 1 ^35 926 bet\veen the ingress and egress. 3 g 's horary motion in latitude.
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