Transactions of the American Philosophical Society
Transactions of the 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.
What to read after Transactions of the American Philosophical Society?
You can find similar books in the "Read Also" column, or choose other free books by American Philosophical Society to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
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.
What to read after Transactions of the American Philosophical Society?
You can find similar books in the "Read Also" column, or choose other free books by American Philosophical Society to read onlineMoreLess
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