Transactions of the American Philosophical Society 1, Ed,2

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23'. 20" the given inclin. of Venus's or- bit to the ecliptic: Is to Radius, " So is S, 242'', 936, the heliocent. dift. of the cent, of the Sun from Venus, at the middle of the tranfit, " To the Sine of 4io",5=i°. 8'. 25", the Sun's difk, from the node of Venus at the ecliptical conjundion.
" As S, of 1°. 8'. 25", the Sun's dift. from the node of Venus, " Is to 10'. io",6i, the geocent. neareft dift. of their centers " So ASTRONOMICAL PAPERS. 75 " So is Rad : to the S, of 8°. 32'. 57",6, the a
...ngle of Venus's vifible path with the ecliptic.
" From 8". 32' . S7"^'> the angle of Venus's vifible path, " Subt. 3. 23. 20, the inclination of Venus's orbit with the eclipt. and the remainder is 5^. 9' • 37")6. Then " As S, 5°. 9' . 2>7''^^ the diff. of the angle of Venus's vifible path and the inclin. of her orbit, &c.
" Is to S, 8°. 32'. 57",6 the angle of Venus's vifible path with the eclipt.
" So is 2^,392375 the given hor. motion of the Sun.
" To 3', 954 12 the hor. motion of Venus.


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