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Two lectures on the parallax and distance of the sun, as deducible from the transit of Venus
Read in Holden-Chapel at Harvard-College in Cambridge, New-England, in March 1769 -
An inquiry into the probable parallax
and magnitude of the fixed stars, from the quantity of light which they afford us, and the particular circumstances of their situation. By the Rev. John Michell, B. D. F. R. S -
Parallaticae commentationis praxeosq[ue] nucleus quidam. Authore Ioanne Dee, Londinensi
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A plain method of determining the parallax of Venus
by her transit over the sun: and from thence, by analogy, the parallax and distance of the sun, and of all the rest of the planets. By James Ferguson -
The whole doctrine of parallaxes explained
and illustrated by an arithemetical [sic] and geometrical construction of the transits of Venus and Mercury over the sun. ... The second edition, corrected and enlarged. By the Rev. Mr. Edward Stone -
A treatise on the parallactic angle, extracted from a letter to the late Earl of Macclesfield on that subject. To which is added an appendix: containing a compleat set of solar and lunar tables, Entitled, Tabulae Dunelmenses, for Computing the Places of those Luminaries, both in, and out of Syzigies
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Two lectures on the parallax and distance of the sun, as deducible from the transit of Venus
Read in Holden-Chapel at Harvard-College in Cambridge, New-England, in March 1769. By John Winthrop, Esq. Hollisian Professor of the Mathematics and Philosophy at Cambridge, and F.R.S. [Three lines in Latin] Published by the general desire of the students -
Animadversions on Dr. Stewart's computation of the sun's distance from the earth
By John Landen, F.R.S -
Notes shewing how to get the angle of parallax of a comet or other phænomenon at two observations
to be taken in any one station or place of the earth and thereby the distance from the earth -
Tables for correcting the apparent distance of the moon and a star from the effects of refraction and parallax. Published by order of the Commissioners of Longitude
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A plain method of determining the parallax of Venus
by her transit over the sun: and from thence, by analogy, the parallex and distance of the sun, and of all the rest of the planets. By James Ferguson