The Twentieth Century Atlas of Popular Astronomy Comprising in Twenty-Two Plates a Complete Series of Illustrations of the Heavenly Bodies

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The orbit of the planet Venus lies in order of distance next nearer to the sun than the earth's. Hence, when Venus is nearest the earth, in inferior con- junction, a method similar to that used with Mars to obtain its parallax, and from it that of the sun, might have been adopted, if it had not been for the fact that Venus in inferior conjunction rises and sets nearl)' at the same time as the sun. Hence Venus is visible only under most unfavourable circumstances, in daylight, when the stars, ex
...cept the very brightest, are invisible. It must be remembered that the position of the planet in such observations as these is fixed by measuring its distance from neighbouring stars.
44 ASTRONOMY.
However, Venus occasionally passes so directly between us and the sun that it moves across or transits the sun's disc appearing as a round black spot on the sun. Two methods have been devised for utilising these transits of Venus to determine the solar parallax.
As early as 1716 Halley suggested the following method.


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