The stationary places of the Planets variable.]

146. If the Earth kept always at _E_, it is evident that the Stationary

places of Mercury and Venus would always be in the same points of the

Heavens where they were before. For example; whilst Mercury _m_ goes

from _h_ to _n_, according to the order of the letters, he appears to

describe the arc _ABCDE_ in the Heavens, direct: and whilst he goes from

_n_ to _h_, he seems to describe the same arc back again, from _E_ to

_A_, retrograde: always at _n_ and _h_ he appears stationary at the same

points _E_ and _A_ as before. But Mercury goes round his Orbit, from _f_

to _f_ again, in 88 days; and yet there are 116 days from any one of his

Conjunctions, or apparent Stations, to the same again: and the places of

these Conjunctions and Stations are found to be about 114 degrees

eastward from the points of the Heavens where they were last before;

which proves, that the Earth has not kept all that time at _E_, but has

had a progressive motion in it’s Orbit from _E_ to _t_. Venus also

differs every time in the places of her Conjunctions and Stations; but

much more than Mercury; because, as Venus describes a much larger Orbit

than Mercury does, the Earth advances so much the farther in it’s annual

path before Venus comes round again.

[Sidenote: The Elongations of all Saturn’s inferiour Planets as seen

from him.]

147. As Mercury and Venus, seen from the Earth, have their respective

Elongations from the Sun, and Stationary places; so has the Earth, seen

from Mars; and Mars, seen from Jupiter; and Jupiter, seen from Saturn.

That is, to every superiour Planet, all the inferiour ones have their

Stations and Elongations; as Venus and Mercury have to the Earth. As

seen from Saturn, Mercury never goes above 2-1/2 degrees from the Sun;

Venus 4-1/3; the Earth 6; Mars 9-1/2; and Jupiter 33-1/4: so that

Mercury, as seen from the Earth, has almost as great a Digression or

Elongation from the Sun, as Jupiter seen from Saturn.

[Sidenote: A proof of the Earth’s annual motion.]

148. Because the Earth’s Orbit is included within the Orbits of Mars,

Jupiter, and Saturn, they are seen on all sides of the Heavens; and are

as often in Opposition to the Sun as in Conjunction with him. If the

Earth stood still, they would always appear direct in their motions,

never retrograde nor stationary. But they seem to go just as often

backward as forward; which, if gravity be allowed to exist, affords a

sufficient proof of the Earth’s annual motion.

[Sidenote: Fig. III.

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