The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar systemHarris, Joseph
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The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar system
Harris, Joseph
Astronomical models; Globes
These different motions observed in the Planets, are easily
illustrated, as followeth: The lesser circle round the Sun is the
orbit of _Mercury_, in which he performs his revolution round the
Sun, in about three months, or while the Earth is going thro’ ¼ part
of her orbit, or from A to N. The numbers 1, 2, 3, _&c._ in the orbit
of _Mercury_, show the spaces he describes in a week nearly, and the
distance AB, BC, DC, _&c._ in the Earth’s orbit, do likewise show her
motion in the same time. The letters A, B, C, _&c._ in the great orb,
are the motions of _Mercury_ in the Heavens, as they appear from the
Earth. Now if the Earth be supposed in A, and _Mercury_ in 12, near his
superior conjunction with the Sun; a spectator on the Earth will see ☿,
as if he were in the point of the Heavens A, and while ☿ is moving from
12 to 1, and from 1 to 2, _&c._ the Earth in the same time also moves
from A to B, and from B to C, _&c._ All which time ☿ appears in the
Heavens to move in a direct motion from A to B, and from B to C, _&c._
but gradually slower, until he arrives near the point G; near this
place he appears stationary, or to stand still; and afterwards (tho’ he
still continues to move uniformly in his own orbit, with a progressive
motion) yet in the sphere of the fixed Stars he will appear to be
retrograde, or to go backwards, as from G to H, from H to I, _&c._
until he has arrived near the point L, where again he will appear to be
stationary; and afterwards to move in a direct motion from L to M, and
from M to N, _&c._
What has been here shewed concerning the motions of _Mercury_, is
also to be understood of the motions of _Venus_; but the conjunctions
of _Venus_ with the Sun do not happen so often as in _Mercury_; for
_Venus_ moving in a larger orbit, and much slower than _Mercury_, does
not so often overtake the Earth. But the retrogradations are much
greater in _Venus_ than they are in _Mercury_, for the same reasons.
[Sidenote: _Fig. 2._]
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