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
History
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
The innermost circle represents the Earth’s orbit, divided into 12
parts, answering to her monthly motion; the greatest circle is in the
orbit of _Jupiter_, which he describes in about 12 years; and therefore
the ¹/₁₂ thereof, from A to N, defines his motion, in one of our years
nearly; and the intermediate divisions, A, B, C, _&c._ his monthly
motion. Let us suppose the Earth to be in the point of her orbit 12,
and _Jupiter_ in A, in his conjunction with the Sun; it is evident
that from the Earth _Jupiter_ will be seen in the great orb, or in the
point of the Heavens A, and while the Earth is moving from 12 to 1, 2,
_&c._ ♃ also moves from A to B, _&c._ all which time he appears in the
Heavens to move with a direct motion from A to B, C, _&c._, until he
comes in opposition to the Earth near the point of the Heavens E, where
he appears to be stationary; after which ♃ again begins to move (tho’
at first with a slow pace) from E through F, H, I to K, where again he
appears to stand still, but afterwards he reassumes his direct motion
from I thro’ K, to M, _&c._
From the construction of the preceding figure it appears, that when
the superior Planets are in conjunction with the Sun, their direct
motion is much quicker than at other times; and that because they
really move from West to East, while the Earth in the opposite part
of the Heavens is carried the same way, and round the same center.
This motion afterwards continually slackens until the Planet comes
almost in opposition to the Sun, when the line joining the Earth and
Planet, will continue for some time nearly parallel to itself, and so
the Planet seems from the Earth to stand still; after which, it begins
to move with a slow motion backward, until it comes into a quartile
aspect with the Sun, when again it will appear to be stationary, for
the above reasons; after that it will resume its direct motion, until
it comes into a conjunction with the Sun, then it will proceed as above
explained. Hence it also appears, that the retrogradations of the
superior Planets are much slower than their direct motions, and their
continuance much shorter; for the Planet, from its last quarter, until
it comes in opposition to the Sun, appears to move the same way with
the Earth, by whom it is then overtaken: After which it begins to go
backwards, but with a slow motion, because the Earth being in the same
part of the Heavens, and moving the same way that the Planet really
does, the apparent motion of the Planet backwards, must thereby be
lessened.
What has been here said concerning the motions of _Jupiter_, is also
to be understood of _Mars_ and _Saturn_. But the retrogradations
of _Saturn_ do oftener happen than those of _Jupiter_, because the
Earth oftener overtakes _Saturn_; and for the same reason, the
regressions of _Jupiter_ do oftener happen than those of _Mars_. But
the retrogradations of _Mars_ are much greater than those of _Jupiter_,
whose are also much greater than those of _Saturn_.
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