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
If before the instrument is put into motion, the satellites of
_Jupiter_ and _Saturn_ be brought into the same right line from their
respective primaries, you will see them, as you turn the handle,
immediately dispersed from one another, according to their different
celerities. Thus one turn of the handle will bring the first of
_Jupiter_’s Moons about ⁴/₇ part round _Jupiter_, while the second has
described but ²/₇ part, the third but above ¹/₇, and the fourth not
quite ¹/₁₆ part, each of its respective orbits. If you turn the handle
until the hour index has moved 18½ hours more, the first satellite will
then be brought into its former position, and so has made one entire
revolution; the second at the same time will be almost diametrically
opposite to the first, and so has made a little more than half of
one revolution; the others will be in different aspects, according
to the length of their periods, as will be plainly exhibited by the
instrument. The same observations may be made with respect to the
satellites of _Saturn_.
The machine is so contrived, that the handle may be turned either way;
and, if before you put it into motion, you observe the aspect (or
situation with respect to each other) of the Planets, and then turn the
handle round any number of times; the same number of revolutions being
made backwards, will bring all the Planets to their former situations.
I shall next proceed to particulars.
_Of the Stations and Retrogradations of the Planets._
[Sidenote: _Retrograde Motion of the Planets._]
The primary Planets, as they all turn round the Sun, at different
distances, and in different times, appear to us from the Earth to have
different motions; as sometimes they appear to move from West to East,
according to the order of the signs, which is called their _Direct
Motion_; then by degrees they slacken their pace, until at last they
lose all their motion, and become _Stationary_, or not to move at all;
that is, they appear in the same place with respect to the fixed Stars
for some time together; after which they again begin to move, but with
a contrary direction, as from East to West, which is called their
_Retrograde Motion_; then again they become stationary, and afterwards
reassume their direct motion. The reason of all these appearances is
very evidently shewn by the _Orrery_.
_Of the Stations_, &c. _of the Inferior Planets._
We shall instance in the Planet _Mercury_, because his motion round the
Sun differs more from the Earth’s than that of _Venus_ does.
Public-domain text, read in full here on John Shaqi.
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