Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematicsFerguson, James
Science
Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematics
Ferguson, James
Astronomy -- Early works to 1800
[Sidenote: Fig. IV. The proportions of the Orbits of the Planets and
Satellites.]
271. In Fig. 4th we have the proportions of the Orbits of Saturn’s five
Satellites, and of Jupiter’s four, to one another, to our Moon’s Orbit,
and to the Disc of the Sun. _S_ is the Sun; _M m_ the Moon’s Orbit (the
Earth supposed to be at _E_;) _J_ Jupiter; _1._ _2._ _3._ _4_ the Orbits
of his four Moons or Satellites; _Sat_ Saturn; and _1._ _2._ _3._ _4._
_5_ the Orbits of his five Moons. Hence it appears, that the Sun would
much more than fill the whole Orbit of the Moon; for the Sun’s diameter
is 763,000 miles, and the diameter of the Moon’s Orbit only 480,000. In
proportion to all these Orbits of the Satellites, the Radius of Saturn’s
annual Orbit would be 21-1/4 yards, of Jupiter’s orbit 11-2/3, and of
the Earth’s 2-1/4, taking them in round numbers.
272. The annexed table shews at once what proportion the Orbits,
Revolutions, and Velocities, of all the Satellites bear to those of
their primary Planets, and what sort of curves the several Satellites
describe. For, those Satellites whose velocities round their primaries
are greater than the velocities of their primaries in open space, make
loops at their conjunctions § 269; appearing retrograde as seen from the
Sun whilst they describe the inferior parts of their Orbits, and direct
whilst they describe the superior. This is the case with Jupiter’s first
and second Satellites, and with Saturn’s first. But those Satellites
whose velocities are less than the velocities of their primary planets
move direct in their whole circumvolutions; which is the case of the
third and fourth Satellites of Jupiter, and of the second, third,
fourth, and fifth Satellites of Saturn, as well as of our Satellite the
Moon: But the Moon is the only Satellite whose motion is always concave
to the Sun. There is a table of this sort in _De la Caile_’s Astronomy,
but it is very different from the above, which I have computed from our
_English_ accounts of the periods and distances of these Planets and
Satellites.
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