Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematics — John Shaqi
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
76. The difference between the Equatoreal and Polar diameters of Jupiter
is 6230 miles; for his equatoreal diameter is to his polar as 13 to 12.
So that his Poles are 3115 miles nearer his center than his Equator is.
This results from his quick motion round his Axis; for the fluids,
together with the light particles, which they can carry or wash away
with them, recede from the Poles which are at rest, towards the Equator
where the motion is quickest, until there be a sufficient number
accumulated to make up the deficiency of gravity occasioned by the
centrifugal force, which always arises from a quick motion round an
axis: and when the weight is made up so, as that all parts of the
surface press equally heavy toward the center, there is an
_equilibrium_, and the equatoreal parts rise no higher. Our Earth being
but a very small Planet, compared to Jupiter, and it’s motion on it’s
Axis being much slower, it is less flattened of course; for the
difference between it’s equatoreal and polar diameters is only as 230 to
229, or 35 miles.
[Sidenote: Place of his Nodes.]
77. Jupiter’s Orbit is 1 degree 20 minutes inclined to the Ecliptic. His
North Node is in the 7th degree of Cancer, and his South Node in the 7th
degree of Capricorn.
[Sidenote: Saturn.
Fig. I.]
78. SATURN, the remotest of all the Planets, is about 777 millions of
miles from the Sun; and, travelling at the rate of 18 thousand miles
every hour, as in the circle marked ♄, performs his annual circuit in 29
years 167 days and 5 hours of our time; which makes only one year to
that Planet. His diameter is 67,000 miles; and therefore he is near 600
times as big as the Earth.
[Sidenote: Fig. V.
His Ring.
PLATE I.]
79. He is surrounded by a thin broad Ring, as an artificial Globe is by
its Horizon. This Ring appears double when seen through a good
telescope, and is represented by the figure in such an oblique view as
it is generally seen. It is inclined 30 degrees to the Ecliptic, and is
about 21 thousand miles in breadth; which is equal to it’s distance from
Saturn on all sides. There is reason to believe that the Ring turns
round it’s Axis, because, when it is almost edge-wise to us, it appears
somewhat thicker on one side of the Planet than on the other; and the
thickest edge has been seen on different sides at different times. But
Saturn having no visible spots on his body, whereby to determine the
time of his turning round his Axis, the length of his days and nights,
and the position of his Axis, are unknown to us.
[Sidenote: His five Moons.
Fig. I.]
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