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: The Sun’s center the only point from which the true motions
and places of the Planets could be seen.]
135. The Sun being the center of all the Planets motions, the only place
from which their motions could be truly seen, is the Sun’s center; where
the observer being supposed not to turn round with the Sun (which, in
this case, we must imagine to be a transparent body) would see all the
Stars at rest, and seemingly equidistant from him. To such an observer
the Planets would appear to move among the fixed Stars, in a simple,
regular, and uniform manner; only, that as in equal times they describe
equal Areas, they would describe spaces somewhat unequal, because they
move in elliptic Orbits § 155. Their motions would also appear to be
what they are in fact, the same way round the Heavens; in paths which
cross at small Angles in different parts of the Heavens, and then
separate a little from one another § 20. So that, if the solar
Astronomer should make the Path or Orbit of any one Planet a standard,
and consider it as having no obliquity § 201, he would judge the paths
of all the rest to be inclined to it; each Planet having one half of
it’s path on one side, and the other half on the opposite side of the
standard Path or Orbit. And if he should ever see all the Planets start
from a conjunction with each other[28]; Mercury would move so much
faster than Venus as to overtake her again (though not in the same point
of the Heavens) in a quantity of time almost equal to 145 of our days
and nights; or, as we commonly call them, _Natural Days_, which include
both the days and nights: Venus would move so much faster than the Earth
as to overtake it again in 585 natural days: the Earth so much faster
than Mars as to overtake him again in 778 such days: Mars is much faster
than Jupiter as to overtake him again in 817 such days: and Jupiter so
much faster than Saturn as to overtake him again in 7236 days, all of
our time.
[Sidenote: The judgment that a solar Astronomer would probably make
concerning the distances and bulks of the Planets.]
Public-domain text, read in full here on John Shaqi.
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