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
136. But as our solar Astronomer could have no idea of measuring the
courses of the Planets by our days, he would very probably take the
period of Mercury, which is the quickest moving Planet, for a measure to
compare the periods of the others by. As all the Stars would appear
quiescent to him, he would never think that they had any dependance upon
the Sun; but could naturally imagine that the Planets have, because they
move round the Sun. And it is by no means improbable, that he would
conclude those Planets whose periods are quickest to move in Orbits
proportionably less than those do which make slower circuits. But being
destitute of a method for finding their Parallaxes, or, more properly
speaking, as they could have no Parallax to him, he could never know any
thing of their real distances or magnitudes. Their relative distances he
might perhaps guess at by their periods, and from thence infer something
of truth concerning their relative bulks, by comparing their apparent
bulks with one another. For example, Jupiter appearing bigger to him
than Mars, he would conclude it to be much bigger in fact; because it
appears so, and must be farther from him, on account of it’s longer
period. Mercury would seem bigger than the Earth; but by comparing it’s
period with the Earth’s, he would conclude that the Earth is much
farther from him than Mercury, and consequently that it must be really
bigger though apparently less; and so of the rest. And, as each Planet
would appear somewhat bigger in one part of it’s Orbit than in the
opposite, and to move quickest when it seems biggest, the observer would
be at no loss to determine that all the Planets move in Orbits of which
the Sun is not precisely in the center.
[Sidenote: The Planetary motions very irregular as seen from the Earth.
PLATE III.]
137. The apparent magnitudes of the Planets continually change as seen
from the Earth, which demonstrates that they approach nearer to it, and
recede farther from it by turns. From these Phenomena, and their
apparent motions among the Stars, they seem to describe looped curves
which never return into themselves, Venus’s path excepted. And if we
were to trace out all their apparent paths, and put the figures of them
together in one diagram, they would appear so anomalous and confused,
that no man in his senses could believe them to be representations of
their real paths; but would immediately conclude, that such apparent
irregularities must be owing to some Optic illusions. And after a good
deal of enquiry, he might perhaps be at a loss to find out the true
cause of these inequalities; especially if he were one of those who
would rather, with the greatest justice, charge frail man with
ignorance, than the Almighty with being the author of such confusion.
[Sidenote: Those of Mercury and Venus represented.
Fig. I.]
Public-domain text, read in full here on John Shaqi.
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