The Study of Astronomy, adapted to the capacities of youth: In twelve familiar dialogues, between a tutor and his pupil: explaining the general phænomena of the heavenly bodies, the theory of the tides, &c. — John Shaqi
The Study of Astronomy, adapted to the capacities of youth: In twelve familiar dialogues, between a tutor and his pupil: explaining the general phænomena of the heavenly bodies, the theory of the tides, &c.Stedman, John, teacher of astronomy
Science
The Study of Astronomy, adapted to the capacities of youth: In twelve familiar dialogues, between a tutor and his pupil: explaining the general phænomena of the heavenly bodies, the theory of the tides, &c.
Stedman, John, teacher of astronomy
Astronomy -- Juvenile literature -- Early works to 1800
DIALOGUE VI.
PUPIL.
Since I was last with you, Sir, I have been thinking of what you then
told me, that the planets perform their revolutions in open space: I
have not the least idea how this can be; if convenient, I shall be happy
to have it explained.
TUTOR. It will be necessary first to inform you, that the orbits or
paths described by the revolution of the planets round the sun, are not
true circles (as Plate II. fig. 2.) but somewhat elliptical, that is,
longer one way than the other, as fig. 3.
PUPIL. This is exceedingly plain.
TUTOR. In a circle, the periphery or circumference is equally distant
from a point within called its center, as A; but an ellipsis has two
points called the focuses or foci, as B C. In one of these, called its
lower focus, is the sun: so that you see in every revolution of the
planet it must be nearer to the sun in one part of its orbit, than it is
in another.
PUPIL. I see it clearly.
TUTOR. Now let S (Plate II. fig. 4.) represent the sun, A B C D a planet
in different parts of its orbit; when it is nearest to the sun, as at A
it is said to be in its _perihelion_; when at B its _aphelion_; but when
at C or D its middle or mean distance, because the distance S C or S D
is the middle between A S the least and B S the greatest distance; and
half the distance between the two focuses is called the _eccentricity_
of its orbit, as S E or E F.
PUPIL. This I will endeavour to understand; but I find it will take me
some time to be perfected in it.
TUTOR. You may study it at your leisure, as it will not prevent our
proceeding to the thing proposed, namely, the laws which govern the
motion of the planets, or ATTRACTION OF GRAVITATION.
PUPIL. By attraction I think you mean that property in bodies whereby
they have a tendency to approach each other. I remember you told me that
the magnet I had the other day attracted the needle.
TUTOR. Yes. And you may recollect that when I took a feather suspended
by a thread, and put it near the conductor of the electrical machine, it
was strongly attracted by it, and adhered to it as long as the machine
was kept in motion.
PUPIL. I remember it well. But what am I to understand by attraction of
gravitation?
TUTOR. The sun, being the largest body, _attracts_ the earth and all the
other planets, they _gravitate_ or have a tendency to approach the sun;
the earth being larger than the moon _attracts_ her, and she
_gravitates_ towards the earth; the planets are attracted by and
gravitate towards each other; a stone when thrown from the earth, by its
attraction and the gravitating power or weight of the stone, is brought
to the earth again; the waters in the ocean gravitate towards the center
of the earth; and it is by this power we stand on all parts of the earth
with our feet pointing to the center.
PUPIL. This information affords me great pleasure.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account