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duplicate proportion of those distances. For instance, if two bodies, at a given distance, attract each other with a certain force, at half the distance, they will attract each other with four times that force; at one third of the distance, with nine times that force; and

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SO on.

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Two bodies at a distance will put one another into motion by the force of attraction; which is inexplicable by us, though made evident to us by experience, and so to be taken as a principle in natural philosophy.

Supposing then the earth the sole body in the universe, and at rest; if God should create the moon, at the same distance that it is now from the earth, the earth and the moon would presently begin to move one towards another in a straight line by this motion of attraction or gravitation.

If a body, that by the attraction of another would niove in a straight line towards it, receives a new motion any ways oblique to the first; it will no longer move in a straight line, according to either of those directions, but in a curve that will partake of both. And this curve will differ, according to the nature and quantity of the forces that concurred to produce it; as, for instance, in many cases it will be such a curve as ends where it began, or recurs into itself; that is, makes up a circle, or an ellipsis or oval very little differing from a circle.

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CHAPTER II.

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To any one, who looks about him in the world, there are obvious several distinct masses of matter, separate from one another; some whereof have discernible motions. These are the sun, the fixed stars, the comets, and the planets, amongst which this earth, which we

VOL. III.

X

inhabit, is one. All these are visible to our naked eyes.

Besides these, telescopes have discovered several fixed stars, invisible to the naked eye; and several other bodies moving about some of the planets; all which were invisible and unknown before the use of

perspective-glasses was found.

The vast distances between these great bodies are called intermundane spaces; in which though there may be some fluid matter, yet it is so thin and subtile, and there is so little of that in respect of the great masses that move in those spaces, that it is as much as nothing

These masses of matter are either luminous, or opake or dark.

Luminous bodies, are such as give light of themselves; and such are the sun and the fixed stars.

Dark or opake bodies, are such as emit no light of themselves, though they are capable of reflecting of it, when it is cast upon them from other bodies; and such are the planets.

There are some opake bodies, as for instance the comets, which, besides the light that they may have from the sun, seem to shine with a light that is nothing else but an accension, which they receive from the sun, in their near approaches to it, in their respective revolutions.

The fixed stars are called fixed, because they als ways keep the same distance one from another.

The sun, at the same distance from us that the fixed stars are, would have the appearance of one of the fixed stars.

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CHAPTER III.

Elfred

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Of our Solar System.

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Our solar system consists of the sun, and the planets and comets moving about it.

The planets are bodies, which appear to us like stars; not that they are luminous bodies, that is, have light in themselves; but they shine by reflecting the light of the sun.

hey are called planets from a Greek word, which signifies wandering; because they change their places, and do not always keep the same distance with one another, nor with the fixed stars, as the fixed stars do.

The planets are either primary, or secondary.

There are six primary planets, viz. Mercury, Venus, the Earth, Mars, Jupiter, and Saturn.

All these move round the sun, which is, as it were, the centre of their motions.

The secondary planets move round about other planets. Besides the moon, which moves about the earth, four moons move about Jupiter, and five about Saturn, which are called their satellites.

The middle distances of the primary planets from the sun are as follows:

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Mercury

32,000,000 Statute miles, Venus Is distant 59,000,000 each 5280 The Earth from the 81,000,000 (English and Mars sun's cen

123,000,000 4943 French Jupiter tre, about 424,000,000 feet. Saturn

777,000,000

The orbits of the planets, and their respective distances from the sun, and from one another, together with the orbit of a comet, may be seen in the figure of the solar system hereunto annexed.

The periodical times of each planet's revolution about the sun are as follows:

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The planets move round about the sun from west to east in the zodiac; or, to speak plainer, are always found amongst some of the stars of those constellations which make the twelve signs of the zodiac.

The motion of the planets about the sun is not perfectly circular, but rather elliptical.

The reason of their motions in curve lines, is the attraction of the sun, or their gravitations towards the sun, (call it which you please); and an oblique or sidelong impulse or motion.

These two motions or tendencies, the one always endeavouring to carry them in a straight line from the circle they move in, and the other endeavouring to draw them in a straight line to the sun, makes that curve line they revolve in.

The motion of the comets about the sun is in a very long slender oval: whereof one of the focuses is the centre of the sun, and the other very much beyond the sphere of Saturn.

The moon moves about the earth, as the earth doth about the sun. So that it hath the centre of its motion in the earth; as the earth hath the centre of its revolution in the sun, about which it moves.

The moon makes its synodical motion about the earth in 29 days, 12 hours, and about 44 minutes.

It is full moon, when, the earth being between the sun and the moon, we see all the enlightened part of the moon; new moon, when, the moon being between

moon.

us and the sun, its enlightened part is turned from us; and half moon, when the moon being in the quadratures, as the astronomers call it, we see but half the enlightened part.

An eclipse of the moon is, when the earth, being between the sun and the moon, hinders the light of the sun from falling upon, and being reflected by, the

If the light of the sun is kept off from the whole body of the moon, it is a total eclipse; if from a part only, it is a partial one.

An eclipse of the sun is, when the moon, being between the sun and the earth, hinders the light of the sun from coming to us.

If the moon hides from us the whole body of the sun, it is a total eclipse; if not, a partial one.

Our solar system is distant from the fixed stars 20,000,000,000 semi-diameters of the earth; or, as Mr. Huygens expresses the distance, in his Cosmotheoros * : the fixed stars are so remote from the earth, that if a cannon-bullet should come from one of the fixed stars with as swift a motion as it hath when it is shot out of the mouth of a cannon, it would be 700,000 years in coming to the earth.

This vast distance so much abates the attraction to those remote bodies, that its operation upon those of our system is not at all sensible, nor would draw away or hinder the return of any of our solar comets; though some of them should go so far from the sun as not to make the revolution about it in less than 1000 years.

It is more suitable to the wisdom, power, and greatness of God, to think that the fixed stars are all of them suns, with systems of inhabitable planets moving about them, to whose inhabitants he displays the marks of his goodness as well as to us; rather than to imagine that those very remote bodies, so little useful to us, were made only for our sake.

* Christiani Huygenii KOXMOOENPOE, sive de terris cælestibus earumque ornatu, conjecturæ, &c. p. m. 137.

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