[A History of Science<br>Volume 2(of 5) by Henry Smith Williams]@TWC D-Link book
A History of Science
Volume 2(of 5)

BOOK II
110/368

Let us then begin our discussion with the consideration that, whatever motion may be attributed to the earth, yet we, as dwellers upon it, and hence as participators in its motion, cannot possibly perceive anything of it, presupposing that we are to consider only earthly things.

On the other hand, it is just as necessary that this same motion belong apparently to all other bodies and visible objects, which, being separated from the earth, do not take part in its motion.

The correct method to discover whether one can ascribe motion to the earth, and what kind of motion, is, therefore, to investigate and observe whether in bodies outside the earth a perceptible motion may be discovered which belongs to all alike.

Because a movement which is perceptible only in the moon, for instance, and has nothing to do with Venus or Jupiter or other stars, cannot possibly be peculiar to the earth, nor can its seat be anywhere else than in the moon.

Now there is one such universal movement which controls all others--namely, that which the sun, moon, the other planets, the fixed stars--in short, the whole universe, with the single exception of the earth--appears to execute from east to west in the space of twenty-four hours.


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