THE EARTH’S ANNUAL MOTION.

In conformity with the Copernican view of our system, we must learn to

look upon the sun as the comparatively motionless centre about which

the earth performs an annual elliptic orbit of the dimensions and

excentricity, and with a velocity, regulated according to a certain

assigned law; the sun occupying one of the foci of the ellipse, and

from that station quietly disseminating on all sides its light and

heat; while the earth travelling round it, and presenting itself

differently to it at different times of the year and day, passes

through the varieties of day and night, summer and winter, which we

enjoy.--_Sir John Herschel’s Outlines of Astronomy._

Laplace has shown that the length of the day has not varied the

hundredth part of a second since the observations of Hipparchus, 2000

years ago.

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