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vatories at Washington, Cambridge, Philadelphia, and Georgetown, are amply provided with instruments, and an efficient corps of observers are constantly occupied in their use.

For a long time to come, one principal object will engage the instruments of the Cincinnati observatory, viz., the exploration of the heavens south of the equator, and the re-measurement of Sturve's double stars in that region. Should this work progress but slowly, let it be remembered that the director of the observatory has no assistant, out of his own immediate family, and must devote a large portion of his time to other duties, far more closely allied to the earth than the stars.

CINCINNATI OBSERVATORY,

Mount Adams, May, 1848.

CONTENTS.

The era of physical astronomy commences, 121. A theore-
tic system proposed and discussed; a central sun and solitary
planet, 122. Planets and satellites added and their effects
considered, 124. How the imagined system may be made the
system of nature, 125. Discussion of the relative motions of
the sun, moon, and earth, under the action of their mutual
influences, 127. The moon's acceleration; motion of her
apsides, nodes, &c., and the discovery of the change in the
figure of the earth's orbit, 129. Perplexity occasioned by the

seeming discrepancy between the observed and computed

motion of the moon's perigee, 135. Finally removed by

Clairault, 138. Changes in the earth's figure occasioned by

its rotation, 141. The form of equilibrium reached, 142.

The precession of the equinoxes caused by the protuberant
matter at the earth's equator, 144. Moon affected by the
redundant matter at the earth's equator, 148. Wonderful
questions answered by an examination of the moon, 149.

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