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.