MERCURY
Will be distinctly visible every evening from the first to the thirteenth of the month, setting at 6:06 p. m. on the evening of the former date, and at very nearly the same hour on the latter date. From the 1st to the 11th its motion is from west to east; on the 11th it is said to be stationary; however, it is actually moving in its orbit about thirty thousand miles per hour; but is approaching us in an almost direct line, and thus seems to be at a stand still. On the same day, it arrives at its greatest distance east of the sun, 19° 16′, and then starts on its journey west, approaching the earth, and coming directly between it and the sun, that is, reaching its inferior conjunction about 3:00 on the afternoon of the 20th. On the 31st it will be so far west as to rise one hour and fourteen minutes earlier than the sun.