MERCURY
Presents us this month with an unusual number of phenomena, none of which, however, are of a striking character. He rises on the 1st at 8:28 a. m.; on the 16th, at 8:55 a. m.; on the 31st, at 7:48 a. m.; sets on the corresponding days at 5:16, 5:53 and 5:20 p. m.; that is, during the entire month setting from one-half hour to one and one-third hours later than the sun; and thus being visible to a careful observer for perhaps ten or twelve days both before and after the 17th, the day on which he reaches his greatest distance (20° 12′) east of the sun. His motion during the first seventeen days is 30° 33′ 44″ direct, and for the remaining fourteen 5° 9′ 55.5″ retrograde. Diameter increases from 5.2″ to 9.6″. At 3:00 p. m. on the 4th he is 1° 26′ south of Mars; on the 19th, at 6:34 a. m., 6° 27′ south of the moon; on the 25th, at 10:00 a. m., stationary; at midnight on the 29th, 2° 25′ north of Mars; and on the 30th, at 5:00 a. m., reaches its nearest point to the sun.