Phases for the month occur in the following order and time (Washington mean time): First quarter on the 2d at 4:09 p. m.; full moon on the 10th at 6:36 a. m.; last quarter on the 18th at 10:46 a. m.; new moon on the 25th at 9:49 a. m. It is also on the meridian on the 1st, 15th and 30th, at 5:18 p. m., 3:38 a. m., 5:03 p. m. respectively. On the 2d it sets at 12:41 a. m.; on the 15th rises at 11:23 p. m.; and on the 29th sets at 11:28 p. m. It is farthest from the earth on the 13th at 1:30 p. m.; and nearest to the earth on the 26th at 3:42 a. m. In latitude 41° 30′ north, its least elevation above the horizon is on the 15th, and its greatest on the 28th; on the former date being 29° 48½′, and on the latter 67° 12½′. There will also be a total eclipse, beginning on the 10th at 4:44 a. m., and ending at 8:33 a. m. The beginning of the part called “total” continues from 5:52 to 7:25 a. m., or one hour and thirty-three minutes. Magnitude nearly 1.5. As the moon sets in the neighborhood of Washington at about 5:30 a. m., only the first part and none of the “totality” will be there visible. Our neighbor, the moon, has one peculiar trait, which we could wish belonged to all our friends. It never “turns its back on you.” Cold it may be, and is often so called, but in darkest hours, and under all circumstances, it presents its face to the earth. It may be only politeness or etiquette, that causes it thus to act; but the fact remains. It may move a trifle, so that we can sometimes see more of it than at others, but four-sevenths is the limit of its surface as seen by man. What may be on the other side has never been revealed. For aught we know, there may be

“Sweet fields arrayed in living green, And rivers of delight.”

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But the probabilities are strongly on the other side. So far as we can discover, no atmosphere is there to catch and hold the rays from the burning sun, and hence it seems that all must be cold and bleak and barren. “Distance lends enchantment to the view,” and it were perhaps better that we should thus enjoy its mild light and gentle influence, than cultivate a closer acquaintance.

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The planet enjoying the distinction of being the nearest to the center of our system is too near the “dazzling brightness” to permit our finding out much about its physical constitution. We suppose, but do not know, that it revolves on its axis. We guess that it has satellites, but no one is certain that he ever saw one of them. We used to think it must be a very warm planet; but now we think it might perhaps be a moderately comfortable place for a mortal to reside. The fact is, what we do not know about it is much more than what we do know; and what we know about it for this month is nearly as follows: On the 1st, 15th, 25th and 30th it will rise after the sun, and will not be visible to the unaided eye; but on the same dates it will set at 6:32, 7:03, 8:37 and 8:35 p. m., respectively, and can therefore be easily seen after sunset from the 20th to the end of the month by anybody who will take the pains to look for it—that is, within the latitude in which most of our readers live. It reaches its most easterly limit (20° 32′) at 9:00 p. m. on the evening of the 25th, and approaches so much nearer to us during the month as to cause its diameter to appear nearly twice as large—that is, to increase from 5″ to 9″. On the 21st at 2:00 a. m. it will be 4° 20′ north of Neptune, and on the 26th at 5:55 p. m., 5° 47′ north of the moon.

The Chautauquan, Vol. 04, April 1884, No. 7 — Part 79