Through the sunlit half can be seen

Through the 19th and 20th centuries, visual exploration through powerful telescopes has fielded a fairly comprehensive picture of the visible side of the moon. The hitherto unseen far side of the moon was first revealed to the world in October 1959 through photographs made by the Soviet Lunik III spacecraft.

This photograph showed that the far side of die moon is similar to the near side except that large lunar Maria is absent. Craters arc now known to cover the entire moon, ranging in size from huge, ringed Maria to those of microscopic size. The entire moon has about 3 trillion craters larger than about 1 m in diameter.

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The moon shows different phases as it moves along its orbit around the earth. Half the moon is always in sunlight, just as half the earth has day while the other half has night. The phases of the moon depend on how much of the sunlit half can be seen at any one time. In the new moon, the face is completely in shadow.

About a week later, the moon is in first quarter, resembling a half-circle; another week later, the full moon shows its fully lighted surface; a week afterward, in its last quarter, the moon appears as a half-circle again. The entire cycle is repeated each lunar month, which is approximately 29.5 days.

The moon is filling when it is farther away from the sun than the earth; it is new when it is closer. When it is more than half-illuminated, it is said to be in gibbous phase. The moon is when it progresses from full to new, and waxing as it proceeds again to full.

Temperatures on its surface are extreme, ranging from a maximum of 127° C (261° F) at lunar noon to a Minimum of-173° C (-279° F) just before lunar dawn. Just before the autumnal equinox on about September 23 during this season the moon rises at a point opposite to the sun, or close to the exact eastern point of die horizon.

Moreover the moon rises only a few minutes later each night, affording on several successive evenings an attractive moonrise close to sunset time and strong moonlight almost all night if the skis not clouded.

The continuance of the moonlight after sunset is useful to farmers in northern latitudes, who are then harvesting their crops. The full moon following the harvest m(X) n, which exhibits the same phenomena in a lesser degree, is called the hunter’s moon. A similar phenomenon to the harvest moon is observed in southern latitudes at the spring equinox on about March 21.