The moon, being a satellite of the earth, revolves around it. At the same time moon also rotates on its axis and the axis of the moon is more or less parallel to the axis of the earth (the axis of the moon is inclined at the angle of about 58 degree 43 inches with respect to the plane of ecliptic).
The moon has a diameter of about 3480 km and has a mass about 1/81 that of the earth. Like that of the earth the moon’s orbit is also elliptical. At its nearest point to the earth the moon is said to be inperigee, and at its farthest, in apogee. Distance between the earth and the moon varies from about 356,000 km at perigee to about 407,000 km at apogee. As the moon completes one revolution around the earth every month, the perigee and apogee are monthly phenomenon unlike perihelion andaphelion that are annual phenomenon.
The moon’s period of revolution with reference to the sun is about 29.53 days (29 days, 12 hour, 44 minutes, and 2.8 seconds) this period is called a synodic month. In term of sidereal time, it takes about 27 and half days (27.32 days, or 27 days, 7 hours, 43 minutes, 11.6 seconds) for the moon to be re-located in exactly the same meridianal position with respect to the stars. This period of about 27 and half days is called the sidereal month and is the time required by the moon to complete one revolution about the earth with respect to the stars. The time taken by the moon in completing one revolution around the earth (synodic month) is longer than one sidereal month because of the fact that while the moon revolves around the earth, the earth also evolved around the sun and thus moon has to travel a longer distance to be re-located exactly in the same position with respect to the earth and the sun.
As mentioned above, just like the earth the moon also rotates on its own axis. The time taken by the moon to complete one rotation on its axis is also exactly one sidereal month. This fact has an important bearing upon the earth-moon relationship. Consequent to this relationship we always see the same face of the moon from the earth also, we can never see from the earth the complete surface of the moon. Only 59 per cent of the total surface of the moon is visible from the earth. The remaining 41 per cent is never seen. In fact at any given time at the most 50 percent of the surface of the moon is visible from the earth and another 9 per cent can be seen from time to time with shift of the apparent edges of the illuminated part of the moon because of the relative motion (liberations) due to changes in the angle of the view from the earth.