The second precession is that of the major axis of the Moon's elliptical orbit ( the line of the apsides from perigee to apogee ), which sidereal month ( the period of time when the Moon completes one revolution with respect to the fixed stars ).
22.
However, during one sidereal month, Earth has revolved part way around the Sun, making the average time between one new moon and the next longer than the sidereal month : it is approximately 29.5 days . This is known as the synodic month and corresponds to what is commonly called the lunar month.
23.
However, during one sidereal month, Earth has revolved part way around the Sun, making the average time between one new moon and the next longer than the sidereal month : it is approximately 29.5 days . This is known as the synodic month and corresponds to what is commonly called the lunar month.
24.
The net effect is that the Moon alternately lags and leads, showing nearly 60 % of its surface over the course of a sidereal month, even though only the same 50 % is visible at any given point in a sidereal month . & mdash; Lomn 19 : 03, 4 March 2010 ( UTC)
25.
The net effect is that the Moon alternately lags and leads, showing nearly 60 % of its surface over the course of a sidereal month, even though only the same 50 % is visible at any given point in a sidereal month . & mdash; Lomn 19 : 03, 4 March 2010 ( UTC)
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