Orbit of The Moon - Lunar Periods

Lunar Periods

See also: Month
Name Value (days) Definition
sidereal month 27.32166155 with respect to the distant stars (13.36874634 passes per solar orbit)
synodic month 29.53058886 with respect to the Sun (phases of the Moon, 12.36874634 passes per solar orbit)
tropical month 27.321582 with respect to the vernal point (precesses in ~26,000 years)
anomalistic month 27.554550 with respect to the perigee (recesses in 3232.6054 days = 8.8504 years)
draconic (nodical) month 27.212220815 with respect to the ascending node (precesses in 6793.4765 days = 18.5996 years)

There are several ways to measure how much time it takes the Moon to complete one orbit. The sidereal month is the time it takes to make one complete orbit with respect to the fixed stars, which is about 27.3 days. In contrast, the synodic month is the time it takes the Moon to reach the same phase, which takes about 29.5 days. The synodic period is longer than the sidereal period because the Earth–Moon system moves a finite distance in its orbit around the Sun during each sidereal month, and a longer time is required to achieve the same relative geometry. Other definitions for the duration of a lunar month include the time it takes to go from perigee to perigee (the anomalistic month), from ascending node to ascending node (the draconic month), and from two successive passes of the same ecliptic longitude (the tropical month). As a result of the slow precession of the lunar orbit, these latter three periods are only slightly different from the sidereal month. The average length of a calendric month (1⁄12 of a year) is about 30.4 days.

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