Convert sidereal month to anomalistic year


sidereal month
anomalistic year


More information from the unit converter

How many sidereal month in 1 anomalistic year? The answer is 13.368865902259. We assume you are converting between sidereal month and anomalistic year. You can view more details on each measurement unit: sidereal month or anomalistic year The SI base unit for time is the second. 1 second is equal to 4.2362262070237E-7 sidereal month, or 3.1687251843163E-8 anomalistic year. Note that rounding errors may occur, so always check the results. Use this page to learn how to convert between months and years. Type in your own numbers in the form to convert the units!



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Quick conversion chart of sidereal month to anomalistic year

1 sidereal month to anomalistic year = 0.0748 anomalistic year

10 sidereal month to anomalistic year = 0.74801 anomalistic year

20 sidereal month to anomalistic year = 1.49601 anomalistic year

30 sidereal month to anomalistic year = 2.24402 anomalistic year

40 sidereal month to anomalistic year = 2.99203 anomalistic year

50 sidereal month to anomalistic year = 3.74003 anomalistic year

100 sidereal month to anomalistic year = 7.48007 anomalistic year

200 sidereal month to anomalistic year = 14.96013 anomalistic year


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Common time conversions


Definition: Month

The sidereal month is defined as the Moon's orbital period in a non-rotating frame of reference (which on average is equal to its rotation period in the same frame). It is about 27.32166 days (27 days, 7 hours, 43 minutes, 11.6 seconds). The exact duration of the orbital period cannot be easily determined, because the 'non-rotating frame of reference' cannot be observed directly. However, it is approximately equal to the time it takes the Moon to pass twice a "fixed" star (different stars give different results because all have proper motions and are not really fixed in position).


Definition: Year

The anomalistic year is the time taken for the Earth to complete one revolution with respect to its apsides. The orbit of the Earth is elliptical; the extreme points, called apsides, are the perihelion, where the Earth is closest to the Sun (January 3 in 2011), and the aphelion, where the Earth is farthest from the Sun (July 4 in 2011). The anomalistic year is usually defined as the time between perihelion passages. Its average duration is 365.259636 days (365 d 6 h 13 min 52.6 s) (at the epoch J2011.0).


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