Convert anomalistic month to sidereal month


anomalistic month
sidereal month


More information from the unit converter

How many anomalistic month in 1 sidereal month? The answer is 0.99154811227318. We assume you are converting between anomalistic month and sidereal month. You can view more details on each measurement unit: anomalistic month or sidereal month The SI base unit for time is the second. 1 second is equal to 4.2004220987365E-7 anomalistic month, or 4.2362262070237E-7 sidereal month. Note that rounding errors may occur, so always check the results. Use this page to learn how to convert between months and months. Type in your own numbers in the form to convert the units!



Date difference between calendar days

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Quick conversion chart of anomalistic month to sidereal month

1 anomalistic month to sidereal month = 1.00852 sidereal month

5 anomalistic month to sidereal month = 5.04262 sidereal month

10 anomalistic month to sidereal month = 10.08524 sidereal month

15 anomalistic month to sidereal month = 15.12786 sidereal month

20 anomalistic month to sidereal month = 20.17048 sidereal month

25 anomalistic month to sidereal month = 25.2131 sidereal month

30 anomalistic month to sidereal month = 30.25572 sidereal month

40 anomalistic month to sidereal month = 40.34096 sidereal month

50 anomalistic month to sidereal month = 50.4262 sidereal month


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Common time conversions


Definition: Month

An anomalistic month is the average time the Moon takes to go from perigee to perigee - the point in the Moon's orbit when it is closest to Earth. An anomalistic month is about 27.55455 days on average.


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).


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