Convert Gaussian year to sidereal month


Years
sidereal month


Did you mean to convert Gregorian year
Julian year
tropical year
sidereal year
anomalistic year
draconic year
lunar year
Gaussian year
to sidereal month

More information from the unit converter

How many Years in 1 sidereal month? The answer is 0.074801221179392. We assume you are converting between Gaussian year and sidereal month. You can view more details on each measurement unit: Years or sidereal month The SI base unit for time is the second. 1 second is equal to 3.1687489347752E-8 Years, 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 years and months. Type in your own numbers in the form to convert the units!



Date difference between calendar days

You may also want to find out how many days are between two dates on the calendar. Use the date calculatorto get your age in days or measure the duration of an event.


Quick conversion chart of Years to sidereal month

1 Years to sidereal month = 13.36877 sidereal month

2 Years to sidereal month = 26.73753 sidereal month

3 Years to sidereal month = 40.1063 sidereal month

4 Years to sidereal month = 53.47506 sidereal month

5 Years to sidereal month = 66.84383 sidereal month

6 Years to sidereal month = 80.21259 sidereal month

7 Years to sidereal month = 93.58136 sidereal month

8 Years to sidereal month = 106.95013 sidereal month

9 Years to sidereal month = 120.31889 sidereal month

10 Years to sidereal month = 133.68766 sidereal month


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Common time conversions


Definition: Year

The Gaussian year is the sidereal year for a planet of negligible mass (relative to the Sun) and unperturbed by other planets that is governed by the Gaussian gravitational constant. Such a planet would be slightly closer to the Sun than Earth's mean distance. Its length is 365.2568983 days (365 d 6 h 9 min 56 s).


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).


Metric conversions and more

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