month (Gregorian average) to day (sidereal) conversion

Conversion number between month (Gregorian average) [mo] and day (sidereal) [d (sidereal)] is 30.520208404671. This means, that month (Gregorian average) is bigger unit than day (sidereal).

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from day (sidereal) to month (Gregorian average) conversion


Enter the number in month (Gregorian average):

Decimal Fraction Exponential Expression
[mo]
eg.: 10.12345 or 1.123e5

Result in day (sidereal)

?
precision [info]
Decimal:
Exponential:

Calculation process of conversion value


High precision conversion

If conversion between month (Gregorian average) to second and second to day (sidereal) is exactly definied, high precision conversion from month (Gregorian average) to day (sidereal) is enabled.

Since definition contain rounded number(s) too, there is no sense for high precision calculation, but if you want, you can enable it. Keep in mind, that converted number will be inaccurate due this rounding error!

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month (Gregorian average) to day (sidereal) conversion chart

Start value: [month (Gregorian average)]
Step size [month (Gregorian average)]
How many lines? (max 100)

visual:
month (Gregorian average)day (sidereal)
00
10305.20208404671
20610.40416809343
30915.60625214014
401220.8083361869
501526.0104202336
601831.2125042803
702136.414588327
802441.6166723737
902746.8187564204
1003052.0208404671
1103357.2229245139
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Multiple conversion

Enter numbers in month (Gregorian average) and click convert button.
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Converted numbers in day (sidereal):
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Details about month (Gregorian average) and day (sidereal) units:

Convert Month (Gregorian average) to other unit:

month (Gregorian average)

Definition of month (Gregorian average) unit: = 30.436875 d. Average Gregorian month is calculated from average Gregorian Year divided by 12 month: 365.2425 days / 12 months × 86400 sec ≈ 2.6297 Ms

Convert Day (sidereal) to other unit:

day (sidereal)

Definition of day (sidereal) unit: ≈ 23 h, 56 min, 4.0916 sec. A sidereal day is the time needed for the Earth to rotate once around its axis so that the distant stars appear in the same position in the sky. This is ~4 minutes shorter than the solar day.


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