How many draconic year in 1 sidereal month? The answer is 0.078823080190714. We assume you are converting between draconic year and sidereal month. You can view more details on each measurement unit: draconic year or sidereal month The SI base unit for time is the second. 1 second is equal to 3.3391239802223E-8 draconic year, 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!
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.
1 draconic year to sidereal month = 12.68664 sidereal month
2 draconic year to sidereal month = 25.37328 sidereal month
3 draconic year to sidereal month = 38.05992 sidereal month
4 draconic year to sidereal month = 50.74656 sidereal month
5 draconic year to sidereal month = 63.4332 sidereal month
6 draconic year to sidereal month = 76.11984 sidereal month
7 draconic year to sidereal month = 88.80648 sidereal month
8 draconic year to sidereal month = 101.49312 sidereal month
9 draconic year to sidereal month = 114.17976 sidereal month
10 draconic year to sidereal month = 126.86639 sidereal month
You can do the reverse unit conversion from sidereal month to draconic year, or enter any two units below:
The draconic year, draconitic year, eclipse year, or ecliptic year is the time taken for the Sun (as seen from the Earth) to complete one revolution with respect to the same lunar node (a point where the Moon's orbit intersects the ecliptic). This period is associated with eclipses: these occur only when both the Sun and the Moon are near these nodes; so eclipses occur within about a month of every half eclipse year. Hence there are two eclipse seasons every eclipse year. The average duration of the eclipse year is 346.620075883 days (346 d 14 h 52 min 54 s) (at the epoch J2000.0).
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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