How many anomalistic year in 1 draconic year? The answer is 0.94896901195784. We assume you are converting between anomalistic year and draconic year. You can view more details on each measurement unit: anomalistic year or draconic year The SI base unit for time is the second. 1 second is equal to 3.1687251843163E-8 anomalistic year, or 3.3391239802223E-8 draconic year. Note that rounding errors may occur, so always check the results. Use this page to learn how to convert between years and years. Type in your own numbers in the form to convert the units!
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1 anomalistic year to draconic year = 1.05378 draconic year
5 anomalistic year to draconic year = 5.26888 draconic year
10 anomalistic year to draconic year = 10.53775 draconic year
15 anomalistic year to draconic year = 15.80663 draconic year
20 anomalistic year to draconic year = 21.0755 draconic year
25 anomalistic year to draconic year = 26.34438 draconic year
30 anomalistic year to draconic year = 31.61326 draconic year
40 anomalistic year to draconic year = 42.15101 draconic year
50 anomalistic year to draconic year = 52.68876 draconic year
You can do the reverse unit conversion from draconic year to anomalistic year, or enter any two units below:
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).
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).
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