Convert draconic year to anomalistic year


draconic year
anomalistic year


More information from the unit converter

How many draconic year in 1 anomalistic year? The answer is 1.0537751890727. We assume you are converting between draconic year and anomalistic year. You can view more details on each measurement unit: draconic year or anomalistic year The SI base unit for time is the second. 1 second is equal to 3.3391239802223E-8 draconic year, or 3.1687251843163E-8 anomalistic 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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Quick conversion chart of draconic year to anomalistic year

1 draconic year to anomalistic year = 0.94897 anomalistic year

5 draconic year to anomalistic year = 4.74485 anomalistic year

10 draconic year to anomalistic year = 9.48969 anomalistic year

20 draconic year to anomalistic year = 18.97938 anomalistic year

30 draconic year to anomalistic year = 28.46907 anomalistic year

40 draconic year to anomalistic year = 37.95876 anomalistic year

50 draconic year to anomalistic year = 47.44845 anomalistic year

75 draconic year to anomalistic year = 71.17268 anomalistic year

100 draconic year to anomalistic year = 94.8969 anomalistic year


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Common time conversions


Definition: Year

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).


Definition: Year

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).


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