How many Gaussian year in 1 draconic year? The answer is 0.94897612473922. We assume you are converting between Gaussian year and draconic year. You can view more details on each measurement unit: Gaussian year or draconic year The SI base unit for time is the second. 1 second is equal to 3.1687489347752E-8 Gaussian 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!
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 Gaussian year to draconic year = 1.05377 draconic year
5 Gaussian year to draconic year = 5.26884 draconic year
10 Gaussian year to draconic year = 10.53767 draconic year
15 Gaussian year to draconic year = 15.80651 draconic year
20 Gaussian year to draconic year = 21.07535 draconic year
25 Gaussian year to draconic year = 26.34418 draconic year
30 Gaussian year to draconic year = 31.61302 draconic year
40 Gaussian year to draconic year = 42.15069 draconic year
50 Gaussian year to draconic year = 52.68836 draconic year
You can do the reverse unit conversion from draconic year to Gaussian year, or enter any two units below:
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).
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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