How many draconic year in 1 Gaussian year?
The answer is 1.0537672907997.

We assume you are converting between **draconic year** and **Gaussian year**.

You can view more details on each measurement unit:

draconic year or
Gaussian year

The SI base unit for **time** is the second.

1 second is equal to 3.3391239802223E-8 draconic year, or 3.1687489347752E-8 Gaussian 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
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to get your age in days or measure the duration of an event.

1 draconic year to Gaussian year = 0.94898 Gaussian year

5 draconic year to Gaussian year = 4.74488 Gaussian year

10 draconic year to Gaussian year = 9.48976 Gaussian year

20 draconic year to Gaussian year = 18.97952 Gaussian year

30 draconic year to Gaussian year = 28.46928 Gaussian year

40 draconic year to Gaussian year = 37.95904 Gaussian year

50 draconic year to Gaussian year = 47.44881 Gaussian year

75 draconic year to Gaussian year = 71.17321 Gaussian year

100 draconic year to Gaussian year = 94.89761 Gaussian year

You can do the reverse unit conversion from Gaussian year to draconic year, or enter any two units below:

draconic year to millisecond

draconic year to second

draconic year to microsecond

draconic year to decade

draconic year to week

draconic year to quarter

draconic year to nanosecond

draconic year to minute

draconic year to century

draconic year to millennium

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 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).

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