Gaussian year
In Astronomy, a Gaussian year is a definite Unité of time like equal to: 365.2568983 D (either 365 D 6 H 9 min 56 S). Historically, it is about the value adopted by Carl Friedrich Gauss for the sidereal Année in its studies on the dynamics of the solar system; the sidereal year has a different value nowadays and that used per Gauss was baptized of its name.
Definition
By definition, a negligible particle of mass which orbits a body of a solar Masse with a period of one Gaussian year has a Equatorial radius of a astronomical Unité.The value of the Gaussian year is derived from the third law of Kepler:
where
-
K is the gravitational Constante of Gauss.
See too
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