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Astronomical constant - Wikipedia, the free encyclopedia

Astronomical constant

From Wikipedia, the free encyclopedia

An astronomical constant is a physical constant used in astronomy. The astronomical constants include units of astronomical distance (the astronomical unit (A.U.), the light year (ly), and the parsec (pc)), units of time (the sidereal year, the tropical year, and the Gregorian year), and various values for distances, masses, etc. (e.g., the mass and the mean radius of the Earth, and the mass, radius, and luminosity of the Sun). The astronomical constants may also be taken to include such physical constants as the speed of light (c), the gravitational constant (G), and the Planck constant (h).

The values of astronomical constants have been recalculated at various times, perhaps most notably by the Canadian-born astronomer Simon Newcomb.

[edit] Table of Astronomical constants

Quantity Symbol Value Uncertainty
Astronomical unit AU 149,597,870,691 m ± 30 m
Light-year ly 9,460,730,472,580,800 m
Parsec pc 3.086×1016 m
Speed of light in vacuum c \, 299 792 458 m·s-1 defined

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