from The American Heritage® Dictionary of the English Language, 4th Edition
- n. The time required for one complete revolution of the earth about the sun, relative to the fixed stars, or 365 days, 6 hours, 9 minutes, 9.54 seconds in units of mean solar time.
from Wiktionary, Creative Commons Attribution/Share-Alike License
- n. The orbital period of the Earth; a measure of the time it takes for the Sun to return to the same position with respect to the stars of the celestial sphere. A sidereal year is about 20.4 minutes longer than the tropical year due to precession of the equinoxes.
from the GNU version of the Collaborative International Dictionary of English
- n. the time in which the sun, departing from any fixed star, returns to the same. This is 365 days, 6 hours, 9 minutes, and 9.3 seconds.
from WordNet 3.0 Copyright 2006 by Princeton University. All rights reserved.
- n. the time for the earth to make one complete revolution around the sun, relative to the fixed stars
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