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parsec |
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parsec (pär`sĕc) [parallax + second], in astronomy, basic unit of length for measuring interstellar and intergalactic distances, equal to 206,265 times the distance from the earth to the sun, 3.26 light-years, or 3.08 × 1013 km (about 19 million million mi). The distance in parsecs of an object from the earth is the reciprocal of the parallax parallax (pâr`əlăks) ..... Click the link for more information. of the object. The nearest star, Proxima Centauri, has a parallax of 0.763" of arc and a distance of about 1.31 parsecs. parsecUnit of measure used by astronomers to express distances to stars and galaxies. It is the distance at which the radius of Earth's orbit would subtend an angle of one second of arc, so an object one parsec away would have a parallax of one second. An object's distance in parsecs is the reciprocal of its parallax in seconds of arc. For example, Alpha Centauri, with a parallax of 0.76 second, is 1.33 parsecs from the Sun and Earth. One parsec equals 3.26 light-years, or 19.2 trillion mi (30.9 trillion km). parsec a unit of astronomical distance equal to the distance from earth at which stellar parallax would be 1 second of arc; equivalent to 3.0857 × 1016 m or 3.262 light years parsec [′pär‚sek] (astronomy) The distance at which a star would have a parallax equal to 1 second of arc; 1 parsec equals 3.258 light-years or 3.08572 × 1013kilometers. Derived from parallax-second.
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| Astronomers estimate that Geminga may lie no more than 30 parsecs, or about 100 light-years, from Earth. However, certain of its characteristics suggest it may be much closer, perhaps as near as 6 parsecs (20 light-years). The R Coronae Borealis shell is 8 parsecs or 26 light-years across, about 20 times as large as any shell previously found around a late-type star such as this. |
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