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    How much time does it take for the Sun to revolve around the center of our galaxy?

    Question #59659. Asked by UT-7. (Sep 29 05 11:56 PM)


    dim_dude

    Does the sun revolve around it? the sun is a star, and a star can't move. At least, I don't think so. I'd really like to know the answer.

    Sep 30 05, 7:32 AM
    UT-7

    Special for you,dim_dude!!!
    http://en.wikipedia.org/wiki/Milky_Way
    The Sun's place in the Milky Way
    The Sun (and therefore the Earth and Solar System) may be found close to the inner rim of the Orion Arm, in the Local Fluff, 8.5±0.5 kpc from the galactic center. The distance between the local arm and the next arm out, the Perseus Arm, is about 6,500 light-years .
    The Apex of the Sun's Way, or the solar apex, refers to the direction that the Sun travels through space in the Milky Way. The general direction of the sun's galactic motion is towards the star Vega near the constellation of Hercules, at an angle of roughly 86 degrees to the direction of the galactic center. The sun's orbit around the galaxy is expected to be roughly elliptical with the addition of perturbations due to the galactic spiral arms and non-uniform mass distributions. We are presently about 8.5 kpc from the center of the galaxy and roughly 1/8 of an orbit before perigalacton (the sun's closest approach to the center, ~8.3 kpc).

    It would take the solar system about 200-250 million years to complete one orbit ("galactic year"), and so is thought to have completed about 20-25 orbits during its lifetime. The orbital speed is 217 km/s, i.e. 1 light-year in ca. 1400 years, and 1 AU in 8 days.



    Sep 30 05, 9:03 AM
    my_baby_love

    The disk of the Galaxy is a flattened, rotating system which contains the Sun and other intermediate-to-young stars. The sun sits about 2/3 of the way from the center to the edge of the disk (about 25,000l.y. by the most modern estimates). The sun revolves around the center of the galaxy about once every 250 million years. The disk also the galaxy about contains atomic (HI) and molecular (H2) gas and dust.

    http://cassfos02.ucsd.edu/public/tutorial/MW.html

    Sep 30 05, 9:03 AM


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