MadSci Network: Astronomy |
Hi Donald, You heard right that we are getting closer to Vega. The Sun's motion is about 20 km/s, pretty close to the direction of Vega, and Vega is approaching the Sun at about 14 km/s. Vega isn't moving directly towards the Sun, however: its transverse velocity (ie at right angles to the line between the Sun and Vega) is about 2.71 AU/year (1 AU= 1 "astronomical unit" = distance from the Earth to the Sun). So the distance of closest approach is (2.71 AU/year)*(time to closest approach), where (time to approach) = (current distance)/(approach speed) I calculate the number of years as about 250 000, so the distance is about 650 000 AU, which is 3.2 parsec or 10.4 light years. This is a little under half the current Vega-Sun distance of 7.8 parsec. So it's not as though Vega will be screaming through the solar system, but it will be about 4 times brighter being only half as far away. This is only a rough calculation, since it assumes that the Sun and Vega will not deviate from their current velocities in the next quarter million years. This isn't quite true, because the other stars in the neighborhood will also have some (small) gravitational effect on both stars. I don't know of any caulcation that attempts to map the local stars' positions out in detail for the next 250000 years. But in principle it could certainly be done. I got the numbers for this calculation from "Abell's Exploration of the Universe", 7th Ed. by Morrison, Wolff and Fraknoi. This college astronomy text is a very good general reference. Pauline
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