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  2. Proper motion - Wikipedia

    en.wikipedia.org/wiki/Proper_motion

    Barnard's Star's transverse speed is 90 km/s and its radial velocity is 111 km/s (perpendicular (at a right, 90° angle), which gives a true or "space" motion of 142 km/s. True or absolute motion is more difficult to measure than the proper motion, because the true transverse velocity involves the product of the proper motion times the distance.

  3. Apparent magnitude - Wikipedia

    en.wikipedia.org/wiki/Apparent_magnitude

    For example, a magnitude 2.0 star is 2.512 times as bright as a magnitude 3.0 star, 6.31 times as magnitude 4.0, and 100 times magnitude 7.0. The brightest astronomical objects have negative apparent magnitudes: for example, Venus at −4.2 or Sirius at −1.46.

  4. Magnitude (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Magnitude_(astronomy)

    An illustration of light sources from magnitude 1 to 3.5, in 0.5 increments. In astronomy, magnitude is a measure of the brightness of an object, usually in a defined passband. An imprecise but systematic determination of the magnitude of objects was introduced in ancient times by Hipparchus. Magnitude values do not have a unit.

  5. Rigel - Wikipedia

    en.wikipedia.org/wiki/Rigel

    It has an apparent magnitude of 6.7, making it 1/400th as bright as Rigel. Two stars in the system can be seen by large telescopes, and the brighter of the two is a spectroscopic binary . These three stars are all blue-white main-sequence stars , each three to four times as massive as the Sun. Rigel and the triple system orbit a common center ...

  6. Vega - Wikipedia

    en.wikipedia.org/wiki/Vega

    Radial velocity (R v) −13.9 ± 0.9 [9] ... Vega is the bright star near the bottom. ... the magnitude scale has been calibrated so that the magnitude of these stars ...

  7. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    Radial velocity (R v) ... although at its extremes it can become as bright as magnitude 0.0 or as faint as magnitude +1.6. Betelgeuse is listed in the ...

  8. Messier 87 - Wikipedia

    en.wikipedia.org/wiki/Messier_87

    Apparent magnitude (V) 8.6 [4] ... with a very bright, 45 ... The escape of the cluster with such a high velocity was speculated to have been the result of a close ...

  9. Gamma Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/Gamma_Cassiopeiae

    Gamma Cassiopeiae has three faint companions, listed in double star catalogues as components B, C, and D. [24] [25] [15] Star B is about 2 arc-seconds distant and magnitude 11, and has a similar space velocity to the bright primary, making it likely to be physically associated.