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    Stars
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    The Magnitude Scale

    The brightness of stars and other objects is given as their magnitude. The magnitude scale of brightness had its beginning centuries ago. Ptolemy, the Egyptian astronomer, gave the approximate magnitude of stars in his catalogue, which appeared in the 2nd century. The brightest stars wer called first-magnitude stars. Dimmer stars were of the second magnitude, and so on to sixth magnitude--the dimmest stars that could be identified.

    When instruments to measure light became available, it was possible to determine differences in brightness exactly, rather than extimating them as Ptolemy had done. It was found that the degree of difference between successive magnitudes amounted to a value of 2.512. A first-magnitude star is about 2.5 times dimmer than a 0-magnitude star; a second-magnitude star is about 6.3 (2.512 X 2.512) times dimmer, and so on.

          Star Magnitude Ratio
          1 2.5 : 1
          2 6.3 : 1
          3 16 : 1
          4 40 : 1
          5 100 : 1
          10 10,000 : 1

    In some of the tables below, magnitude values are given. Those objects having the highest magnitudes are the dimmest; those with smaller numbers are brighter. In some cases the object is so bright it has a negative magnitude. Such objects are much brighter than the brightest stars.

          Sun -26.8
          Full Moon -12.0
          Venus at brightest -4.0
          Sirius -1.4
          Rigel +0.1
          Polaris +2.0

    Spectrum Classification

    One way of classifying stars is by the light spectra they produce. These are then put in order, form the very hottest stars to the coolest, and categorized by letter designations.

    Initially, A type stars were thought to be the hottest stars; B type stars the second hottest; and so on. Improved measuring techniques and greater knowledge resulted in a rearrangement of classes-thus the departure from alphabetical order. Examples of each spectral type, including range in temperature and some of the principal materials found, are given below.

      Type Name Temp. Range (K) Abundant Materials Color
      O Naos 30,000 - 60,000 Helium Blue-white
      B Spica 12,000 - 25,000 Helium Blue-white
      A Vega 8,000 - 11,000 Hydrogen White
      F Procyon 6,200 - 7,200 Hydrogen, metals Yellow-white
      G Sun 4,600 - 6,000 Hydrogen, metals Yellow
      K Arcturus 3,500 - 4,900 Calcium Orange
      M Antares 2,600 - 3,500 Titanium Orange-red
      R Variables 2,000 - 3,000 Zirconium Red
      N Alpha Cygni 2,000 - 3,000 Carbon Deep red

    The 25 Brightest Stars

          Name Constellation Apparent Magnitude
          Sun - -26.80
          Sirius Canis Major -1.43
          Canopus Carina -0.73
          Alpha Centauri Centaurus -0.27
          Arcturus Boötes -0.06
          Vega Lyra 0.04
          Capella Auriga 0.09
          Rigel Orion 0.15
          Procyon Canis Major 0.37
          Achernar Eridanus 0.53
          Beta Centauri Centaurus 0.66
          Betelgeuse Orion 0.70
          Altair Aquila 0.80
          Aldebaran Taurus 0.85
          Alpha Crucis Crux 0.87
          Antares Scorpius 0.98
          Spica Virgo 1.00
          Fomalhaut Piscis Austrinus 1.16
          Pollux Gemini 1.16
          Deneb Cygnus 1.26-26.8
          Beta Crucis Crux 1.31
          Regulus Leo 1.36
          Adhara Canis Major 1.49
          Castor Gemini 1.59
          Shaula Scorpio 1.62

    The 15 Nearest Stars

          Name Distance (light years) Apparent Magnitude Spectral Type
          Sun - -26.8 G
          Alpha Centauri 4.3 0.3 G
          Barnard's Star 5.9 9.5 M
          Wolf 359 7.6 13.5 M
          Lalande 21185 8.1 7.5 M
          Sirius 8.6 -1.4 A
          Luyten 8.9 12.5 M
          Ross 154 9.4 10.6 M
          Ross 248 10.3 12.2 M
          Epsilon Eridani 10.7 3.7 K
          Luyten 789-6 10.8 12.2 M
          Ross 128 10.8 11.1 M
          61 Cygni 11.2 5.2 K
          Epsilon Indi 11.2 4.7 K
          Procyon 11.4 0.3 F