The Heavens Above: A Popular Handbook of AstronomyRolfe, W. J. (William James)
Science
The Heavens Above: A Popular Handbook of Astronomy
Rolfe, W. J. (William James)
Astronomy
III. THE STELLAR UNIVERSE.
I. GENERAL ASPECT OF THE HEAVENS.
322. _The Magnitude of the Stars._--The stars that are visible to the
naked eye are divided into six classes, according to their brightness.
The brightest stars are called stars of the _first magnitude_; the next
brightest, those of the _second magnitude_; and so on to the _sixth
magnitude_. The last magnitude includes the faintest stars that are
visible to the naked eye on the most favorable night. Stars which are
fainter than those of the sixth magnitude can be seen only with the
telescope, and are called _telescopic stars_. Telescopic stars are also
divided into magnitudes; the division extending to the _sixteenth_
magnitude, or the faintest stars that can be seen with the most powerful
telescopes.
The classification of stars according to magnitudes has reference only
to their brightness, and not at all to their actual size. A sixth
magnitude star may actually be larger than a first magnitude star; its
want of brilliancy being due to its greater distance, or to its inferior
luminosity, or to both of these causes.
None of the stars present any sensible disk, even in the most powerful
telescope: they all appear as mere points of light. The larger the
telescope, the greater is its power of revealing faint stars; not
because it makes these stars appear larger, but because of its greater
light-gathering power. This power increases with the size of the
object-glass of the telescope, which plays the part of a gigantic pupil
of the eye.
The classification of the stars into magnitudes is not made in
accordance with any very accurate estimate of their brightness. The
stars which are classed together in the same magnitude are far from
being equally bright.
The stars of each lower magnitude are about two-fifths as bright as
those of the magnitude above. The ratio of diminution is about a third
from the higher magnitude down to the fifth. Were the ratio two-fifths
exact, it would take about
2-1/2 stars of the 2d magnitude to make one of the 1st.
6 stars of the 3d magnitude to make one of the 1st.
16 stars of the 4th magnitude to make one of the 1st.
40 stars of the 5th magnitude to make one of the 1st.
100 stars of the 6th magnitude to make one of the 1st.
10,000 stars of the 11th magnitude to make one of the 1st.
1,000,000 stars of the 16th magnitude to make one of the 1st.
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