STAR CLASSIFICATION Stars appear to the naked eye as spiky, twinkling lights or scintillation,
especially at night. The stars near the horizon also seem to
flash and change color. The twinkling and flashing effects are not due
to the stars themselves but to the Earth's atmosphere. Turbulent
air currents cause the star's light to dance around. The spikiness of
star images is due to optical effects in the observer's eyes. In
reality, stars are spheres of gas similar to our own Sun. Stars are
held together by gravity.
Astronomers classify stars in two ways. The
first classification uses the star’s spectrum, the color(s)
of light that the star emits. A star’s spectrum is caused by the
temperature in the outer layers of the star. If the star is hot, it
looks blue. If it is cool, it looks red. The chart below shows the
basic classification of stars by spectral type. The
temperatures for stars are measured in a unit called, Kelvin.
The temperature of a star in degrees Centigrade is equal to its
temperature in degrees Kelvin plus 273. In other words, real hot!
Try to guess what
temperature and spectral type our Sun is from the chart below.
|
The Sun
|
Spectral Type |
Color |
temperature (K) |
Example |
O |
BLUE |
40,000-25,000 |
Zeta Puppis |
B |
BLUE |
25,000-11,000 |
Spica
Regulus
Rigel |
A |
BLUE-WHITE |
11,000-7,500 |
Vega, Daneb
Sirius |
F |
WHITE |
7,500-6,000 |
Canopus, Procyon
Polaris |
G |
YELLOW-WHITE |
6,000-5,000 |
Alpha Centauri |
K |
ORANGE |
5,000-3,500 |
|
M |
RED |
3,500-3,000 |
|
|
|