The Greeks had a system of classifying stars according tot heir brightness. The main Greek astronomer to use magnitudes was Ptolemy.
But the modern system of magnitudes was devised by Norman Pogson. A 1st magnitude star is defined as being 100 times brighter than a 6th magnitude star. A difference of one magnitude is equivalent to 2.512 times brighter or fainter.
The system was originally devised by Hipparcus, and defined more precisely in modern times.
Two ways are by temperature and brightness
No. Stars vary greatly in size and brightness.
A star's brightness is known as its magnitude. Stars with lower magnitude numbers are brighter than stars with a higher magnitude number.
relative "brightness" is based on distance, size, and temperature
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Two ways are by temperature and brightness
Two ways are by temperature and brightness
Stars are classified by their color, temperatures, sizes, and brightness, it could also be by composition and radiation.Scientists classify stars by color, luminosity, and temperature.
No. Stars vary greatly in size and brightness.
spectrum and temperature
A star's brightness is known as its magnitude. Stars with lower magnitude numbers are brighter than stars with a higher magnitude number.
relative "brightness" is based on distance, size, and temperature
no
Magnitude.
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The brightness is very similar to the temperature, the brightness relies on the temperature
Stars are classified by four different characteristics. Apparent magnitude (brightness) and absolute magnitude (how bright it would appear at 10 parsecs from the earth). Luminosity, another measure of brightness, compares the star to the sun's brightness. Spectral classifications are measured by the star's temperatures. Finally stars are signed a number by scientists through the Morgan-Keenan System.