A good example of a white star is Sirius, Deneb, Altair or Vega.
Epsilon Orionis and Rigel
The color of a star determines the heat of the star. For example; a white dwarf star does not produce nearly as much heat as our sun does. However, one day, our sun will turn into a white dwarf star. When this happens there will not be enough heat to live on Earth.
a white dwarf star
the color of the star regulus is blue-white
A white star has a temperature range of between 7,500-10,000 K. A blue white star has an even higher temperature range, and a blue star has the highest.
Epsilon Orionis and Rigel
The color of a star determines the heat of the star. For example; a white dwarf star does not produce nearly as much heat as our sun does. However, one day, our sun will turn into a white dwarf star. When this happens there will not be enough heat to live on Earth.
The obvious reason is that the specific star has bigger density compared with the Sun. For example, that star could be a "white dwarf star". A white dwarf mostly contains "electron degenerate matter", which is very dense. A white dwarf is a small dense star.
a white dwarf star
The White Star Line
White dwarf stars are hot , but not very bright, because they are so small. An example is "Sirius B", the companion of "Sirius A", the brightest star in the sky.
For example, the white light from the Sun is really a mixture of several colors.
the color of the star regulus is blue-white
The White Star line
You have to make the entire field the color of the element. For example if you use Saints the field has to be white because the element color is white.
The White Star Line.
the color of the star regulus is blue-white