Understanding White Dwarf Temperature

In summary, the white Dwarf classification system is defined by a letter and a temperature. However, there is some overlap in temperature for certain classifications. DA white dwarfs are not precisely defined by their spectra, and there is no known statistical relationship between their temperature and other stellar measurements. Masses of white dwarfs can be measured by studying binary systems, and there is a theoretical relationship between mass and radius. There is no fundamental relationship between mass and temperature, as white dwarfs are slowly cooling off due to the lack of fusion energy.
  • #1
piareround
79
0
So after a long time I finally figured out how the white Dwarf classification system works.

Basically its first the letter D
Followed by a temperature


Correct me if I am wrong but, DO, DB, DC, DZ white dwarfs are associated with a specific effective temperature of the star. However, White dwarf stars are no precisely definable by their spectra. In fact, seems that DA and DQ actually overlap in temperature with the other spectral classifications in the table.

Therefor this got me wondering...

Is their even a known statistical relationship for DA white dwarf stars that relates their Temperature to the stars Mass, Luminosity, Radius, or any other stellar measurements?

If not then how to scientist measure the radius and mass of white dwarfs when they are like 50-100 pc away.

Please can some one help me out here >>;
 
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  • #2
Wikipedia is always a good place to start on topics like this:

http://en.wikipedia.org/wiki/White_dwarf

As far as measuring the properties, masses are usually measured by finding white dwarfs that are part of a binary system. Then from measuring the orbital dynamics, one can determine the masses of the two stars. Once the mass is known, there is a theoretical relationship between mass and radius (see above reference) that allows you to determine the radius. This can also be checked by measuring the luminosity and using the Stefan Boltzmann relation, together with the measured temperature, to calculate the radius.
I don't think there is a fundamental relationship between mass and temperature, as there is for main sequence stars. Since white dwarfs are no longer producing fusion energy, there are slowly cooling off. So their temperature also depends on how old they are.
 
  • #3
Thanks PhyzGuy, I really appreciate the help with understanding this. ^^
 

What is a white dwarf?

A white dwarf is a small, dense star that is the end stage of evolution for most stars. It is made up of leftover material from the star's core, compressed into a small size.

Why are white dwarfs so hot?

White dwarfs are hot because they are still radiating heat from their previous life as a larger star. They do not generate energy through fusion like main sequence stars, so they gradually cool over time.

What determines the temperature of a white dwarf?

The temperature of a white dwarf is primarily determined by its mass. The more massive the white dwarf, the higher its temperature will be. Other factors such as composition and age can also play a role.

How do scientists measure the temperature of a white dwarf?

Scientists can use a variety of methods to measure the temperature of a white dwarf. One common method is to study the white dwarf's spectrum, which can reveal its surface temperature. Another method is to track changes in the white dwarf's luminosity over time.

Why is understanding white dwarf temperature important?

Understanding white dwarf temperature is important for several reasons. It can help us better understand the life cycle of stars and the processes that occur during their evolution. It can also provide important insights into the properties of matter at extreme densities and temperatures.

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