Density of White Dwarfs: Questions & Answers

  • A
  • Thread starter K. Doc Holiday
  • Start date
  • Tags
    Density
In summary, White Dwarfs are incredibly dense objects that are the remnants of low to medium mass stars. They are made up mostly of carbon and oxygen, with a thin layer of hydrogen and helium on their surface. The density of a White Dwarf is incredibly high, with some measuring up to one ton per cubic centimeter. This extreme density is a result of the gravitational collapse that occurs when the star runs out of nuclear fuel. White Dwarfs are also known for their small size and high temperatures, with some reaching temperatures of over 100,000 degrees Celsius. Despite their small size, White Dwarfs have a mass comparable to that of our sun, making them some of the densest objects in the universe.
  • #1
K. Doc Holiday
32
13
White dwarfs are about the size of the Earth but they are 200,000 to 400,000 times more dense. (They contain almost as much mass as the sun.)

Question one: can we duplicate this density in a lab? If so, when did we accomplish that?

Matter normally comes in five forms; the common 3 are solid, liquid and gas. The uncommon forms are the Bose - Einstein condensate and plasma. (One at extremely low temp the other at extremely high.)

Are white dwarfs composed of one or more of these 5? Or at these densities can we assume a more exotic form of matter is present?

For example, is it possible that they are composed, at least partially, of matter which has overcome electron degeneracy?

In other words, is it theoretically possible that the only way to compact matter to a density 200,000 times more dense than solid granite is to strip the electrons, leaving only atomic nuclei?

I apologize in advance for asking such stupid questions and i appreciate everyone's patience.
 
  • Like
Likes Delta2
Astronomy news on Phys.org
  • #2
I really don't think we've ever come any close to white dwarf density in laboratory. I don't know if something like that can be momentarily achieved in situations like the core of a nuclear explosion or such extreme circumstances; it's certainly not something you can reach with a really big hydraulic press.

White dwarfs are composed exactly of matter that's stabilised against gravitational collapse by electron degeneracy pressure. When they go beyond 1.4 solar masses the pressure isn't enough any more and that makes the electrons and protons merge, forming neutrons, thus forming a neutron star, stabilised by the neutron degeneracy pressure. What you suggested would not work for a simple reason: Coulomb's force. Ordinary matter stripped of all its electrons would be entirely positive and experience such crazy Coulombic repulsion there would be no way for it to be compressed easily. It would, instead, be impossibly hard to do so. This comes to mind: https://what-if.xkcd.com/140/.
 
  • Like
Likes stoomart
  • #3
K. Doc Holiday said:
Are white dwarfs composed of one or more of these 5? Or at these densities can we assume a more exotic form of matter is present?

The white dwarf is held up by degeneracy pressure, but the temperature is so high that, unlike in a solid metal, the atoms are completely ionized and form a degenerate gas. A degenerate gas is essentially an entirely different state or phase than anything else.

K. Doc Holiday said:
For example, is it possible that they are composed, at least partially, of matter which has overcome electron degeneracy?

What do you mean by "overcoming" the degeneracy?
 

What is the density of a white dwarf?

The average density of a white dwarf star is about one million times that of water, or about 1 ton per cubic centimeter.

How does the density of a white dwarf compare to other stars?

White dwarfs are some of the densest objects in the universe, with densities that are 100,000 times higher than the Sun's.

What determines the density of a white dwarf?

The density of a white dwarf is determined by its mass. The more massive the star, the higher its density will be.

What is the Chandrasekhar limit and how does it relate to the density of white dwarfs?

The Chandrasekhar limit is the maximum mass that a white dwarf can have before it collapses into a neutron star or black hole. It is directly related to the density of the white dwarf, as a higher density means a higher mass and vice versa.

Can the density of a white dwarf change?

The density of a white dwarf remains relatively constant throughout its lifetime, as it is supported by electron degeneracy pressure. However, it can increase if the white dwarf accretes mass from a companion star, leading to a potential collapse into a supernova or neutron star.

Similar threads

Replies
1
Views
2K
  • Astronomy and Astrophysics
2
Replies
49
Views
2K
  • Astronomy and Astrophysics
Replies
2
Views
2K
  • Astronomy and Astrophysics
Replies
9
Views
1K
  • Astronomy and Astrophysics
Replies
2
Views
1K
  • Astronomy and Astrophysics
Replies
5
Views
2K
  • Astronomy and Astrophysics
Replies
2
Views
5K
  • High Energy, Nuclear, Particle Physics
Replies
9
Views
3K
Replies
15
Views
4K
  • Advanced Physics Homework Help
Replies
3
Views
2K
Back
Top