An electron degenerate gas in a white dwarf is a state of matter where electrons are densely packed together, leading to a high degeneracy pressure that supports the white dwarf against the inward pull of gravity. This degenerate gas behaves differently from a classical gas and is characterized by the Pauli exclusion principle, which prevents two electrons from occupying the same quantum state.
A degenerate gas is a state of matter where particles are tightly packed together and follow quantum mechanical principles. This type of gas has unique properties such as high density, low temperature, and pressure. The behavior of a degenerate gas is characterized by the exclusion principle, which states that no two particles can occupy the same quantum state. This leads to unusual behaviors such as superfluidity and superconductivity.
That's called a "black dwarf". Such objects are hypothetical; they are not expected to exist yet, since it takes a white dwarf longer, to cool down to a black dwarf, than the current age of the Universe.
The energy source of a white dwarf is primarily from nuclear reactions involving the fusion of helium nuclei, also known as the triple-alpha process. This process converts helium into heavier elements like carbon and oxygen, releasing energy in the form of heat and light. As a white dwarf no longer undergoes significant nuclear fusion, the energy it radiates gradually comes from stored thermal energy.
The element with the electron configuration of 1s22s22p63s23p6 is neon, which has atomic number 10 and is a noble gas.
This is a chemical element. You can find the how many electron in a single atom by using a periodic table.
The pressure within the white dwarf. The situation is somewhat different from normal gas pressure; the kind of pressure within a white dwarf is called "degenerate pressure".
None of the above. White dwarfs and the black dwarfs they will become consist of a unique state of matter called electron degenerate matter.
Not normally. A white dwarf is the remnant of a star in which fusion has stopped. If, however, a white dwarf has a close binary companion star it can accrete gas from that companion. If enough gas collects on the white dwarf it can ignite a complex reaction change between the hydrogen gas and the carbon, nitrogen, and oxygen of the surface. Unlike the steady fusion in a main sequence star, the fusion on a white dwarf is a runaway reaction that results in a massive explosion called a nova, which drives away the accreted gas and ends fusion. If the white dwarf is massive enough the accretion of gas can trigger carbon fusion inside the white dwarf, resulting in an even larger explosion called a type Ia supernova, which destroys the white dwarf.
The gas being used as a fuel source for white dwarfs is primarily hydrogen. During nuclear fusion reactions in the core of a white dwarf, hydrogen atoms are fused together to form helium, releasing energy in the process.
Since white dwarf, like all stars, are made up of plasma (ionized gas), they have no craters on their surfaces.
The most likely way to reignite fusion in a white dwarf is for gas from a close binary companion to be pulled to it by gravity. As the gas collects the white dwarf heats up and may either ignite fusion in the hydrogen or in the carbon of the white dwarf itself.
stars are not always white there are many different types of star for example: Black Dwarf Red Giant White Dwarf Blue Giant Neutron they are all varying colors because of the configurations of gas and energy of particals. however 97% of our galaxy's stars are the fabled white dwarf these are white because they are expelling there entire energy at once, the white dwarf is the final stage of a stars life, aside from the purely theoretical black dwarf
Ceres is a dwarf planet. There is no such thing as a gas dwarf planet - Yet!
A supernova is a star that has exploded into dust and gas. A white-dwarf is a small, hot, dense star nearing the end of its life, that did not have enough mass to go supernova. So the answer is "none".
A degenerate gas is a state of matter where particles are tightly packed together and follow quantum mechanical principles. This type of gas has unique properties such as high density, low temperature, and pressure. The behavior of a degenerate gas is characterized by the exclusion principle, which states that no two particles can occupy the same quantum state. This leads to unusual behaviors such as superfluidity and superconductivity.
No, a white dwarf cannot kill you. White dwarfs are very dense stellar remnants that have exhausted their nuclear fuel and no longer undergo fusion reactions. They do not pose any direct threat to life on Earth.
Depending on the distance between the binary pair, it is possible for the white dwarf to draw gas from it's companion causing the star to reach the Chandrasekhar limit causing the white dwarf to explode as a nova or a type La supernova.