Try Collapsar' derived from "Collapsed Star"
Also black holes are often referred to as singularities.
neutron stars are also known as pulsars, magnetars, and hyperneutron stars depending on it's characteristics
PSR J0108-1431 is our closest (discovered) neutron star at a distance of about 424 light years from us.
The most famous is CP1919 better known as LGM-1 for Little Green Men. The first pulsar to be observed.
Pulsar
Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.
The very definition of a black hole is a stellar body dense enough to have an escape velocity greater than that of light -- in other words, light that comes close enough to its event horizon will be trapped around it forever. If a star dies and it has enough mass to be compressed to a high-enough mass-to-radius-squared ratio to have such a high escape velocity, then a black hole will result. Otherwise, it will become a neutron star -- extremely dense, to be sure, but not dense enough to trap light, and therefore not as dense as a black hole.
The stars solar mass, or relative size to the sun. If its gravity is big enough, when it does condense in on itself, it will create a black hole. If not, it will form a highly dense clump of matter, or a Neutron Star If the stars mass is more than 3 solar masses, it will form a black hole. If it is less, it will form a neutron star
A nova is created when additional material is accreted onto the hot surface of a white dwarf.If sufficient material is accreted that pushes the mass of the white dwarf over the Chandrasekhar limit of about 1.38 solar masses a type Ia supernova will occur.See related questions.
Well, they don't affect us directly... But it's interesting to know that most stars - and pressumably that will include our Sun - will end up as a white dwarf, eventually. The exception is the most massive stars, which become neutron stars or black holes.
A cooled white dwarf is a black dwarf. I think you are thinking of a neutron star which has nothing to do with a white dwarf.
The Neutron stage follows the White Dwarf stage of star development.
Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.Then, depending on the remaining mass of the star, it will collapse into a white dwarf, a neutron star (aka pulsar), or a black hole.
A white dwarf is much larger than a neutron star.
* white dwarf * neutron star * black hole
It can be a black hole or a Neutron Star
A black hole, a neutron star, or a white dwarf.
The long-term fate of the sun according to current theories in stellar evolution, is to become a white dwarf. It lacks the mass to further collapse into a neutron star or black hole.
Nebule > Star > Red Giant > Red Dwarf > White Dwarf > Supernova > Neutron Star > Black Hole.
According to current theories of stellar evolution, because of the Sun's mass and chemistry most likely it will become a white dwarf. It simply lacks the weight to become a neutron star or black hole.
No. A neutron star is many times denser than a white dwarf.
its original mass when it formed