A white dwarf who's progenitor star was about the same mass as our Sun will leave behind a stellar remnant around the size of our Earth.
Obviously if the progenitor star was larger or smaller, then the stellar remnant will also be larger or smaller.
A white dwarf has far more mass than any planet. Jupiter is the most massive planet in the solar system and so would be the "closest" in mass to a white dwarf, but it is still hundreds of times lass massive.
Difficult to know for sure. Brown dwarf stars are small and dim, and it's possible that there is one relatively close by that we've never noticed.
The nearest known brown dwarf star is Epsilon Indi Bb, one of two brown dwarf stars orbiting the star Epsilon Indi. It would not be detectable at all if it were not so close to the parent star, and it is possible that there are other solitary brown dwarf stars that are closer. Epsilon Indi is about 12 light-years away.
In fact, there have been suggestions that a brown dwarf star tentatively named "Nemesis" may be distantly orbiting the Sun, occasionally coming close enough to perturb clusters of comets from the Oort Cloud and dropping them into the inner solar system. Nothing like this has been discovered, however, and the idea has been generally discredited.
white dwarf's are stars not just one white dwarfs are a completion of a star so it can be close or far
I'm pretty sure it is Sirius A. It is 8.6 light years (50,556,179,654,736 miles) away. It is also a binary system. It's sister star is Sirius B and it is a white dwarf.
If I am correct it is called sirius b
Aldebaran is a red giant star 65 light years away.
The dwarf planet Eris truly deserves its designation as "dwarf planet"; it is less than one quarter of Earth's diameter, and about one percent of Earth's mass.
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.
Re the radius, what units are the 10.4 in.(A white dwarf is a small star composed mostly of electron-degenerate matter. They are very dense; a white dwarf's mass is comparable to that of the Sun and its volume is comparable to that of the Earth).The density of matter in a white dwarf is, very roughly, 1,000,000 times greater than the average density of the Sun, or approximately 106 grams (1 tonne) per cubic centimeter.There is a limiting mass that no white dwarf can exceed called the Chandrasekhar limit, beyond which electron degeneracy pressure cannot support the object against collapse at which point it turns into a Type 1a supernova.
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.
A yellow dwarf star, is a star on the main sequence that has a temperature range of between 5,200 to 6,000 Kelvin. It has a spectral class of G or possibly F.Our Sun is a yellow dwarf - much as you may not believe it, it is a dwarf compared to other stars!!See related question for a size comparison
No. A white dwarf is the collapsed remnant of the core of a low to medium mass star. It has a mass comparable to that of a star, but is about the size of a small planet.
A white dwarf is the remnant of a low to medium mass star.
A neutron star is smaller, but has a greater mass. A typical white dwarf is about the size of a terrestrial planet. A typical neutron star is a few miles across.
Venus
it is exactly the same as a planet but its diameter and mass are not great enough to be considered a planet.
No. A white dwarf is the remnant of a low to medium mass star.
A white dwarf could not become a red dwarf. A white dwarf is a remnant of a dead star. A red dwarf is a star with a very low mass.
A white dwarf, also called a degenerate dwarf, is a small star composed mostly of electron-degenerate matter. They are very dense; a white dwarf's mass is comparable to that of the Sun and its volume is comparable to that of the Earth.
Not necessarily. A white dwarf is simply the remains of a low to medium mass star that has died. A red dwarf is a low mass star. Since red dwarfs last longer than medium mass stars, one could easily be older than a white dwarf.
Eris with a mass of 1.7×1022 kg.
Venus
white dwarf