It takes several hundred trillion years of a white dwarf to cool.
It is estimated to take at least several hundred trillion years.
There are small hot stars - White dwarfs, neutron stars but by furtue that they are hot, means they are not near the end of their lives. It takes a long long time for all the residual heat to escape into the Universe. So, there are NO hot stars near the end of it's life.
Billions of years - longer than the life of our universe has passed from now (21st century).
A White Dwarf star starts as a small to intermediate size star, like our Sun is currently. That eventually becomes a red giant star. Eventually that blows off everything but the hot very dense core of "electron degenerate matter". What is left is a hot ball of mainly carbon and oxygen that will eventually cool and dim and turn into a black dwarf star. A white dwarf has a second chance of life and death in a close binary star system, where the white dwarf draws mass from the companion star. Once the mass of the white dwarf reaches the Chandrasekhar limit of approximately 1.38 solar masses or roughly 140% of the mass of our Sun, the core can no longer hold the gravitational pressure and a Type 1a Supernova may occur. A Red Dwarf star is a " Main Sequence " star, but with very low mass and luminosity. You need a telescope to see one. However, they make up about 80% of all stars and they have very long lifetimes.
White dwarf stars are calculated to continue emitting energy for incredibly long amounts of time. It is believed that they can do so for longer than the age of the universe, hence, none have cooled off to black dwarf status yet. Some white dwarfs have been found around 100 light years from Earth and are thought to be the oldest known stars at 11 to 12 billion years old.
It is estimated to take at least several hundred trillion years.
In that case, it will basically stop emitting any radiation. No star has had time so far to become a black dwarf - the Universe is too young for that. This is because it takes a white dwarf a long, long time to cool down.
Yes. When they are first created after a "normal" star ends it life, they are white because they are very hot. Over time they will slowly cool and in doing so turn from white to yellow, to orange, then red, brown and eventually black.The cooling process takes billion of years. So long in fact that no white dwarf ever created, has had enough time to cool down completely.
A white dwarf is the remnant of a star that has lost most of it mass. When it is formed it is very hot indeed but, as it now has insufficient mas to carry on fusion, it begins to cool down. For objects as massive as stars, even dwarfs, this cooling down takes a long time but eventually a white dwarf will cool down completely and become a black dwarf. Red dwarfs are never very hot as they have barely sufficient mass to effect fusion so don't do it very vigorously. However the fact that they go about their fusion slowly means they can maintain their meager temperatures for a long long time indeed. Some red dwarfs are older than the calculated age of the universe. (which is an interesting paradox) a nova What this person^^^^^ is really trying to say is that : The hottest star is white dwarf.
All Dwarf hamster are short-haired. The Russian Dwarf, Winter White, Chinese Dwarf, Roborovski's dwarf, etc. The long-haired hamsters are Syrians.
Yes, as long as you do it right.
A brown dwarf will never become a black dwarf. A black dwarf is what becomes of a white dwarf. This process takes hundreds of trillions of years.
None. Nor will there by any for a very long time. In about 7 billion years the sun will become a white dwarf, which ten, over the course of trillions of years, cool to become a black dwarf. At that point our solar system (or what is left of it) will have exactly one black dwarf
Yes, but it will take many, many billions of years. White dwarves no longer produce energy, and will gradually cool down. However, there is a lot of energy in a white dwarf, and a small surface are to dissipate that energy, so it will take very long.
Low to medium mass Stars will become white dwarfs, where the mass is up to 8 solar masses (8 times the mass of our sun). There are two types of white dwarf stars; - low mass stars with a solar mass less than 0.5 will become helium white dwarfs. The temperature of these will not be high enough to fuse helium into carbon. - low to medium stars with a solar mass between 0.5 and 8 will become Carbon-Oxygen white dwarfs. Any star larger than 8 solar masses cannot become a white dwarf.
Based on current theories of stellar evolution, billions of years in the future our Sun will expand to a red giant, shed much of its outer envelope, and become a white dwarf. After this it will probably cool over an extremely long time and likely end up as a black dwarf.
There are small hot stars - White dwarfs, neutron stars but by furtue that they are hot, means they are not near the end of their lives. It takes a long long time for all the residual heat to escape into the Universe. So, there are NO hot stars near the end of it's life.