White dwarfs become novae when they accrete matter from a companion star's outer layers. This matter builds up on the surface of the white dwarf until a critical temperature and pressure is reached, triggering a runaway nuclear fusion reaction. This explosion releases a vast amount of energy and causes the white dwarf to temporarily brighten significantly.
No. Stars become white dwarfs after dying.
Stars that have ejected a planetary nebula eventually become white dwarfs. These are core remnants of low to medium mass stars that have exhausted their nuclear fuel. White dwarfs gradually cool down over billions of years to become black dwarfs.
Type I novae occur in binary star systems where one star is a white dwarf and the other is a normal star. The white dwarf accretes material from the normal star until it reaches a critical mass, causing a thermonuclear explosion. Type II novae, on the other hand, involve the collapse and explosion of a massive star at the end of its life cycle.
White dwarfs shine for billions of years before they cool completely. As they cool, they become dimmer and eventually fade into darkness, becoming black dwarfs. However, the process of a white dwarf cooling into a black dwarf takes trillions of years.
All white dwarfs do not have about the same mass. White dwarfs vary in mass because the stars they form from are not all the same mass.
No. Stars become white dwarfs after dying.
Stars that have ejected a planetary nebula eventually become white dwarfs. These are core remnants of low to medium mass stars that have exhausted their nuclear fuel. White dwarfs gradually cool down over billions of years to become black dwarfs.
Red dwarfs have not yet evolved into white dwarfs because red dwarfs are much less massive than other types of stars that do become white dwarfs. Red dwarfs are the smallest and coolest stars, and they have not burned through their fuel quickly enough to go through the stage of becoming a white dwarf. It will take billions of years for a red dwarf to cool and fade into a white dwarf.
Stars that become white dwarfs die but become black holes . Neutron stars are born from a Super Nova that stored its energy and became a neutron star.
Black dwarfs. [See related question]
Dying stars eventually shrink into white dwarfs (which as they age eventually become red dwarfs and then brown dwarfs - but this takes an extremely long time).
None of the above. White dwarfs and the black dwarfs they will become consist of a unique state of matter called electron degenerate matter.
They are called white dwarfs because when they form, although not replenishing their energy supply any more, they are still hot enough to shine. Overt time (a long time) however, they will cool down and become 'black dwarfs' which no longer emit light in visible wavelengths.
Those are dwarf stars, which start out as white dwarfs and as they (very slowly) cool, become red dwarfs and eventually brown dwarfs.
Type I novae occur in binary star systems where one star is a white dwarf and the other is a normal star. The white dwarf accretes material from the normal star until it reaches a critical mass, causing a thermonuclear explosion. Type II novae, on the other hand, involve the collapse and explosion of a massive star at the end of its life cycle.
Did Snow White ever had sex with the dwarfs
According to astronomers and authors Jonathan Weiner and Carl Sagan, white dwarfs - which have been an accepted entities by all astronomers for decades - require an amount of time to "cool down" that well exceeds the current age of the universe - hence there hasn't been enough time for any of them to cool down yet and become "black dwarfs".