A nova is a cataclysmic nuclear explosion caused by the accretion of hydrogen onto the surface of a white dwarf star. Nova are not to be confused with Type Ia supernovae which do explode [See Link]
Yes, when a star undergoes a nova, it expels material into space, which can eventually form a white dwarf. A white dwarf is the remnant core of a star that has exhausted its nuclear fuel and collapsed under gravity. Novae are different from supernovae, which are more energetic and can leave behind other remnants like neutron stars or black holes.
No. It is not nearly massive enough. When the sun dies it will leave behind a remnant called a white dwarf.
No. When the sun dies it will expel its outer layers in a series of gradual pulses and leave behind a white dwarf.
After a low-mass or medium-mass star dies, it will typically leave behind a remnant called a white dwarf. A white dwarf is a dense, Earth-sized core made primarily of carbon and oxygen. It gradually cools and fades over billions of years.
No, a dead star is different from a black dwarf. A black dwarf is a type of stellar remnant, but not all stars become black dwarfs. When a star dies it will leave behind a white dwarf, a neutron star, or a black dwarf as a remnant depending on its mass. Given enough time a white dwarf will eventually cool to a black dwarf. The universe is not old enough for this cooling to have happened yet.
A white dwarf supernova occurs when a white dwarf star in a binary system accretes material from a companion star, causing it to exceed the Chandrasekhar limit (1.4 solar masses). The core then undergoes a runaway nuclear fusion reaction, leading to a catastrophic explosion that destroys the white dwarf.
The Sun will leave behind a white dwarf as its final stellar corpse. After exhausting its nuclear fuel, it will shed its outer layers, creating a planetary nebula, while the remaining core will cool and shrink to form the white dwarf. This dense, Earth-sized remnant will eventually fade away over billions of years, ultimately becoming a cold, dark object known as a black dwarf, though the universe is not old enough for any black dwarfs to exist yet.
An average star like our sun will eventually become a red giant as it exhausts its nuclear fuel. After that, it will shed its outer layers to form a planetary nebula and leave behind a dense core called a white dwarf.
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.
Generally yes, however in some rare cases such as yellow supergiants, they will explode as a supernova and leave behind, either a black hole or a neutron star.
The white trails left behind jets are known as contrails.
Neutron Star