A nebula does not directly turn into a white dwarf. A nebula will collapse to form stars. Low to medium mass stars become white dwarfs after they die.
Some are the result of a supernova and do not collapse, they merely dissipate over time. The Crab Nebula is the most prominent example of this.
After a planetary nebula occurs, the core of the star collapses and becomes a white dwarf. This white dwarf slowly cools down over billions of years until it eventually becomes a cold, dark remnant known as a black dwarf.
A star with a low mass will go through these stages: 1. Protostar nebula 2. Main sequence (as a red dwarf) 3. Red giant 4. Planetary nebula 5. White dwarf (6. Black dwarf is theorized to occur after white dwarf)
The central star of the Ring Nebula is a white dwarf known as HD 229236. It is the remnant core of a low to intermediate mass star that has exhausted its nuclear fuel and shed its outer layers. The white dwarf is hot and compact, surrounded by the colorful nebula that was once its outer layers.
The central star of the Ring Nebula, also known as Messier 57, is a white dwarf. A white dwarf is a dense, compact stellar remnant that is left behind after a star like our Sun exhausts its nuclear fuel and sheds its outer layers.
When a planetary nebula dissipates, what remains is the core of the star that has shed its outer layers. This core, known as a white dwarf, is extremely dense and hot, gradually cooling over billions of years. The planetary nebula itself, which is the glowing gas and dust expelled by the dying star, eventually disperses into space.
A White Dwarf Star remains.
What actually happens to the types of stars is that the low mass will turn into a white dwarf and the medium mass will turn into a black dwarf and reproduce a nebula
Yes, but it can also make a black hole or a white dwarf.
After a planetary nebula occurs, the core of the star collapses and becomes a white dwarf. This white dwarf slowly cools down over billions of years until it eventually becomes a cold, dark remnant known as a black dwarf.
A star with a low mass will go through these stages: 1. Protostar nebula 2. Main sequence (as a red dwarf) 3. Red giant 4. Planetary nebula 5. White dwarf (6. Black dwarf is theorized to occur after white dwarf)
No, the star usually will become a white dwarf or explode .
A white dwarf is the core of a dead star. As the star runs out of fuel, it expands into a red giant, as the shell of the red giant became a planetary nebula, and the core shrinks and became a white dwarf.
The central star of the Ring Nebula is a white dwarf known as HD 229236. It is the remnant core of a low to intermediate mass star that has exhausted its nuclear fuel and shed its outer layers. The white dwarf is hot and compact, surrounded by the colorful nebula that was once its outer layers.
A white dwarf. Basically, a red dwarf just gets cooler and cooler until it has consumed all of its hydrogen. Then it becomes a white dwarf star. It will then dissipate any remaining heat into space and eventually become a "black dwarf".
in the middle of a nebula lies a glowing neutron star or a white dwarf with highly concentrated mass at extremely high densities.
Nebula protostar mid sized star red giant nova white dwarf black dwarf:)
The white dwarf still has a lot of mass ( about 80% of the original star), but it only has a small size( less than two Earths). A huge volume of material forms a nebula which gradually disperses. This type of nebula is (confusingly) called a "planetary nebula".