An average star, which is what our sun is, will actively fuse hydrogen into helium for a few billion years (exact time varies based on mass), then it slowly expands int a giant star. Then, the star's outer layer of gases puff off and become a planetary nebula, where its hot core is exposed as a white dwarf. The star reddens and cools, then stops burning and becomes a black dwarf.
Yes, Nebula's die. They die when they get to close to Black Holes.
As the universe ages, interstellar space undergoes significant changes due to stellar processes. Stars form, evolve, and eventually die, often in supernova explosions that enrich the interstellar medium with heavy elements. This enrichment facilitates the formation of new stars and planetary systems, while the expansion of the universe leads to an increasing distance between galaxies. Over generations, the composition and density of interstellar space evolve, influencing star formation rates and the overall structure of galaxies.
Stars will either grow brighter just before they go out, if they supernova, or they will evolve into white dwarfs, which slowly fade into black dwarfs over the course of billions of years. Most likely what you saw was caused by atmospheric refraction; similar to a mirage.
A high mass protostar will eventually evolve into a massive star like a red supergiant, followed by a supernova explosion. After the supernova event, the remnants may form a neutron star or a black hole.
The mass of a star is the fundamental quality that indicates its ultimate fate. A star's mass determines whether it will end its life as a white dwarf, neutron star, or black hole. More massive stars are likely to undergo supernova explosions and collapse into neutron stars or black holes, while lower-mass stars will evolve into white dwarfs.
the answer is white dwarf
The main sequence stage of a sunlike star typically lasts for about 10 billion years. It is during this stage that the star fuses hydrogen into helium in its core, maintaining a balance between the force of gravity pulling in and the energy produced by nuclear fusion pushing out.
When a sunlike star exhausts its hydrogen fuel, it expands into a red giant. During this phase, the star's core contracts and heats up, allowing helium fusion to begin. As it expands, the outer layers cool and become more luminous, giving the star its red appearance. Eventually, the outer layers are ejected, leaving behind a hot core that becomes a white dwarf.
What causes star to evolve is mass.
A sunlike star goes through the following stages in its life cycle: nebula, protostar, main sequence star, red giant, planetary nebula, and finally white dwarf. During the main sequence stage, the star fuses hydrogen into helium in its core, releasing energy. Once it exhausts its hydrogen fuel, it expands into a red giant before shedding its outer layers to form a planetary nebula. The remaining core becomes a white dwarf, cooling down over billions of years.
take care of it and what to evolve into a : toddler - 1 hour teen - 1 day adult - 1 day oldie - ? ( they've not yet got one they all die )
i don't think you can get him/her on your Tamma music star . sorry
You have to go to Luminous Springs to evolve any pokemon. Buneary requires a 2 star IQ to evolve
A large, compact star is typically a white dwarf, neutron star, or black hole. White dwarfs are the remnants of low to medium mass stars, neutron stars are the ultra-dense cores left behind after a supernova explosion of massive stars, and black holes are the collapsed cores of massive stars with gravity so strong that not even light can escape.
After a supergiant star, the star can evolve into a supernova, which is a massive explosion that signals the end of the star's life. Depending on the mass of the star, it can then collapse into a neutron star or a black hole.
All I know is that you need to use an item to evolve Rioulu
yes fire-star will die