Nebulae are associated with the end of a star's life cycle, as they are shells matter that blown off a star, usually in a series of events, when a star is in its death throws.
The starting nebula of a medium star cycle and a large star cycle differs primarily in mass and density. Medium stars, like our Sun, typically form from nebulae that have a lower mass and are less dense, allowing for a more gradual accumulation of material. In contrast, large stars originate from more massive and denser nebulae, which can lead to a faster and more violent formation process. This difference in initial conditions influences their subsequent life cycles and eventual fates.
Nebulae (gas and dust) protostar (formed by immense pressure in nebulae) ^ becomes either a Brown dwarf (basicall dead :P) or a Main sequence star which becomes: A Red giant (when MSS runs out f hydrogen ) if red giant is small it becomes a white dwarf and does nothing or a planetary nebulae if it's a big one it either becomes a Neutron star or a Black hole
The first stage in a star's life cycle is the nebula stage, where a cloud of gas and dust in space begins to collapse under its own gravity. This collapse leads to the formation of a protostar, which will eventually become a full-fledged star through nuclear fusion.
No, a protostar is basically the BEGINNING of a star's life cycle.
Nebulae are star factories because they are vast clouds of dust and gas in space that can collapse under their own gravitational forces, leading to the formation of new stars. Within nebulae, gas and dust particles come together to form protostars, which eventually evolve into full-fledged stars through the process of nuclear fusion. This ongoing cycle of star formation within nebulae replenishes galaxies with new stars and contributes to the overall creation and evolution of stellar systems.
A nebula is a cloud of gas (hydrogen) and dust in space. Nebulae are the birthplaces of stars.
The starting nebula of a medium star cycle and a large star cycle differs primarily in mass and density. Medium stars, like our Sun, typically form from nebulae that have a lower mass and are less dense, allowing for a more gradual accumulation of material. In contrast, large stars originate from more massive and denser nebulae, which can lead to a faster and more violent formation process. This difference in initial conditions influences their subsequent life cycles and eventual fates.
What is capella star life cycle
The "star life cycle" refers to stars. Earth is not a star.
Nebulae (gas and dust) protostar (formed by immense pressure in nebulae) ^ becomes either a Brown dwarf (basicall dead :P) or a Main sequence star which becomes: A Red giant (when MSS runs out f hydrogen ) if red giant is small it becomes a white dwarf and does nothing or a planetary nebulae if it's a big one it either becomes a Neutron star or a Black hole
The first stage in a star's life cycle is the nebula stage, where a cloud of gas and dust in space begins to collapse under its own gravity. This collapse leads to the formation of a protostar, which will eventually become a full-fledged star through nuclear fusion.
Planetary Nebulae
Nebulae (gas and dust) protostar (formed by immense pressure in nebulae) ^ becomes either a Brown dwarf (basicall dead :P) or a Main sequence star which becomes: A Red giant (when MSS runs out f hydrogen ) if red giant is small it becomes a white dwarf and does nothing or a planetary nebulae if it's a big one it either becomes a Neutron star or a Black hole
No, a protostar is basically the BEGINNING of a star's life cycle.
Nebulae are star factories because they are vast clouds of dust and gas in space that can collapse under their own gravitational forces, leading to the formation of new stars. Within nebulae, gas and dust particles come together to form protostars, which eventually evolve into full-fledged stars through the process of nuclear fusion. This ongoing cycle of star formation within nebulae replenishes galaxies with new stars and contributes to the overall creation and evolution of stellar systems.
They are created by nebulae.
Planetary Nebula are the outer layers of a star that are lost when the star changes from a red giant to a white dwarf. A star is a luminous globe of gas producing its own heat and light by nuclear reactions (nuclear fusion). They are born from nebulae and consist mostly of hydrogen and helium gas.