Nothing, there is no astronomy at Stonehenge, just a single alignment. So no headaches there then!
The next nuclear fusion cycle after helium fusion in a massive star is carbon fusion. This process involves fusing helium nuclei to form carbon. Carbon fusion typically occurs in the core of a massive star after helium fusion is completed.
a star with 2-3 stellar masses would become a red supergiant then a supernova and then become a neutron star.
At the end of its life cycle, a large mass star undergoes a supernova explosion after exhausting its nuclear fuel. This explosion disperses the outer layers of the star into space, while the core collapses under gravity, potentially forming a neutron star or a black hole. The remnant can have a profound impact on its surroundings, enriching the interstellar medium with heavy elements and triggering the formation of new stars.
mass
The stages in a star's life cycle are: formation from a nebula, main sequence (where it fuses hydrogen into helium), red giant or supergiant phase, depending on the star's mass, and finally either collapse into a white dwarf, neutron star, or black hole. This life cycle is accurate for most stars, including our Sun.
Nobody "invented" it, the life cycle of stars happens naturally.
The next nuclear fusion cycle after helium fusion in a massive star is carbon fusion. This process involves fusing helium nuclei to form carbon. Carbon fusion typically occurs in the core of a massive star after helium fusion is completed.
What is capella star life cycle
The "star life cycle" refers to stars. Earth is not a star.
a star with 2-3 stellar masses would become a red supergiant then a supernova and then become a neutron star.
Our Sun is in the hydrogen fusion cycle of an average, mid-size, main sequence star. I have no idea what state YOUR Sun happens to be in.
No, a protostar is basically the BEGINNING of a star's life cycle.
Life cycle of a sun like star. A sun like star will start out as a nebula to a protostar to a main sequence star to a red giant and into a white dwarf and will simply fade out.
At the end of its life cycle, a large mass star undergoes a supernova explosion after exhausting its nuclear fuel. This explosion disperses the outer layers of the star into space, while the core collapses under gravity, potentially forming a neutron star or a black hole. The remnant can have a profound impact on its surroundings, enriching the interstellar medium with heavy elements and triggering the formation of new stars.
The "protostar". That's not classed as a true star, but I think that's the answer.
its mass
A dog.