our Sun will eventually become a red giant and a white dwarf....
Once the sun finishes fusing Hydrogen into helium it will start fusing helium. It will need more pressure to do this so it will expand. But it will cool a little as it expands. It all has to do with equilibrium. Our sun will become a red giant and expand to about half way between earth's orbit and mars' orbit. This will not happen for another 5 billion years or so supposedly since as far as we can tell stars like our sun stay in the main sequence for 10 billion years give or take and our sun is about 5 billion years old or so.
The sun is currently in the main sequence stage. Next, it will evolve into a red giant as it depletes its hydrogen fuel and starts burning helium in its core.
When the Sun exhausts its hydrogen fuel in the core and finishes the main sequence stage, it will enter the red giant phase. During this stage, the core will contract and heat up, causing the outer layers to expand significantly. Eventually, the Sun will shed its outer layers, creating a planetary nebula, while the core will remain as a white dwarf.
After the main sequence stage, a star like the sun will enter the red giant phase where its core contracts and the outer layers expand. This is followed by the helium fusion stage where the star burns helium in its core. Ultimately, the fate of a star depends on its mass, which determines if it will become a white dwarf, neutron star, or black hole.
main sequence
The main sequence stage is a point in the stellar evolution of stars in the universe at which every star converts hydrogen into helium in its cores and releases huge amounts of energy.
its to the right of the middle of the main sequence.
main sequence
The sun is currently in the main sequence stage. Next, it will evolve into a red giant as it depletes its hydrogen fuel and starts burning helium in its core.
red giant
When the Sun exhausts its hydrogen fuel in the core and finishes the main sequence stage, it will enter the red giant phase. During this stage, the core will contract and heat up, causing the outer layers to expand significantly. Eventually, the Sun will shed its outer layers, creating a planetary nebula, while the core will remain as a white dwarf.
A protostar generates energy by friction whereas a main sequence star generates energy by fusion.
A protostar generates energy by friction whereas a main sequence star generates energy by fusion.
Because there not that hot
After the main sequence stage, a star like the sun will enter the red giant phase where its core contracts and the outer layers expand. This is followed by the helium fusion stage where the star burns helium in its core. Ultimately, the fate of a star depends on its mass, which determines if it will become a white dwarf, neutron star, or black hole.
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Main Sequence
The "main sequence".