When the sun exhausts the hydrogen in its core and become a red giant.
The sun is powered by nuclear fusion in its core, converting hydrogen into helium. Eventually it will run out of hydrogen fuel and start fusing helium, leading to its expansion into a red giant and eventually shedding its outer layers, forming a planetary nebula. This process will happen in about 5 billion years.
Our sun, Sol, uses hydrogen for fuel.
The next stage in the Sun's evolution is the red giant phase. This occurs when the Sun runs out of hydrogen fuel in its core and starts burning helium. During this phase, the Sun will expand and become larger, eventually engulfing Mercury, Venus, and possibly Earth.
Hydrogen is the fuel used by the sun, helium is the waste produced by hydrogen use in the fusion process
Our Sun will eventually become a red giant, not a red supergiant. As it exhausts its hydrogen fuel in about 5 billion years, it will expand and cool, turning into a red giant. A red supergiant, on the other hand, is a larger star that has significantly more mass than the Sun and undergoes a different evolutionary path.
Yes. It will eventually. The sun has enough hydrogen in its core to remain as a main sequence star for about 5 billion years. After that it will alternate between fusing helium in its core and hydrogen in a shell around the core for about 2 billions. Then it will shed its outer layers and leave behind a degenerate remnant called a white dwarf.
Proxima Centauri is a "red dwarf" star. Its composition is similar to the Sun, but with less mass and it's much smaller than the Sun. It has lower core and surface temperatures. The Sun will eventually start to use helium as well as hydrogen as its fuel It will become a red giant then a white dwarf. Red dwarfs don't have a high enough core temperature to use helium as as "fuel". Proxima Centauri will not become a red giant. It will go straight to the white dwarf stage, once it has used up its hydrogen "fuel".
The hydrogen in the Sun is fuel for the nuclear fusion reaction.
As the hydrogen in the sun decreases, helium increases. Eventually, there won't beenough hydrogen remaining to maintain the sun's present rate of energy production.At that point, the sun will undergo drastic changes in its size and energy output that will,first, cook any life remaining on Earth at that time, and eventually, incinerate the Earth itself.
Hydrogen
The sun is powered by nuclear fusion in its core, converting hydrogen into helium. Eventually it will run out of hydrogen fuel and start fusing helium, leading to its expansion into a red giant and eventually shedding its outer layers, forming a planetary nebula. This process will happen in about 5 billion years.
Most scientists believe that the Sun will continue to radiate for another 5 billion years. This is because the Sun is in the middle of its main sequence phase, where it fuses hydrogen into helium. Once the hydrogen fuel runs out, the Sun will evolve into a red giant and eventually become a white dwarf.
Our sun, Sol, uses hydrogen for fuel.
It will run out of hydrogen fuel eventually, so will die. Not for a few billion years yet though scientist reckon.
By that time earth will be no more:c, but just to answer your question, it will eventually become a black dwarf.
no hydrogen is not affected by the sun because hydrogen can be combined with helium it creates a fuel source but it is not affected by hydrogen by it self so no hydrogen is not affected by the sun
The expectation is that some day in the (to us) far future, most of the hydrogen in the sun will have been converted to helium (and higher weight atoms). At that point, the sun will be "exhausted" since the energy of the sun comes primarily from the fusion of the hydrogen - when there is no hydrogen left to fuse, the sun will have run out of "fuel".