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the hydrogen and helium in the sun will continue to thermonuclear fuse until they end up creating lead, collapsing in on itself because of its immense mass.

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What will happen to the relative amounts of hydrogen and helium in the sun over the next few billion years?

Over the next few billion years, the hydrogen content in the sun will decrease as it fuses into helium through nuclear fusion. This process will cause the relative amount of helium to increase in the sun over time.


Why will the sun burn out?

The sun generates energy by fusing hydrogen into helium. Eventually it will run out of hydrogen. However, this won't happen for several billion years.


What will happen to the amounts of hydrogen and helium in the sun over the next few billion years?

well the sun will slowley expand to as much as it could reach earths atomsphere and explode. But hopefully by the next couple of billion years we will have found life on other planets and solar systems.


What will happen to the relative amounts of hydrogen and helium in the sun over the next few years?

Over the next few years, the amount of helium in the sun will gradually increase as hydrogen fuses into helium in its core through nuclear fusion. This process is part of the sun's natural life cycle and will continue until a significant portion of the hydrogen fuel is depleted.


What are the Sun's main atmospheric gases?

The Sun's atmosphere is primarily composed of hydrogen and helium. These two gases make up over 98% of the Sun's total mass. Other gases present in smaller amounts include oxygen, carbon, neon, and iron.


What is The most abundant ingrediant of sun and Jupiter?

(H) Hydrogen makes up the majority of the Sun and Jupiter with small amounts of He (Helium)


What property do hydrogen and helium have in common?

Hydrogen and helium are both present in significant amounts in the universe. They are also both light gases that have low atomic masses.


What substances or elements are the sun made of?

About 70% hydrogen, 28% helium, and the remainder is "trace" amounts of every other element. We believe that the universe was originally mostly hydrogen, with a little helium and a trace of lithium. Over the course of about 10 billion years, generations of stars formed from the hydrogen, fused the hydrogen into helium, and then blew themselves apart in titanic supernova explosions that created, in the instant of the explosion, every element heavier than lithium. Our solar system formed about 4.5 billion years ago, born from the hydrogen gas from space and the dust and debris from every star that lived and died before then.


How is your sun powered?

The Sun is powered by nuclear fusion which requires extremely high temperatures to happen. Hydrogen is fused into helium releasing incredible amounts of energy which is counteracted by gravity.


What types of minerals or gases are found on the Sun?

The Sun primarily consists of hydrogen and helium gases. It also contains small amounts of other elements, such as carbon, oxygen, and nitrogen. The Sun's core is thought to contain heavier elements like iron and nickel, but these are found in trace amounts compared to hydrogen and helium.


What kind of gas is in Jupiter's atmosphere?

Jupiter's atmosphere is primarily composed of hydrogen and helium, with smaller amounts of methane, ammonia, and water vapor. The high concentration of hydrogen and helium gives Jupiter its characteristic colors and properties.


What major gaseous substances are in Jupiter and Saturn?

Jupiter and Saturn primarily consist of hydrogen and helium, with trace amounts of other gases such as methane, ammonia, and water vapor. These gas giants have thick atmospheres that are mostly composed of hydrogen and helium.