The sun keeps shining and throwing out masses of heat, and calculations show that the fusion of hydrogen to form helium would enable it, and other stars, to keep going for billions of years. Of course we can't get there to examine it closely, but I think the evidence is mainly based on not being able to account for it any other way. Try the question in 'Sun and Stars' category to see if an astronomer can give you a better answer.
No, it is not possible to manufacture helium. Helium is a naturally occurring element that is produced through the process of nuclear fusion in stars.
A star primarily possesses nuclear energy in the form of fusion reactions occurring in its core. This fusion process converts hydrogen into helium, releasing large amounts of energy in the form of radiation, heat, and light.
The Sun is a massive ball of plasma that shines due to nuclear fusion reactions occurring in its core, releasing energy in the form of light and heat.
Sun's energy is primarily the result of nuclear fusion reactions occurring in its core. These reactions fuse hydrogen atoms together to form helium, releasing a large amount of energy in the process. This energy is what powers the Sun and provides light and heat to our solar system.
The Sun's energy comes from nuclear fusion reactions occurring in its core. This process involves the combining of hydrogen atoms to form helium, releasing vast amounts of energy in the form of light and heat.
How can temperature either help fusion to occur or prevent fusion from occurring?
Nuclear fusion
Yes, a red giant is a stage in the life cycle of a star where fusion reactions are occurring in its core. The core of a red giant star typically consists of helium undergoing fusion into heavier elements like carbon and oxygen.
Double fertilization + syngamy occurring in angiosperms is called triple fusion.
The sun is currently a main sequence star.
Nuclear fusion: mainly of hydrogen into helium. To a lesser extent there is fusion of helium into larger elements - all the way to iron.
The very center of the core, where nuclear fusion is occurring; millions of degrees.
Primarily stars, more specifically stars where fusion is occurring.
The energy output of the sun can be estimated based on the rate of nuclear fusion occurring in its core. This energy output is crucial for sustaining life on Earth and understanding the sun's role in the solar system.
Creation of synthetic elements in the laboratory is not based on nuclear fusion.
You would look for high-energy electromagnetic radiation like gamma rays emitted from the star. This type of radiation is produced during nuclear fusion reactions when light atomic nuclei combine to form heavier nuclei and release energy. Detection of gamma rays can provide evidence that nuclear fusion is taking place in the core of a star.
Like all stars, Betelgeuse emits light because it is very hot. The heat for that light comes from nuclear fusion reactions occurring in the star. Unlike in most other stars, the fusion is occurring in a shell around the core rather than in the core itself.