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What stars burn up hydrogen?
All main sequence stars fuse hydrogen.
What gas is formed when hydrogen atoms fuse?
The gas formed when hydrogen atoms fuse is helium. Stars do this.
How do atoms make stars burn?
The enormous heat and pressure at the center of a star causes atoms to fuse together, releasing enormous amounts of energy. Most stars fuse hydrogen, but larger stars that have exhausted the hydrogen in their cores may fuse heavy elements.
Is helium naturally produced in stars?
Yes, stars fuse Hydrogen atoms to make Helium in a natural process.
How do most stars make light?
Well Stars use 4 atoms of Hydrogen and 1 atom of Helium fuse together.
What does a star primarily burn in its lifetime?
Most stars, for most of their existence, fuse hydrogen into helium.
What stars have left the main sequence?
The main sequence stars are stars that fuse hydrogen, so the stars that have left the main sequence are the ones that have basically run out of hydrogen. They are the Red Giant stars, Supergiant stars and White Dwarf stars.
Is it true stars like the sun burn hydrogen producing helium?
All stars fuse hydrogen into helium - the slight difference in atomic weight between 4 hydrogen atoms and one helium atom, is given off as radiation.
What chemical is inside the sun?
Hydrogen is in the sun, when the hydrogen atoms fuse (join together) they make helium in stars. this gives out lots of heat and light.
Hydrogen atoms fuse and become what?
Hydrogen atoms fuse to become helium atoms during the process of nuclear fusion in stars. This process releases a large amount of energy and is the source of the sun's energy.
What kind of stars are mainly composed of hydrogen?
Main sequence stars, like our Sun, are mainly composed of hydrogen. These stars fuse hydrogen into helium in their cores, releasing energy in the form of light and heat. This process allows them to shine bright in the sky.
What element is formed when hydrogen nuclei fuse together?
When hydrogen nuclei fuse together, they can form helium. This fusion process is the energy source for stars, including our sun, where hydrogen nuclei combine to form helium through a series of nuclear reactions.
