A Red GIant.
Stars like our sun and hydrogen bombs produce energy through nuclear fusion.
No, not all stars turn hydrogen into helium. Stars like our Sun do convert hydrogen into helium through nuclear fusion in their cores. However, more massive stars can undergo further fusion reactions involving helium, producing heavier elements like carbon, oxygen, and even iron.
Massive Stars Use Their Hydrogen Much Faster Than Stars Like The Sun Do.
The two main elements in stars are Hydrogen and Helium. Stars start out as mostly Hydrogen and produce Helium. There are less amounts of heavier elements like Oxygen, Neon and Iron in stars
When hydrogen stocks run out
No, carbon was not the first atom created after the Big Bang. The first atoms that formed were hydrogen and helium, and heavier elements like carbon were produced later through processes like stellar nucleosynthesis in the cores of stars.
Yes, stars have cores where nuclear fusion reactions occur. This is where the immense pressure and temperature allow hydrogen atoms to fuse into helium, releasing energy in the form of light and heat. The core is the hottest and densest part of a star.
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.
Stars like the sun become red giants as they exhaust their core hydrogen fuel, causing the core to contract and the outer layers to expand. This expansion results in the outer layers cooling and emitting more red light, hence the term "red giant." The star's outer envelope eventually expands to a point where it engulfs the inner planets in the solar system.
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.
The first stars are called population III stars as they were the first stars created - about 400 million years - after the big bang. They consisted of hydrogen and helium only (and maybe a small amount of lithium) and would have been massive. As such, their lifespan would only have been in the millions of years, rather than the billions of years for the current population I stars (Like our Sun). To date, no population III stars have been observed and thus have not been named.
Stars' energy comes from the fusion of hydrogen atoms into helium atoms, initially.