Most stars, for most of their existence, fuse hydrogen into helium.
The larger a star the shorter the lifetime because, larger stars burn out more quickly.
The mass of the star. The bigger it is, the faster it will burn through its fuel supply.
It will burn out eventually, but that will be very far from now, not in our lifetime.
When a star is at the end of its lifetime its mass increases.
Nothing that you will notice in your lifetime . In millions of years, the sun , being a star will first expand , burning up the earth and then reduce and burn out.
Stellar evolution is the term for the changes a star undergoes during its lifetime.
Burn time is time from power on to power off, but the lifetime is time from the first using to not available.
The life of a star depends on the amount of hydrogen a star has left. Simple answer the larger the star the shorter the life span for example: stars like our Sun can be expected to live 8-12 billion years a more massive star like Beetlegeuse can expect to live 100-400 million years and the most massive stars like S. Doradus and VY Canis Majoris can expect to live just a few million years. The larger the star the more fuel it consumes. Due to contrary belief not all stars burn hydrogen some stars burn helium others burn carbon some even burn oxygen this is all based off the core temperature the hotter the core the more elements it can burn
When a star is at the end of its lifetime its mass increases.
The mass of the star
The chemicals (usually hydrogen and helium) that fuel the reactions in the star that creates heat and light have a finite lifetime. Our own sun is expected to only last for about another 6,000 years.
The chemicals (usually hydrogen and helium) that fuel the reactions in the star that creates heat and light have a finite lifetime. Our own sun is expected to only last for about another 6,000 years.