The steps in a low-mass star evolution are the main sequence, red giant, nebula, and a white dwarf.
What is a star?
This is a type of celestial body composed of gas that differs from other celestial bodies due to their composition and constant fusion processes. This constant fusion causes stars to change or evolve.
How do low-mass stars evolve?
The steps in their evolution include:
- Main sequence: This is the first stage of evolution and in this stage, stars are considered simply average stars. Due to this, this is usually the longest phase.
- Red giant: After billions of years of fusion, the helium of the star expands, this leads to the general expansion of the star that is composed of a carbon core surrounded by a layer of hydrogen.
- Nebula: Gravity pulls hydrogen and this causes hydrogen to sping, which changes the appearance of the star.
- White dwarf: This is considered the final stage and in this stage, only the core remains.
Note: This question is incomplete because the steps are missing; due to this, the answer is based on general knowledge.
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