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The energy from stars, like our Sun, comes from a process called nuclearfusion. In the star’s core, hydrogen changes into helium, creating energy. A star can do this for millions or billions of years. When the hydrogen runs out, the star starts fusing helium into heavier elements like carbon and oxygen. It continues to change fuels until it reaches iron.
As these fusion processes happen, the star’s layers change. In older stars, the outer layer often has leftover hydrogen. Inside, there are layers of helium, carbon, and oxygen, ending with an iron core.
When the star runs out of silicon and sulfur, fusion stops. This happens because fusing iron and heavier elements does not create energy. Low-mass stars, like our Sun, stop shining and become cinders. Heavy stars go through a supernova, a powerful explosion. Gravity takes over, collapsing the star’s mass. The core becomes a neutron star or a black hole, while outer layers are blown away, possibly forming new stars or planets.
In 2021, a supernova named SN2021yfj surprised researchers. It showed all its layers had been expelled before exploding. Scientists are trying to understand how this happened.