During this stage, the sun will remain on the main sequence by burning hydrogen in a shell around the inert helium core, but the changes in its internal structure set the stage for a dramatic transformation. The remaining core, composed primarily of carbon and oxygen, will collapse under gravity but will be prevented from becoming a neutron star or black hole due to its low mass.
Sun Future Heat Devastation Earth: What Happens When the Sun Dies Out
6 billion years, the star has approximately 5 to 6 billion years of stable energy production remaining before the core hydrogen is exhausted. It will shed layers of its outer atmosphere into space, creating a spectacular cloud of gas and dust known as a planetary nebula.
The nebula disperses the elements necessary for future star and planet formation, continuing the cosmic cycle of life. 4 billion years from now.
Sun's Future Heat: Earth's Devastation When the Sun Leaves the Main Sequence
Instead, it will stabilize as a dense, hot remnant known as a white dwarf. The Main Sequence: Our Sun's Prime Currently, the sun is in a stable phase known as the main sequence, where it fuses hydrogen into helium in its core.
More About When will the sun die out
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