* Gravity: The immense mass of the sun creates an incredibly strong gravitational pull, trying to crush the sun inwards.
* Nuclear Fusion: The intense heat and pressure at the sun's core cause hydrogen atoms to fuse into helium, releasing a tremendous amount of energy that pushes outwards.
This balance, known as hydrostatic equilibrium, keeps the sun stable. The outward pressure from nuclear fusion perfectly counteracts the inward pull of gravity, preventing the sun from collapsing in on itself.
Here's a simplified breakdown:
1. Gravity tries to squeeze the sun.
2. Squeezing creates heat and pressure.
3. Heat and pressure cause nuclear fusion.
4. Nuclear fusion releases energy that pushes outwards.
5. Outward pressure balances gravity.
This delicate equilibrium is what allows the sun to shine steadily for billions of years.