New posts in Stellar Physics

Why do later fusion stages in a star last shorter?

Why does a star die once it has iron?

Can a hydrogen cloud directly collapse to form a black hole?

Can a neutron star become a black hole via cooling?

Is the mass of an individual star almost constant throughout its life?

Why is the Sun called an "average star"?

Why are some stars very large (i.e., $r \geq 1000 \ R_{\odot}$) but not super massive?

How is hydrostatic pressure overcome when a star is formed?

Why is the Sun almost perfectly spherical?

Density of the Sun