Question

place the events that occur at the end of a solar - mass stars life in chronological order, starting with when the star depletes all hydrogen in its core and ending with an object of temperature close to 0 k. core hydrogen depleted inert carbon core (white dwarf) becomes visible double - shell burning of hydrogen and helium helium fusion begins in core final stages of mass loss via stellar winds planetary nebula dissipates away black dwarf temperature close to 0 k

Explanation:

When a solar - mass star depletes core hydrogen, helium fusion starts in the core. Then double - shell burning of hydrogen and helium occurs. As the star evolves, it loses mass via stellar winds in the final stages. After that, the planetary nebula dissipates, the inert carbon core (white dwarf) becomes visible, and eventually, it cools to a black dwarf with a temperature close to 0 K.

Answer:

1. Helium fusion begins in core
2. Double - shell burning of hydrogen and helium
3. Final stages of mass loss via stellar winds
4. Planetary nebula dissipates away
5. Inert carbon core (white dwarf) becomes visible
6. Black dwarf