SOFF X · AIHujjatingizni AI yaratsinSovg'ani olingMahsulot tavsifi
Protostars form from dense regions of gas and dust, collapsing under gravity and heating up as they gather more material. Once a protostar reaches a critical temperature and pressure, nuclear fusion ignites, converting hydrogen into helium and releasing energy. The majority of stars, including our sun, are main sequence stars, where the force of gravity is balanced by the energy produced through fusion.
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