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physics astrophysics (astrophysics (the solar system (the sun (clouds of…
physics astrophysics
astrophysics
the solar system
the sun
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main sequence
Materials continued to collide (come together) until the temperature and pressure were high enough for hydrogen nuclei to start fusing and form helium (in nuclear fusion).
The star then went into a stable period, called a ‘main star sequence’.
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stable
The Sun is still in its stable main sequence phase.
In this phase, the outward force of the energy released by nuclear fusion is balanced by the force of gravity pulling the Sun inwards.
the sun is at the centre of the solar system. planets, moons, asteroids and comets orbit the sun
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