Respuesta :

Given what we know, we can confirm that the next life cycle phase for a G-type main-sequence star like our Sun after it collapses like a “soufflé” is that of a white dwarf star.

What we know about white dwarf stars.

  • Stars use a balance of gravity and internal forces to stay in their main sequence phase.
  • Then the internal forces diminish as a star uses up all of the fuel it has to produce nuclear fusion.
  • When this happens the star collapses under its own weight and can become a white dwarf.
  • White dwarf stars provide low amounts of light and are extremely dense.

Therefore, we can confirm that once our sun has collapsed onto itself, it will likely become a white dwarf star, packing all of its mass into the size of about our Earth.

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