Stars evolve to the upper left along the main sequence, after forming in the middle.
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Q7: A stage 4 protostar may temporarily be
Q8: Rotation causes the cocoon of dust to
Q9: Magnetic fields enhance the collapse of a
Q10: It takes about 1032 hydrogen atoms to
Q11: As a protostar evolves from stage 4
Q13: A protostar of 20 solar masses will
Q14: Brown dwarfs most commonly form in the
Q15: Rotation of the protostar helps generate the
Q16: Many of the brightest stars we see
Q17: Collisions between galaxies tend to destroy, not
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