Every red dwarf star that ever joined the main sequence is still there today.
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Q14: When a star becomes a red giant,
Q15: All planetary nebulae are slowly expanding spherical
Q16: The shell ejection in making a planetary
Q17: Low mass stars should produce white dwarfs,
Q18: The Sun will get brighter in the
Q20: Eventually, all low mass stars will become
Q21: Refer to the figure above. What is
Q22: What is a planetary nebula?
A)the bipolar jets
Q23: At which stage in a Sun-like star's
Q24: What spectral type of star that is
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