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We can't be sure, because low-mass stars are very dim, and we can't see them. They "live" darn near forever. We think there are very great number of them, but because we can hardly detect them, we can't be sure. In fact, the IAU recently tripled their estimate of the number of stars in the universe, because of the difficulty of seeing brown-dwarf stars.

There are probably relatively few very high mass stars at any one time; high-mass stars burn very brightly, can be seen from very great distances, and die very early - and messy! - deaths, in supernova explosions.

If I had to guess - and this is ONLY a guess! - I would guess that 85% of all stars are low mass, 1% or fewer are "high mass", and the remaining 14% are in that vague middle.

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14y ago

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