Math 2.0

Astronomy and astrophysics Star formation and the interstellar medium Concept

Initial mass function

Summary

The initial mass function describes how the masses of stars are distributed when a population of stars is born. It is a density on the range of stellar masses, usually normalised to the number or to the total mass of stars. Above about one solar mass it is close to a power law, with many more low-mass stars than high-mass stars. It sets how much light, how many supernovae and how much chemical enrichment a stellar population produces.

Further reading

  1. Web https://en.wikipedia.org/wiki/Initial_mass_function
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Changed3 November 2026

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