Vogt–Russell theorem

The Vogt–Russell theorem states that the structure of a star, in hydrostatic and thermal equilibrium with all energy derived from nuclear reactions, is uniquely determined by its mass and the distribution of chemical elements throughout its interior.^[1] Although referred to as a theorem, the Vogt–Russell theorem has never been formally proved. The theorem is named after astronomers Heinrich Vogt and Henry Norris Russell, who devised it independently.

References[edit]

^ Carroll, Bradley W. & Ostlie, Dale A. (28 July 2006). An Introduction to Modern Astrophysics (Second ed.). Addison-Wesley. p. 333. ISBN 978-0805304022.

This article about stellar astronomy is a stub. You can help Wikipedia by expanding it.

[1] Carroll, Bradley W. & Ostlie, Dale A. (28 July 2006). An Introduction to Modern Astrophysics (Second ed.). Addison-Wesley. p. 333. ISBN 978-0805304022.

[1]