Astrophysics

Astrophysics is the analysis of the physical structure and evolution of objects studied by means of astronomical observations (e.g., stars, galaxies, radio sources, X-ray sources, quasi-stellar objects). The physical structure of such objects depends on a balance of gravitation, radiation pressure, and centrifugal forces, while their evolution depends on their initial composition and the reactions that take place between matter and radiation. In particular, nuclear reactions create new elements in the interior of stars and provide their major energy source. Detailed analysis discloses important relations between the color of light emitted by a star and its total radiation output; this relation changes with the age of the star. At its life's end, a star may die in a supernova explosion, or it may end up as a white dwarf star, neutron star, or black hole, depending on its mass.

See also ASTRONOMY; BLACK HOLE; COSMOLOGY, PHYSICAL ASPECTS; GRAVITATION

GEORGE F. R. ELLIS