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A star is a massive, compact body of plasma in outer space that is currently producing or has produced energy through nuclear fusion. The most familiar and closest star to the Earth is the Sun. Unlike a planet, from which most light is reflected, a star emits light because of its intense heat. Stellar astronomy is the study of stars.

Individual stars differ from each other due to their total mass, their composition, and their age. The total mass determines the course of evolution of a star, as well as its eventual fate. A Hertzsprung-Russell diagram shows the pattern of the temperature of stars against their absolute magnitude, and can be used to determine the overall age of a star and the stage in its evolution. Initially, stars are composed primarily of hydrogen, with some helium and heavier trace elements that determine the metallicity of a star. Over the course of a star's evolution, a portion of the hydrogen is converted into heavier elements through the process of nuclear fusion. Part of the matter is then recycled back into the interstellar environment, where it is used to form a new generation of more metal-rich stars.

Multi-star systems consist of two or more stars that are gravitationally bound, and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution. For example, a nova occurs when a white dwarf accretes matter from a companion star.

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Research Plus: Brown Dwarf - Online encyclopedia article.
Meta Description: [ Brown Dwarf, type of body in space that is smaller than a star but more massive than a planet. Brown dwarfs do not have enough mass to start... ]

A Brown Dwarf Solar flare - Article on the surprise solar flare of a brown dwarf star detected by NASA's Chandra X-ray Observatory.

500 Accreting White Dwarfs - Deep research from the TeSRE Institute - an Italian body who analyze observations in the IR, optical, X-ray and gamma ray energy bands.

Astronomy 162: White Dwarfs and Novae - Short on text, but contains excellent images, diagrams and a table of the brightest white dwarfs

Chandra X-Ray Observatory: Brown Dwarf Stars - Introduction and data on brown dwarf stars.

Coronae of Dwarf Stars - Highly mathematical explanation of how to calculate the coronae of dwarf stars.

Cosmic census finds universe full of brown dwarfs - Details the surprising amount of brown dwarf stars in the universe. CNN article
Meta Description: [ Once considered rare, brown dwarves populate the cosmos with surprising regularity, according to astronomers studying the elusive objects, which occupy a limbo between stars and planets. ]

Echelle Spectra for White Dwarfs - Contains final processed IUE SWP echelle spectra for all 55 hot white dwarfs

404 European Workshop on White Dwarfs - Conference in Kiel, Germany in July 19-23, 2004. Tentative topic list and contact information.

NASA: White Dwarfs Introduction - Easy to understand and includes images
Meta Description: [ This site is intended for students age 14 and up, and for anyone interested in learning about our universe. ]

Royal Observatory Greenwich: White Dwarfs - Explains stellar stability and evolution, electron degeneracy, the observation and evolution of white dwarfs, and the white dwarf Sirius B.

500 White Dwarfs Lecture - The origin and general characteristics of white dwarfs. High School level.

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