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brown dwarf star (s) (noun), brown dwarf stars (pl)
A gaseous body or object smaller in mass than a star, but larger than a planet and heavier than a star..
2. An object less massive than a star, but heavier than a planet: A brown dwarf star is a theoretical "star" and does not have enough mass to ignite nuclear reactions at their centers, but shine by heat released during their contraction from a gas cloud.

Some astronomers believe that vast numbers of brown dwarf stars exist throughout the galaxy, but because of the difficulty in detecting them, none of them were discovered until 1995, when U.S. astronomers discovered a brown dwarf, in the constellation Lepus (Hare).

This entry is located in the following unit: Astronomy and related astronomical terms (page 5)