Final answer:
A brown dwarf is an object intermediate between a planet and a star, with not enough mass to begin nuclear reactions in its core. It falls within a specific mass range and is capable of deuterium fusion, but not hydrogen fusion.
Step-by-step explanation:
A brown dwarf is a celestial object intermediate in size between a planet and a star. It has not enough mass to begin nuclear reactions in its core, so it falls between the mass range of about 1/100 of the mass of the Sun up to the lower mass limit for self-sustaining nuclear reactions, which is about 1/12 the mass of the Sun. Brown dwarfs are capable of deuterium fusion, but not hydrogen fusion, making them different from true stars.