The coolest true stars are thought to have surface temperatures
around 2,600 K. One example of such a star is Gliese 105C,
imaged by the Hubble Space Telescope in 1995.
The main factor determining a star's surface temperature is its
mass. Theory puts the lower mass limit for a star at 8% the Sun's
mass. Below this limit, it is impossible for the centre of a clump
of gas contracting under gravity to heat up sufficiently for
spontaneous nuclear fusion to start and maintain itself.
Potential stars that fail because their mass is below this limit are
called brown dwarfs. Gliese 105C appears to be a true low-mass
star, and not a brown dwarf. Its mass is put at 8-9% of the Sun's.
Gliese 105C is the binary companion of larger star, Gliese 105A,
also known as HD 16160.
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