z_The "THD94H" Red Dwarf
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Owner:
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Landbehrt
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Released:
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Saturday, November 19, 2011
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Origin:
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Québec, Canada
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Recently Spotted:
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Unknown Location
This is not collectible.
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This is a racing Travel Bug. It has to move fast, often and far. Drop it as soon as possible in the most popular caches, easy to find and with easy access. This Travel Bug loves traditional caches and hates mystery caches. And please, DON'T KEEP IT! Thanks!
The name of this Travel Bug is "The "THD94H" Red Dwarf". This is a racing Travel Bug. It has to move fast, often and far. Drop it as soon as possible in the most popular caches, easy to find and with easy access. This Travel Bug loves traditional caches and hates mystery caches. And please, DON'T KEEP IT! Thanks!
According to the Hertzsprung-Russell diagram, a red dwarf star is a small and relatively cool star, of the main sequence, either late K or M spectral type.
They constitute the vast majority of stars and have a mass of less than half that of the Sun (down to about 0.075 solar masses, which are brown dwarfs) and a surface temperature of less than 4,000 K.
Stellar models indicate that red dwarfs are fully convective so that the nuclear fuel hydrogen is constantly remixed to be burned to helium. They therefore develop very slowly, having a constant luminosity and spectral type for some hundreds of billions of years, until their fuel is depleted. Because of the comparatively short age of the universe, no red dwarfs of advanced evolutionary stages exist in the current era.
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