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Red dwarves have very low mass, less than 40% of that of our own sun. As a result, they have relatively low temperatures in their cores such that energy is generated at a very slow rate through hydrugen fusion into helium. Very little light is emitted, even the largest red dwarf emits less than 10% of that of our sun.

The biggest difference between a red dwarf and our own sun is the total absence of a metallic core.

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Mostly hydrogen, like any other star which is still burning.

wierd shut up


All stars are "mostly hydrogen, with some helium". Most stars have traces of heavier elements, and the exact proportion is different for every star and every stage of the star's life. When stars get large proportions of heavier elements, they are near the end of their lives.
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