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Stars fuse Hydrogen into heavier elements (main sequence stars fuse hydrogen into helium).

If you were to weigh the mass of the hydrogen before the fusion process and the mass of the helium which is the result of the helium process then you would find the the helium has less mass than the hydrogen.

This lost mass is converted into energy (heat and light) in the core of the star in line with Einstein's famous equation E-MC2, where E= the energy that comes out and M= the mass lost and C2 is the speed of light in a vacuum (299,792,458 metres per second,) multiplied by itself.

Our sun loses mass a the rate of 4.26 million metric tons per second so if you multiply this by C2 you can see just how much energy the sun is producing each second. (384.6 yotta watts (3.846×1026

W), or 9.192×1010 megatons of TNT per second).

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