Sky Matters: Without thermonuclear fusion there is no me — or you

Calculations revealed that the enormous energy emitted by the Sun requires the fusion of four million tonnes of hydrogen into helium every second — but the Sun is big enough to do this for an incredible 10 billion years.
There has been a lot of news coverage recently about “thermonuclear fusion” following a successful demonstration of its capabilities at the Lawrence Livermore laboratories in the US.
Fusion is a process whereby hydrogen nuclei are smashed together at super-high temperatures of around 15 million centigrade, causing them to stick together (or “fuse”). The hydrogen is also converted to helium in the process and furthermore the process releases energy.