Concept
Nuclear fusion — where it appears
The joining of light nuclei into heavier ones, releasing the difference in binding energy. In a star it is regulated by a thermostat — expansion cools the core when the rate rises — which fails only where the pressure has stopped depending on the temperature.
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
The furnace that runs cooler than a compost heap
The Sun's core produces 276 watts per cubic metre. A human body produces more. The Sun is bright because it is enormous, and its fusion is astonishingly slow — which is exactly why it lasts.
A star is held up by its own weight
A star has a central temperature because it has a central pressure, and it has a central pressure because everything above is pressing down. The nuclear reactions do not set that temperature — they obey it.
Named alongside it
The objects these essays reach for when they reach for this one.
Binding energyCNO cycleEddington limitEffective temperatureGravitational potentialHydrostatic equilibriumMain sequenceMetallicityProton proton chainQuantum tunnellingStellar radius