Hermann von Helmholtz

Definition and stakes

Portrait of Edmund Taylor Whittaker Edmund Taylor Whittaker A History of the Theories of Aether and Electricity (1910)

This energy may be either dissipated as heat in conformity to Joule's law, or otherwise utilized in the outer circuit.
The importance of these principles was emphasized by Hermann von Helmholtz (b. 1821, d. 1894) , in a memoir which was published in 1847, and which will be more fully noticed presently, and by W. Thomson (Lord Kelvin) in 1851 [32] ; the equations have subsequently received only one important modification, which is due to Helmholtz.
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Arthur Berry A Short History of Astronomy (1898)

The obvious explanation of the sun as a furnace deriving its heat from combustion is found to be totally inadequate when put to the test of figures, as the sun could in this way be kept going at most for a few thousand years. The explanation now generally accepted was first given by the great German physicist Hermann von Helmholtz (1821–1894) in a popular lecture in 1854. The sun possesses an immense store of energy in the form of the mutual gravitation of its parts; if from any cause it shrinks, a certain amount of gravitational energy is necessarily lost and takes some other form.
Source: Wikisource

Portrait of Hermann von Helmholtz Hermann von Helmholtz On the Conservation of Force

All change in nature amounts to this, that force can change its form and locality without its quantity being changed. The universe possesses, once for all, a store of force which is not altered by any changed of phenomena, can neither be increased nor diminished, and which maintains any change which takes place on it.
You see how, starting from considerations based on the immediate practical interests of technical work, we have been led up to a universal natural law, which, as far as all previous experience extends, rules and embraces all natural processes
Source: Wikisource

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