The Origin of Heat Energy On Earth
Earth's proximity to the Sun is the reason that almost everything near Earth's surface is warm with a temperature substantially above absolute zero. Solar radiation constantly replenishes heat energy that Earth loses into space and a relatively stable state of near equilibrium is achieved. Because of the wide variety of heat diffusion mechanisms (one of which is black-body radiation which occurs at the speed of light), objects on Earth rarely vary too far from the global mean surface and air temperature of 287 to 288 K (14 to 15 °C). The more an object's or system's temperature varies from this average, the more rapidly it tends to come back into equilibrium with the ambient environment.
Read more about this topic: Thermal Energy
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—Robert Frost (1874–1963)
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—David Hume (1711–1776)
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—Philip Dormer Stanhope, 4th Earl Chesterfield (1694–1773)
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—Friedrich Nietzsche (1844–1900)