On the surface of the earth the sunlight has had to pass through the atmosphere, and in perfectly bright sunshine it is estimated that only three-fifths of the heat is transmitted. Any surface is also radiating out into surroundings which are at about 300° absolute. Taking into account these two facts, we find that the upper limit to a non-conducting surface in full sunshine on the earth is about 365° absolute, or only a few degrees less than the boiling point of water. +Effective Temperature of Space.+--The last problem we will attack by means of the fourth power law is the estimation of the effective temperature of space, _i.e._ the temperature of a full absorber shielded from the sun and far away from any planet. It is estimated by experiment that zenith sun radiation is five million times the radiation from the stars. This estimate is only very rough, as the radiation from the stars is so minute. As the sun only occupies one 94,000th part of the heavens, the radiation from a sunbright hemisphere would be five million times 94,000 times starlight, _i.e._ 470,000,000,000 times. The temperature of the sun is therefore the fourth root of this quantity times the effective temperature of space, _i.e._ about 700 times. Since the temperature of the sun is about 6200°, the temperature of space is a little under 10° absolute; _i.e._ lower than -263° C. {56} +Note on Absolute Temperature.+--It is found that, if a gas such as air has its temperature raised or lowered while its pressure is kept uniform, for every one degree centigrade rise or fall its volume is increased or decreased by one two hundred and seventy-third of its volume at freezing point, _i.e._ at 0° centigrade. If therefore it continued in the same way right down to -273° centigrade, its volume would be reduced to zero at this temperature. This temperature is therefore called the absolute zero of temperature, and temperatures reckoned from it are called absolute temperatures. To get absolute temperatures from centigrade temperatures we evidently need to add 273°. {57} CHAPTER VI THE TRANSFORMATION OF ABSORBED RADIATION No account of radiation would be complete without mentioning what becomes of the radiation which bodies absorb, but a good deal of the subject is in so uncertain a state that very little space will be devoted to it.