Cambridge | March 16 1858
My dear Sir,
I sent by last evening’s post a copy of my memoir on the temperature of the earth and planets.1 I may mention a point which may be liable to be mistaken. You will find two kinds of heat spoken of and designated respectively by Ho and Hi and radiating from a spherical envelope, which represents the external sources of radiant heat falling on the earth. Hi is supposed to have the power of radiating completely thro’ a certain imaginary shell (which may represent the earth's atmosphere) so that the shell is supposed completely diathermanous2 for this kind of heat; but it is not diathermanous for Ho which represents in fact all the heat from whatever source which is absorbed by the imaginary shell. In the actual case it represents the portion of the solar and stellar heat which is absorbed by the atmosphere. My reasoning and conclusions do not depend on the ratio of Hi to Ho so far at least as regards the nature of these conclusions. It is of no consequence whether it be 100: 5 or 100: 25.
Yours very truly | W. Hopkins.
RI MS JT/1/TYP/2/613
LT Typescript Only
a copy of my memoir on the temperature of the earth and planets: W. Hopkins, ‘On the External Temperature of the Earth, and the Other Planets of the Solar System’, Transactions of the Cambridge Philosophical Society, 9 (1855), pp. 628–72.
diathermanous: having the property of freely transmitting radiant heat (OED).
Please cite as “Tyndall1499,” in Ɛpsilon: The John Tyndall Collection accessed on