Chapter
1 II | Barbicane, viz., that the temperature inside the projectile was
2 III | atmosphere can temper, either in temperature or brilliancy, the projectile
3 III | withstood a very much higher temperature than this as it slid through
4 III | producing substance at a temperature of above 400°. But there
5 V | not strike direct. This temperature is only the temperature
6 V | temperature is only the temperature produced by the radiation
7 V | modified that excessive temperature; hence the compensation
8 V | asked Nicholl, “is the temperature of the planetary spaces
9 V | replied Barbicane; “the temperature which was observed in the
10 V | another savant, estimates the temperature of space at 250° Fahrenheit
11 V | the contrary, a very high temperature. But, when we arrive in
12 VI | to stop suddenly?”~“Her temperature would be raised to such
13 VI | restored by radiation, their temperature can only be that of the
14 XIII | transition from cold to heat, the temperature falling in an instant from
15 XIV | and a considerably lower temperature was the result. The humidity
16 XIV | heat. The projectile’s low temperature was no longer endurable.
17 XIV | we have had, at least in temperature. Now we are blinded with
18 XIV | asked Nicholl, “what is the temperature outside?”~“Exactly that
19 XIV | good position to verify the temperature of space, and see if Fourier
20 XIV | level of the surrounding temperature. Then it was rapidly pulled
21 XIV | That was the undoubted temperature of the starry space. Such
22 XV | lowness of the surrounding temperature obliged them to consume
23 XV | Regnaut’s apparatus raised the temperature of the interior of the projectile
24 XVIII| days created differences of temperature insupportable to organization,
25 XVIII| know what diminution of temperature the earth undergoes in the
26 XVIII| calculations, this mean temperature will after a period of 400,
|