The Day After Death; Or, Our Future Life According to Science (New Edition)Figuier, Louis
Religion
The Day After Death; Or, Our Future Life According to Science (New Edition)
Figuier, Louis
Cosmology; Future life; Transmigration
It takes three years to circumnavigate the earth. To circumnavigate the
solar globe, under similar conditions, would take three hundred years.
If human life be not more prolonged in the sun than on the earth, an
existence would not suffice to enable a traveller to become acquainted
with the surface of the globe he inhabits.
[Illustration: Fig. 1.--Comparative Dimensions of the Sun and the
Planets.]
Weight is thirty times more intense on the surface of the sun than on
the earth. We know that a body which falls upon the earth traverses, in
the first second of its fall, a space of four metres, nine centimetres.
In the sun a falling body traverses 144 metres in the first second of
its fall. It follows from this, that a human body, if transported to
the sun, would weigh about 2000 kilogrammes, the weight of an elephant.
The body of a dog or of a horse would weigh twenty-eight times as much
as upon our earth, so that these animals would remain fixed to the
surface. The conditions of nature must therefore be entirely different
in the sun from what they are in the group of planets to which the
earth belongs.
The sun sheds rays from perpetual fire, a characteristic that
appertains to him alone among all the stars of our world. Of himself
he burns, and sheds abroad light and heat. The other stars are neither
warm nor luminous, and if the sun did not exist, they would be plunged
into eternal darkness and eternal cold. This privilege alone ought to
make us comprehend the immense importance of the central star.
The light and heat which emanate from the sun are constant; they are
never interrupted, and they never lose their force. Thus, a second
characteristic--constancy of illumination--separates the sun from all
the other celestial bodies of our world.
The intensity of the real heat of the sun has been measured by the
physicists. This result was attained in an endeavour to determine by
experience the quantity of heat which accumulates in a given time,
upon a certain portion of the earth's surface, exposed to the sun's
rays, and adding to that element the quantities of heat which would be
absorbed by the atmospheric air, the ethereal spaces, and the soil.
Pouillet, the French physicist, who undertook this critical
investigation, arrived at certain results, which he states as follows:
"If the total quantity of heat emitted by the sun was exclusively
employed to melt a layer of ice applied to the solar globe, and
covering it completely in all its parts, that quantity of heat
would be able to melt, in one minute, a layer of eleven metres,
eighty centimetres, and in one day a layer of seventeen kilometres
in thickness."
"'This same quantity of heat,' says Professor Tyndall, 'would boil
2900 milliards of cubical kilometres of water, at the temperature
of ice.'"
Public-domain text, read in full here on John Shaqi.
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