Omega by Camille Flammarion (books to read to be successful .TXT) ๐
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Born in 1842, Camille Flammarion was a French astronomer who wrote many popular books about science and astronomy, together with a number of novels which we would now consider to be science fiction. He was a contemporary of H. G. Wells and Jules Verne, though his works never achieved their level of popularity.
Omega: The Last Days of the World is an English translation of Flammarionโs novel La Fin du Monde, published in 1893. The bookโs fictional premise is the discovery of a comet on a collision course with the Earth in the 25th century. However, this is mostly a pretext on which Flammarion can hang his interesting scientific speculations about how the world will end, together with philosophical thoughts about war and religion. Much of the scientific description he uses in the book, while accurately representing the knowledge and thinking of his time, has today been superseded by modern discoveries. For example, we now know the source of the Sunโs energy to be nuclear fusion rather than being due to gravitational contraction and the constant infall of meteorites.
When talking about the ills of society, however, Flammarion could well be talking about todayโs world. For example, he excoriates the vast waste of societyโs resources on war, and demonstrates how much more productive each nationโs economy would be without it. He also depicts the media of his future world as having been entirely taken over by commercial interests, publishing only what will excite the greatest number of readers rather than serving the public interest.
Omega ranges over a vast period of time, from prehistory through to millions of years in the future when mankind has been reduced to the last two doomed individuals. Nevertheless, the book ends on a hopeful and inspiring note.
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- Author: Camille Flammarion
Read book online ยซOmega by Camille Flammarion (books to read to be successful .TXT) ๐ยป. Author - Camille Flammarion
โBut, gentlemen, from the point of view of vegetable and animal life, this half of one percent of aqueous vapor is of supreme importance, and so far as temperature and climate are concerned, I do not hesitate to assert that it is more essential than all the rest of the atmosphere.
โThe heat waves, coming from the Sun to the Earth, which warm the soil and are thence returned and scattered through the atmosphere into space, in their passage through the air meet with the oxygen and nitrogen atoms and with the molecules of aqueous vapor. These molecules are so thinly scattered (for they occupy but the hundredth part of the space occupied by the others), that one might infer that the retention of any heat whatever is due rather to the nitrogen and oxygen than to the aqueous vapor. Indeed, if we consider the atoms alone, we find two hundred oxygen and nitrogen atoms for one of aqueous vapor. Well, this one atom has eighty times more energy, more effective power to retain radiant heat, than the two hundred others; consequently, a molecule of the vapor of water is 16,000 times more effective than a molecule of dry air, in absorbing and in radiating heatโ โfor these two properties are reciprocally proportional.
โTo diminish by any great amount the number of these invisible molecules of the vapor of water, is to immediately render the Earth uninhabitable, notwithstanding its oxygen; even the equatorial and tropical regions will suddenly lose their heat and will be condemned to the cold of mountain summits covered with perpetual snow and frost: in place of luxurious plants, of flowers and fruits, of birds and nests, of the life which swarms in the sea and upon the land; instead of murmuring brooks and limpid rivers, of lakes and seas, we shall be surrounded only by ice in the midst of a vast desertโ โand when I say we, gentlemen, you understand we shall not linger long as witnesses, for the very blood would freeze in our veins and arteries, and every human heart would soon cease to beat. Such would be the consequences of the suppression of this half hundredth part of aqueous vapor which, disseminated through the atmosphere, beneficently protects and preserves all terrestrial life as in a hothouse.
โThe principles of thermodynamics prove that the temperature of space is 273ยฐ below zero. And this, gentlemen, is the more than glacial cold in which our planet will sleep when it shall have lost this airy garment in whose sheltering warmth it is today enwrapped. Such is the fate with which the gradual loss of the Earthโs water threatens the world, and this death by cold will be inevitably ours, if our earthly sojourn is long enough.
โThis end is all the more certain, because not only the aqueous vapor is diminishing, but also the oxygen and nitrogen, in brief, the entire atmosphere. Little by little the oxygen becomes fixed in the various oxides which are constantly forming on the Earthโs surface; this is the case also with the nitrogen, which disappears in the soil and vegetation, never wholly regaining a gaseous state; and the atmosphere penetrates by its weight into the land and sea, descending into subterranean depths. Little by little, from century to century, it grows less. Once, as for example in the early primary period, it was of vast extent; the Earth was almost wholly covered by water, only the first granite upheaval broke the surface of the universal ocean, and the atmosphere was saturated with a quantity of aqueous vapor immeasurably greater than that it now holds. This is the explanation of the high temperature of those bygone days, when the tropical plants of our time, the tree ferns, such as the calamites, the equisetaceae, the sigillaria and the lepidodendrons flourished as luxuriously at the poles as at the equator. Today, both the atmosphere and aqueous vapor have considerably diminished in amount. In the future they are destined to disappear. Jupiter, which is still in its primary period, possesses an immense atmosphere full of vapors. The Moon does not appear to have any at all, so that the temperature is always below the freezing point, even in the sunlight, and the atmosphere of Mars is sensibly rarer than ours.
โAs to the time which must elapse before this reign of cold caused by the diminution of the aqueous atmosphere which surrounds the globe, I also would adopt the period of 10,000,000 years, as estimated by the speaker who preceded me. Such, ladies, are the stages of world-life which nature seems to have marked out, at least for the planetary system to which we belong. I conclude, therefore, that the fate of the Earth will be the same as that of the Moon, and that when it loses the airy garment which now guarantees it against the loss of the heat received from the Sun, it will perish with cold.โ
At this point the chancellor of the Columbian academy, who had come that very day from Bogota by an electric airship to participate in the discussion, requested permission to speak. It was known that he had founded on the very equator itself, at an enormous altitude, an observatory overlooking the entire planet, from which one might see both the celestial poles at the same time, and which he had named in honor of a French astronomer who had devoted his whole life to making known his favorite science and to establishing its great philosophical importance. He was received with marked sympathy and attention.
โGentlemen,โ he said, on reaching the desk, โin these two sessions
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