The Destinies of the Stars
The Destinies of the Stars
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In our eReader you can find the full English version of the book. Read The Destinies of the Stars Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book The Destinies of the Stars
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Rather the immobility of the nebulae is due to the frequent collisions between the molecules in any quantity of gas even if it be attenuated to such a high degree as in the nebulae. Thus, the molecules strike a balance, as it were, against each other so that the different parts of the gas accumula- The Riddle of the Milky Way 57 tions shortly are brought to rest relative to each other. The irregular gas mists around the Milky Way form therefore a continuous whole. A different condition obtains ...in regard to condensed stellar bodies such as the stars. They may in the densest throng move during billions of years before they collide; but they might on the other hand enter nebulous masses and thereby suffer gradual retardation. We now refer to stars moving outside of the vapour clouds. They are therefore imrestricted and the longer they have obeyed gravitation without impeding encounters with nebulous matter, in other words the longer the time elapsed since they emerged from the gas accumulations which gave them birth, the swifter is their motion.
What to read after The Destinies of the Stars?
You can find similar books in the "Read Also" column, or choose other free books by Arrhenius, Svante, 1859-1927 to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
Rather the immobility of the nebulae is due to the frequent collisions between the molecules in any quantity of gas even if it be attenuated to such a high degree as in the nebulae. Thus, the molecules strike a balance, as it were, against each other so that the different parts of the gas accumula- The Riddle of the Milky Way 57 tions shortly are brought to rest relative to each other. The irregular gas mists around the Milky Way form therefore a continuous whole. A different condition obtains ...in regard to condensed stellar bodies such as the stars. They may in the densest throng move during billions of years before they collide; but they might on the other hand enter nebulous masses and thereby suffer gradual retardation. We now refer to stars moving outside of the vapour clouds. They are therefore imrestricted and the longer they have obeyed gravitation without impeding encounters with nebulous matter, in other words the longer the time elapsed since they emerged from the gas accumulations which gave them birth, the swifter is their motion.
What to read after The Destinies of the Stars?
You can find similar books in the "Read Also" column, or choose other free books by Arrhenius, Svante, 1859-1927 to read onlineMoreLess
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