Read e-book online A Short History of Nearly Everything (Краткая история почти PDF

By Bill Bryson

ISBN-10: 0375432000

ISBN-13: 9780375432002

One of many world’s so much liked and bestselling writers takes his final trip -- into the main fascinating and intractable questions that technology seeks to answer.
In A stroll within the Woods, invoice Bryson trekked the Appalachian path -- good, such a lot of it. In In A Sunburned kingdom, he faced probably the most deadly flora and fauna Australia has to supply. Now, in his greatest e-book, he confronts his maximum problem: to appreciate -- and, if attainable, resolution -- the oldest, greatest questions we have now posed in regards to the universe and ourselves. Taking as territory every thing from the massive Bang to the increase of civilization, Bryson seeks to appreciate how we acquired from there being not anything in any respect to there being us. accordingly, he has hooked up himself to a number of the world’s so much complex (and frequently obsessed) archaeologists, anthropologists, and mathematicians, vacationing to their places of work, laboratories, and box camps. He has learn (or attempted to learn) their books, pestered them with questions, apprenticed himself to their strong minds. a brief heritage of approximately every thing is the list of this quest, and it's a occasionally profound, occasionally humorous, and constantly supremely transparent and unique event within the geographical regions of human wisdom, as merely invoice Bryson can render it. technology hasn't ever been extra concerning or unique.

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Additional info for A Short History of Nearly Everything (Краткая история почти всего на свете) + audio

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But Betelgeuse is fifty thousand light-years away. Only half a dozen times in recorded history have supernovae been close enough to be visible to the naked eye. One was a blast in 1054 that created the Crab Nebula. Another, in 1604, made a star bright enough to be seen during the day for over three weeks. The most recent was in 1987, when a supernova flared in a zone of the cosmos known as the Large Magellanic Cloud, but that was only barely visible and only in the southern hemisphere—and it was a comfortably safe 169,000 light-years away.

Newton’s laws explained so many things—the slosh and roll of ocean tides, the motions of planets, why cannonballs trace a particular trajectory before thudding back to Earth, why we aren’t flung into space as the planet spins beneath us at hundreds of miles an hour2—that it took a while for all their implications to seep in. But one revelation became almost immediately controversial. This was the suggestion that the Earth is not quite round. According to Newton’s theory, the centrifugal force of the Earth’s spin should result in a slight flattening at the poles and a bulging at the equator, which would make the planet slightly oblate.

Triangulation, their chosen method, was a popular technique based on the geometric fact that if you know the length of one side of a triangle and the angles of two corners, you can work out all its other dimensions without leaving your chair. Suppose, by way of example, that you and I decided we wished to know how far it is to the Moon. Using triangulation, the first thing we must do is put some distance between us, so let's say for argument that you stay in Paris and I go to Moscow and we both look at the Moon at the same time.

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