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A Short History of Nearly Everything 
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  • One of the world's most beloved and bestselling writers takes his ultimate journey-into the most intriguing and intractable questions that science seeks to answer.

    In A Walk in the Woods, Bill Bryson trekked the Appalachian Trail-well, most of it. In In A Sunburned Country, he confronted some of the most lethal wildlife Australia has to offer. Now, in his biggest book, he confronts his greatest challenge: to understand-and, if possible, answer-the oldest, biggest questions we have posed about the universe and ourselves. Taking as territory everything from the Big Bang to the rise of civilization, Bryson seeks to understand how we got from there being nothing at all to there being us. To that end, he has attached himself to a host of the world's most advanced (and often obsessed) archaeologists, anthropologists, and mathematicians, travelling to their offices, laboratories, and field camps. He has read (or tried to read) their books, pestered them with questions, apprenticed himself to their powerful minds. A Short History of Nearly Everything is the record of this quest, and it is a sometimes profound, sometimes funny, and always supremely clear and entertaining adventure in the realms of human knowledge, as only Bill Bryson can render it. Science has never been more involving or entertaining.


    ÀÌ Ã¥¿¡ ½ñ¾ÆÁø Âù»ç´Â ³Ê¹« ȣȭ·Ó´Ù. "½ºÆ¼ºì ȣŷÀÇ <½Ã°£ÀÇ ¿ª»ç> ÀÌ·¡ ÃÖ´ëÀÇ È­Á¦°¡ µÈ °úÇб³¾ç¼­", "¡¸´º¿å ŸÀÓ½º ºÏ¸®ºä¡¹º£½ºÆ®¼¿·¯ ¸ñ·Ï¿¡ 22ÁÖ µ¿¾È ·©Å©!", "¿µ±¹°ú ¹Ì±¹ÀÇ ¾Æ¸¶Á¸´åÄÄ¿¡¼­ ÀÚ¿¬°úÇÐ ¼­ÀûÀ¸·Î´Â ÀÌ·ÊÀûÀ¸·Î Ãâ°£ÈÄ ÆǸżøÀ§ 1À§". ÀÌ·± °úÇÐÃ¥Àº ÈçÄ¡ ¾Ê´Ù.

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    Ã¥ Á¦¸ñ '°ÅÀÇ ¸ðµç °ÍÀÇ ¿ª»ç'´Â °ÅÁþ¸»ÀÌ ¾Æ´Ï´Ù. »ý¹°°ú ÀηùÀÇ ¿ª»ç¸¦ Àç¹Õ°í ½±°Ô ¾Ë°í ½ÍÀº »ç¶÷Àº <³ª¸¦ ºÎ¸£´Â ½£>ÀÇ ±× È°´ÞÇÑ ÀÔ½ÉÀ» ¹Ï°í(±×·¸´Ù! ±× ºô ºê¶óÀ̽¼ÀÌ´Ù) ÀÌ Ã¥À» »ç¶ó. Àü¹®°¡¸¦ À§Çؼ­¶ó¸é ºô ºê¶óÀ̽¼ÀÌ ÀÌ Ã¥À» ¾²Áöµµ ¾Ê¾Ò´Ù.¡°Stylish [and] stunningly accurate prose. We learn what the material world is like from the smallest quark to the largest galaxy and at all the levels in between . . . brims with strange and amazing facts . . . destined to become a modern classic of science writing.¡± ¡ªThe New York Times ¡°Bryson has made a career writing hilarious travelogues, and in many ways his latest is more of the same, except that this time Bryson hikes through the world of science.¡± ¡ªPeople ¡°Bryson is surprisingly precise, brilliantly eccentric and nicely eloquent . . . a gifted storyteller has dared to retell the world¡¯s biggest story.¡± ¡ªSeattle Times ¡°Hefty, highly researched and eminently readable.¡± ¡ªSimon Winchester, The Glob...
  • Part I: Lost in the Cosmos
    1. How to Build a Universe
    2. Welcome to the Solar System
    3. The Reverend Evans's Universe

    Part II: The Size of the Earth
    4. The Measure of Things
    5. The Stone-Breakers
    6. Science Red in Tooth and Claw
    7. Elemental Matters

    Part III: A New Age Dawns
    8. Einstein's Universe
    9. The Mighty Atom
    10. Getting the Lead Out
    11. Muster Mark's Quarks
    12. The Earth Moves

    Part IV: Dangerous Planet
    13. Bang!
    14. The Fire Below
    15. Dangerous Beauty

    Part V: Life Itself
    16. Lonely Planet
    17. Into the Troposphere
    18. The Bounding Main
    19. The Rise of Life
    20. Small World
    21. Life Goes On
    22. Good-bye to All That
    23. The Richness of Being
    24. Cells
    25. Darwin's Singular Notion
    26. The Stuff of Life

    Part VI: The Road to Us
    27. Ice Time
    28. The Mysterious Biped
    29. The Restless Ape
    30. Good-bye

    Notes
    Bibliography
    Index Acknowledgments Introduction 1 Pt. I Lost in the Cosmos 7 1 ...
  • 1 HOW TO BUILD A UNIVERSE

    NO MATTER HOW hard you try you will never be able to grasp just how tiny, how spatially unassuming, is a proton. It is just way too small.

    A proton is an infinitesimal part of an atom, which is itself of course an insubstantial thing. Protons are so small that a little dib of ink like the dot on this i can hold something in the region of 500,000,000,000 of them, rather more than the number of seconds contained in half a million years. So protons are exceedingly microscopic, to say the very least.

    Now imagine if you can (and of course you can't) shrinking one of those protons down to a billionth of its normal size into a space so small that it would make a proton look enormous. Now pack into that tiny, tiny space about an ounce of matter. Excellent. You are ready to start a universe.

    I'm assuming of course that you wish to build an inflationary universe. If you'd prefer instead to build a more old-fashioned, standard Big Bang universe, you'll need additional materials. In fact, you will need to gather up everything there is-every last mote and particle of matter between here and the edge of creation-and squeeze it into a spot so infinitesimally compact that it has no dimensions at all. It is known as a singularity.

    In either case, get ready for a really big bang. Naturally, you will wish to retire to a safe place to observe the spectacle. Unfortunately, there is nowhere to retire to because outside the singularity there is no where. When the universe begins to expand, it won't be spreading out to fill a larger emptiness. The only space that exists is the space it creates as it goes.

    It is natural but wrong to visualize the singularity as a kind of pregnant dot hanging in a dark, boundless void. But there is no space, no darkness. The singularity has no "around" around it. There is no space for it to occupy, no place for it to be. We can't even ask how long it has been there-whether it has just lately popped into being, like a good idea, or whether it has been there forever, quietly awaiting the right moment. Time doesn't exist. There is no past for it to emerge from.

    And so, from nothing, our universe begins.

    In a single blinding pulse, a moment of glory much too swift and expansive for any form of words, the singularity assumes heavenly dimensions, space beyond conception. In the first lively second (a second that many cosmologists will devote careers to shaving into ever-finer wafers) is produced gravity and the other forces that govern physics. In less than a minute the universe is a million billion miles across and growing fast. There is a lot of heat now, ten billion degrees of it, enough to begin the nuclear reactions that create the lighter elements-principally hydrogen and helium, with a dash (about one atom in a hundred million) of lithium. In three minutes, 98 percent of all the matter there is or will ever be has been produced. We have a universe. It is a place of the most wondrous and g...
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