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Powers of Ten

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    [ Music ]
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    A picnic near the lakeside in Chicago is the
    start of a lazy afternoon early one October.
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    We begin with a scene one meter wide,
    which we view from just one meter away.
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    Now every 10 seconds, we will
    look from 10 times farther away
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    and our field of view will be 10 times wider.
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    This square is 10 meters wide
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    and in 10 seconds the next
    square will be 10 times as wide.
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    Our picture will center on the picnickers
    even after they've been lost to sight.
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    100 meters wide, the distance a man
    can run in 10 seconds, cars crowd the highway,
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    power boats lie at their docks, the
    colorful bleachers are Soldier's Field.
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    This square is a kilometer wide,
    1000 meters, the distance
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    a racing car can travel in 10 seconds.
    We see the great city
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    on the lakeshore.
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    10 to the fourth meters, 10 kilometers,
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    the distance a supersonic
    airplane can travel in 10 seconds.
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    We see first, the rounded end of Lake
    Michigan, then the whole Great Lake.
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    10 to the fifth meters, the distance an
    orbiting satellite covers in 10 seconds.
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    Long parades of clouds, the
    day's weather in the Middle West.
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    10 to the sixth, a one with
    six zeros, a million meters.
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    Soon the Earth will show
    as a solid sphere.
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    [ Music ]
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    We are able to see the whole Earth now
    just over a minute along the journey.
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    The Earth diminishes into the distance but
    those background stars are so much farther
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    away that they do not yet appear to move.
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    [ Music ]
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    A line extends at the true speed of light.
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    In one second, it half-crosses
    the tilted orbit of the moon.
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    [ Music ]
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    Now we mark a small part of the path
    in which the Earth moves about the Sun.
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    Now the orbital paths of the neighbor
    planets, Venus, and Mars, then Mercury.
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    Entering our field of view is the
    glowing center of our solar system,
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    the Sun.
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    Followed by the massive outer
    planets swinging wide in their big orbits.
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    [ Music ]
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    That odd orbit belongs to Pluto; a
    fringe of myriad comets too faint
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    to see completes the solar system.
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    [ Music ]
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    10 to the 14, as the solar system shrinks
    to one bright point in the distance,
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    our Sun is plainly now only one
    among the stars. Looking back from here,
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    we note four southern constellations
    still much as they appear
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    from the far side of the Earth.
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    [ Music ]
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    This square's 10 to the 16 meters, one
    light year not yet out to the next star.
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    Our last 10 second step took us 10 light
    years further; the next will be 100.
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    Our perspective changes so
    much in each step now
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    that even the background
    stars will appear to converge.
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    At last, we pass the bright star
    Arcturus and some stars of the Dipper.
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    Normal but quite unfamiliar, stars
    and clouds of gas surround us
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    as we traverse the Milky Way galaxy.
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    [ Music ]
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    Giant steps carry us into
    the outskirts of the galaxy.
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    And as we pull away, we begin to
    see the great flat spiral facing us.
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    The time and path we chose to
    leave Chicago has brought us
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    out of the galaxy along a course
    nearly perpendicular to its disc.
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    [ Music ]
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    But two little satellite galaxies
    of our own are the
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    clouds of Magellan. 10 to the 22nd
    power, a million light years.
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    [ Music ]
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    Groups of galaxies bring a new level
    of structure to the scene.
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    Glowing points are no longer single stars
    but whole galaxies of stars seen as one.
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    We pass the big Virgo cluster
    of galaxies, among many others.
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    A hundred million light years
    out, as we approach the limit
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    of our vision, we pause to start back home.
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    This lonely scene, the galaxies like
    dust, is what most of space looks like.
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    This emptiness is normal.
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    The richness of our own neighborhood
    is the exception.
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    The trip back to the picnic on the lakefront
    will be a sped-up version reducing the
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    distance of the Earth's surface by one
    power of 10 every two seconds.
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    And each two seconds will appear to cover
    90% of the remaining distance back to Earth.
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    Notice the alternation between great
    activity and relative inactivity,
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    a rhythm that will continue all the way
    into our next goal, a proton in the nucleus
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    of a carbon atom beneath the skin on the
    hand of the sleeping man at the picnic.
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    [ Music ]
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    10 to the ninth meters, 10 to the eighth,
    seven, six, five, four, three, two, one,
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    we are back at our starting point.
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    We slow up at one meter, 10 to the 0 power.
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    [ Music ]
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    Now we reduce the distance to our final
    destination by 90% every 10 seconds.
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    Each step much smaller
    than the one before.
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    [ Music ]
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    At 10 to the minus two, one 100th
    of a meter, one centimeter,
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    we approach the surface of the hand.
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    [ Music ]
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    In a few seconds, we'll be entering
    the skin, crossing layer after layer
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    from the outermost dead cells
    into a tiny blood vessel within.
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    Skin layers vanish in turn.
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    An outer layer of cells, felty collagen.
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    The capillary containing red blood
    cells and roughly lymphocyte.
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    We enter the white cell.
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    Among its vital organelles, the porous
    wall of the cell nucleus appears.
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    [ Music ]
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    The nucleus within holds the heredity
    of the man in the coiled coils of DNA.
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    As we close in, we come to
    the double helix itself.
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    A molecule like a long twisted ladder
    whose rungs of paired bases spell out
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    twice, in an alphabet of four letters,
    words of a powerful genetic message.
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    At the atomic scale, the interplay of
    form and motion becomes more visible.
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    We focus on one commonplace group
    of three hydrogen atoms bonded
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    by electrical forces to a carbon atom.
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    Four electrons make up the outer
    shell of the carbon itself.
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    They appear in quantum motion
    as a swarm of shimmering points.
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    At 10 to the -10 meters, one angstrom,
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    we find ourselves right among
    those outer electrons.
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    Now we come upon the two inner
    electrons held in a tighter swarm.
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    As we draw towards the atom's attracting
    center, we enter upon a vast interspace.
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    [ Music ]
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    At last, the carbon nucleus,
    so massive and so small.
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    This carbon nucleus is made up
    of six protons and six neutrons.
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    We are in the domain of universal modules.
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    There are protons and neutrons in
    every nucleus, electrons in every atom.
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    Atoms bonded into every molecule
    out to the farthest galaxy.
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    [ Music ]
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    As a single proton fills our scene
    we reach the edge of present understanding,
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    are these some quarks
    at intense interaction?
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    Our journey has taken us
    through 40 powers of 10.
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    If now the field is one unit, then when
    we saw many clusters of galaxies together,
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    it was 10 to the 40th,
    or one and 40 zeros.
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    [ Music ]
Title:
Powers of Ten
Video Language:
English
Duration:
09:01
Jessica Lund edited English subtitles for Powers of Ten
Laura Hamrick edited English subtitles for Powers of Ten
Laura Hamrick edited English subtitles for Powers of Ten
Alexandra Davis edited English subtitles for Powers of Ten
Alexandra Davis edited English subtitles for Powers of Ten
Alexandra Davis edited English subtitles for Powers of Ten
Alexandra Davis edited English subtitles for Powers of Ten
Alexandra Davis edited English subtitles for Powers of Ten
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