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The (in)visible Universe | Roberto Battiston | TEDxBergamo

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    Light, where does light come from?
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    All the light around us,
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    even the one coming from
    these lit objects
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    comes from the sky.
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    One way or another it reached us,
    maybe some time ago, from the sky.
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    Light comes from cosmos only.
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    From which cosmos? From the one around us.
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    From this sky, that we cannot see
    in our city.
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    Bergamo cannot see this sky,
    you can see this sky in Africa only.
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    You see it in the dark, when the city
    doesn't illuminate night sky.
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    If you happen to go in southern world,
    you can see this sky.
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    Well, let's imagine to be some time ago,
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    two and half million years ago.
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    There will even been a first hominid
    in his evolution phase
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    who raised up from the ground
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    and he realized what he got
    above his head.
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    Imagine that moment,
    an important moment for our history
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    that comes from the remote ancient times.
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    From that moment onwards, man always had
    with him in his culture
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    the awareness of universe
    and of light coming from the sky.
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    Let's have a quantum leap.
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    You know this profile very well.
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    It's Stonehenge profile.
    What Stonehenge is?
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    It is an achievement
    of a primitive people.
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    About 4,500 years ago,
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    then practically before History begins.
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    It is an example on how the study,
    the sky observation,
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    had shaped the human culture.
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    In order to make this particular
    building system,
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    that ancient people did a huge effort,
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    they brought very heavy stones
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    from dozens, perhaps hundreds
    kilometers far away,
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    to structure them
    in a very large circular frame.
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    Why?
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    In order to watch stars.
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    To see planet motion,
    to understand when it is sow time,
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    when to harvest.
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    In order to do rituals
    related to mythologies,
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    just related to information
    coming from the sky.
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    Sky always shaped our culture:
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    Mayan, Egyptian and
    all the humanity history
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    and, according to this example,
    using technology,
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    most advanced features at that age.
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    Let's have another jump,
    about 2,300 years.
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    We are in the Mediterranean Sea,
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    a Greek-Roman ship
    carries some goods
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    between Greece and Italy
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    and it sinks in front of Kythera Island,
    a Peloponnese island.
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    In 1906, at previous century beginning,
    this wreck was found
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    and while collecting the wreck stuff,
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    in the hold of a 2,200 years old ship
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    at that point,
    apart from the usual amphorae,
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    structures like these were found,
    some sort of small wheels
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    completely covered with limestone,
    brought to Athens museum
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    and left there for 60 years long.
    Nobody knows what they were.
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    60 years later, they make them
    radio-graphs with x-ray
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    and discover within those wheels
    some very thin gears
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    like clocks of 1600 century,
    but we are in 200 b.C. century.
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    This was some sort of astrolabe,
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    a system which allowed
    to powerful people of that time
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    to compute planet motion,
    above all sun and moon eclipses.
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    Imagine what does it mean
    for a General, or for a politician,
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    to know when the sun is going to hide,
    when the moon is going to be overshadowed.
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    An incredibly sophisticated technology.
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    Marcus T. Cicero told us that
    two of this machine type,
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    were available at that time,
    in the Greek-Roman civilization.
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    We found one of them undersea,
    an extraordinary good luck!
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    Another example of how technology,
    the more advanced one,
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    had been made available,
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    but for what?
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    In order to study, to understand the sky.
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    Let's have another jump.
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    This is an Almagesto page.
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    Almagesto was a sort of encyclopedia,
    like the Britannica one,
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    where all the information known
    to mankind were collected
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    in one thousand years between
    the end of Roman Empire
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    and half of first millennium.
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    As you can see from these images,
    Earth is perfectly shaped.
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    It has all its continents: North and
    South America, even Australia.
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    What's the problem?
    It is at the center of the world.
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    All the celestial spheres surround it.
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    The one carrying the Sun,
    the one carrying the Moon,
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    the various planets, gradually up to
    the sphere that leads to the fixed stars.
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    Indeed, being in 1550, America
    was discovered by Columbus in 1492,
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    but it is not yet a clear understanding
    where this planet stands
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    within the Universe.
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    Indeed, we have to wait until 1609,
    when Galileo,
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    using this small spyglass which
    you can buy with 50€ in a general store,
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    understood that some satellites
    were turning around a planet, Jupiter,
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    and that they were drilling, ruining,
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    they were destroying
    celestial spheres harmony.
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    At the end Earth found
    its position in the Universe.
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    The Sun was not turning around the Earth,
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    but Earth was turning around Sun.
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    Spyglass, the technology of that moment,
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    now, the technological development
    leads to extraordinary progresses.
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    This is a previous century spyglass,
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    it is the spyglass through which Hubble
    looked at our galaxy for a long time,
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    he took pictures of our set of Stars,
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    that then it was thought to be
    the whole Universe
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    and while studying some small stars,
    a bit blurry,
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    from night to night he understood
    that other galaxies exist,
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    very, very far away.
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    From night to night
    Universe expanded
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    by a factor of a thousand more
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    and from then on
    we continued expanding it,
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    up to, pretty much, to its origins.
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    This by using a telescope clearly
    very much powerful than Galileo's one.
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    Today we have in space
    the telescope of telescopes:
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    Hubble telescope,
    which looks at the Universe
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    using extraordinarily favorable conditions
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    being able to do observations
    from the space
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    and this picture you can see
    on the right side
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    is a Cosmos pinhead
    on our head above
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    hugely magnified by Hubble
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    and we can see early galaxies,
    early protostars,
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    we can see an Universe how it was
    billions and billions of years ago.
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    I told you that technology is fundamental
    to understand the Universe around us
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    but you'll see how amazing
    is the pace
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    of technology evolution
    in the last century.
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    Last century allowed us to do much greater
    advancements
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    than in thousands and billions of years
    before now.
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    You can see this picture,
    we are in Scrovegni Chapel
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    and we see how in 1301 Giotto
    painted a wonderful series of paintings
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    including the Nativity and you can value
    this painting beauty
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    because we can see the shape,
    the persons images,
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    animals, a hut perspective
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    but above the hut we see a ugly comet
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    some sort of reddish shapeless small ball
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    and we wonder why a so great painter
    as Giotto was
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    had drawn a so ugly comet.
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    Because he had seen it in the sky,
    because in that moment he saw
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    that star passing on his head.
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    It is Halley comet, which passes
    each 76 years
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    and in 1301 it was passing
    on this painter's head
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    who precisely copied it.
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    In fact, these photo in 1910,
    first ones of this comet,
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    show us a structure totally similar
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    to the painted one by Giotto in 1300.
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    In 1986, 76 years later,
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    man was able to make
    his artificial satellites
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    his remote-controlled robots
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    which literally went to pinch the tail
    of Giotto comet
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    In order to see how it is made.
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    600 years to go from eye to photography,
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    76 years to pass from photography
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    to the ability to reach Halley comet.
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    Technology, technology.
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    These gentlemen are Penzias and Wilson,
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    two engineers who become famous
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    because substantially they authored
    a paper which says:
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    we tried to build an electronic equipment
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    with a very low environmental noise
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    which had practically to measure
    no one of any noise types
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    and we hear a continuous, deafening noise,
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    coming everywhere from the universe.
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    This equipment has its own ear,
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    which is an antenna, a sort of
    a big radio antenna,
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    which allowed them to realize that
    their noise comes from everywhere.
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    They don't know what they had found,
    published this finding
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    and after a few later,
    others understood
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    that they were listening to
    the Big Bang echo
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    and they awarded Nobel prize for that.
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    A noise which is actually the echo
    of the initial big explosion.
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    Today, we perform studies of the same kind
    using more powerful equipments.
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    This stratospheric balloon studied
    that Big Bang echo,
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    understanding that it has
    a very particular structure.
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    If you wear glasses in order to see
    the Big Bang
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    they are a sort of someway
    special Goggle glasses,
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    made by scientists studying these things
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    and you get out to see the sky,
    you'll see a pocked one,
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    as it had measles.
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    That measles is the detail
    of Big Bang explosion,
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    as you can see it 300,000 years later.
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    Maybe you have seen
    a picture like this
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    In the headlines of main newspapers:
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    a satellite named Plank
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    completed this picture of the sky
    affected by measles,
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    Big Bang measles,
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    this is just a sky, which revealed
    280,000 years,
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    300,000 years after Big Bang.
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    But recently you read on newspapers
    this unbelievable thing,
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    an equipment located at South Pole
    did much more.
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    It found in this picture
    of 300,000 years ago
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    a mark of something that happened
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    1 billionth of second after
    the initial explosion.
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    These polarized light circles in the sky
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    are telling us what happened
    just at the beginning of time.
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    Technology. But what happened
    over the past 50 years?
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    A very big revolution.
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    We learned how to see the Universe colours
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    which are not visible to human eyes
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    and above all not visible from the Earth.
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    The Universe seen by Galileo, Hubble,
    using telescopes,
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    is sending us the light
    which goes through atmosphere.
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    This light is a visible light which
    goes fairly through the air.
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    Radio waves seen by Penzias and Wilson
    are like the ones done by cellular phones,
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    they fairly go through the air.
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    But there are many other waves
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    that cannot go through the air,
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    and, in order to see them, we have
    to go out, literally, from the atmosphere.
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    Over the past 50 years we were able
    to do so systematically
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    and we were able to get all the colors
    of an otherwise invisible Universe.
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    For instance this picture you can see
    if we shift to visible light
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    is the Universe, Milky Way,
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    which dominates our viewpoint,
    seen from the Earth,
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    by the first hominids' eyes,
    by Galileo's eyes and Hubble's ones.
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    in the visible range.
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    It has some structure,
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    We cannot see it clearly as a whole,
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    but it has these features.
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    If we shift in the infrared range,
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    which is a frequency that doesn't go
    through the atmosphere,
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    we can see a totally different shape.
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    In the microwaves range,
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    the ones of the microwaves oven
    we have in our kitchen,
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    again it changes completely.
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    In the radiowaves range, the one
    we can see from Earth, too,
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    where are Penzias and Wilson measures,
    it changes again;
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    some set of cold gas
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    which appear and give out
    that kind of radio light.
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    In the ultraviolet range,
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    which is a color not going easily
    through atmosphere,
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    all a series of stars appear which are
    otherwise invisible in the visible range.
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    In the x-rays range,
    our Universe changes again,
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    it looks completely different
    with very hot sources.
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    To finish in the gamma rays range,
    which are those nuclear explosions,
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    where some objects are exploding
    in a nuclear way
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    inexhaustibly, since millions
    and millions years.
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    This is the Universe we have
    in front of our eyes
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    a Universe full of colours,
    that 50 years ago we don't know.
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    This is the part of an invisible Universe
    which has become a visible one,
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    which has unveiled during
    the last 50 years,
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    thanks to people work
    like Riccardo Giacconi,
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    an Italian who awarded Nobel prize in 2002
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    because he found Universe
    made of X-ray sources,
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    nobody believed it,
    "He can't do this experiment."
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    He stubbornly insisted,
    he went to America
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    and he made this satellite,
    put into orbit
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    and he saw first X-rays sources.
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    Or this satellite called Fermi,
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    as a tribute to our great physicist
    in 40-50 years,
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    which literally observes
    the very hot Universe
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    along an endless nuclear explosion.
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    Or these even more modern equipments
    called "Cherenkov-light" tools
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    which look at light
    with a so ultimate color
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    that we aren't able even
    to produce it in our labs
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    a terribly high energy
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    produced in some cases
    by those sources, energy monsters,
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    which are somewhere In our Universe.
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    This partially explains because
    we have so many satellites,
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    each is an eye looking at
    different colours
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    looking at different distances,
    looking at a short or long distance
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    reaching visible Universe borders,
    unto Big Bang touching.
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    Then we now have these beautiful pictures
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    of the Milky Way, but of the Universe, too
    in all the imaginable colours.
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    This is our Universe,
    become visible over the past 60 years,
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    previously its 90%
    was completely unreachable.
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    We finished, did we reach
    science fulfillment?
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    Do we get visible limits?
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    No, we don't.
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    We indeed don't yet know what is
    the true dark Universe.
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    There is a so dark Universe that
    light cannot be released,
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    not only released light
    doesn't go through atmosphere.
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    It is a Universe substantially invisible
    for any light type.
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    Then we recently learned
    over the past 50 years,
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    many things about the Universe.
  • 15:45 - 15:49
    We know it is flat, homogeneous,
    isotropic, made of radiation,
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    matter, protons, neutrons,
    as we are,
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    but we knows that is 4% only of the whole.
  • 15:56 - 15:58
    It exists a component, called dark matter,
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    that we know is about 23%,
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    six more times plenteous than usual matter
  • 16:05 - 16:08
    and it is in this room, it goes across us,
    but we cannot see it.
  • 16:09 - 16:13
    Not only, we understood that there is
    another 73%,
  • 16:13 - 16:16
    which is vacuum-hidden energy,
    absolutely unknown
  • 16:16 - 16:19
    beside that it exists.
  • 16:19 - 16:21
    Among other things, primeval anti-matter
  • 16:21 - 16:23
    that symbolizes Big Bang
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    has gone away and we don't know
    where it has been.
  • 16:26 - 16:29
    So we learned to look at
    all the Universe colours
  • 16:29 - 16:31
    but while we are doing so,
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    we discovered that about 95%
    of the Universe,
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    which is literally here, but invisible,
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    using all the techniques we invented
  • 16:41 - 16:43
    over the past 50 years,
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    So we know that we don't know,
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    we never have been
    so consciously ignorant
  • 16:49 - 16:52
    about nature.
  • 16:53 - 16:57
    So, after a century
    of extraordinary growth
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    after a literally exploding technology
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    that opened us all the Universe colours,
  • 17:03 - 17:05
    we reached a new board, a new border,
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    we know that 95% of what is around us
    should still be discovered.
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    So we are on the new millennium
    thresholds
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    when we have still to discover most things
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    which are around us.
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    So my meaning for this TEDx Talk is,
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    "AAA. We know that 95% of Universe
    is invisible at all.
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    Looking for ideas to understand
    what is made of."
  • 17:35 - 17:37
    Thank you.
  • 17:38 - 17:40
    (Applause)
Title:
The (in)visible Universe | Roberto Battiston | TEDxBergamo
Description:

This talk was held at a TEDx event using TED talks format, but organized indipendently by a local community. For additionl info, please see at http://ted.com/tedx

Roberto Battiston was born in 1956 in Trento-Italy. since 1993 he is professor of General Physics at Engineering Faculty of Perugia University and since 2012 professor of Experimental Physics at Physics Dept. in Trento.
For more than 30 yers active in international scientific collaborations about experimental physics on fundamantal particles interactions in accelerators or in space (Strong , Weak and Electromagnetic interaction Physics, Study of Space cosmic rays).

He was eputy spokesperson for AMS, the big experiment to search space antimatter, instalìed on ISS spacestation, on May 2011, during STS134 mission. He authored more than 400 papers published on international journals and 3 patents. In additon he organizes numerous congress on space sciences (Trento 1999, Elba 2002, Washington 2003, Beijing 2006, CERN 2012).

He also carries out activities for scientific publications, collaborating with newspapers (La Stampa, Il Corriere della Sera, Il Sole 24 Ore) and magazines (L'Indice, Le Scienze). For years In the latter he is writing a monthly column
and a blog "Stars and Particles".

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Video Language:
Italian
Team:
closed TED
Project:
TEDxTalks
Duration:
17:46

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