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We're all stardust -- and why that should make you feel awesome | Dr. Natalie Hinkel | TEDxNashville

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    I am a planetary astrophysicist.
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    (Cheers) (Applause)
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    Thank you.
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    But I will be the first to tell you
    that I made that title up.
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    (Laughter)
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    You see, I had to make up a title
    to describe what it is that I do.
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    So I got my PhD in astrophysics
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    because I look at the properties of stars
    that are near to the Sun.
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    But I also look at planets and how
    those planets and stars interact.
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    You see, up until about 25 years ago,
    the term "planetary scientist"
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    meant only people who studied the planets
    within our own solar system.
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    But it was in 1992 that the first planet
    outside of our solar system,
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    or exoplanet, was discovered.
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    So, there's no name for somebody
    who studies what I study,
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    and today there are
    3,593 known exoplanets.
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    (Whoo!)
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    It's a lot.
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    So this field that I'm in,
    it is very young.
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    If it was a person, it would
    barely be old enough to drink.
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    (Laughter)
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    Whereas astronomy in general,
    which is the study of celestial bodies,
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    has been around for thousands of years.
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    It is the oldest of the natural sciences.
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    So today we're only just learning
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    about all the crazy possible planets
    that can exist out there.
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    There are some planets
    that actually share a star,
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    so they have two stars over the same one.
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    And there are some,
    like what you see on this picture,
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    that are so close to their planet
    that they have a period of ten hours.
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    The Earth's period is 365 days.
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    So that's pretty nuts.
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    So we're only just now
    really beginning to understand
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    all the weird physical
    and geometric properties
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    that exist between a star and a planet.
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    But I don't look at just how
    a star and a planet move
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    with respect to one another.
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    I study how they chemically interact.
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    But let me explain.
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    From the Big Bang, the only elements
    that we got were hydrogen and helium.
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    So there is none of these
    carbon or oxygen or iron.
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    There's none of that.
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    So what happened
    was that the Big Bang went off,
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    and there was hydrogen and helium
    shot all over the universe.
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    But it did so in an uneven way
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    until it formed
    these giant pockets of gas,
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    which is sort of what you're
    seeing in this video.
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    Eventually this gas collapsed
    in on itself and formed stars.
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    But these stars were massive,
    they were just absolutely huge.
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    They were about a thousand times
    bigger than the Sun.
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    (Laughter)
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    So this is like saying our Sun is a grape,
    and these massive stars were as a cat.
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    (Laughter)
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    Except less furry.
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    But it was within these first stars
    that you were able to have
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    high enough temperatures
    and densities that you had fusion.
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    So for the first time, elements were
    slamming together, and they were sticking.
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    So you have hydrogen,
    which has one proton,
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    and helium, which has two protons,
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    and they slam together,
    and suddenly you have lithium,
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    and then beryllium, and then carbon.
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    But these first stars,
    they lived hard and died young,
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    so they exploded out everywhere.
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    But they took all of these new elements
    that they created inside of them,
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    and they shot them out,
    also into the universe.
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    So a second generation of stars was formed
    mostly out of hydrogen and helium,
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    but also with these seeds of carbon
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    that they could continue
    the process of fusion.
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    Our Periodic Table
    was compiled by looking at stars
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    who lived and died at different times.
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    This one here is color-coded and was done
    by a colleague of mine, Jennifer Johnson,
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    and what she did was she color-coded it
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    to show the different ways
    in which these elements could be formed.
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    So you see that a few of them are blue
    because they came from the Big Bang,
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    but most of them come
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    from either two stars circling
    each other and then exploding,
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    or just one exploding as a supernova.
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    So, our Sun is created out of the original
    hydrogen and helium from the Big Bang,
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    but also out of many of these elements.
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    And at the same time that the Sun
    was formed, were also planets.
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    So that's everything
    from Mercury to Neptune,
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    even the dwarf Pluto.
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    But it was on the Earth
    that life blossomed,
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    and out of that life came humanity.
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    But our humanity is really rooted
    in the properties of our planet.
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    So when you think about it,
    people are made up of raw ingredients,
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    these elements that are so basic to life,
    which were created in stars.
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    We are carbon-based beings,
    the bones made of calcium.
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    And we walk on iron silicates
    on the ground,
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    and we breathe oxygen,
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    like right now, you're breathing,
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    I could see it.
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    (Laughter)
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    That came from a star.
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    So we're all stardust.
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    Quite literally.
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    But we can also do a thing
    that is similar to other stars,
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    in that we can create other elements.
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    [Tennessine]
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    (Applause) (Cheers)
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    For example, tennessine,
    which you may or may not have heard of.
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    So this is Ts 117, and it was named
    after the great state of Tennessee
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    because a number of Vanderbilt scientists
    were part of the discovery team.
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    I'm often asked the question:
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    "How can you look into outer space
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    when there are so many
    problems here on Earth?
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    Doesn't it make you feel small?"
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    And my answer to that
    question is always no.
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    It doesn't make me feel small,
    it makes me feel empowered.
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    Because I know all of the things,
    all of the events
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    that might have happened,
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    and all of the events that did happen
    in order to create life.
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    You see, it's important for us as people
    to know where we came from,
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    whether it's our parents, our ancestors,
    our planet, the birth star,
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    or the stellar nursery.
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    Knowing our root is a fundamental drive
    that is so important to humanity.
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    And it's by using the scientific method
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    that we're able to come up
    with a hypothesis
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    that can explain how the solar system
    got to be where it is today.
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    So for example, it's currently thought
    that a supernova must have gone off
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    4.6 billion years ago
    as the solar system was forming.
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    We're then able to collect data
    about nearby stars and planets
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    such that we can understand
    their basic properties.
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    So now we've found that there
    are specific elements in meteorites,
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    and also at the bottom of the ocean,
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    that could have only come
    from a supernova.
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    There, and with the help
    of our peers reviewing our data,
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    we're able to deduce the fact
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    that this supernova
    must have acted like a huge blender.
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    So it took the gas, and the dust,
    and all of these new elements,
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    and it swirled it together
    until it made something
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    that was palatable
    or habitable for life.
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    It's by looking at thousands of planets
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    and millions of stars
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    that we're able to see what a unique
    cocktail of basic elements was needed
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    in order to create a planet
    that could sustain life.
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    Then there were even more unique
    circumstances that were needed
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    to create that life.
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    In other words, we are
    a mathematical anomaly,
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    a rarity in the universe.
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    And while there's probably
    life in the universe,
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    maybe even our Milky Way galaxy,
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    that life is going to be inherently
    different from our own
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    because they were affected by events
    that never happened for us.
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    And it's going to take quite a lot
    to actually detect that life
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    because we need to be able to find,
    fund and develop the new technologies.
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    So thinking about the statistical
    likelihood of our existence,
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    it doesn't make me feel small,
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    it reminds me of all the possibilities
    that exist in outer space.
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    When we were undergrads, we'd walk
    at night from the library to the dorm,
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    and we'd look up at stars.
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    And I'd look up at Orion in particular.
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    In our classes, we learned that two stars
    that are shooting through space,
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    they're probably never going to collide,
    no matter the circumstances.
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    And that the inside of a star
    has a structure like an onion,
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    it's like shells.
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    So over time, I realize
    that these constellations
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    changed from being just these dots
    in the sky to being distinct characters.
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    I could see them, being
    at different distances from us,
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    and they shone in different colors,
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    and they were rotating
    at different speeds.
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    Some of them had planets
    that were so close to them
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    that it was hard to fathom.
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    And others shared their planet
    with another star.
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    When you look up in the sky,
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    it's like zooming from the Earth
    into outer space.
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    Except, instead of seeing
    data or pictures,
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    you're seeing questions and possibilities.
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    Regularly looking outside of our world
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    gives you a perspective
    that's so easy to forget.
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    There were so many events
    that had to happen
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    in exactly the right sequence
    in order for me to be with you today.
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    If even one of those things was different,
    say that the Earth was closer to the Sun,
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    or that the Moon didn't exist,
    then maybe life wouldn't have happened.
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    Realizing the statistical odds
    of our existence,
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    it helps to have
    all of the day-to-day drama,
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    anxieties, and insecurities
    just fall away.
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    It reminds you who you are.
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    A mathematical anomaly
    in a sea of gas, stars and planets.
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    And what I do is I study those stars
    and planets in order to try to understand
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    how they formed and how they evolved.
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    And maybe, just maybe, to discover life.
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    But you don't have to be
    a planetary astrophysicist
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    in order to feel inspired
    or empowered by outer space.
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    All you need to do is look up and remember
    that there are so many things going on
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    outside of the right here
    and the right now.
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    There's stars being born,
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    planets colliding,
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    galaxies rotating,
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    all of which are beautiful
    as you can see.
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    And they have nothing to do with you.
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    (Laughter)
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    Or so you think.
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    But these were the exact events
    that had to happen
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    in order for the Milky Way
    galaxy to be formed,
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    for a supernova to go off,
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    for the Earth to rotate around the Sun,
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    and for us to exist.
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    Thank you.
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    (Applause) (Cheers)
Title:
We're all stardust -- and why that should make you feel awesome | Dr. Natalie Hinkel | TEDxNashville
Description:

According to planetary astrophysicist Dr. Natalie Hinkel, exploring outer space makes us realize all of the possibilities for galaxies, stars, planets -- even life. The basic elements created within stars, or the raw ingredients required for life on Earth, needed to be present at exactly the right times in order for humans to exist -- which is pretty empowering, when you think about it.

Dr. Natalie Hinkel is a researcher at Vanderbilt University, studying the composition of nearby stars and how that may affect the make-up of planets orbiting those stars. She got her bachelor’s degree in physics and math at Oberlin College. Her work has brought to light a number of important (and technical) truths within the field, which she has sought to explain by leading multiple international collaborations. Natalie also observes planets that are outside of the solar system, or exoplanets, by using the Cerro Tololo Interamerican Telescope in Chile. She has studied exotic systems where planets orbit two stars (think Tatooine!) and what life would be like on an exomoon (which has yet to be discovered!). Her PhD is in Astrophysics from the School of Earth and Space Exploration, which combines the fields of geology, planetary science, and astronomy, at Arizona State University. Natalie has put together the largest catalog of element abundances measured in stars near to the Sun, called the Hypatia Catalog; it contains +65 elements in over 6000 stars: https://www.youtube.com/watch?v=lbYYcZtRiXE

This talk was given at a TEDx event using the TED conference format but independently organized by a local community. Learn more at http://ted.com/tedx

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Video Language:
English
Team:
closed TED
Project:
TEDxTalks
Duration:
12:15

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