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LIFE BEYOND II: The Museum of Alien Life (4K)

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    Sᴜᴘᴘᴏʀᴛᴇᴅ ʙʏ
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    Sᴜᴘᴘᴏʀᴛᴇᴅ ʙʏ
    Protocol Labs
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    Sᴜᴘᴘᴏʀᴛᴇᴅ ʙʏ
    Protocol Labs
    Follow your curiosity.
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    Sᴜᴘᴘᴏʀᴛᴇᴅ ʙʏ
    Protocol Labs
    Follow your curiosity.
    Lead humanity forward.
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    Protocol Labs
    Follow your curiosity.
    Lead humanity forward.
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    Follow your curiosity.
    Lead humanity forward.
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    In all the universe,
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    In all the universe,
    there stands only one known tree of life.
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    Does it stand alone?
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    Does it stand alone?
    Or is it part of a vast cosmic wilderness?
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    Imagine a museum
    containing every type of life in the universe.
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    What strange things would such a museum hold?
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    What is possible under the laws of nature?
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    LIFE
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    LIFE BEYOND
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    CHAPTER II
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    CHAPTER II
    The Museum Of Alien Life
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    To have any hope-
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    of finding alien life,
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    we have to know what to look for.
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    But where do we begin?
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    How do we narrow down...
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    a seemingly infinite set-
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    of possibilities?
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    There's one thing we know for sure...
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    nature will have to play-
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    by her own rules.
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    No matter how strange-
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    alien life might be...
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    is going to be limited-
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    by the same physical,
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    and chemical laws that we are...
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    6_
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    6 C_
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    6 CO_
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    6 CO₂
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    6 CO₂ +
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    6 CO₂ + 6
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    6 CO₂ + 6 H_
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    6 CO₂ + 6 H₂_
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    6 CO₂ + 6 H₂O_
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    6 CO₂ + 6 H₂O +
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    6 CO₂ + 6 H₂O + L
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    6 CO₂ + 6 H₂O + Li
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    6 CO₂ + 6 H₂O + Lig_
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    6 CO₂ + 6 H₂O + Ligh_
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    6 CO₂ + 6 H₂O + Light_
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    6 CO₂ + 6 H₂O + Light →
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    6 CO₂ + 6 H₂O + Light → C
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    6 CO₂ + 6 H₂O + Light → C₆
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    6 CO₂ + 6 H₂O + Light → C₆H_
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    6 CO₂ + 6 H₂O + Light → C₆H₁_
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    6 CO₂ + 6 H₂O + Light → C₆H₁₂_
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    6 CO₂ + 6 H₂O + Light → C₆H₁₂O
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    6 CO₂ + 6 H₂O + Light → C₆H₁₂O₆
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    6 CO₂ + 6 H₂O + Light → C₆H₁₂O₆ +
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    6 CO₂ + 6 H₂O + Light → C₆H₁₂O₆ + 6_
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    6 CO₂ + 6 H₂O + Light → C₆H₁₂O₆ + 6 O_
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    6 CO₂ + 6 H₂O + Light → C₆H₁₂O₆ + 6 O₂
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    On top of this,
    6 CO₂ + 6 H₂O + Light → C₆H₁₂O₆ + 6 O₂
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    On top of this,
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    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ →_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅O_
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +
    each alien environment-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2C_
    will further limit-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO_
    will further limit-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ +_
    will further limit-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + E
    will further limit-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + En
    will further limit-
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    ⁴⁵⁸ ʜʏᴅʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Ene
    will further limit-
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    ⁴⁵⁸ ᴏxʏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Ener_
    will further limit-
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    ⁴⁵⁸ ᴏxʏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Energ_
    will further limit-
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    ⁴⁵⁸ ᴏxʏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Energy_
    will further limit-
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    ⁴⁵⁸ ᴏxʏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Energy
    will further limit-
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    ⁴⁵⁸ ᴏxʏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Energy
    what kinds of life forms-
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    ⁴⁵⁸ ᴏxʏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Energy
    can evolve there.
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    ⁴⁵⁸ ɴɪʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Energy
    can evolve there.
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    ⁴⁰⁵⁰ ɴɪʀᴏɢᴇɴ | C₆H₁₂O₆ → 2C₂H₅OH +2CO₂ + Energy
    can evolve there.
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    Despite these natural boundaries,
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    the possibilities...
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    are staggering to imagine.
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    Trillions of planets...
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    each a unique cauldron of chemicals,
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    undergoing their own...
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    complex evolution.
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    To guide our thinking,
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    this museum of alien life-
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    will be divided into two exhibits...
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    Life as we know it,
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    Life as we know it,
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    home to beings-
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    with bio-chemistries like ours.
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    EXHIBIT II
    Life As We Know Don't It
    ᴱˣᵒᵗⁱᶜ ᴮⁱᵒᶜʰᵉᵐⁱˢᵗʳⁱᵉˢ
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    EXHIBIT II
    Life As We Know Don't It
    ᴱˣᵒᵗⁱᶜ ᴮⁱᵒᶜʰᵉᵐⁱˢᵗʳⁱᵉˢ
    And life as we don't know it,
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    EXHIBIT II
    Life As We Know Don't It
    ᴱˣᵒᵗⁱᶜ ᴮⁱᵒᶜʰᵉᵐⁱˢᵗʳⁱᵉˢ
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    EXHIBIT II
    Life As We Know Don't It
    ᴱˣᵒᵗⁱᶜ ᴮⁱᵒᶜʰᵉᵐⁱˢᵗʳⁱᵉˢ
    home to beings-
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    EXHIBIT II
    Life As We Know Don't It
    ᴱˣᵒᵗⁱᶜ ᴮⁱᵒᶜʰᵉᵐⁱˢᵗʳⁱᵉˢ
    that challenge our concept...
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    EXHIBIT II
    Life As We Know Don't It
    ᴱˣᵒᵗⁱᶜ ᴮⁱᵒᶜʰᵉᵐⁱˢᵗʳⁱᵉˢ
    to of life itself.
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    Before we venture-
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    too far into the unknown,
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    we have to ask ourselves...
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    What if alien life-
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    is more like us...
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    than we think?
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    EXHIBIT I
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    EXHIBIT I
    Life As We Know It
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    If there's one feature-
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    that unites us...
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    with these other specimens-
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    in this museum,
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    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
  • 4:20 - 4:21
    EXHIBIT I
    Life As We Know It
    ᶜᵃʳᵇᵒⁿ ᵃⁿᵈ ʷᵃᵗᵉʳ ᵇᵃˢᵉᵈ
    it's carbon...
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    Carbon
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    Carbon
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    S_
    Carbon ⁴ᵗʰ
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    ᴀ_ Sᴜ_
    Carbon ⁴ᵗʰ ᵐ
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    C_
    ᴀᴛ_ Sᴜʙ_
    Carbon ⁴ᵗʰ ᵐᵒ
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    R_ C_
    ᴀᴛᴏ_ Sᴜʙʟ
    Carbon ⁴ᵗʰ ᵐᵒˢ
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    R +_ C_
    ᴀᴛᴏᴍ Sᴜʙʟɪ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ
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    R + 7:_ C
    ᴀᴛᴏᴍɪ Sᴜʙʟɪᴍ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃ
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    R + 7: 9 C
    ᴀᴛᴏᴍɪᴄ Sᴜʙʟɪᴍᴀ_
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇ
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    R + 7: 9: C 0
    ᴀᴛᴏᴍɪᴄ ᴡ_ Sᴜʙʟɪᴍᴀᴛ_
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘ
  • 4:23 - 4:23
    R + 7: 9: 5 C 0_
    ᴀᴛᴏᴍɪᴄ ᴡᴇ_ Sᴜʙʟɪᴍᴀᴛɪ_
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿ
  • 4:23 - 4:23
    R + 7: 9: 56_ C 0_
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪ_ Sᴜʙʟɪᴍᴀᴛɪᴏ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈ
  • 4:23 - 4:23
    R + 7: 9: 56._ C 0_
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜ Sᴜʙʟɪᴍᴀᴛɪᴏɴ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃ
  • 4:23 - 4:23
    R + 7: 9: 56.2_ C 0
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 00
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏ_
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 00
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪ_
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 00_
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴ_
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 00_
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂. Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 00_
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ:
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:23 - 4:23
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:23 - 4:24
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:24 - 4:25
    R + 7: 9: 56.25: Period 2
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:25 - 4:26
    R + 7: 9: 56.25: Period 2
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    Carbon is ubiquitous,
  • 4:26 - 4:26
    R + 7: 9: 56.25: Period 2
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:26 - 4:27
    R + 7: 9: 56.25: Period 2
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    it's one o' tho most-
  • 4:27 - 4:28
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    it's one o' tho most-
  • 4:28 - 4:29
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    common elements in the universe,
  • 4:29 - 4:29
    R + 7: 9: 56.25: Group 14
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    common elements in the universe,
  • 4:29 - 4:30
    R + 7: 9: 56.25: Group 14
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:30 - 4:30
    R + 7: 9: 56.25: Group 14
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    and is very good at forming-
  • 4:30 - 4:31
    R + 7: 9: 56.25: [He] 2s² 2p²
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    and is very good at forming-
  • 4:31 - 4:32
    R + 7: 9: 56.25: [He] 2s² 2p²
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    large stable molecules.
  • 4:32 - 4:33
    R + 7: 9: 56.25
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    large stable molecules.
  • 4:33 - 4:34
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    large stable molecules.
  • 4:34 - 4:35
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:35 - 4:37
    R + 7: 9: 56.25: Period 2
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:37 - 4:37
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:37 - 4:39
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    Carbon has the rare ability-
  • 4:39 - 4:39
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    to form four way bounds-
  • 4:39 - 4:40
    R + 7: 9: 56.25: Group 14
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    to form four way bounds-
  • 4:40 - 4:41
    R + 7: 9: 56.25: Group 14
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    with other elements...
  • 4:41 - 4:42
    R + 7: 9: 56.25: [He] 2s² 2p²
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    with other elements...
  • 4:42 - 4:42
    R + 7: 9: 56.25: [He] 2s² 2p²
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
  • 4:42 - 4:42
    R + 7: 9: 56.25: [He] 2s² 2p²
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    and to bind to itself-
  • 4:42 - 4:43
    R + 7: 9: 56.25
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    and to bind to itself-
  • 4:43 - 4:43
    R + 7: 9: 56.25
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    in long stable chains...
  • 4:43 - 4:45
    R + 7: 9: 56.25: C 006
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: ₁₂.₀₁₁ Sᴜʙʟɪᴍᴀᴛɪᴏɴ ᴘᴏɪɴᴛ: ³⁹¹⁵ ᴷ
    Carbon ⁴ᵗʰ ᵐᵒˢᵗ ᵃᵇᵘⁿᵈᵃⁿᵗ ᵉˡᵉᵐᵉⁿᵗ
    in long stable chains...
  • 4:46 - 4:47
    enabling the formation-
  • 4:48 - 4:51
    of huge complex molecules.
  • 4:56 - 4:58
    This versatility makes-
  • 4:58 - 4:59
    carbon the center piece...
  • 4:59 - 5:01
    in the moleculary machinery of life.
  • 5:03 - 5:05
    And the same carbon compounds,
  • 5:05 - 5:06
    that we use have been-
  • 5:06 - 5:09
    found far from Earth,
  • 5:09 - 5:10
    clinging to meteorites...
  • 5:11 - 5:11
    G
  • 5:11 - 5:11
    Gl
  • 5:11 - 5:11
    Gly_
  • 5:11 - 5:11
    Glyc_
  • 5:11 - 5:11
    ᵃᵐ Glyc_
  • 5:11 - 5:11
    ᵃᵐⁱ Glyc_
  • 5:11 - 5:11
    ᵃᵐⁱⁿ Glyc_
  • 5:11 - 5:11
    ᵃᵐⁱⁿᵒ Glyci_
  • 5:11 - 5:11
    ᵃᵐⁱⁿᵒ ᵃ Glyci_
  • 5:11 - 5:11
    ᵃᵐⁱⁿᵒ ᵃᶜ Glycin
  • 5:11 - 5:11
    ᵃᵐⁱⁿᵒ ᵃᶜⁱ Glycin
  • 5:11 - 5:12
    ᵃᵐⁱⁿᵒ ᵃᶜⁱᵈ Glycine
  • 5:12 - 5:15
    ᵃᵐⁱⁿᵒ ᵃᶜⁱᵈ Glycine
    to floating in far off clouds...
  • 5:15 - 5:15
    ᵃᵐⁱⁿᵒ ᵃᶜⁱᵈ Glycine
  • 5:15 - 5:16
    ᵃᵐⁱⁿᵒ ᵃᶜⁱᵈ Glycine
    of cosmic dust.
  • 5:16 - 5:18
    ᵃᵐⁱⁿᵒ ᵃᶜⁱᵈ Glycine
  • 5:18 - 5:20
    ᵃᵐⁱⁿᵒ ᵃᶜⁱᵈ Glycine
    The building blocks of life...
  • 5:21 - 5:22
    Drifting like snow...
  • 5:22 - 5:24
    through the universe.
  • 5:30 - 5:31
    And if alien life...
  • 5:31 - 5:32
    has selected other-
  • 5:33 - 5:34
    carbon compounds...
  • 5:34 - 5:35
    for the biochemistry,
  • 5:36 - 5:38
    they will have plenty to choose from.
  • 5:40 - 5:41
    Z DNA | B DNA
  • 5:42 - 5:44
    Scientists recently identified-
  • 5:44 - 5:46
    over a million possible-
  • 5:46 - 5:48
    alternatives to DNA...
  • 5:48 - 5:51
    all carbon based.
  • 5:58 - 5:59
    If we ever discover-
  • 5:59 - 6:01
    other carbon based life forms,
  • 6:02 - 6:06
    we will be fundamentally related.
  • 6:08 - 6:11
    They will be our cosmic brother.
  • 6:13 - 6:15
    But would they look anything like us?
  • 6:20 - 6:22
    If they hail from Earth like planets,
  • 6:23 - 6:24
    we could share even more in common,
  • 6:25 - 6:28
    than just our biochemistry.
  • 6:30 - 6:31
    What would life be like-
  • 6:31 - 6:32
    on another planets,
  • 6:32 - 6:33
    if it is evolved?
  • 6:33 - 6:34
    Would it be like,
  • 6:35 - 6:37
    the world today here on Earth?
  • 6:37 - 6:40
    Or would be completely different?
  • 6:40 - 6:41
    There are those,
  • 6:41 - 6:42
    who argue that...
  • 6:42 - 6:44
    from the argument of convergent evolution,
  • 6:45 - 6:46
    if conditions on other planets-
  • 6:46 - 6:47
    are similar to here,
  • 6:48 - 6:48
    then we will see-
  • 6:48 - 6:50
    very similar life forms...
  • 6:54 - 6:57
    Animal and plant-like organisms,
  • 6:57 - 7:00
    that look very familiar.
  • 7:12 - 7:13
    On Earth,
  • 7:13 - 7:15
    certain features like eyesight,
  • 7:15 - 7:17
    echo-location and flight...
  • 7:17 - 7:19
    have evolved multiple times,
  • 7:19 - 7:20
    independently...
  • 7:20 - 7:22
    in different species.
  • 7:24 - 7:26
    This process of convergent evolution...
  • 7:26 - 7:29
    could extend to alien planets like Earth,
  • 7:29 - 7:31
    where creatures face similar-
  • 7:31 - 7:35
    environmental pressures.
  • 7:35 - 7:37
    It's no guarantee,
  • 7:37 - 7:39
    but there could be certain-
  • 7:39 - 7:42
    universalities of life...
  • 7:44 - 7:46
    the greatest hits of evolution...
  • 7:46 - 7:49
    on repeat across the universe.
  • 7:58 - 7:59
    Each feature would be a tune-
  • 7:59 - 8:02
    to its local environment.
  • 8:03 - 8:04
    Dimly lit planets...
  • 8:04 - 8:06
    would produce huge eyes-
  • 8:06 - 8:08
    to suck in extra light,
  • 8:08 - 8:11
    like nocturnal mammals.
  • 8:14 - 8:15
    Some people have gone-
  • 8:15 - 8:16
    so far as to say...
  • 8:17 - 8:18
    that human type organism,
  • 8:19 - 8:19
    humanoids,
  • 8:19 - 8:22
    will occur on other planets.
  • 8:26 - 8:27
    The existence of other-
  • 8:27 - 8:29
    human-like organisms...
  • 8:29 - 8:30
    seems unlikely,
  • 8:30 - 8:31
    given the long...
  • 8:31 - 8:33
    convoluted chain of events-
  • 8:33 - 8:34
    that produced us.
  • 8:35 - 8:37
    But we can't rule it out.
  • 8:41 - 8:42
    If just one in every-
  • 8:42 - 8:45
    100 trillion Earth-like planets produced-
  • 8:45 - 8:46
    a human-like form...
  • 8:46 - 8:47
    There could still be-
  • 8:47 - 8:48
    thousands of creatures-
  • 8:48 - 8:51
    like us out there...
  • 9:02 - 9:07
    But in reality, we are more likely to find
    something lower on the food chain.
  • 9:10 - 9:11
    Convergent evolution-
  • 9:11 - 9:14
    is also rampant in plant life...
  • 9:14 - 9:16
    and C₄ photosynthesis-
  • 9:16 - 9:17
    has arisen independently,
  • 9:17 - 9:19
    over 40 times...
  • 9:21 - 9:23
    Would alien plants-
  • 9:23 - 9:24
    look like ours...
  • 9:24 - 9:26
    or something else entirely?
  • 9:37 - 9:37
    On Earth,
  • 9:38 - 9:39
    plants appear green...
  • 9:39 - 9:40
    because they absorb-
  • 9:40 - 9:41
    the other wavelengths,
  • 9:41 - 9:44
    in the Sun's light spectrum.
  • 9:45 - 9:49
    But stars come in many colors...
  • 9:52 - 9:54
    and alien plants would evolve-
  • 9:54 - 9:55
    different pigments...
  • 9:55 - 9:59
    to adapt to their sun's unique spectrum.
  • 10:04 - 10:06
    Plants feeding off hotter stars-
  • 10:06 - 10:08
    could appear redder,
  • 10:08 - 10:09
    by absorbing their-
  • 10:09 - 10:11
    energy rich bluer light
  • 10:20 - 10:22
    Around dim Red Dwarfs stars,
  • 10:22 - 10:25
    vegetation could appear black,
  • 10:25 - 10:27
    adapted to absorb all-
  • 10:27 - 10:29
    visible wavelengths of light.
  • 10:45 - 10:46
    Earth itself-
  • 10:46 - 10:48
    may have once appeared purple,
  • 10:48 - 10:49
    due a pigment called retinal,
  • 10:49 - 10:50
    ʀᴇᴛɪɴᴀʟ
    due a pigment called retinal,
  • 10:50 - 10:50
    ʀᴇᴛɪɴᴀʟ
  • 10:50 - 10:50
    ʀᴇᴛɪɴᴀʟ
    that was an early-
  • 10:50 - 10:51
    ʀᴇᴛɪɴᴀʟ
    precursor to chlorophyll.
  • 10:51 - 10:51
    ʀᴇᴛɪɴᴀʟ | ᴄʜʟᴏʀᴏᴘʜʏʟʟ ᴅ
    precursor to chlorophyll.
  • 10:51 - 10:52
    ʀᴇᴛɪɴᴀʟ | ᴄʜʟᴏʀᴏᴘʜʏʟʟ ᴅ
    precursor to chlorophyll.
  • 10:52 - 10:53
    ʀᴇᴛɪɴᴀʟ | ᴄʜʟᴏʀᴏᴘʜʏʟʟ ᴅ ʀᴇᴛɪɴᴀʟ ᵖʰᵒᵗᵒˢʸⁿᵗʰᵉᵗⁱᶜ ᵖⁱᵍᵐᵉⁿᵗ
    precursor to chlorophyll.
  • 10:53 - 10:55
    ʀᴇᴛɪɴᴀʟ | ᴄʜʟᴏʀᴏᴘʜʏʟʟ ᴅ ʀᴇᴛɪɴᴀʟ ᵖʰᵒᵗᵒˢʸⁿᵗʰᵉᵗⁱᶜ ᵖⁱᵍᵐᵉⁿᵗ
  • 10:55 - 10:56
    ʀᴇᴛɪɴᴀʟ | ᴄʜʟᴏʀᴏᴘʜʏʟʟ ᴅ ʀᴇᴛɪɴᴀʟ ᵖʰᵒᵗᵒˢʸⁿᵗʰᵉᵗⁱᶜ ᵖⁱᵍᵐᵉⁿᵗ
    Some think that retinal's-
  • 10:56 - 10:57
    ʀᴇᴛɪɴᴀʟ | ᴄʜʟᴏʀᴏᴘʜʏʟʟ ᴅ ʀᴇᴛɪɴᴀʟ ᵖʰᵒᵗᵒˢʸⁿᵗʰᵉᵗⁱᶜ ᵖⁱᵍᵐᵉⁿᵗ
    molecular simplicity...
  • 10:57 - 10:58
    molecular simplicity...
  • 10:58 - 10:59
    could make it a more-
  • 10:59 - 11:01
    universal pigment.
  • 11:04 - 11:05
    If so,
  • 11:05 - 11:06
    we may find-
  • 11:06 - 11:07
    that purple...
  • 11:08 - 11:08
    is life's-
  • 11:08 - 11:09
    favorite color...
  • 11:20 - 11:22
    But the color of alien vegetation...
  • 11:22 - 11:24
    is more than just a curiosity,
  • 11:26 - 11:27
    it's chemical information-
  • 11:27 - 11:28
    that could be seen...
  • 11:28 - 11:30
    from light years away.
  • 11:34 - 11:36
    Earth plants leave a signature bump,
  • 11:37 - 11:39
    in the light reflected off our planet.
  • 11:40 - 11:42
    Finding a similar signal...
  • 11:42 - 11:43
    from another world could point the way...
  • 11:44 - 11:47
    to alien vegetation.
  • 11:50 - 11:51
    Perhaps-
  • 11:51 - 11:52
    this will be our...
  • 11:52 - 11:54
    first glimpse at alien life,
  • 11:55 - 11:56
    a vibrant hue...
  • 11:57 - 11:59
    cast by a distant world.
  • 12:12 - 12:19
    But the biggest influence on life won't be its host star;
    it will be its home planet.
  • 12:21 - 12:21
    What happens,
  • 12:21 - 12:22
    when you change the day-length...
  • 12:23 - 12:23
    of a planet?
  • 12:23 - 12:24
    What happens,
  • 12:24 - 12:24
    when you change-
  • 12:24 - 12:25
    the tilt of a planet?
  • 12:26 - 12:26
    What happens,
  • 12:26 - 12:27
    when you change-
  • 12:27 - 12:28
    the shape of the orbit?
  • 12:28 - 12:28
    What happens,
  • 12:28 - 12:29
    when you change-
  • 12:29 - 12:31
    the gravity of a planet?
  • 12:34 - 12:36
    Planets with long,
  • 12:36 - 12:37
    elliptical orbits...
  • 12:37 - 12:40
    would see drastic seasons.
  • 12:41 - 12:42
    There could be worlds...
  • 12:42 - 12:43
    did that appear dead-
  • 12:43 - 12:45
    for the thousands of years,
  • 12:45 - 12:47
    then suddenly...
  • 12:47 - 12:48
    spring to life.
  • 13:02 - 13:04
    Most of the rocky planets...
  • 13:04 - 13:05
    discovered so far-
  • 13:05 - 13:06
    have been massive-
  • 13:06 - 13:08
    "Super Earths".
  • 13:09 - 13:09
    G
  • 13:09 - 13:09
    GJ
  • 13:09 - 13:09
    GJ 3
  • 13:09 - 13:09
    GJ 35
  • 13:09 - 13:10
    GJ 357
  • 13:10 - 13:10
    GJ 357 D
  • 13:10 - 13:10
    GJ 357 D
    ˢ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄
  • 13:10 - 13:10
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜
  • 13:10 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³
  • 13:11 - 13:11
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`
  • 13:11 - 13:13
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
  • 13:13 - 13:14
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    How would life evolve...
  • 13:14 - 13:16
    GJ 357 D
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 357
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜ ⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 357
    ˢᵘᵖᵉʳ ᵉᵃʳᵗ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 357
    ˢᵘᵖᵉʳ ᵉᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 35
    ˢᵘᵖᵉʳ ᵉᵃ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃʳ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 35
    ˢᵘᵖᵉʳ ᵉ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉᵃ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds
  • 13:16 - 13:16
    GJ 35
    ˢᵘᵖᵉʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸᵉ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ: ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 3
    ˢᵘᵖᵉ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ ʸ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳᵗ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 3
    ˢᵘᵖ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰᵗ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱᵃʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ 3
    ˢᵘ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍʰ
    ᵐᵃˢˢ᠄ ˜⁷× ᴱᵃ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`ᶜ
    on these worlds?
  • 13:16 - 13:16
    GJ
    ˢ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱᵍ
    ᵐᵃˢˢ᠄ ˜⁷ˣ ᴱ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³`
    on these worlds?
  • 13:16 - 13:16
    GJ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡⁱ
    ᵐᵃˢˢ᠄ ˜⁷ˣ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵³
    on these worlds?
  • 13:16 - 13:16
    G
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹ ˡ
    ᵐᵃˢˢ᠄ ˜⁷
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻⁵
    on these worlds?
  • 13:16 - 13:16
    G
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³¹
    ᵐᵃˢˢ᠄ ˜
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜⁻
    on these worlds?
  • 13:16 - 13:16
    G
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜³
    ᵐᵃˢˢ᠄
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ˜
    on these worlds?
  • 13:16 - 13:16
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜
    ᵐᵃˢˢ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄
    on these worlds?
  • 13:16 - 13:16
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
    ᵐᵃˢ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ
    on these worlds?
  • 13:16 - 13:16
    ᵈⁱˢᵗᵃⁿᶜᵉ
    ᵐᵃ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳ
    on these worlds?
  • 13:16 - 13:16
    ᵈⁱˢᵗᵃⁿᶜ

    ᵗᵉᵐᵖᵉʳᵃᵗᵘ
    on these worlds?
  • 13:16 - 13:16
    ᵈⁱˢᵗᵃⁿ
    ᵗᵉᵐᵖᵉʳᵃᵗ
  • 13:16 - 13:16
    ᵈⁱˢᵗᵃ
    ᵗᵉᵐᵖᵉʳᵃ
  • 13:16 - 13:16
    ᵈⁱˢᵗ
    ᵗᵉᵐᵖᵉʳ
  • 13:16 - 13:16
    ᵈⁱˢ
    ᵗᵉᵐᵖᵉ
  • 13:16 - 13:16
    ᵈⁱ
    ᵗᵉᵐᵖ
  • 13:16 - 13:16

    ᵗᵉᵐ
  • 13:16 - 13:16
    ᵗᵉ
  • 13:16 - 13:16
  • 13:19 - 13:19
    In the seas,
  • 13:20 - 13:21
    gravity may not matter-
  • 13:21 - 13:22
    much at all.
  • 13:30 - 13:31
    A high-gravity planet...
  • 13:31 - 13:32
    isn't high-gravity all over,
  • 13:34 - 13:34
    If you're in the sea,
  • 13:34 - 13:36
    and that's where all life starts...
  • 13:36 - 13:38
    there's very nearly no gravity,
  • 13:38 - 13:39
    'cuz you're much the density-
  • 13:39 - 13:43
    as the stuff around you.
  • 13:43 - 13:44
    It's when the animals-
  • 13:44 - 13:45
    come out on land,
  • 13:46 - 13:48
    that they feel the gravity.
  • 13:52 - 13:53
    High g-force...
  • 13:53 - 13:54
    would necessitate-
  • 13:54 - 13:56
    large bones and muscle mass,
  • 13:56 - 13:59
    in complex life on land...
  • 14:00 - 14:01
    They would also demand-
  • 14:01 - 14:04
    a more robust circulatory system.
  • 14:05 - 14:06
    And plant life could be stunted...
  • 14:06 - 14:09
    by the energy cost of carrying nutrients-
  • 14:09 - 14:13
    under stronger gravity.
  • 14:17 - 14:19
    Low-gravity planets...
  • 14:19 - 14:19
    would more easily-
  • 14:19 - 14:22
    lose their atmospheres to space,
  • 14:22 - 14:23
    and lack a magnetic field-
  • 14:23 - 14:25
    to protect from cosmic rays.
  • 14:36 - 14:37
    But smaller worlds-
  • 14:37 - 14:39
    could be home to secret oases...
  • 14:46 - 14:47
    Huge cave systems...
  • 14:48 - 14:51
    that provide hide-outs for life.
  • 15:02 - 15:11
    With steadier temperatures and protection from cosmic rays,
    life could thrive underground on planets with deadly surfaces.
  • 15:27 - 15:28
    The smallest possible-
  • 15:28 - 15:29
    habitable planets...
  • 15:29 - 15:32
    are estimated at 2.5%-
  • 15:32 - 15:35
    Earth's mass.
  • 15:35 - 15:38
    If surface life does evolve on these worlds,
  • 15:39 - 15:41
    it could be a sight to behold.
  • 15:45 - 15:47
    Plant life could grow to towering heights,
  • 15:47 - 15:49
    able to carry nutrients higher,
  • 15:49 - 15:51
    at lesser gravity.
  • 15:59 - 16:00
    And without the need...
  • 16:00 - 16:01
    for bulky skeletons-
  • 16:01 - 16:02
    and muscle mass,
  • 16:03 - 16:04
    animals could have body types,
  • 16:04 - 16:07
    that boggle the mind.
  • 16:22 - 16:28
    Despite our eager imaginations, large complex lifeforms
    are probably a cosmic rarity.
  • 16:31 - 16:32
    Here on Earth,
  • 16:32 - 16:34
    it took three billion years-
  • 16:34 - 16:35
    for evolution...
  • 16:35 - 16:37
    to produce complex plant and animal life.
  • 16:40 - 16:42
    Simple organisms are hardier,
  • 16:42 - 16:43
    more adaptable...
  • 16:43 - 16:46
    and more widespread.
  • 16:48 - 16:50
    The largest collection-
  • 16:50 - 16:50
    in the museum-
  • 16:50 - 16:51
    of alien life...
  • 16:51 - 16:52
    would likely be...
  • 16:52 - 16:55
    the "Hall of Microbes".
  • 17:10 - 17:11
    Yet finding even-
  • 17:11 - 17:13
    the tiniest alien microbe...
  • 17:13 - 17:16
    would be a profound discovery.
  • 17:30 - 17:32
    And bite-sized life...
  • 17:32 - 17:35
    could leave a big footprint.
  • 17:36 - 17:37
    Like stromatolites on Earth,
  • 17:37 - 17:39
    layers of microbes...
  • 17:39 - 17:39
    could build up into-
  • 17:39 - 17:41
    huge rock mounds over time.
  • 17:42 - 17:44
    Leaving behind eery structures.
  • 17:49 - 17:50
    And in big enough numbers,
  • 17:50 - 17:52
    some alien bacteria...
  • 17:52 - 17:54
    could leave a distinct biosignature,
  • 17:56 - 17:57
    by exhaling gases-
  • 17:57 - 17:59
    that wouldn't coexist naturally...
  • 17:59 - 18:00
    Like oxygen...
  • 18:00 - 18:03
    and methane.
  • 18:07 - 18:08
    There's ways-
  • 18:08 - 18:09
    to make oxygen without life.
  • 18:09 - 18:09
    There's ways-
  • 18:09 - 18:10
    to make-
  • 18:10 - 18:11
    methane without life.
  • 18:11 - 18:11
    But to have them-
  • 18:11 - 18:13
    in the atmosphere together?
  • 18:13 - 18:14
    Is almost impossible...
  • 18:14 - 18:15
    unless you've got biology-
  • 18:15 - 18:16
    making those gases-
  • 18:16 - 18:16
    at the surface.
  • 18:17 - 18:18
    And it would have,
  • 18:18 - 18:20
    a imprint on the planet's-
  • 18:20 - 18:21
    spectrum of colors.
  • 18:23 - 18:25
    Next generation space telescopes-
  • 18:25 - 18:28
    could find a signal like this,
  • 18:28 - 18:32
    on a world not far from home.
  • 18:32 - 18:34
    The closest Sun-like star-
  • 18:34 - 18:36
    with an Earth-like exoplanet,
  • 18:36 - 18:38
    in the habitable zone...
  • 18:38 - 18:39
    is probably only-
  • 18:39 - 18:40
    20 light years away...
  • 18:40 - 18:41
    and can be seen...
  • 18:41 - 18:42
    with a naked eye.
  • 18:46 - 18:52
    But there may be an even easier target to aim for
    than tiny Earth-like planets.
  • 18:55 - 19:02
    The brown dwarfs: too small to be stars, to big to be planets.
  • 19:06 - 19:07
    Most Brown Dwarfs...
  • 19:07 - 19:09
    are too hot to support life-
  • 19:09 - 19:10
    as we know it.
  • 19:11 - 19:13
    But some are just cold enough.
  • 19:14 - 19:14
    W
  • 19:14 - 19:14
    WI
  • 19:14 - 19:14
    WIS
  • 19:14 - 19:14
    WISE
  • 19:14 - 19:14
    WISE 0
  • 19:14 - 19:14
    WISE 08
  • 19:14 - 19:14
    WISE 085
  • 19:14 - 19:14
    WISE 0855
  • 19:14 - 19:14
    WISE 0855-
  • 19:14 - 19:14
    WISE 0855-0
  • 19:14 - 19:14
    WISE 0855-07
  • 19:14 - 19:14
    WISE 0855-071
  • 19:14 - 19:14
    WISE 0855-0714
  • 19:14 - 19:14
    WISE 0855-0714
    ˢ
  • 19:14 - 19:15
    WISE 0855-0714
    ˢᵘ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷
  • 19:15 - 19:15
    WISE 0855-0714
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱ
  • 19:15 - 19:15
    WISE 0855-0714
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    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻¹³`ᶜ
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    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻¹³`ᶜ
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    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻¹³`ᶜ
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    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
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    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
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    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
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    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻¹³`ᶜ
  • 19:22 - 19:22
    WISE 085
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻¹³`
  • 19:22 - 19:22
    WISE 085
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻¹³
  • 19:22 - 19:22
    WISE 085
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻¹
  • 19:22 - 19:22
    WISE 085
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻ ⁻
  • 19:22 - 19:22
    WISE 085
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉʳ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻
  • 19:22 - 19:22
    WISE 085
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗᵉ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰ ⁻
  • 19:22 - 19:22
    WISE 085
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱᵗ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵⁰
  • 19:22 - 19:22
    WISE 08
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖⁱ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻⁵
  • 19:22 - 19:22
    WISE 08
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃʳ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘᵖ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻
  • 19:22 - 19:22
    WISE 08
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉᵃ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲᵘ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄
  • 19:22 - 19:22
    WISE 08
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸᵉ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ ʲ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ
  • 19:22 - 19:22
    WISE 08
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ ʸ
    ᵐᵃˢˢ᠄ ³⁻¹⁰ˣ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳ
  • 19:22 - 19:22
    WISE 0
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰᵗ
    ᵐᵃˢˢ᠄ ³⁻¹⁰
    ᵗᵉᵐᵖᵉʳᵃᵗᵘ
  • 19:22 - 19:22
    WISE 0
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳᶠ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍʰ
    ᵐᵃˢˢ᠄ ³⁻¹
    ᵗᵉᵐᵖᵉʳᵃᵗ
  • 19:22 - 19:22
    WISE 0
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱᵍ
    ᵐᵃˢˢ᠄ ³⁻
    ᵗᵉᵐᵖᵉʳᵃ
  • 19:22 - 19:22
    WISE 0
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷᵃ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡⁱ
    ᵐᵃˢˢ᠄ ³
    ᵗᵉᵐᵖᵉʳ
  • 19:22 - 19:22
    WISE 0
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈʷ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷ ˡ
    ᵐᵃˢˢ᠄
    ᵗᵉᵐᵖᵉ
  • 19:22 - 19:22
    WISE 0
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ ᵈ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ⁷
    ᵐᵃˢˢ
    ᵗᵉᵐᵖ
  • 19:22 - 19:22
    WISE
    ˢᵘᵇ⁻ᵇʳᵒʷⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
    ᵐᵃˢ
    ᵗᵉᵐ
  • 19:22 - 19:22
    WISE
    ˢᵘᵇ⁻ᵇʳᵒʷ
    ᵈⁱˢᵗᵃⁿᶜᵉ
    ᵐᵃ
    ᵗᵉ
  • 19:22 - 19:23
    WIS
    ˢᵘᵇ⁻ᵇʳᵒ
    ᵈⁱˢᵗᵃⁿᶜ

  • 19:23 - 19:23
    WIS
    ˢᵘᵇ⁻ᵇʳ
    ᵈⁱˢᵗᵃⁿ
  • 19:23 - 19:23
    WIS
    ˢᵘᵇ⁻ᵇ
    ᵈⁱˢᵗᵃ
  • 19:23 - 19:23
    WIS
    ˢᵘᵇ⁻
    ᵈⁱˢᵗ
  • 19:23 - 19:23
    WIS
    ˢᵘᵇ
    ᵈⁱˢ
  • 19:23 - 19:23
    WI
    ˢᵘ
    ᵈⁱ
  • 19:23 - 19:23
    WI
    ˢ
  • 19:23 - 19:23
    WI
    ˢ
  • 19:23 - 19:23
    WI
  • 19:23 - 19:23
    W
  • 19:24 - 19:26
    All the prime elements for life...
  • 19:26 - 19:27
    have been detected-
  • 19:27 - 19:29
    inside their atmospheres.
  • 19:31 - 19:33
    And within these clouds,
  • 19:33 - 19:34
    some layers-
  • 19:34 - 19:36
    would provide ideal temperatures-
  • 19:36 - 19:40
    and pressures for habitability.
  • 19:46 - 19:47
    There could be photosynthetic-
  • 19:47 - 19:49
    plankton in these skies,
  • 19:50 - 19:54
    kept aloft by churning upwinds.
  • 19:57 - 19:59
    And within enough force,
  • 19:59 - 20:01
    these upwinds could even support larger...
  • 20:01 - 20:04
    more complex life.
  • 20:06 - 20:08
    Predators...
  • 20:16 - 20:24
    There are over 25 billion brown dwarfs in our galaxy alone,
    and their sizes will make them easier targets for study.
  • 20:27 - 20:35
    The first specimen we discover from the museum of life
    may not be from a planet at all.
  • 20:44 - 20:47
    This raises a crucial question...
  • 20:48 - 20:48
    what if we've-
  • 20:48 - 20:49
    been looking in...
  • 20:49 - 20:51
    all the wrong places?
  • 20:52 - 20:53
    What if nature...
  • 20:53 - 20:57
    has other ideas?
  • 20:59 - 21:01
    EXHIBIT II
  • 21:01 - 21:03
    EXHIBIT II
    Life As We Know Don't It
  • 21:03 - 21:08
    EXHIBIT II
    Life As We Know Don't It
    ᴱˣᵒᵗⁱᶜ ᴮⁱᵒᶜʰᵉᵐⁱˢᵗʳⁱᵉˢ
  • 21:21 - 21:22
    Most of the Universe...
  • 21:22 - 21:24
    is too cold or too hot-
  • 21:24 - 21:25
    for liquid water,
  • 21:25 - 21:26
    and the biochemistry-
  • 21:26 - 21:27
    that supports life...
  • 21:27 - 21:29
    as we know it.
  • 21:31 - 21:34
    But in case our biases are misleading,
  • 21:35 - 21:38
    we have to cast a wide net.
  • 21:39 - 21:40
    To search for life-
  • 21:40 - 21:42
    outside the habitable zone,
  • 21:42 - 21:43
    in places that seem-
  • 21:43 - 21:47
    wildly hostile to us.
  • 21:49 - 21:51
    Exotic environments...
  • 21:51 - 21:53
    will demand exotic biochemistries.
  • 21:53 - 21:55
    And while no element-
  • 21:55 - 21:57
    can match carbon's versatility,
  • 21:57 - 21:59
    one contender is a front runner.
  • 22:00 - 22:00
    Silicon
  • 22:00 - 22:01
    Silicon
  • 22:01 - 22:01
    M
    Silicon
  • 22:01 - 22:01
    M
    Silicon
  • 22:01 - 22:01
    Mᴇ
    Silicon
  • 22:01 - 22:01
    Mᴇʟ_
    Silicon
  • 22:01 - 22:01
    Mᴇʟᴛ_
    Silicon ᴰᵉ
  • 22:01 - 22:01
    Mᴇʟᴛɪ_
    Silicon ᴰᵉ
  • 22:01 - 22:01
    Mᴇʟᴛɪɴ_
    Silicon ᴰᵉⁿ
  • 22:01 - 22:01
    Mᴇʟᴛɪɴ_
    Silicon ᴰᵉⁿ
  • 22:01 - 22:01
    Mᴇʟᴛɪɴ
    Silicon ᴰᵉⁿ
  • 22:01 - 22:01
    R_
    ᴀ_ Mᴇʟᴛɪɴɢ_
    Silicon ᴰᵉⁿˢ
  • 22:01 - 22:01
    R_
    ᴀ_ Mᴇʟᴛɪɴɢ_
    Silicon ᴰᵉⁿˢ
  • 22:01 - 22:01
    R_
    ᴀᴛ_ Mᴇʟᴛɪɴɢ ᴘ_
    Silicon ᴰᵉⁿˢ
  • 22:01 - 22:01
    R_
    ᴀᴛ_ Mᴇʟᴛɪɴɢ ᴘᴏ_
    Silicon ᴰᵉⁿˢⁱ
  • 22:01 - 22:01
    R
    ᴀᴛ Mᴇʟᴛɪɴɢᴘᴏ
    Silicon ᴰᵉⁿˢⁱ
  • 22:01 - 22:01
    R
    ᴀᴛᴏ Mᴇʟᴛɪɴɢ ᴘᴏɪ
    Silicon ᴰᵉⁿˢⁱᵗ
  • 22:01 - 22:01
    R_
    ᴀᴛᴏ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴ_
    Silicon ᴰᵉⁿˢⁱᵗ
  • 22:01 - 22:01
    R_
    ᴀᴛᴏ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ_
    Silicon ᴰᵉⁿˢⁱᵗ
  • 22:01 - 22:01
    R +_
    ᴀᴛᴏᴍ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ:_
    Silicon ᴰᵉⁿˢⁱᵗʸ
  • 22:01 - 22:01
    R +
    ᴀᴛᴏᴍ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ:
    Silicon ᴰᵉⁿˢⁱᵗʸ
  • 22:01 - 22:01
    R +
    ᴀᴛᴏᴍɪ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ:
    Silicon ᴰᵉⁿˢⁱᵗʸ
  • 22:01 - 22:01
    R +
    ᴀᴛᴏᴍɪ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ:
    Silicon ᴰᵉⁿˢⁱᵗʸ
  • 22:01 - 22:01
    R +_
    ᴀᴛᴏᴍɪ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹
    Silicon ᴰᵉⁿˢⁱᵗʸ
  • 22:01 - 22:01
    R +_
    ᴀᴛᴏᴍɪ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄
  • 22:01 - 22:01
    R +_
    ᴀᴛᴏᴍɪ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄
  • 22:01 - 22:01
    R +
    ᴀᴛᴏᴍɪᴄ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄
  • 22:01 - 22:01
    R +
    ᴀᴛᴏᴍɪᴄ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄
  • 22:01 - 22:01
    R +
    ᴀᴛᴏᴍɪᴄ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²
  • 22:01 - 22:01
    R + 7_
    ᴀᴛᴏᴍɪᴄ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²
  • 22:01 - 22:01
    R + 7_
    ᴀᴛᴏᴍɪᴄ ᴡ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²
  • 22:01 - 22:01
    R + 7_
    ᴀᴛᴏᴍɪᴄ ᴡ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ
    Silicon ᴰᵉⁿˢᶦⁱᵗʸ᠄
  • 22:01 - 22:01
    R + 7:
    ᴀᴛᴏᴍɪᴄ ᴡ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙
  • 22:01 - 22:01
    R + 7:
    ᴀᴛᴏᴍɪᴄ ᴡᴇ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙
  • 22:01 - 22:01
    R + 7:
    ᴀᴛᴏᴍɪᴄ ᴡᴇ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙
  • 22:01 - 22:01
    R + 7:_
    ᴀᴛᴏᴍɪᴄ ᴡᴇ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ B_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³
  • 22:01 - 22:01
    R + 7:_
    ᴀᴛᴏᴍɪᴄ ᴡᴇ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ B_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³
  • 22:01 - 22:01
    R + 7:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏ_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²
  • 22:01 - 22:01
    R + 7: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹
  • 22:01 - 22:01
    R + 7: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹
  • 22:01 - 22:01
    R + 7: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹
  • 22:01 - 22:01
    R + 7:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟ_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹
  • 22:01 - 22:02
    R + 7:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪ_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰
  • 22:02 - 22:02
    R + 7:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴ_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰
  • 22:02 - 22:02
    R + 7: 9 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰
  • 22:02 - 22:02
    R + 7: 9 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰
  • 22:02 - 22:02
    R + 7: 9 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰
  • 22:02 - 22:02
    R + 7: 9:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏ_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ
  • 22:02 - 22:02
    R + 7: 9:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏ_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ
  • 22:02 - 22:02
    R + 7: 9:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ:_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪ_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ
  • 22:02 - 22:02
    R + 7: 9: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕
  • 22:02 - 22:02
    R + 7: 9: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕
  • 22:02 - 22:02
    R + 7: 9: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ:
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜ
  • 22:02 - 22:02
    R + 7: 9:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ:_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ:_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜ
  • 22:02 - 22:02
    R + 7: 9:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 2_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ:_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜ
  • 22:02 - 22:02
    R + 7: 9:_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 2_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ:_
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜ
  • 22:02 - 22:02
    R + 7: 9: 5 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 2 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ
  • 22:02 - 22:02
    R + 7: 9: 56 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28._ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56._ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28._ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56._ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.0_ Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56.2 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.0 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56.2 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.08 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56.25 Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.08 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:02
    R + 7: 9: 56.25_ Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:02 - 22:03
    R + 7: 9: 56.25: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:03 - 22:05
    R + 7: 9: 56.25: Period 3
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:05 - 22:07
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:07 - 22:07
    R + 7: 9: 56.25: Metalloid
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:07 - 22:08
    R + 7: 9: 56.25: Metalloid
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    At first glance...
  • 22:08 - 22:09
    R + 7: 9: 56.25: Metalloid
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    silicon seem similar to carbon.
  • 22:09 - 22:11
    R + 7: 9: 56.25: 3.9936
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    silicon seem similar to carbon.
  • 22:11 - 22:11
    R + 7: 9: 56.25: 3.9936
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:11 - 22:11
    R + 7: 9: 56.25:
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:11 - 22:13
    R + 7: 9: 56.25: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:13 - 22:13
    R + 7: 9: 56.25: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    It forms the same four-way bonds
  • 22:13 - 22:15
    R + 7: 9: 56.25: Period 3
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    It forms the same four-way bonds
  • 22:15 - 22:15
    R + 7: 9: 56.25: Period 3
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    and is also abundant in the Universe.
  • 22:15 - 22:17
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    and is also abundant in the Universe.
  • 22:17 - 22:17
    R + 7: 9: 56.25: P-block
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:17 - 22:19
    R + 7: 9: 56.25: Metalloid
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:19 - 22:19
    R + 7: 9: 56.25: 3.9936
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
  • 22:19 - 22:20
    R + 7: 9: 56.25: 3.9936
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    But a closer look...
  • 22:20 - 22:21
    R + 7: 9: 56.25: 3.9936
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    reveals that these-
  • 22:21 - 22:21
    R + 7: 9: 56.25:
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    reveals that these-
  • 22:21 - 22:22
    R + 7: 9: 56.25:
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    two elements are false twins...
  • 22:22 - 22:23
    R + 7: 9: 56.25: Si 014
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    two elements are false twins...
  • 22:23 - 22:24
    R + 7: 9: 56.25: Period 3
    ᴀᴛᴏᴍɪᴄ ᴡᴇɪɢʜᴛ: 28.086 Mᴇʟᴛɪɴɢ ᴘᴏɪɴᴛ: ¹⁶⁸⁷ ᴷ ∕ Bᴏɪʟɪɴɢ ᴘᴏɪɴᴛ: ³⁵³⁸ ᴷ
    Silicon ᴰᵉⁿˢⁱᵗʸ᠄ ²˙³²⁹⁰ ᵍ∕ᶜᵐ³
    two elements are false twins...
  • 22:27 - 22:29
    Silicon bonds are weaker,
  • 22:29 - 22:30
    and less prone to forming-
  • 22:30 - 22:34
    large complex molecules.
  • 22:36 - 22:37
    Despite this,
  • 22:38 - 22:39
    they can withstand a wider range-
  • 22:39 - 22:40
    of temperatures,
  • 22:41 - 22:44
    opening up intriguing possibilities.
  • 22:47 - 22:49
    Life based on the silicon atom-
  • 22:49 - 22:50
    instead of carbon,
  • 22:51 - 22:52
    would be more resistant-
  • 22:52 - 22:54
    to the extreme cold.
  • 22:55 - 22:56
    Providing a whole...
  • 22:56 - 23:00
    new range of weird forms.
  • 23:01 - 23:03
    But silicon has a problem...
  • 23:04 - 23:06
    in the presence of oxygen,
  • 23:06 - 23:08
    it binds into solid rock.
  • 23:10 - 23:12
    To avoid turning to stone,
  • 23:12 - 23:13
    silicon beings might be-
  • 23:13 - 23:13
    T
    silicon beings might be-
  • 23:13 - 23:13
    TI
    silicon beings might be-
  • 23:13 - 23:13
    TIT
    silicon beings might be-
  • 23:13 - 23:13
    TITA
    silicon beings might be-
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    TITAN
    silicon beings might be-
  • 23:14 - 23:14
    TITAN
    ˢ
  • 23:14 - 23:14
    TITAN
    ˢᵃ
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗ
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ

    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙²
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ

    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗ
    confined to oxygen free environments.˙
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ

    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹
    confined to oxygen free environments.
  • 23:14 - 23:14
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`
    confined to oxygen free environments.
  • 23:14 - 23:16
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
    confined to oxygen free environments.
  • 23:16 - 23:16
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
  • 23:16 - 23:18
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
    Like Saturn's frigid moon,
  • 23:18 - 23:18
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
  • 23:18 - 23:20
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
    Titan.
  • 23:20 - 23:23
    TITAN
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
  • 23:23 - 23:23
    TITA
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`ᶜ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹`
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷⁹
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹⁷
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻¹
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ⁻
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    ᵗᵉ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ

    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗʰ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TIT
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳᵗ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃʳ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉᵃ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ ᵉ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³ˣ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²³
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰²
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄ ˙⁰
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ᠄
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢˢ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃˢ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    ᵐᵃ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ

    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏᵐ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ ᵏ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒⁿ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱᵒ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡⁱ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    TI
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡˡ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱˡ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐⁱ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙² ᵐ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙²
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹˙
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜᵉ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿᶜ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃⁿ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗᵃ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢᵗ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱˢ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    ᵈⁱ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ

    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒⁿ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒᵒ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐᵒ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ ᵐ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃⁿ
    Its vast lakes of liquid...
  • 23:23 - 23:23
    T
    ˢᵃᵗᵘʳⁿⁱᵃ
    Its vast lakes of liquid...
  • 23:23 - 23:24
    T
    ˢᵃᵗᵘʳⁿⁱ
    Its vast lakes of liquid...
  • 23:24 - 23:24
    ˢᵃᵗᵘʳⁿ
    Its vast lakes of liquid...
  • 23:24 - 23:24
    ˢᵃᵗᵘʳ
    Its vast lakes of liquid...
  • 23:24 - 23:24
    ˢᵃᵗᵘ
    Its vast lakes of liquid...
  • 23:24 - 23:24
    ˢᵃᵗ
    Its vast lakes of liquid...
  • 23:24 - 23:24
    ˢᵃ
    Its vast lakes of liquid...
  • 23:24 - 23:24
    ˢ
    Its vast lakes of liquid...
  • 23:24 - 23:24
    Its vast lakes of liquid...
  • 23:24 - 23:26
    methane and ethane-
  • 23:26 - 23:27
    could be an ideal medium-
  • 23:27 - 23:29
    for silicon-based life,
  • 23:29 - 23:36
    or other radical biochemistries.
  • 23:37 - 23:39
    Without ample sunlight,
  • 23:39 - 23:41
    beings on worlds like Titan...
  • 23:41 - 23:43
    would likely be chemosynthetic.
  • 23:43 - 23:44
    Deriving their energy-
  • 23:44 - 23:48
    by breaking down rocks.
  • 24:01 - 24:02
    Such life forms-
  • 24:02 - 24:05
    could have ultra slow metabolisms...
  • 24:05 - 24:06
    and life cycles measured-
  • 24:06 - 24:12
    in millions of years.
  • 24:16 - 24:21
    And frozen worlds aren't the only possible harbor for exotic life.
  • 24:22 - 24:23
    C
  • 24:23 - 24:23
    Co
  • 24:23 - 24:23
    CoR
  • 24:23 - 24:23
    CoRo
  • 24:23 - 24:23
    CoRoT
  • 24:23 - 24:23
    CoRoT-
  • 24:23 - 24:23
    CoRoT-7
  • 24:23 - 24:23
    CoRoT-7B
  • 24:23 - 24:23
    CoRoT-7B
    ˢ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ
  • 24:23 - 24:23
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸ
  • 24:23 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶
  • 24:24 - 24:24
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`
  • 24:24 - 24:26
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
  • 24:26 - 24:27
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
    In high temperatures,
  • 24:27 - 24:29
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
    typically rigid silicon-
  • 24:29 - 24:29
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
  • 24:29 - 24:30
    CoRoT-7B
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
    oxygen bonds become more...
  • 24:30 - 24:30
    CoRoT-7
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
    flexible and reactive.
  • 24:30 - 24:30
    CoRoT-
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
    flexible and reactive.
  • 24:30 - 24:31
    CoRoT
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`ᶜ
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶`
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²⁶
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵²
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹⁵
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻¹
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶⁻
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²⁶
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰²
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹⁰
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄ ¹
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ᠄
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳᵉ
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘʳ
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗᵘ
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃᵗ
    flexible and reactive.
  • 24:31 - 24:31
    CoRo
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳᵃ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉʳ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖᵉ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐᵖ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉᵐ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    ᵗᵉ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ

    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗʰ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳᵗ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃʳ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉᵃ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ ᵉ
    flexible and reactive.
  • 24:31 - 24:31
    CoR
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸ˣ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜⁸
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄ ˜
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ᠄
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢˢ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃˢ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ᵐᵃ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ

    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉᵃ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸᵉ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ ʸ
    flexible and reactive.
  • 24:31 - 24:31
    Co
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰᵗ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍʰ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱᵍ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡⁱ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰ ˡ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²⁰
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵²
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜⁵
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ˜
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜᵉ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿᶜ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃⁿ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗᵃ
    flexible and reactive.
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢᵗ
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱˢ
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
    ᵈⁱ
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
  • 24:31 - 24:31
    C
    ˢᵘᵖᵉʳ ᵉᵃʳᵗʰ
  • 24:31 - 24:31
    ˢᵘᵖᵉʳ ᵉᵃʳᵗ
  • 24:31 - 24:31
    ˢᵘᵖᵉʳ ᵉᵃʳ
  • 24:31 - 24:31
    ˢᵘᵖᵉʳ ᵉᵃ
  • 24:31 - 24:31
    ˢᵘᵖᵉʳ ᵉ
  • 24:31 - 24:31
    ˢᵘᵖᵉʳ
  • 24:31 - 24:31
    ˢᵘᵖᵉ
  • 24:31 - 24:31
    ˢᵘᵖ
  • 24:31 - 24:31
    ˢᵘ
  • 24:31 - 24:31
    ˢ
  • 24:33 - 24:36
    Triggering more dynamic chemistry.
  • 24:40 - 24:41
    This has led to a-
  • 24:41 - 24:43
    truly bizarre proposal...
  • 24:43 - 24:45
    silicon-based life forms,
  • 24:45 - 24:46
    that live inside-
  • 24:46 - 24:48
    molten silicate rock.
  • 25:01 - 25:02
    In theory,
  • 25:02 - 25:03
    these forms could even-
  • 25:03 - 25:04
    exist deep beneath the Earth...
  • 25:04 - 25:06
    inside magma chambers,
  • 25:06 - 25:11
    as part of a shadow biosphere.
  • 25:12 - 25:13
    If so...
  • 25:13 - 25:15
    then the aliens are right-
  • 25:15 - 25:18
    under our noses.
  • 25:21 - 25:22
    Other shadow biospheres-
  • 25:22 - 25:23
    have been proposed...
  • 25:23 - 25:25
    forms of life...
  • 25:25 - 25:25
    living alongside us-
  • 25:25 - 25:26
    that we don't even-
  • 25:26 - 25:27
    know are here.
  • 25:27 - 25:30
    Including tiny RNA-based life,
  • 25:30 - 25:32
    small enough to go undetected-
  • 25:32 - 25:34
    by existing instruments.
  • 25:44 - 25:45
    [Many billion years ago]
  • 25:47 - 25:49
    Clouds of dust and empty space,
  • 25:49 - 25:50
    might seem like the last place-
  • 25:50 - 25:53
    you did expect to find anything living.
  • 25:54 - 25:54
    Astronomical Plasma
  • 25:54 - 25:55
    Astronomical Plasma
    But when cosmic dust-
  • 25:55 - 25:57
    Astronomical Plasma
    makes contact with plasma,
  • 25:57 - 25:57
    Astronomical Plasma ⁱⁿᵗᵉʳˢᵗᵉˡˡᵃʳ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    makes contact with plasma,
  • 25:57 - 25:58
    Astronomical Plasma ⁱⁿᵗᵉʳˢᵗᵉˡˡᵃʳ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
  • 25:58 - 25:59
    Astronomical Plasma ⁱⁿᵗᵉʳˢᵗᵉˡˡᵃʳ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    a type of ionized gas...
  • 25:59 - 26:02
    Astronomical Plasma ⁱⁿᵗᵉʳˢᵗᵉˡˡᵃʳ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    something strange happens.
  • 26:02 - 26:02
    Astronomical Plasma ⁱⁿᵗᵉʳˢᵗᵉˡˡᵃʳ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
  • 26:06 - 26:08
    In simulated conditions dust particles,
  • 26:08 - 26:10
    have been seen spontaneously...
  • 26:10 - 26:11
    self-organizing into-
  • 26:11 - 26:12
    helical structures-
  • 26:12 - 26:14
    that resemble DNA.
  • 26:19 - 26:20
    These plasma crystals-
  • 26:20 - 26:21
    even begin to exhibit-
  • 26:21 - 26:23
    life-like behavior...
  • 26:24 - 26:25
    replicating,
  • 26:25 - 26:26
    evolving into more...
  • 26:26 - 26:27
    stable forms-
  • 26:27 - 26:29
    and passing on information.
  • 26:36 - 26:39
    Could these crystals be considered alive?
  • 26:42 - 26:48
    To some researchers, they meet all the criteria
    to qualify as inorganic life forms.
  • 26:52 - 26:57
    So far, we have only ever seen them in computer simulations.
  • 26:59 - 27:04
    But some speculate we could find them
    among the ice particles in the rings of Uranus.
  • 27:12 - 27:12
    Space Plasma
  • 27:12 - 27:13
    Space Plasma
    Plasma is the most-
  • 27:13 - 27:15
    Space Plasma
    common state of matter...
  • 27:15 - 27:15
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
  • 27:15 - 27:16
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    in the Universe.
  • 27:16 - 27:17
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
  • 27:17 - 27:19
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    If complex evolving-
  • 27:19 - 27:21
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    plasma crystals really exist?
  • 27:21 - 27:23
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    and if they can be considered life,
  • 27:23 - 27:23
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
  • 27:23 - 27:27
    Space Plasma ⁱⁿᵗᵉʳ⁻ ˢᵒˡᵃʳ ˢʸˢᵗᵉᵐ ⁱᵒⁿⁱᶻᵉᵈ ᵍᵃˢ
    they could be its most common form.
  • 27:39 - 27:47
    Or perhaps life is lurking in the polar opposite environment:
    inside the hearts of dead stars.
  • 27:51 - 27:53
    When massive suns explode,
  • 27:53 - 27:54
    some collapase into-
  • 27:54 - 27:55
    ultra dense cores...
  • 27:55 - 27:55
    P
    ultra dense cores...
  • 27:55 - 27:55
    PS
    ultra dense cores...
  • 27:55 - 27:55
    PSR
  • 27:55 - 27:56
    PSR B
    called neutron stars.
  • 27:56 - 27:56
    PSR B1
    called neutron stars.
  • 27:56 - 27:56
    PSR B15
    called neutron stars.
  • 27:56 - 27:56
    PSR B150
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-5
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ

    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ
    called neutron stars.
  • 27:56 - 27:56
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄
    called neutron stars.
  • 27:56 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢ
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉ
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜ
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒ
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿ
    called neutron stars.
  • 27:57 - 27:57
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    called neutron stars.
  • 27:57 - 27:58
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
  • 27:58 - 28:00
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    Hulking masses of atomic nuclei,
  • 28:00 - 28:00
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
  • 28:00 - 28:03
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    crammed together like sardines.
  • 28:03 - 28:05
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
  • 28:05 - 28:07
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    Conditions on the surface-
  • 28:07 - 28:08
    PSR B1509-58
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    are mind-boggling...
  • 28:08 - 28:08
    PSR B1509-5
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    are mind-boggling...
  • 28:08 - 28:08
    PSR B1509-
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    are mind-boggling...
  • 28:08 - 28:08
    PSR B1509
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
    are mind-boggling...
  • 28:08 - 28:08
    PSR B150
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
  • 28:08 - 28:08
    PSR B15
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
  • 28:08 - 28:08
    PSR B1
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿᵈ
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒⁿ
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜᵒ
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉᶜ
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈᶦˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡᶦᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖᶦⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢᵉ
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕ˢ
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷∕
  • 28:08 - 28:08
    PSR B
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜⁷
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄ ˜
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ᠄
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗᵉ
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃᵗ
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳᵃ
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ ʳ
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖⁱⁿ
  • 28:08 - 28:08
    PSR
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖᶦ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢᵖ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
    ˢ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳˢ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃʳ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉᵃ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸᵉ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ ʸ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰᵗ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍʰ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱᵍ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡⁱ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰ ˡ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰⁰
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰⁰
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷⁰
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹⁷
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄ ¹
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ᠄
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜᵉ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿᶜ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃⁿ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗᵃ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢᵗ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱˢ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
    ᵈⁱ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃʳ
  • 28:08 - 28:08
    PS
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢᵃ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡˢ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘˡ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖᵘ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕ ᵖ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ ∕
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃʳ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗᵃ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢᵗ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ ˢ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒⁿ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳᵒ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗʳ
  • 28:08 - 28:08
    P
    ⁿᵉᵘᵗ
  • 28:08 - 28:08
    P
    ⁿᵉᵘ
  • 28:08 - 28:08
    P
    ⁿᵉ
  • 28:08 - 28:08
    P
  • 28:08 - 28:08
    P
  • 28:09 - 28:11
    gravity is a hundred billion times...
  • 28:11 - 28:12
    stronger than Earths.
  • 28:16 - 28:18
    But beneath their iron nuclei crust lies,
  • 28:18 - 28:20
    something strange...
  • 28:21 - 28:23
    a hot dense sea...
  • 28:23 - 28:26
    of neutrons and subatomic particles.
  • 28:34 - 28:36
    Stripped of their electron shells-
  • 28:36 - 28:38
    these nuclei would obey entirely...
  • 28:38 - 28:40
    different laws of chemistry,
  • 28:40 - 28:43
    based not on the electromagnetic force,
  • 28:43 - 28:45
    but the strong nuclear force...
  • 28:45 - 28:48
    which binds nuclei together.
  • 28:49 - 28:51
    In theory...
  • 28:51 - 28:52
    these particles could link-up to form-
  • 28:52 - 28:54
    larger macronuclei...
  • 28:54 - 28:55
    which could then-
  • 28:55 - 28:57
    combine into even bigger-
  • 28:57 - 28:58
    super nuclei.
  • 29:07 - 29:08
    If so...
  • 29:08 - 29:10
    then this bewildering environment,
  • 29:10 - 29:11
    would mimic the basic-
  • 29:11 - 29:12
    conditions for life.
  • 29:12 - 29:14
    Heavy nucleon molecules,
  • 29:14 - 29:16
    floating in a complex-
  • 29:16 - 29:17
    particle ocean.
  • 29:23 - 29:24
    Some scientists have-
  • 29:24 - 29:25
    proposed the unimaginable...
  • 29:26 - 29:28
    exotic life forms...
  • 29:28 - 29:29
    drifting through the-
  • 29:29 - 29:31
    strange particle sea,
  • 29:31 - 29:32
    living evolving...
  • 29:32 - 29:35
    and dying on incomprehensibly-
  • 29:35 - 29:37
    fast time scales...
  • 29:56 - 30:01
    There's probably no chance of ever detecting
    such a strange breed of life.
  • 30:03 - 30:08
    But there may be hope for finding an even more exotic form.
  • 30:19 - 30:20
    Life is not something-
  • 30:20 - 30:24
    that has to evolve naturally.
  • 30:26 - 30:29
    It can be designed.
  • 30:41 - 30:43
    And once intelligence-
  • 30:43 - 30:44
    is introduced into the-
  • 30:44 - 30:46
    evolutionary process,
  • 30:46 - 30:48
    a Pandora's box is opened.
  • 31:06 - 31:07
    Free from typical...
  • 31:07 - 31:09
    biological limitations,
  • 31:09 - 31:11
    synthetic and machine-based life-
  • 31:11 - 31:12
    could be the most...
  • 31:12 - 31:15
    successful of all.
  • 31:16 - 31:17
    It could thrive...
  • 31:17 - 31:18
    almost anywhere,
  • 31:18 - 31:21
    including the vaccum of space,
  • 31:21 - 31:23
    opening up vast frontiers...
  • 31:23 - 31:26
    unavailable to biological organisms.
  • 31:32 - 31:33
    And compared to the glacial pace-
  • 31:33 - 31:35
    of natural selection,
  • 31:35 - 31:37
    technical evolution-
  • 31:37 - 31:38
    allows exponentially...
  • 31:38 - 31:39
    faster growth,
  • 31:39 - 31:43
    adaptability and resilience.
  • 31:56 - 31:57
    By some estimates,
  • 31:57 - 31:58
    autonomous self-
  • 31:58 - 31:59
    replicating machines...
  • 31:59 - 32:00
    could colonize...
  • 32:00 - 32:02
    an entire galaxy-
  • 32:02 - 32:02
    in as little...
  • 32:02 - 32:05
    as a million years.
  • 32:19 - 32:20
    We can't predict...
  • 32:20 - 32:21
    how hyper-intelligent life-
  • 32:21 - 32:23
    would organize itself,
  • 32:26 - 32:27
    but in theory,
  • 32:27 - 32:28
    there could be-
  • 32:28 - 32:31
    convergent evolution at play.
  • 32:32 - 32:34
    The electrical properties of Silicon-
  • 32:34 - 32:36
    might make it a universal basis...
  • 32:36 - 32:39
    for machine intelligence,
  • 32:39 - 32:40
    a redemption...
  • 32:40 - 32:45
    for its biological shortcomings.
  • 33:03 - 33:05
    With all its potential advantages,
  • 33:05 - 33:08
    With all its potential advantages, machine life may even be a universal endpoint:
  • 33:08 - 33:15
    With all its potential advantages, machine life may even be a universal endpoint:
    the apex of evolutionary process.
  • 33:53 - 33:55
    As the universe ages,
  • 33:55 - 33:57
    perhaps machine intelligence...
  • 33:57 - 33:58
    would come to dominate,
  • 33:59 - 34:00
    and naturally occurring-
  • 34:00 - 34:02
    biological life will be viewed...
  • 34:02 - 34:04
    as a quaint starting point.
  • 34:09 - 34:10
    Perhaps...
  • 34:10 - 34:11
    we ourselves...
  • 34:11 - 34:13
    will lead this transition,
  • 34:13 - 34:14
    and the great human experiment...
  • 34:15 - 34:15
    would be merely...
  • 34:15 - 34:16
    a first link-
  • 34:16 - 34:17
    in a sprawling,
  • 34:17 - 34:24
    intergalactic chain of life.
  • 34:51 - 35:02
    In the end, we are still the only beings we know of
    in the museum of alien life.
  • 35:07 - 35:10
    To truly know ourselves, we will have to know:
  • 35:10 - 35:13
    To truly know ourselves, we will have to know:
    are we the only ones?
  • 35:27 - 35:29
    Loren Eiseley has said...
  • 35:29 - 35:30
    that one does not
  • 35:30 - 35:32
    meet oneself...
  • 35:32 - 35:33
    until one catches...
  • 35:33 - 35:35
    the reflection from an eye-
  • 35:35 - 35:36
    other than human.
  • 35:39 - 35:40
    One day that eye-
  • 35:40 - 35:41
    maybe that...
  • 35:41 - 35:42
    of an intelligent alien.
  • 35:46 - 35:47
    And the sooner-
  • 35:47 - 35:48
    we eschew our...
  • 35:48 - 35:52
    narrow view of evolution,
  • 35:52 - 35:53
    the sooner-
  • 35:53 - 35:54
    we can...
  • 35:54 - 35:56
    truly explore,
  • 35:56 - 35:58
    our ultimate origins...
  • 35:58 - 36:02
    and destinations.
  • 36:04 - 36:07
    We have seen what could be out there.
  • 36:10 - 36:13
    And we know how we might find it.
  • 36:16 - 36:19
    There is only one thing left to do.
  • 36:22 - 36:26
    Go looking.
  • 36:27 - 36:28
    End Credit In 3...
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    End Credit In 2...
  • 36:29 - 36:30
    End Credit In 1...
  • 36:30 - 36:31
    End Credit In 0.99...
  • 36:31 - 36:31
    End Credit In 0.98...
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    End Credit In 0.97...
  • 36:31 - 36:31
    End Credit In 0.96...
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    End Credit In 0.95...
  • 36:31 - 36:31
    End Credit In 0.94...
  • 36:31 - 36:31
    End Credit In 0.93...
  • 36:31 - 36:31
    End Credit In 0.92...
  • 36:31 - 36:31
    End Credit In 0.92...
  • 36:31 - 36:31
    End Credit In 0.91...
  • 36:31 - 36:31
    End Credit In 0.90...
  • 36:31 - 36:31
    End Credit In 0.89...
  • 36:31 - 36:31
    End Credit In 0.89...
  • 36:31 - 36:31
    End Credit In 0.88...
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    End Credit In 0.87...
  • 36:31 - 36:31
    End Credit In 0.86...
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    End Credit In 0.85...
  • 36:31 - 36:31
    End Credit In 0.84...
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    End Credit In 0.83...
  • 36:31 - 36:31
    End Credit In 0.82...
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    End Credit In 0.82...
  • 36:31 - 36:31
    End Credit In 0.81...
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    End Credit In 0.80...
  • 36:31 - 36:31
    End Credit In 0.79...
  • 36:31 - 36:31
    End Credit In 0.78...
  • 36:31 - 36:31
    End Credit In 0.77...
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    End Credit In 0.76...
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    End Credit In 0.75...
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    End Credit In 0.74...
  • 36:31 - 36:31
    End Credit In 0.73...
  • 36:31 - 36:31
    End Credit In 0.72...
  • 36:31 - 36:31
    End Credit In 0.71...
  • 36:31 - 36:31
    End Credit In 0.70...
  • 36:31 - 36:31
    End Credit In 0.69...
  • 36:31 - 36:31
    End Credit In 0.68...
  • 36:31 - 36:31
    End Credit In 0.67...
  • 36:31 - 36:31
    End Credit In 0.67...
  • 36:31 - 36:31
    End Credit In 0.66...
  • 36:31 - 36:31
    End Credit In 0.65...
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    End Credit In 0.64...
  • 36:31 - 36:31
    End Credit In 0.64...
  • 36:31 - 36:31
    End Credit In 0.63...
  • 36:31 - 36:31
    End Credit In 0.62...
  • 36:31 - 36:31
    End Credit In 0.61...
  • 36:31 - 36:31
    End Credit In 0.60...
  • 36:31 - 36:31
    End Credit In 0.59...
  • 36:31 - 36:31
    End Credit In 0.58...
  • 36:31 - 36:31
    End Credit In 0.57...
  • 36:31 - 36:31
    End Credit In 0.57...
  • 36:31 - 36:31
    End Credit In 0.56...
  • 36:31 - 36:31
    End Credit In 0.54...
  • 36:31 - 36:31
    End Credit In 0.53...
  • 36:31 - 36:31
    End Credit In 0.52...
  • 36:31 - 36:31
    End Credit In 0.51...
  • 36:31 - 36:31
    End Credit In 0.50...
  • 36:31 - 36:31
    End Credit In 0.49...
  • 36:31 - 36:31
    End Credit In 0.48...
  • 36:31 - 36:31
    End Credit In 0.47...
  • 36:31 - 36:31
    End Credit In 0.46...
  • 36:31 - 36:31
    End Credit In 0.45...
  • 36:31 - 36:31
    End Credit In 0.44...
  • 36:31 - 36:31
    End Credit In 0.43...
  • 36:31 - 36:31
    End Credit In 0.42...
  • 36:31 - 36:31
    End Credit In 0.41...
  • 36:31 - 36:31
    End Credit In 0.41...
  • 36:31 - 36:31
    End Credit In 0.40...
  • 36:31 - 36:31
    End Credit In 0.40...
  • 36:31 - 36:31
    End Credit In 0.39...
  • 36:31 - 36:31
    End Credit In 0.38...
  • 36:31 - 36:31
    End Credit In 0.37...
  • 36:31 - 36:31
    End Credit In 0.36...
  • 36:31 - 36:31
    End Credit In 0.35...
  • 36:31 - 36:31
    End Credit In 0.34...
  • 36:31 - 36:31
    End Credit In 0.33...
  • 36:31 - 36:31
    End Credit In 0.32...
  • 36:31 - 36:31
    End Credit In 0.31...
  • 36:31 - 36:31
    End Credit In 0.31...
  • 36:31 - 36:31
    End Credit In 0.30...
  • 36:31 - 36:31
    End Credit In 0.29...
  • 36:31 - 36:31
    End Credit In 0.28...
  • 36:31 - 36:31
    End Credit In 0.27...
  • 36:31 - 36:31
    End Credit In 0.26...
  • 36:31 - 36:31
    End Credit In 0.25...
  • 36:31 - 36:31
    End Credit In 0.24...
  • 36:31 - 36:31
    End Credit In 0.23...
  • 36:31 - 36:31
    End Credit In 0.22...
  • 36:31 - 36:31
    End Credit In 0.21...
  • 36:31 - 36:31
    End Credit In 0.20...
  • 36:31 - 36:31
    End Credit In 0.19...
  • 36:31 - 36:31
    End Credit In 0.18...
  • 36:31 - 36:31
    End Credit In 0.17...
  • 36:31 - 36:31
    End Credit In 0.16...
  • 36:31 - 36:31
    End Credit In 0.15...
  • 36:31 - 36:31
    End Credit In 0.14...
  • 36:31 - 36:31
    End Credit In 0.13...
  • 36:31 - 36:31
    End Credit In 0.13...
  • 36:31 - 36:31
    End Credit In 0.12...
  • 36:31 - 36:31
    End Credit In 0.11...
  • 36:31 - 36:31
    End Credit In 0.10...
  • 36:31 - 36:31
    End Credit In 0.09...
  • 36:31 - 36:31
    End Credit In 0.08...
  • 36:31 - 36:31
    End Credit In 0.07...
  • 36:31 - 36:31
    End Credit In 0.06...
  • 36:31 - 36:31
    End Credit In 0.05...
  • 36:31 - 36:31
    End Credit In 0.05...
  • 36:31 - 36:31
    End Credit In 0.04...
  • 36:31 - 36:31
    End Credit In 0.03...
  • 36:31 - 36:31
    End Credit In 0.03...
  • 36:31 - 36:31
    End Credit In 0.02...
  • 36:31 - 36:31
    End Credit In 0.01...
  • 36:33 - 36:34
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34

    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴ

    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪ
    ᴇʀ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪs
    ᴇʀɴ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ
    ᴇʀɴᴇ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇs

    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀ
    ᴇʀ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏ
    ᴇʀɪ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏs
    ᴇʀɪᴄ

    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ
    ᴇʀɪᴄᴋ
    ᴋɪ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊ
    ᴇʀɪᴄᴋ s
    ᴋɪʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀ
    ᴇʀɪᴄᴋ sᴏ
    ᴋɪʟʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:34
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄ
    ᴇʀɪᴄᴋ sᴏᴀ
    ᴋɪʟʟᴇ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:34 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋ
    ᴇʀɪᴄᴋ sᴏᴀʀ
    ᴋɪʟʟᴇʀ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇ
    ᴋɪʟʟᴇʀɢ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs
    ᴋɪʟʟᴇʀɢʜ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰ
    ᴋɪʟʟᴇʀɢʜᴏ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪ
    ᴋɪʟʟᴇʀɢʜᴏᴜ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢᴜ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢᴜᴇ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢᴜᴇɪ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢᴜᴇɪʀ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢᴜᴇɪʀᴇ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:35
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢᴜᴇɪʀᴇᴅ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:35 - 36:37
    ᴄᴀᴘᴛɪᴏɴɪsᴛ :
    ᴇʀɴᴇsʀʏsᴛ ᴊᴀᴄᴋɪɴɴ
    ᴇʀɪᴄᴋ sᴏᴀʀᴇs ꜰɪɢᴜᴇɪʀᴇᴅᴏ
    ᴋɪʟʟᴇʀɢʜᴏᴜʟ
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:37 - 36:41
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
  • 36:41 - 36:43
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
    Sᴜᴘᴘᴏʀᴛᴇᴅ ʙʏ
  • 36:43 - 36:49
    𝐇𝐀𝐍𝐃 𝐂𝐑𝐀𝐅𝐓𝐄𝐃 𝐁𝐘 𝐌𝐄𝐋𝐎𝐃𝐘𝐒𝐇𝐄𝐄𝐏
    Sᴜᴘᴘᴏʀᴛᴇᴅ ʙʏ
    Protocol Labs
  • 36:49 - 36:50
    Sᴜᴘᴘᴏʀᴛᴇᴅ ʙʏ
    Protocol Labs
    ɴᴀʀʀᴀᴛᴇᴅ ʙʏ
  • 36:50 - 36:51
    Protocol Labs
    ɴᴀʀʀᴀᴛᴇᴅ ʙʏ
    Will Crowley
  • 36:51 - 36:53
    ɴᴀʀʀᴀᴛᴇᴅ ʙʏ
    Will Crowley
    ᴄᴏɴᴄᴇᴘᴛ, ᴍᴜsɪᴄ, & ᴠɪsᴜᴀʟs ʙʏ
  • 36:53 - 36:54
    Will Crowley
    ᴄᴏɴᴄᴇᴘᴛ, ᴍᴜsɪᴄ, & ᴠɪsᴜᴀʟs ʙʏ
    Melodysheep (John D. Boswell)
  • 36:54 - 36:55
    ᴄᴏɴᴄᴇᴘᴛ, ᴍᴜsɪᴄ, & ᴠɪsᴜᴀʟs ʙʏ
    Melodysheep (John D. Boswell)
    ᴡɪᴛʜ ᴀᴅᴅɪᴛɪᴏɴᴀʟ ᴠɪsᴜᴀʟs ʙʏ
  • 36:55 - 36:56
    Melodysheep (John D. Boswell)
    ᴡɪᴛʜ ᴀᴅᴅɪᴛɪᴏɴᴀʟ ᴠɪsᴜᴀʟs ʙʏ
    Lynn Huberty
  • 36:56 - 36:57
    ᴡɪᴛʜ ᴀᴅᴅɪᴛɪᴏɴᴀʟ ᴠɪsᴜᴀʟs ʙʏ
    Lynn Huberty
    Tim Stupak
  • 36:57 - 36:57
    Lynn Huberty
    Tim Stupak
    NASA
  • 36:57 - 36:59
    Tim Stupak
    NASA
    Evolve
  • 36:59 - 37:00
    NASA
    Evolve
    sᴏᴜɴᴅʙɪᴛᴇs ꜰʀᴏᴍ
  • 37:00 - 37:01
    Evolve
    sᴏᴜɴᴅʙɪᴛᴇs ꜰʀᴏᴍ
    Nick Lane
  • 37:01 - 37:02
    sᴏᴜɴᴅʙɪᴛᴇs ꜰʀᴏᴍ
    Nick Lane
    Jonathan Losos
  • 37:02 - 37:02
    Nick Lane
    Jonathan Losos
    Caleb Scharf
  • 37:02 - 37:03
    Jonathan Losos
    Caleb Scharf
    Jack Cohen
  • 37:03 - 37:05
    Caleb Scharf
    Jack Cohen
    Jill Tarter
  • 37:05 - 37:06
    Jack Cohen
    Jill Tarter
    sᴘᴇᴄɪᴀʟ ᴛʜᴀɴᴋs ᴛᴏ
  • 37:06 - 37:07
    Jill Tarter
    sᴘᴇᴄɪᴀʟ ᴛʜᴀɴᴋs ᴛᴏ
    Juan Benet
  • 37:07 - 37:07
    sᴘᴇᴄɪᴀʟ ᴛʜᴀɴᴋs ᴛᴏ
    Juan Benet
    Rowdy Jansen
  • 37:07 - 37:08
    Juan Benet
    Rowdy Jansen
    Lynn Huberty
  • 37:08 - 37:09
    Rowdy Jansen
    Lynn Huberty
    Tim Stupak
  • 37:09 - 37:10
    Lynn Huberty
    Tim Stupak
    Joel Edwards
  • 37:10 - 37:11
    Tim Stupak
    Joel Edwards
    Melodysheep Patreon supporters
  • 37:11 - 37:12
    Joel Edwards
    Melodysheep Patreon supporters
    sᴜᴘᴘᴏʀᴛ ᴛʜɪs ᴘʀᴏᴅᴜᴄᴛɪᴏɴ ᴀᴛ
  • 37:12 - 37:14
    Melodysheep Patreon supporters
    sᴜᴘᴘᴏʀᴛ ᴛʜɪs ᴘʀᴏᴅᴜᴄᴛɪᴏɴ ᴀᴛ
    patreon.com/melodysheep
  • 37:14 - 37:14
    sᴜᴘᴘᴏʀᴛ ᴛʜɪs ᴘʀᴏᴅᴜᴄᴛɪᴏɴ ᴀᴛ
    patreon.com/melodysheep
    Melodysheep.com
  • 37:14 - 37:15
    patreon.com/melodysheep
    Melodysheep.com
    Twitter: @musicalscience
  • 37:15 - 37:17
    Melodysheep.com
    Twitter: @musicalscience
    Instagram: @melodysheep
  • 37:17 - 37:18
    Twitter: @musicalscience
    Instagram: @melodysheep
    ᵃⁿ
  • 37:18 - 37:19
    Instagram: @melodysheep
    ᵃⁿ
    Amber Mountain Studios
  • 37:19 - 37:28
    ᵃⁿ
    Amber Mountain Studios
    ᴘʀᴏᴅᴜᴄᴛɪᴏɴ
  • 37:30 - 37:37
    ɴᴇxᴛ ᴏɴ ʟɪꜰᴇ ʙᴇʏᴏɴᴅ:
    Making contact with intelligent life
    Intergalactic civilizations
    Surviving the end of the universe
  • 37:39 - 37:46
    sᴏᴜɴᴅᴛʀᴀᴄᴋ ᴄᴏᴍɪɴɢ ᴛᴏ ᴀʟʟ ᴍᴀᴊᴏʀ ᴍᴜsɪᴄ ᴘʟᴀᴛꜰᴏʀᴍs
  • 37:47 - 37:54
    sᴜᴘᴘᴏʀᴛ ᴛʜᴇ ɴᴇxᴛ ᴄʜᴀᴘᴛᴇʀ ᴀᴛ:
    patreon.com/melodysheep
Titre:
LIFE BEYOND II: The Museum of Alien Life (4K)
Description:

Soundtrack: https://bit.ly/3lo7cnH Support this project on Patreon: http://patreon.com/melodysheep

What if there was a museum that contained every type of life form in the universe? This experience takes you on a tour through the possible forms alien life might take, from the eerily familiar to the utterly exotic, ranging from the inside of the Earth to the most hostile corners of the universe.

New research is upending our idea of life and where it could be hiding: not just on Earth-like planets, where beings could mimic what our planet has produced, but in far flung places like the hearts of dead stars and the rings of gas giant planets. Nowhere in the universe is off limits.

Only when we know what else is out there will we truly know ourselves. This thought experiment will give us a glimpse into what could be out there, how we might find it, and just how far nature’s imagination might stretch.

Big thanks to Protocol Labs for their continued support of this series: https://protocol.ai.

Concept, visuals, and score by melodysheep, aka John D. Boswell. Narrated by Will Crowley. Additional visuals by Lynn Huberty, Tim Stupak, NASA, and Evolve. Featuring soundbites from Nick Lane, Jonathan Losos, Caleb Scharf, Jack Cohen, and Jill Tarter.

Featuring clips from Lynn Huberty’s amazing film “SHYAMA”: https://bit.ly/3d6xtUF

Thanks especially to:
Lynn Huberty
Juan Benet
Rowdy Jansen
Eddy Adams: http://www.eddyadams.com
Kimi Ushida: http://Eff.org
Gregory Cohen: www.DesignFirebrand.com
Eric Capuano: http://reconinfosec.com
John Maier
Logan
Ali Aljumayd
Caleb Levesque
Eric Malette
Brandon Sanders
Tim Stupak

And to all my supporters on Patreon: Ada Cerna, Adam Orand, Ajish Balakrishnan, Aksel Tjønn, Ali Akın Kurnaz, Andrew Edwards, Andrew Valenti, Antoine C, Antoni Simelio, Augustas Babelis, Bhisham Mahtani, Bradley Gallant, Brant Stokes, Daniel Saltzman, Caleb Levesque, Case K., Cheshire 2e du nom, Chinmay Kumar, Chris Wilken, Christian Oehne, Christina Winikoff, Christopher Heald, Chung Tran, Colin Glover, Corentin Kerisit, Cozza38, Crystal, Dan Alvesved, Danaos Christopoulos, Dave LeCompte, Davee Hallinan, David Lyneham, david p boswell, David Southpaw, denise frey, Derick Yan, Dexter, dixon1829, Don Loristo, Dylan Webb, Eico Neumann, Eyubed Balcha, Ezri Dax, Gaétan Marras, Gary Wei, geekiskhan, Genesplicer, Giulia C., Håkon A. Hjortland, Hans Husurianto, Henry R. Seymour, Heribert Breidsamer, ilkercan Kaya, Iota Katari, is8ac, Jackie Pham, James O'Connor, Jayson Hale, Jean Neyrial, Jessica Turner, Jimpy, JM_Borg, Jordan Swickard, Jose Contreras, Joshua Oram, JousterL, Julian Büttner, Julio Hernández Camero, kaynen brown, Kristin & Alan Cameron, Laine Boswell, Lars Støttrup Nielsen, Laura, Laura Liddington, Layne Burnett, LemonHead, Lennart Klootwijk, Leo Botinelly, Leonard van Vliet, lloll887, Manu Galán García, Maraiu, Marco Cardamone, Mark Christopher, Mark T., Markus Oinonen, Marlin Balzer, Martin Majernik, Matthew Jacoby, Matthew Ullrich, Maxime Marois, Mehdi Bennani, Michael Li, Michelle Wilcox, Mike Norkus, Mind Wave, Mitchel Humpherys, Mohammed Aldaabil, Nathan, Nicholas Martin, Nikita Temryazansky, Nina Atesh, Nina Barton, Ninel, Patrick Keim, Patrick Schouten, Peycho Ivanov, PonWer, Preston Maness, Radu Turcan, Ramsey Elbasheer, Randall Bollig, Raz, RedOptics, Reg Reyes, Richard Sundvall, Richard Williams, Rob Phillips, Robin Kuenkel, Runi Winther Johnsen, Samih Fadli, Sandra, Sandro Heinimann, Scarlet Fortuna, Silas Rech, SilverFolfy, Smoka_Lad, SpartanLegends, Stefan, SunaScorpion, SymeSynth, The Cleaner, The Fellowship of Doge, TheHumungus, Timothé Wegiersky, Timothy E Plum, Trevor Robertson, Verissimus, Vinh Vo, Virgile Coulot, Whitney Champion, William Ronholm, Wise Doane, Wolfgang Bernecker, Yannic, ZAB, Алексей Козловский

Sources coming soon.

Peace and love,

melodysheeep
http://melodysheep.com
twitter: @musicalscience
instagram: @melodysheep_

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Langue de la vidéo:
English
Durée:
38:00

sous-titres en English

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