full transcript
From the Ted Talk by Fabio Pacucci: Newton's three-body problem explained
Unscramble the Blue Letters
In 2009, two researchers ran a simple experiment. They took everything we know about our solar system and calculated where every planet would be up to 5 billion years in the future. To do so they ran over 2,000 numerical simulations with the same exact itiainl conditions except for one difference: the distance between Mercury and the Sun, modified by less than a millimeter from one simulation to the next. Shockingly, in about 1 percent of their slnuaimtois, Mercury’s obirt changed so dtlcslariay that it could plunge into the Sun or collide with vuens. Worse yet, in one simulation it destabilized the entire inner solar system. This was no error; the astonishing variety in results reelavs the tutrh that our solar system may be much less stable than it seems.
Open Cloze
In 2009, two researchers ran a simple experiment. They took everything we know about our solar system and calculated where every planet would be up to 5 billion years in the future. To do so they ran over 2,000 numerical simulations with the same exact _______ conditions except for one difference: the distance between Mercury and the Sun, modified by less than a millimeter from one simulation to the next. Shockingly, in about 1 percent of their ___________, Mercury’s _____ changed so ___________ that it could plunge into the Sun or collide with _____. Worse yet, in one simulation it destabilized the entire inner solar system. This was no error; the astonishing variety in results _______ the _____ that our solar system may be much less stable than it seems.
Solution
- initial
- truth
- reveals
- drastically
- orbit
- venus
- simulations
Original Text
In 2009, two researchers ran a simple experiment. They took everything we know about our solar system and calculated where every planet would be up to 5 billion years in the future. To do so they ran over 2,000 numerical simulations with the same exact initial conditions except for one difference: the distance between Mercury and the Sun, modified by less than a millimeter from one simulation to the next. Shockingly, in about 1 percent of their simulations, Mercury’s orbit changed so drastically that it could plunge into the Sun or collide with Venus. Worse yet, in one simulation it destabilized the entire inner solar system. This was no error; the astonishing variety in results reveals the truth that our solar system may be much less stable than it seems.
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