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  • It took Clyde Tombaugh half a year

  • of manually looking at photographic

  • plates, contains over two million stars

  • before he discovered Pluto.

  • and its in our own solar system.

  • So how on earth, does one find a planet orbiting a distant star?

  • You could just look,

  • but stars are so far away,

  • and so bright compared to their planets,

  • that its really hard to just look at one, and see a planet orbiting it.

  • Direct discovery of new exoplanets by

  • just looking, is essentially limited to

  • relatively nearby stars,

  • with very large planets, very far away from them.

  • Think 10 times the size of jupiter, and an orbit at least as big.

  • The vast majority of exoplanets,

  • have been found indirectly, by observing their effects on their parents stars.

  • For example, a planet passing in front of a star will make

  • that star darker for a little while.

  • and the amount it darkens, will tell you about the size of the planet, relative to the size of the star.

  • of course this only works if the planets orbit is tilted perfectly to pass between us and its star.

  • and on average less than 1% of earth like planets will have this convenient orbital orientation.

  • We have managed to find a lot of exoplanets this way,

  • by exhaustive satellite searches.

  • but you could instead have a look at the effect planets have on the motion of stars.

  • as we know, planets don't orbit stars.

  • Rather, both orbit around their combined centre of mass.

  • Stars are so heavy, so often the centre of mass is inside the star,

  • but the star will nonetheless be moving.

  • That motion manifests itself as a teeny tiny wobble,

  • in the velocity of the star relative to us.

  • which we determine by carefully measuring the red or blue doppler shift

  • of the stars light

  • both these indirect methods are most effective at finding big planets,

  • close to their stars,

  • because the speeds involved, and the amount of light blocked

  • are greater, and also because close planets orbit more often

  • so we don't have to wait as long to notice their effects.

  • There are other more complicated and fancy methods which can find planets

  • which are harder to notice by a star wobbling or star light blocking

  • and all of these together have helped to discover

  • more than 1800 exoplanets

  • as of 2014.

  • Sorry pluto, you've been Ex-ed out!

  • This video is brought to you in part by Audible.com,

  • The leading provider of audio books across all types of literature, including

  • fiction, non-fiction and periodicals.

  • If you go to audible.com/minutephysics,

  • you can try Audible out by downloading a free audiobook of your choice.

  • I would like to recommend the book 'Foundation'.

  • It's the opening act of Isaac Asimov's

  • opening saga about the impending collapse of interstellar civilisation.

  • You can download your free audiobook at Audible.com/minutephysics

  • and I would like to say thanks to Audible for helping me continue to make these videos.

It took Clyde Tombaugh half a year

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B1 中級

外惑星の探し方 (How to Find an Exoplanet)

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    林宜悉 に公開 2021 年 01 月 14 日
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