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    Why Don't We Know If There Are More Planets Around Alpha Centauri?
    By Robert Cooper | October 24th 2012 11:11 AM | 4 comments | Print | E-mail | Track Comments
    About Robert

    I have given up on categories. I did a BA in physics, a PhD in molecular biology, and now a postdoc in a bioengineering department. So call that...

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    Alpha Centauri is the closest star system to Earth other than our own sun.  So one would think if it had planets, we would know by now, right?  Wrong, apparently.  Astronomers just announced the discovery of an Earth-sized planet in Alpha Centauri, although it's closer to its star than Mercury is to our sun, so unlikely to have life.  However, there may actually be even more planets further out from the star!  So why are we only just now discovering planets in our nearest neighboring solar system, and why don't we know yet if there are more?

    Two reasons: planetary mass, and distance from the star.  Unfortunately, the smaller a planet is, and the further it is from its star, the more difficult it is to detect.  This is because of the way we spot planets – by looking for the way they make their stars wobble.  Imagine swinging a heavy bucket around you in circles.  The bucket goes around, but you wobble too, just like planets make the stars they orbit wobble.  As the star wobbles towards us and away from us, there is a doppler shift in the star's light, similar to how a car horn coming at you sounds higher-pitched than a car horn moving away from you.  The size of the doppler shift depends on how fast the star is wobbling.

    Ok, some quick math here.  The momentum of a system is conserved, so the star's maximum momentum while wobbling towards us equals the planet's maximum momentum while orbiting away from us, or (lower case for the planet, upper case for the star).  So the velocity of the star is
    Ok good, but what's the velocity of the planet, v?  Well, for an orbit to be stable, the gravitational force on the planet   has to equal the centripetal force to keep it in orbit, .  Set those two equal and solve for v, and you get
    Now, combining equations 1 and 2, we can see how the star's wobble velocity depends on the planet's size and orbit:
    So smaller planets (small m) make a smaller wobble, and planets that are further out (large r) make a smaller wobble.  Since finding this Earth-sized planet that's so super-close to its star already "pushed our technique to the limit", finding Earth-like planets farther out where life (as we know it) could exist will be even tricker.  But techniques keep on pushing, so stay tuned!


    Pretty good article.  You broke it down in a way that anyone who knows algebra should understand with minimal effort.  

    Science advances as much by mistakes as by plans.
    Thanks!  Got a head start by TAing an astrobiology course last year.
    Astrobiology is big and going to get bigger. If you get up to Northern California, I will introduce you to UCSC's Dave Deamer, who writes here on the subject (and various books too).
    Hmm, that sounds like fun.  Astrobio isn't really my main focus, but it is interesting (I actually did the course mainly for the Yellowstone field trip looking for extremophiles)