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Two Planets Found Sharing One Orbit

dweezil-n0xad writes "Buried in the flood of data from the Kepler telescope is a planetary system unlike any seen before. Two of its apparent planets share the same orbit around their star. If the discovery is confirmed, it would bolster a theory that Earth once shared its orbit with a Mars-sized body that later crashed into it, resulting in the moon's formation."

33 of 175 comments (clear)

  1. Time for another IAU meeting by edalytical · · Score: 4, Funny

    Quick, we need to redefine the meaning of "planet" yet again.

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    1. Re:Time for another IAU meeting by painandgreed · · Score: 5, Interesting

      Quick, we need to redefine the meaning of "planet" yet again.

      Possibly. As neither has "cleared its neighbourhood" of other masses in their neighborhood, they might be back to being called planetoids like Pluto. Both are to be considered "dwarf planets" until they collide and one becomes obviously dominant. There's already bits that cover things like this, but people are already arguing about the exampled in our own solar system. I be something like this would cause even more hub bub and another conference to further define the meaning of planet yet again.

    2. Re:Time for another IAU meeting by Anonymous Coward · · Score: 3, Insightful

      Quick, we need to redefine the meaning of "planet" yet again.

      Yeah... because it's been changed so many times, right? And for no good reason to boot, right?

      Truth is, the term "planet" has only really been defined once, a few years ago. before that, we had an intuitive idea of what a "planet" was; we included Pluto, as it appeared to be a comparatively unique object, but then we found that Pluto isn't unique and that there is no reason to believe that we wouldn't have millions (at least!) of planets, since there'll be that many objects that all share Pluto's characteristics and that'll have the same right to be called "planet".

      Not a good solution, obviously, so we looked for something different and came up with a better, precise definition. And yes, that meant that Pluto lost its "planet" status... but that's happened before; Ceres was considered a planet when it was first found. Until, that is, people noticed that it was just one of a ton of objects that would then also have to be called "planets" if Ceres was one. Sound familiar? It's basically exactly Pluto's situation.

      Now maybe you don't see keeping the number of planets down as a worthwhile goal, but personally, I think that if you're thinking that the four major rocky planets in the inner solar system and the four gas giants in the outer solar system do not stand out from millions of asteroids and Kuiper belt objects, then you're deluded. They do.

      Doesn't mean the remaining objects aren't interesting, mind you, but that's just you attaching too much significance to the label "planet" in the first place.

    3. Re:Time for another IAU meeting by Anonymous Coward · · Score: 3, Funny

      There can only be one!

    4. Re:Time for another IAU meeting by Jiro · · Score: 2, Interesting

      That's not what "clearing the neighborhood" is defined as. "Clearing the neighborhood" contains an exemption for other objects under the first object's gravitational influence.

      If there are two objects in one orbit *and* the objects stay that way because of some complicated gravitational interaction, they are exempt from "clearing the neighborhood" and can still count as planets. In order to not count as planets you'd have to have two objects in the same orbit that just stay there because they happen to be in the same orbit, without any gravitational forces keeping it that way.

      It's highly likely that these two objects are staying in that orbit because of gravitational interactions, and therefore they are probably planets.

      Or they would be, except that the definition of "planet" used to disqualify Pluto specifically says it only applies to our own solar system. It couldn't be applied to other systems anyway, since we can't see enough smaller objects in other solar systems to know whether the neighborhood has been cleared or not. Currently, the definition used outside the solar system has problems at its lower size limits.

    5. Re:Time for another IAU meeting by Ambiguous+Coward · · Score: 4, Interesting

      Is an estimated minimum of 2 million more years not stable enough for you? With the two planets orbiting their star about every 10 earth days, that's over 70 million orbits, at minimum. What makes this an interesting find it that it IS unlikely, and it does NOT require external forces. Hence there's an article about it. :)

      As referenced by TFA: http://en.wikipedia.org/wiki/Lagrange_point

      Unless you're claiming that nothing is stable because y'know, entropy, man!

      --
      Their may be a grammatical error, misspeling, or evn a typo in this post.
    6. Re:Time for another IAU meeting by Artifakt · · Score: 4, Informative

      The definition that makes Pluto a dwarf planet specifically apples only to our solar system, and the part that calls for clearing the orbit was inserted in case a Kuiper belt object actually bigger than Mercury was found later, so the IAU would not have to debate the subject again, not as a straight-forward rule based on any physical fact. Incidentally, the belt is named after Kuiper because he was a. the third major working astronomer to propose such as zone, and b. the first to be fundamentally wrong about its nature, as he claimed such a belt could not still exist.
            All the debate about how to define a an extra-solar planet will be driven by the very people who have totally screwed up any rational, scientific definitions when it comes to our own solar system. Expect a rule about how planets in the 'northern' part of the galaxy must have an eccentricity of less than 5.2%, and planets in the direction of Virgo are allowed 7.1%, but only if they move in square orbits on alternate St. Swithen'sdays.

      --
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    7. Re:Time for another IAU meeting by rrohbeck · · Score: 4, Funny

      Nothing is stable. All orbits change chaotically in the long term.
      Corollary: There are no planets.

    8. Re:Time for another IAU meeting by sumdumass · · Score: 2

      Well, it pointless to start or maintain an argument because of this discover. what they are observing is the Death star beta production facility. It just took a long time for the light to eventually reach us. But then again, it all happened A long time ago in a galaxy far, far away.

    9. Re:Time for another IAU meeting by cowboy76Spain · · Score: 2

      Even with the center of mass of each planet exactly in the L point of the other, then if the planet has a radius of 100km, parts of it will be 100kms away from the lagrange point --> inestability, whatever long it takes to become catastrophic.

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    10. Re:Time for another IAU meeting by Brucelet · · Score: 2

      The L4 and L5 points are actually stable equilibria, meaning that a body a very short distance away from the L-point will circle it. I would guess instability is more likely to come from effects like orbits being not perfectly planar and circular, and perturbations from other bodies in the system, rather than from being not quite on the L-point.

    11. Re:Time for another IAU meeting by Narcogen · · Score: 2

      Other fun facts about the universe: The universe contains no population, no money, and no sex*.

      (*Actually there is quite a lot of this.)

      Corollary: sex is entropy.

      Corollary to the corollary: Slashdot is immune to entropy.

    12. Re:Time for another IAU meeting by Sabalon · · Score: 2

      In my best Jean Luc Picard: There....are...nine...planets!

    13. Re:Time for another IAU meeting by gnasher719 · · Score: 2

      Even with the center of mass of each planet exactly in the L point of the other, then if the planet has a radius of 100km, parts of it will be 100kms away from the lagrange point --> inestability, whatever long it takes to become catastrophic.

      Actually, two earth sized masses on opposing sides of the sun will stabilise each other.

  2. You can't explain that! by bunratty · · Score: 4, Funny

    This is more liberal lies. Bill O'Reilly told me that you can't explain that!

    --
    What a fool believes, he sees, no wise man has the power to reason away.
  3. Re:And bolster my theory by Issildur03 · · Score: 4, Funny

    Check Wikipedia.

  4. Re:And bolster my theory by dweezil-n0xad · · Score: 4, Informative

    That there's a duplicate Earth on the exact opposite side of the Sun!

    OK, just for the fun of it: what would be the most efficient method to check this hypothesis?

    That would be STEREO.

  5. Re:And bolster my theory by MartinSchou · · Score: 2

    That would be in the L3 point, and that one is highly unstable, and a planet in L3 would be knocked out of it whenever Jupiter or Mars is close by.

    L4 and L5 is much more likely, but not for a duplicate Earth, as we would be able to see it from here.

  6. Gravity of an Earth-size body at L3 by tepples · · Score: 5, Informative

    That there's a duplicate Earth on the exact opposite side of the Sun!

    OK, just for the fun of it: what would be the most efficient method to check this hypothesis?

    By checking how its gravity would effect other planets in the same star system. For background: Counter-Earth on Wikipedia, Lagrangian point L3 on Wikipedia, and Counter-Earth on TV Tropes. Executive summary: We don't have one, and we know this because if we did, we'd be able to detect its pull. Furthermore, such an orbit would be unstable.

    1. Re:Gravity of an Earth-size body at L3 by Issildur03 · · Score: 4, Funny

      Checking Wiki worked! :)

  7. First? by jc42 · · Score: 5, Informative

    It's not clear that this is anything new. A number of astronomers have suggested that we should treat the Earth/Luna and Pluto/Charon pairs as "double planets" sharing an orbit. And there's a pair of Saturn's moons that share an orbit. Of course, whether these are counterexamples depends on the picky, legalistic details of how you define the term "planet", which we've discussed to death here on /. already. Fun as such pseudo-arguments may be, the fact is that they're not terribly significant.

    Thus, for the Pluto/Charon pair, reclassifying Pluto as a "dwarf planet" make it especially an edge case, since it still includes the term "planet" in its classification. But they're both large, spherical bodies in a single orbit around the sun, while also orbiting each other.

    The Earth/Luna pair is a bit of a mathematical curiosity. One of the arguments supporting calling our moon a "planet" orbiting the sun is that its orbit is everywhere convex with respect to the sun. You'd expect a "moon" to have a much more wiggly orbit, parts of which are curved away from the sun, and this is true of the other objects in the solar system that we call moons. OTOH, the barycenter of the Earth/Luna pair is (slightly) inside the Earth, which can be used with some definitions to say that it's really a satellite of the Earth.

    And, of course, Saturn's two moons in a single orbit can be disqualified because they're obviously not "planets". They're not even big enough to be spheroidal, which is required by most definitions of a planet.

    But the fact remains that our solar system contains at least three example of paired bodies sharing an orbit about their primary, and periodically exchanging the lead position. The mechanics of such orbits have been long understood, and astrophysicists can tell you when such orbits are stable. So while this may be "news" in the sense that it's about such orbits around another star, it's hardly news in the astrophysics sense.

    What'll be interesting news is the discovery of three astronomical bodies in a "Scottish reel" orbit, which was proved possible several years ago, but to my knowledge hasn't actually been observed yet. Possible places to find them are in the asteroid belt, in Jupiter's "Trojan" asteroid clumps, and in the Kuiper Belt.

    --
    Those who do study history are doomed to stand helplessly by while everyone else repeats it.
    1. Re:First? by Ambiguous+Coward · · Score: 4, Informative

      What'll be interesting news is the discovery of three astronomical bodies in a "Scottish reel" orbit, which was proved possible several years ago, but to my knowledge hasn't actually been observed yet. Possible places to find them are in the asteroid belt, in Jupiter's "Trojan" asteroid clumps, and in the Kuiper Belt.

      I googled "scottish reel orbit" and of course the first result was your own post. However, I did come across this, for those who are interested: http://faculty.ifmo.ru/butikov/Projects/Collection3.html

      --
      Their may be a grammatical error, misspeling, or evn a typo in this post.
  8. Re:right.... by WrongSizeGlass · · Score: 2

    how is this amazing. there are an infinite amount of things in the skies... I wouldn't be surprised to see a new Galaxy that had an outline shaped like a Penis

    I think they've already found one in the Porn Cluster ... I think it's called the Sheen Galaxy.

  9. Re:As well as by Weedhopper · · Score: 2

    Yes. Please say nothing more of Gor, thank you.

  10. Keplerian Occultations by kenwd0elq · · Score: 4, Insightful

    The problem with the planet detection methods used by the Kepler team is that it is all calculated based on occultations; the slight dimming of the star's light as a planet passes between that star and the Kepler satellite. This only works if the planet in question is 1) HUGE or 2) very close to the star or 3) the Earth just HAPPENS to be in the plane of the planet's orbit around the star. That's why we're discovering so many enormous planets with orbital periods in the range of only a few days. But the nice thing about the Kepler data seems to be that it's eliminating many of the "it could NEVER have happened that way!" explanations. With upwards of 500 billion stars in the Milky Way galaxy and we've looked only at a few thousand, it looks more and more that ANYTHING is possible when it comes to planetary formation.

    1. Re:Keplerian Occultations by Nyeerrmm · · Score: 2

      The distance from the star doesn't matter much for occultation methods. The difference between the Earth orbital radius and the Jupiter orbital radius from tens or hundreds of light years is negligible. The place where the radius does make a difference is in the time to repeat an observation. To get the orbital period of a planet in an Earthlike orbit will take around a year, while a jupiterlike orbit would require 16 years. The "wobble" method that found the first planets is the one that is really sensitive to hot Jupiters.

      Also, Kepler was specifically sized (and placed above the atmosphere) to be sensitive enough to detect Earth-sized planets around Sun-like stars.

      As you point out, the orbit plane is a problem, but often these things can be de-biased. If you assumed that ecliptic plane distributions were uniform it would be easy to extrapolate Kepler statistics to get a good estimate of the general population. While that uniform distribution is probably not true (I just don't know), a combination of models and distributions of ecliptic plane angles from other detection methods may give enough information to get a good estimate. The point isn't to detect every planet out there, but to get an estimate of the total number and distribution.

  11. two planets one orbit by frisket · · Score: 4, Funny
    I googled "two planets one orbit" and was shocked by the sick porn it brought up.

    Oh, sorry, typed it wrong...

  12. It's not a real planet . . . . until . . . by PolygamousRanchKid+ · · Score: 2, Interesting

    Captain Kirk beams down there, takes his shirt off, and gets the chick. Wait, two planets? Wait a second, we'll have to fly in a second, evil, Captain Kirk from a parallel universe. And how about a Spock with a beard? Does Ryanair fly there? Can we get a discount rate for two? Well, knowing them, they'll charge an extra exorbitant fee for Spock's beard. And the plane won't even land in the parallel universe, but in another universe, "Really close by!"

    --
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  13. Re:And bolster my theory by Lloyd_Bryant · · Score: 4, Funny

    .htraE ylno eht si sihT .tuoba gniklat er`uoy tahw wonk t'nod I .uoy rof taht dexiF

    --
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  14. Note that these planets do not orbit each other by robbak · · Score: 2

    These planets are at the stable lagrange points, not in orbit with each other.

    Which, by the way, is perfectly fine with regards to the IAU's definition. These planets have cleared their orbit nicely, and are gravitationally bound to each other.

    --
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  15. Dwarf planet? by niew · · Score: 2

    Both are to be considered "dwarf planets"

    We prefer the term "little planets"... (you insensitive clod!)

  16. This is probably a horseshoe orbit pair by viking80 · · Score: 2

    Two planets orbiting the same star is arguably only possible with horseshoe orbits. If two objects are of similar size so on cannot say one orbits the other, it is described a a double body rather than primary and satellite.

    A Lagrangian moon will likely develop into a horseshoe orbit over time.

    --
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  17. Re:And bolster my theory by d3ac0n · · Score: 2

    Strictly speaking, the planets would not actually share a common orbit. At least, in order for the orbit to be stable, that is. What you would actually have are two counter-rotating elliptical orbits in precise resonance with one another. To picture this, imagine a two component Venn Diagram using ellipses instead of circles. The Sun would be in the precise center, with the outer edges of the ellipses being the planetary orbits.

    This is the ONLY way that we could have an orbiting "companion" planet that is hidden from view all the time when viewed from Earth.

    Of course, having two resonant and opposing elliptical orbits creates a VERY large area that needs to be free of any gravitational perturbation. I don't know if such a planet could exist in our Solar System without interference from Mars.

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