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Potential 'Avatar' Gas Giant Exoplanet Discovered

Luminary Crush writes "A gas giant of approximately 1.5 Mj (Jupiter Mass) was discovered on October 22nd around the binary star system HD 176051B. It's not known with certainty which component of the binary system the planet is in orbit around at this point as both stars in HD 176051B are relatively Sol-sized (1.07 and .71 solar masses). Named 176051B b, this new exoplanet orbits within the star system's habitable zone, and if mapped onto our solar system with relative distance from our Sun it would place the large planet between Earth and Mars. While it's unlikely that such a gas giant could host life as we know it (though it's hypothesized), the location of the big planet opens up the intriguing idea of the realization of some of science fiction's famously habitable moons, Pandora and Endor. Look no further than our own solar system to see moons with the potential ingredients for life — just add heat."

142 comments

  1. how far away is it? by ionix5891 · · Score: 0

    Captain Jean-Luc Picard: Estimated time of arrival, Mr. Data?

    1. Re:how far away is it? by cappp · · Score: 1

      TFA claims "15.99 (± 0.13) pc" which is what, like one and a little Kessel Runs in the 'Falcon.

    2. Re:how far away is it? by Anonymous Coward · · Score: 0

      Yes, but in how many parsecs can you run it?

    3. Re:how far away is it? by Lanteran · · Score: 2, Informative

      in a fusion powered orion, it falls far short of the 50 year rule; 500 years with current technology. If we found a plentiful antimatter source, we could cut this to about 60 years.

      --
      "People don't want to learn linux" hasn't been a valid excuse since '03.
    4. Re:how far away is it? by SharpFang · · Score: 4, Interesting

      Note, if we get an efficient engine that can keep accelerating (no "idle flight" period), it would be 60-70 years for earth-based observers, but much shorter for the crew. The speed limit of 1c is relevant to surrounding universe, but from the spaceship crew standpoints, the engine power - acceleration - speed - distance - travel time relation behaves in mostly newtonian way. If they expend power needed to travel at 10c according to newtonian mechanics, it will take (in their perception) 1/10 the time of travel at 1c to get there.

      --
      45 5F E1 04 22 CA 29 C4 93 3F 95 05 2B 79 2A B2
    5. Re:how far away is it? by ledow · · Score: 3, Interesting

      If we found a plentiful antimatter source, and built something never yet produced but only really theorised (i.e. an antimatter-based propulsion of any kind), and make it into a fairly compact but reliable propulsion system, of which one example is bought and attached to a particular extra-solar-capable chassis (of which the only two ever produced were made in the 70's and are currently used to transport a couple of LP's in a random direction that we have no control over any longer), etc. etc. etc.

      As with anything to do with extra-solar propulsion, we won't see it for many, many decades and when we do, almost all our extra-solar attempts will be embarrassingly overtaken by the next-decade's attempt that will go faster (and the original mission will either have to keep going to somewhere that will be already colonised / studied even if it takes several generations, or turn back and spend their entire lives and those of their grandchildren trying to get back to Earth, or have to "merge" with the new attempt and thus have spent all their lives in a tin can when they could have just sat on Earth).

      The best solution, if we were to put all our efforts to getting to any such system (which seems unlikely and extraordinarily risky), would be something based on the "water-in-the-desert" method. Go a bit of the way. Leave a small cache of supplies / fuel / resources. Return. Go again, but a tiny bit further, and leave more stuff. Go again and leave more stuff. When we have sufficient stuff cached, make a SECOND cache and so on.

      In spacecraft terms, that means making something that can get to the moon easily. When we have that as an ordinary operational service, we can make trips to the next planet ready. When we have regular trips to all the planets, we can start veering slightly out of the solar system. When we have that ready, we can actually aim for the next best system by firing our best ships at it. They *will* get overtaken, but we can overtake them with an almost-empty ship with better technology, absorb their knowledge/resources and continue on the journey. Then the next ship will overtake that, pick them all up, melt down the old ship for repair-metal and continue. Eventually the people would get to some other system but we can't *ever* expect to just shoot something at the stars and expect it to work.

      This isn't the Moon (a mere ten-times the Equator's distance, and your average reindeer can travel the distance of the equator about 2-3 times during his life, your car should be able to do about four-equators-worth of travel easily before it finally dies (all of mine have), etc.). This is another solar system (the NEAREST of which is 4.37 light years, which is 1,033,339,810 (and a bit) equators. A BILLION equators. And that's the NEAREST damn thing, and quite boring really.

      50 years is way, way, way, optimistic for even a probe to another systems (hell, we've only "recently" done it with a probe out of the solar system at all, or a probe on another planet) - such a propulsion system would basically solve every energy need on Earth, so it's not a "small" development. To be honest, even 100, or 150, or 200 years, is being optimistic. Sometimes optimism pays off but we're not even just talking about doing something which we haven't done, at all, anywhere, in over 40 years - set foot on something that you could, theoretically, drive to within a few years in an ordinary car if you could pave a road there. We're talking about improving the entire accomplishments of all space travel by several (possibly dozen) orders of magnitude in only 2, 3 or 4 times the entire history of space travel itself (i.e. somewhere so far away that parts of a car would probably have destroyed themselves through their own radioactive half-life before it got even close).

      If we could do that with cars, extrapolating from the 60's, then we'd all be driving 1000mph cars that get 500mpg (actually, probably a LOT more than that).

      It's not *impossible*, it's just silver-suits and three-course-meal

    6. Re:how far away is it? by biryokumaru · · Score: 1

      Or a little less than a typical Kessel Run.

      --
      When you're afraid to download music illegally in your own home, then the terrorists have won!
    7. Re:how far away is it? by sznupi · · Score: 1

      I'm not even so sure about overtaking; even our extrasolar spacecraft from the 70's could have been noticeably faster (using instead of medium launcher something like, say, Saturn V with NERVA upper stage and, on the probe, nuclear reactor with ion thruster) - it just didn't make sense for the primary mission (would limit flyby times), it would be quite a bit more expensive.

      It's not just the tech that keeps us firmly on Earth now. And in the future - despite our wishes, it might very well be that the best practical thing allowed by this Universe is some variant of nuclear propulsion (or for small unmanned - starwisps for example; still at best around an order of magnitude less than c, anyway), all our data so far certainly strongly suggests it. And technologically, if we really wanted to, we can have capabilities for interstellar probe decently soon.

      But as you say, it would require basically whole GDP of the planet for the next few generations.

      (BTW you assume too big of a final hop in the "cache / gradual" approach, IMHO - there are many more outposts and local resource sources possible along the way, in the Oort cloud; estimations put their number maybe even at one trillion; I guess that's how our colonization will in the end look like, very gradual over the course of millennia - and with some groups eventually hitching a ride in an Oort cloud of another close-passing star. Maybe some embryo colonization ships, at most - one every few decades shouldn't put too much of a strain on the system)

      --
      One that hath name thou can not otter
    8. Re:how far away is it? by a_hanso · · Score: 1

      how many libraries-of-congress-burned-per-second would the energy requirement for that be?

    9. Re:how far away is it? by rossdee · · Score: 1

      Even if we had Bussard ramscoops it still takes a while to get anywhere. I am assuming that you can't accelerate much faster than 10m per second squared without it being too hard on the crew. Of course once you get close to c the time is slowed down for the crew, but it will take a year to get up to those speeds.

    10. Re:how far away is it? by SharpFang · · Score: 3, Insightful

      Yes, but the "nice 1g" (wow, artificial gravity problem solved!) gives us about 1 light year/year^2 acceleration. That is, gain/loss of 1c per year.

      About 4 years to Proxima Centauri. 50 light years in mere 7 "subjective" years. 40 years of crew life would give 800 light years of travel distance. About 1000 parsecs in a lifetime.

      Sure, we would still need engines that can provide sustained 1g. We're nowhere near that. We have rocket monstrosities that are barely survivable at 8g and more for minutes a time, and tiny farts of ~1N that can work for many years a time. Nothing in between. I believe a pure sustained fusion rocket might be capable of reaching Centauri stars, but that's still a long way away.

      --
      45 5F E1 04 22 CA 29 C4 93 3F 95 05 2B 79 2A B2
    11. Re:how far away is it? by silvermink · · Score: 1

      If they expend power needed to travel at 10c according to newtonian mechanics, it will take (in their perception) 1/10 the time of travel at 1c to get there.

      I don't quite understand what you mean here, it makes little sense talking about newtonian mechanics when the speed is near 1c. If travelling at 1c the Universe will be infintesimally short to the traveller (due to length contraction), and thus wherever he goes he will be there in no-time.

    12. Re:how far away is it? by John+Hasler · · Score: 1

      If travelling at 1c the Universe will be infintesimally short to the traveller (due to length contraction), and thus wherever he goes he will be there in no-time.

      Exactly. And if he travels very close to c the universe will be very short and thus wherever he goes he will be there in a very short time. Thus relativity makes it possible to reach any point in a finite universe in human-scale time (but go fast enough and each proton you hit will be as massive as a star).

      --
      Warning: this article may contain humor, sarcasm, parody, and perhaps even irony. Read at your own risk.
    13. Re:how far away is it? by SharpFang · · Score: 1

      Yes, but achieving precisely 1c would require infinite energy. We don't have that much. But if you double the energy, the perceived travel time will be reduced according to old Newtonian equations. So what if it's in fact the distance that got shortened, instead of speed being increased, ds/dt. You spent enough energy to travel at 2c according to Newton, and in your frame of reference you will get there in half the time as if you were traveling at 1c.

      It may be moot for Earth people (50 light years is still 50 years of flight no matter how much energy they pump into the engines), but it means no need for hibernation/cryogenics for the travelers (who will perceive the 50 years as 7 years of ship time).

      --
      45 5F E1 04 22 CA 29 C4 93 3F 95 05 2B 79 2A B2
    14. Re:how far away is it? by Jesse_vd · · Score: 1

      would you not have to start decelerating about halfway there?

    15. Re:how far away is it? by bill_mcgonigle · · Score: 1

      I believe a pure sustained fusion rocket might be capable of reaching Centauri stars

      The fusion drive is probably the easy part. What to do about hitting a grain of sand at .5c seems to be the harder one.

      --
      My God, it's Full of Source!
      OUTSIDE_IP=$(dig +short my.ip @outsideip.net)
    16. Re:how far away is it? by Teancum · · Score: 2

      Looking back at historical examples of human migration on vast scales, the typical amount of time that somebody relocated from say one continent to another was usually on the scale of months, to perhaps a year or two. A trip from Germany or Poland to California in the 1850's took approximately about a year, including travel by ship to one of the eastern US ports, and then overland on foot or wagon.

      I note this because that is about the current level of technology in terms of travel to various destinations around the Solar System at the moment, and one of the reasons why I think it is going to be comparatively trivial to make the trip to locations of that nature. Interstellar distances are going to take a leap of logic to move out that far and even with "exotic" but physically possible (Relativity equations don't keep you from making the trip as you suggest) modes of travel. At least right now, if you make a trip to Mars you can cut your losses and return to the Earth even using a Hohmann transfer orbit doing a minimal delta-v flight in a lifetime.... you can do several trips of that nature, much less something with more exotic propulsion like a nuclear rocket engine or something else similar.

      Somebody making a trip to Alpha Centauri might be able to make a return trip... if they really care to. But by the time they return home nearly everybody that they cared for would be dead from old age including newborn infants they might have known before they left.

      As you have suggested here, it is something possible and within 800 lightyears I'm fairly certain that we might be able to find a place at least as habitable as Mars that would be worth the trip out there to build homes and make a life. My question is.... why would we?

      Life would have to be getting pretty ugly here in the Solar System for somebody to be that motivated to travel those kinds of distances.

    17. Re:how far away is it? by Anonymous Coward · · Score: 0

      A "faster" ship has to accelerate catch up to, then decelerate to the slower ship's speed, then accelerate again back to the "faster" speed in your hop scenario. The problem is the amount of fuel it'd take to decelerate to pick up the cache, then accelerate again to continue will almost certainly make the operation not worth it. Also this would make things like gravity assists unusable, unless you're willing to wait centuries for a gravity slingshot in the same direction as the last vehicle. Not using a gravity slingshot would be a gross waste of resources, especially since the faster you go, the tighter you can make the slingshot maneuver, and the more speed you can gain. Also since everything in space moves, a slow ship aimed at a star would more likely be aimed at an "empty spot" and the star will be there when it gets there, a faster ship on the same trajectory would get there too early. Remember space isn't like a car where you can just hit the brakes, then speed back up at will. Nor can you just "turn". Inertia limits much of what you can accomplish in free space, any anything that can accelerate fast enough to make inertia not be a huge issue would likely be able to travel at fast enough speeds to not need caches in space.

    18. Re:how far away is it? by Lanteran · · Score: 1

      The 'rule' so to speak isn't for the crew's time experience; it's designed to make sure that its not passed by a faster ship while its still on the way there. I had honestly forgotten, but yeah flying at 90% the speed of light, the crew would only be experiencing a fraction of the time as observed from earth; but again, you don't want to get passed by a faster ship.

      --
      "People don't want to learn linux" hasn't been a valid excuse since '03.
    19. Re:how far away is it? by SharpFang · · Score: 2, Interesting

      Yes, these calculations include that.
      4 light years to Proxima, top speed of 2c at halfway point, averaged speed 1c, 4 years to get there. It would be much shorter for a speedy fly-by, accelerating all the time.

      --
      45 5F E1 04 22 CA 29 C4 93 3F 95 05 2B 79 2A B2
    20. Re:how far away is it? by SharpFang · · Score: 3, Interesting

      There are 6 billion people. Do you really believe none could be found desperate/crazy/naive enough to want to go there?

      btw, Centauri at 1g roundtrip would take 8 traveler's years and only ~12 earth years. Not quite as bad.

      Still, with E=mc^2, to get 1kg to 2c equivalent you need to burn 2kg of matter in a nuclear fusion entirely. Plus whatever is needed to bring last of that fuel near the 2c... rocket fuel equations apply. That's why Proxima may be still within reach, further places - not quite.

      --
      45 5F E1 04 22 CA 29 C4 93 3F 95 05 2B 79 2A B2
    21. Re:how far away is it? by SharpFang · · Score: 1

      I believe if much faster travel is invented during the flight time, a ship will be sent to pick up all the travellers and bring them to destination quickly...

      --
      45 5F E1 04 22 CA 29 C4 93 3F 95 05 2B 79 2A B2
    22. Re:how far away is it? by lul_wat · · Score: 2, Funny

      I'm having a dilemma on whether this should get modded 'Informative'.

      --
      Divide a cake by zero. Is it still a cake?
    23. Re:how far away is it? by RockDoctor · · Score: 1

      Looking back at historical examples of human migration on vast scales,

      Who has ever seriously proposed moving vast numbers of humans between the planets, let alone the stars? Seriously, move a minimal number and breed up a new population at the far end - the work is unskilled and the workforce are generally willing to do overtime.

      A trip from Germany or Poland to California in the 1850's took approximately about a year, including travel by ship to one of the eastern US ports, and then overland on foot or wagon.

      As a point of fact, I suspect that the trip more often (mode or median ; pick either) took closer to a generation, with people travelling to get onto a boat, using the boat, getting off the boat, settling in the city or in the East somewhere (because they need to make money, approximately now!), finding that was horrible, then moving on to try the lands out West in the next generation.

      Not many fleeing a shitty situation in Europe would have been in a situation to sit around and save enough additional money for a wagon and homesteading supplies before leaving the country they're fleeing. As soon as they'd got the boat fare plus a small amount of "travel cash" (maybe as jewellery, not cash, but WTF) then they'd be away.

      --
      Birds are not dinosaur descendants;birds are dinosaurs, for all useful meanings of "birds", "are" and "dinosaurs"
  2. How is this related to Avatar? by The_mad_linguist · · Score: 4, Insightful

    So, it's a much farther distance (50 ly), has a binary system (instead of a triple system), and the planet is bigger than Jupiter (instead of smaller).

    How is this related to Polyphemus from Avatar more, than, say, Bespin? ... come to think of it, both Avatar and this discovery are both overhyped. Objection withdrawn.

    1. Re:How is this related to Avatar? by Anonymous Coward · · Score: 0

      new bullshit detected to attract founding, name everything exo avatarish

    2. Re:How is this related to Avatar? by siddesu · · Score: 1

      The planet has heavy traces of Unobtainium in its Spectre, of course.

    3. Re:How is this related to Avatar? by Anonymous Coward · · Score: 0

      And when will we get there?

      Given that the warp-drive will be invented in 2063:

      2063-2011= 52 years before we get the technology.
      Probably warp 1 will be the initial speed of the drive and that equals to 26x the speed of light.
      Distance is 50LY/26, so about 2 years to get there.

      I would say that we should be there in 54 to 55 years. Assuming that FLT is ready for prime time in 2063...
      I'm sure that Virgin Galactic and Scaled Composites are working on a joint venture as we speak.

    4. Re:How is this related to Avatar? by Lord+Lode · · Score: 1

      The advanced high res 3-D telescopes have discovered blue creatures wandering on this planet, in 3-D!

    5. Re:How is this related to Avatar? by noidentity · · Score: 1

      What the hell does Avatar mean in this context, anyway? Is it a class of planets or something?

    6. Re:How is this related to Avatar? by GameboyRMH · · Score: 1

      Yes, Class-M, as in Marketingtastic.

      --
      "When information is power, privacy is freedom" - Jah-Wren Ryel
  3. Well what are we waiting for? by Anonymous Coward · · Score: 0

    Let's go mine the #$@! outta it.

    1. Re:Well what are we waiting for? by JDeane · · Score: 1

      They just needed to use neutron bombs on those Navi and mine the stuff in peace....

      Damned blue people always getting in the way of progress, first it was the Smurfs and now these Navi things!

      Nuke them from orbit, its the only way to be sure!

  4. Simple question... by Burnhard · · Score: 1

    What size does a planet have to be to become a star? Is it 3 x Jupiter?

    1. Re:Simple question... by hcpxvi · · Score: 1

      What kind of a unit is Jupiter masses anyway? How much is that in Humvees?

    2. Re:Simple question... by MollyB · · Score: 4, Informative

      short answer: If [Jupiter] were about sixty times more massive than it is, it would indeed be a star!

    3. Re:Simple question... by beelsebob · · Score: 2, Informative

      The minimum size of a star is thought to be about 83 times the mass of jupiter.

    4. Re:Simple question... by Anonymous Coward · · Score: 0

      What kind of a unit is Jupiter masses anyway? How much is that in Humvees?

      Jupiter is a pretty average gas giant and there are a fudgeload more of them in other systems. It makes sense to compare their sizes to Jupiter; apart from giving things a decent scale, it's more intelligent than saying '153.31 Earth Masses' or whatever it would be.

      Speaking of which, what kind of measurement is Humvees?

    5. Re:Simple question... by EmagGeek · · Score: 1

      I didn't know mass was a unit of size. :p

    6. Re:Simple question... by buchner.johannes · · Score: 1

      plus/minus 10 jupiter masses. The distinction between planets and brown dwarfs is really fuzzy.
      Even Jupiter emits more light in some frequencies than it receives from the sun.

      --
      NB: The message above might reflect my opinion right now, but not necessarily tomorrow or next year.
    7. Re:Simple question... by Danieljury3 · · Score: 1

      A brown dwarf is between 13 and 75-80 Jupiter masses but is classed as a sub stellar object as it cannot sustain hydrogen fusion so a star is probably more than 80 Jupiter masses. http://en.wikipedia.org/wiki/Brown_dwarf http://en.wikipedia.org/wiki/Substellar_object

    8. Re:Simple question... by Anonymous Coward · · Score: 0

      To elaborate on the correct answer of '83' above:

      Up to 13 Jupiter masses is classified as a planet
      Roughly 13 Jupiter masses is the minimum to be classified as a Brown Dwarf (based on the idea that this is the mass required to fuse deuterium, which brown dwarfs do before entering their cooling phase)
      Roughly 83 Jupiter masses is the minimum mass for sustained hydrogen fusion, at which point it's classified as a star

      Note that there is at least one object which is not quite accounted for in the current mass based definition of a Brown Dwarf. It is Cha 110913 which appears to chemically be a brown dwarf, but may be as small as 8 Jupiter masses.

      On the high end there is no discrepancy (that I'm aware of), since the sustained hydrogen fusion requirement to be considered a star is tightly tied to mass.

    9. Re:Simple question... by SharpFang · · Score: 1

      I think the threshold is not mass but origin/temperature. That is, a gas giant that is ablaze with thermonuclear fusion (or was in the past) is a star. Of course this is possible only above certain size/mass but there may be biggest gas giants slightly bigger than smallest stars.

      --
      45 5F E1 04 22 CA 29 C4 93 3F 95 05 2B 79 2A B2
    10. Re:Simple question... by sznupi · · Score: 1

      Even Jupiter emits more light in some frequencies than it receives from the sun.

      More generally, it radiates more energy than it receives from the Sun (with a different mechanism than in a star of course)

      --
      One that hath name thou can not otter
    11. Re:Simple question... by beelsebob · · Score: 4, Informative

      I didn't know mass was a unit at all ;)

      When talking about how big something needs to be to become a star though, mass is pretty much your only useful measure.

    12. Re:Simple question... by Burnhard · · Score: 1

      Yes, but I suppose I meant how much mass of gassy stuff (hydrogen mostly) in this general location would it require for it to collapse under gravity and eventually form a star. By star I mean a radiating body powered by nuclear fusion, prevented from blowing apart by the counter-acting force of gravity. I originally requested this mass in units of masses of Jupiter, given it's a lot easier to visualise than SI units. I'm guessing you can't form a star by simply twiddling the variables mass/density; you do need a certain amount of mass for the star to be viable over some period of time (let us say for the sake of argument, 1 Earth year :p).

    13. Re:Simple question... by gmuslera · · Score: 2, Informative

      1 x the mass of Jupiter... you just need to add enough monoliths.

    14. Re:Simple question... by Geoffrey.landis · · Score: 1

      Even Jupiter emits more light in some frequencies than it receives from the sun.

      More generally, it radiates more energy than it receives from the Sun (with a different mechanism than in a star of course)

      Most planets radiate more heat than they receive from the sun, of course. Including Earth, which generates internal heat by radioactive decay and radiates it away as part of its infrared output.

      --
      http://www.geoffreylandis.com
    15. Re:Simple question... by sznupi · · Score: 1

      Jupiter appears to be near the breakaway point. Saturn, despite being much further, might receive more energy from the Sun than it radiates. Earth receives four orders of magnitude more than it generates internally.

      --
      One that hath name thou can not otter
    16. Re:Simple question... by Surt · · Score: 1

      http://en.wikipedia.org/wiki/Star#Mass claims you can't get below 75, but it depends on how much metal you are willing to allow your 'gas giant' to contain.

      --
      "Who is the Journal of Quantum Physics going to believe?" --Stephen Hawking
    17. Re:Simple question... by Surt · · Score: 1

      http://en.wikipedia.org/wiki/Star#Mass

      Claims 75X mass of jupiter (depending on the extent to which you are willing to allow your planet to have a metal core rather than be mostly gas).

      --
      "Who is the Journal of Quantum Physics going to believe?" --Stephen Hawking
    18. Re:Simple question... by Surt · · Score: 1

      It is when you think about compacting it down into the smallest volume such that nuclear fusion starts up.

      --
      "Who is the Journal of Quantum Physics going to believe?" --Stephen Hawking
    19. Re:Simple question... by Have+Brain+Will+Rent · · Score: 1

      I would have thought density would be significant, not just total mass, since you can take that mass and spread it out so thinly that it isn't going to do anything significant (form a star, a black hole or whatever).

      --
      The tyrant will always find a pretext for his tyranny - Aesop
    20. Re:Simple question... by beelsebob · · Score: 1

      Well yes and no, the point is that below that mass, there isn't enough material to sustain fusion the way a star does. Sure there are a few more constraints, but mass is the relevant one here.

    21. Re:Simple question... by bhiestand · · Score: 1

      I would have thought density would be significant, not just total mass, since you can take that mass and spread it out so thinly that it isn't going to do anything significant (form a star, a black hole or whatever).

      IANAA/P, but I believe gravity tends to solve that problem when left to its own devices.

      --
      SWM seeks new sig for a brief fling
    22. Re:Simple question... by Have+Brain+Will+Rent · · Score: 1

      Not necessarily... that is why there's the question of whether the universe would keep expanding despite gravitational forces - all particles continuing to recede forever - or would collapse in upon itself due to gravitational force. Think "escape velocity".

      --
      The tyrant will always find a pretext for his tyranny - Aesop
    23. Re:Simple question... by RockDoctor · · Score: 1

      The distinction between planets and brown dwarfs is really fuzzy.

      No it's not. The distinction is at the point where the accreting planet achieves sufficient mass to start to burn lithium. Finding out what that mass is is moderately fuzzy (it almost certainly varies with metallicity of the progenitor material) ; measuring masses is also moderately fuzzy (i. sinand all that jazz) ; determining if the object is depleted in lithium compared to it's progenitor material is also fuzzy. But the criterion is not fuzzy.

      To use the traditional car analogy - you can argue whether the cop's speed gun was reading correctly ; you can argue that you were on this side of the change-of-speed limit sign, not that side, and therefore that the ticket doesn't apply. But there is no fuzziness about the speed limit itself.

      Even Jupiter emits more light in some frequencies than it receives from the sun.

      True, but not relevant. The Sun probably puts out more near-UV than it does far-IR, because of it's high temperature. Jupiter's low temperature would then make it brighter in (say) the far-IR than the Sun. (This is proposed as a way of detecting extra-solar planets, BTW.)

      What you mean to say, probably, is that when summed over a wide range of wavelengths, Jupiter emits more energy than impinges on it from the Sun. Which means that Jupiter is radiating some internal heat. But that's OK, it just means that it's a big planet which acquired a lot of energy from the infall of it's component materials, and is taking it's time about radiating the heat away.

      --
      Birds are not dinosaur descendants;birds are dinosaurs, for all useful meanings of "birds", "are" and "dinosaurs"
  5. Isn't this one even better..? by Anonymous Coward · · Score: 0
  6. SI Units by EmagGeek · · Score: 2, Informative

    1.5 Jupiter Masses = 2.8479 * 10^27 kg, in case anyone was wondering.

  7. Navi and Ewoks breeding? by Anonymous Coward · · Score: 0

    Navi and Ewoks in the same planetary system. That's some really disturbing fan and slash fiction.

    1. Re:Navi and Ewoks breeding? by CyberDragon777 · · Score: 1, Funny

      Navi = tall
      Ewoks = small and furry

      Navi + Ewoks = Wookiees?

      --
      We both said a lot of things that you are going to regret.
    2. Re:Navi and Ewoks breeding? by arielCo · · Score: 1

      Navi + Ewok + ??

      --
      This post contains no rudeness or derision of any kind. All arguments are friendly. Terms and exclusions may apply.
  8. Big Just by ultranova · · Score: 1

    Look no further than our own solar system to see moons with the potential ingredients for life -- just add heat.

    That's a rather big "just", since gas giants require cold to form. They're made of hydrogen and helium, which simply doesn't "stick" to a small proto-planet if the temperature is anywhere near the melting point of water. Of course, you could heat the environment of an already-existing gas giant, but how would that happen?

    --

    Forget magic. Any technology distinguishable from divine power is insufficiently advanced.

    1. Re:Big Just by BeanThere · · Score: 1

      Read that sentence you quoted again, he's talking about the moons of the gas giants, not the gas giants themselves. If you want to colonize the moon, does it matter if the main planet is a gas giant or not? It just has to exist as something for the moon to orbit around.

    2. Re:Big Just by prefect42 · · Score: 1

      Hot moon orbiting a cold giant sounds potentially trixy. Orbit would also be fairly important, or else you'd freeze your nuts off behind the giant.

      --

      jh

    3. Re:Big Just by ultranova · · Score: 1

      Read that sentence you quoted again, he's talking about the moons of the gas giants, not the gas giants themselves. If you want to colonize the moon, does it matter if the main planet is a gas giant or not? It just has to exist as something for the moon to orbit around.

      Yes, he's talking about the moons of the gas giants, which tend to be located rather near the gas giant itself, as far as distances in solar system's scale are concerned. Because they are near the giant, they are about as far from their sun as the giant is. If they're about as far from their sun as the giant, they get about as much solar radiation per square meter, and should thus be about as warm (or cold). In other words, if the gas giant is really really cold, so will the moon be.

      And we aren't talking about colonizing moons, we are talking about life evolving in one. So double fail on your part.

      --

      Forget magic. Any technology distinguishable from divine power is insufficiently advanced.

    4. Re:Big Just by sznupi · · Score: 2, Insightful

      ...and yet we sort of have just such a thing in our system - a moon hot to the point of being, by far, the most volcanically active body in the system.

      All this ignoring how many extrasolar hot Jupiters and hot Neptunes we're discovering - you people really never heard about them, about planetary migration in general?

      --
      One that hath name thou can not otter
    5. Re:Big Just by Anonymous Coward · · Score: 0

      Of course, you could heat the environment of an already-existing gas giant, but how would that happen?

      Maybe (I don't know how to verify this) if you can drop a small black hole (about the mass of our Moon) into the center of that gas giant, gas would fall in towards it, get compressed somewhere ahead of the hole's event horizon and start fusing. Radiation pressure from the fusion reaction and from the black hole itself might be enough to keep things near equilibrium for a while - keep most of the fusing gas shell (shall we call it an accretion shell?) hovering beyond the hole's static limit. It would be beautiful - a tiny black hole surrounded by a very small shell of fusing gas which heats up the rest of the gas giant. One VERY dim, VERY lightweight red dwarf, coming up.

      Dunno if it's possible, though :(. Maybe I should beer-up a physics grad to run the numbers for me. It would make for a nice gimmick in a space-opera.

    6. Re:Big Just by sznupi · · Score: 2, Interesting

      Of course, you could heat the environment of an already-existing gas giant, but how would that happen?

      Yeah, how in the universe this could ever be possible?

      --
      One that hath name thou can not otter
    7. Re:Big Just by prefect42 · · Score: 1

      But do you end up with a nice stable temperature like you would with a sphericalish orbiting body getting its heat from a star?

      I know some of the volcanically active moons get crushed in different ways during their long orbits round their body, but I'd have thought that'd lead to fairly major temperature variations.

      I know remarkably little about astrophysics ;)

      --

      jh

    8. Re:Big Just by sznupi · · Score: 1

      Conditions on Io seem fairly stable...

      Plus any differences during "long" orbits of practically any moon getting appreciable tidal heating are insignificant compared to the basic facts of heat retention, slow rates of convection, etc.

      --
      One that hath name thou can not otter
    9. Re:Big Just by prefect42 · · Score: 1

      Right. But it still makes for quite a lively surface compare to a star heated object doesn't it? A quick google suggests variation from 90-170K with small areas of volcanoes being far hotter (1500K).

      Or would a larger and more atmosphered moon smooth off that variation a fair bit?

      --

      jh

    10. Re:Big Just by sznupi · · Score: 1

      Yes, Io is simply heated far too much than what we would consider "nice" and is too small to retain any appreciable atmosphere (it does tend to stabilize temperatures on Earth, works wonders on Venus which has a day on the order of one year). Doesn't change how it's a good case scenario for extending habitable zones of perhaps millions solar systems just in our galaxy.

      --
      One that hath name thou can not otter
    11. Re:Big Just by sznupi · · Score: 1

      Not really fusion, mostly "friction" of matter in the accretion disk. Wouldn't be very long-lived. Wouldn't be dim; in fact, it would most likely hugely outshine the central star of the system.

      (and you know, we have many decent examples of what happens when a black hole appears inside a place with a lot of matter; the "fusing gas shell" in turn can't be really supported on anything)

      --
      One that hath name thou can not otter
    12. Re:Big Just by Anonymous Coward · · Score: 0

      Wow. Thanks for answering, in the first place. Us ACs aren't normally granted that courtesy.

      No fusion? That's... disappointing. I was kinda hoping that the accretion shell (it can't really be a disk since there's matter falling in from all sides, unlike in a binary system of star + black hole companion) would float itself away from the black hole by "simply" trying to explode all the time. I found this and I thought hey! that's interesting!

      You are basically saying that all of the planet would simply fall in towards the black hole and rather quickly at that... are you sure? A very small black hole would probably add mass slower and much of the added mass would come right back out in the form of radiation.

      I'd be curious about the many examples... afaik no black hole that small has ever been found.

    13. Re:Big Just by sznupi · · Score: 1

      It forms a disk just due to conservation of angular momentum and how the matter on initially, what is in essence, high inclination orbit around the black hole (the parts starting "far" from the equator) can't really keep that "orbit". Nucleosynthesis doesn't appear to be major way of energy release around black holes. Singularity doesn't need to be very large to get things quickly going where there's a lot of mass available; just large enough - and when that is the case, there doesn't appear to be a mechanism which would maintain equilibrium (you miss again how the proposed "shell" wouldn't be supported on anything, would want to escape in all directions, also towards the event horizon; and why shell/disk would be different, anyway?)
      But I didn't say all of the planet would simply fall in - yes, there should be also an "explosion", that's what it will make it quite bright on the scale of a galaxy; certainly nothing like in the recent Star Trek...

      (to register and log in isn't much of a problem?)

      --
      One that hath name thou can not otter
    14. Re:Big Just by BeanThere · · Score: 1

      If they're about as far from their sun as the giant, they get about as much solar radiation per square meter, and should thus be about as warm (or cold). In other words, if the gas giant is really really cold, so will the moon be.

      Exactly. So? Where did anything I say contradict that? Read the summary. He's saying that if this planet is close enough to be warm, so will the moons be warm.

      And we aren't talking about colonizing moons, we are talking about life evolving in one. So double fail on your part.

      Uh, nope, quote the SUMMARY: "the location of the big planet opens up the intriguing idea of the realization of some of science fiction's famously habitable moons". Not that there's any difference anyway; the point is whether or not it can meaningfully support life.

    15. Re:Big Just by BeanThere · · Score: 1

      Who says it's cold? Do you think that just because the gas giants in our solar system are cold, every gas giant in the universe is? Ours are cold because of their distance from our sun. Read the summary.

    16. Re:Big Just by prefect42 · · Score: 1

      So for the non astrophysicist, how does a gas giant form that close the the star where it's "warm"?

      --

      jh

    17. Re:Big Just by mcgrew · · Score: 1

      It would have to be orbiting something close enough and massive enough to cause tides; otherwise, how would the chemicals that create life mix?

    18. Re:Big Just by ultranova · · Score: 1

      ...and yet we sort of have just such a thing in our system - a moon hot to the point of being, by far, the most volcanically active body in the system.

      If you're talking about Io, it has average surface temperature of 110 Kelvin (-163.15 degrees Celsius or -261.67 degrees Fahrenheit), and even max is 113 Kelvin. That's not habitable by any water-based lifeform.

      --

      Forget magic. Any technology distinguishable from divine power is insufficiently advanced.

    19. Re:Big Just by sznupi · · Score: 1

      A temperature close to all other Galilean moons (or indeed all moons of Jupiter) - that's because of small size and hence tenuous atmosphere (also magnetosphere of Jupiter stripping it) unable to retain heat, not lack of heating.

      --
      One that hath name thou can not otter
  9. We might have found Pandora? by Troggie87 · · Score: 1

    So if we launch all of our nukes now, how long would they take to get there? Goddamn furries.

    1. Re:We might have found Pandora? by Anonymous Coward · · Score: 0

      If we time it right we may have enough time to develop FTL travel, and be there to watch the explosion!

    2. Re:We might have found Pandora? by Magada · · Score: 1

      If we do develop FTL travel, some tree-hugging idiot is bound to jump into the past and try to stop the nukes from ever being launched.

      --
      Something bad is coming when people are suddenly anxious to tell the truth.
    3. Re:We might have found Pandora? by sznupi · · Score: 1

      /me looks around...does the Universe seem greatly influenced, by some "civilization" from the "future" that developed FTL, via processes not following the expected natural ones?

      Nope; quite likely no FTL possible in this Universe (unless one wishes to subscribe to one quote of sir Arthur C. Clarke, "it may be that our role on this planet is not to worship god, but to create him")

      --
      One that hath name thou can not otter
    4. Re:We might have found Pandora? by gmuslera · · Score: 1

      We already created one, and all humanity worships it, even if can't do FTL. And if well is not based in very advanced technology, people think that with enough of it they can do magic.

      We call it money.

    5. Re:We might have found Pandora? by vlm · · Score: 1

      We already created one, and all humanity worships it, even if can't do FTL. And if well is not based in very advanced technology, people think that with enough of it they can do magic.

      We call it money.

      Geeze I thought you were going to say "Apple Inc" not boring old "money".

      --
      "Science flies us to the moon. Religion flies us into buildings." - Victor Stenger
    6. Re:We might have found Pandora? by Magada · · Score: 1

      Such a civilization might have even traveled right back to the big bang and influenced things so that the physical constants come out as they have and everything comes to pass as it has (as seen from our perspective). You wouldn't be able to tell the difference if they did, so the discussion is moot anyway.

      --
      Something bad is coming when people are suddenly anxious to tell the truth.
    7. Re:We might have found Pandora? by sznupi · · Score: 1

      Not exactly moot, if it still means no FTL for us anyway.

      --
      One that hath name thou can not otter
  10. Intelligent life... by Slur · · Score: 2, Interesting

    If intelligent life evolved out of a moon ecosystem where the main source of heat was tectonic stress, and the main liquid was methane or ammonia, you can bet they'd kick our ass.

    --
    -- thinkyhead software and media
    1. Re:Intelligent life... by MichaelSmith · · Score: 2, Funny

      If intelligent life evolved out of a moon ecosystem where the main source of heat was tectonic stress, and the main liquid was methane or ammonia, you can bet they'd kick our ass.

      ...slowly.

    2. Re:Intelligent life... by Anonymous Coward · · Score: 0

      I'm genuinely curious: On what basis do you make this statement?

    3. Re:Intelligent life... by Ceyx · · Score: 2, Interesting

      There is a very nice SCI-FI story about life in strange locations here, it is called "Passages in the Void"

      http://localroger.com/revelation-passage/

       

    4. Re:Intelligent life... by gman003 · · Score: 1

      Sure - on their home turf. But they'd probably find oxygen toxic, or start overheating at -40 degrees, or something else. That's part of evolution - you can't evolve resistance or tolerance to something you are never exposed to (thus explaining why plutonium is highly toxic to humans even disregarding the radiation issues). So no need to worry about an alien invasion yet - they'd need as much equipment to survive on Earth as we would to survive on Titan.

    5. Re:Intelligent life... by Have+Brain+Will+Rent · · Score: 1

      Until we dropped the oxygen bomb and a lit match.

      --
      The tyrant will always find a pretext for his tyranny - Aesop
    6. Re:Intelligent life... by TheVision · · Score: 1

      (thus explaining why plutonium is highly toxic to humans even disregarding the radiation issues).

      Citation needed, because the NRC says:

      In general, however, plutonium isotopic mixtures that are commonly encountered in the nuclear fuel cycle, nuclear weapons programs, or thermoelectric generator applications exhibit much higher radiological toxicity than chemical toxicity.

    7. Re:Intelligent life... by Anonymous Coward · · Score: 0

      I don't know much about chemistry and plutonium (aside from the obvious), but your quote does imply that it has chemical toxicity, just that the radiological is worse. The GP says plutonium is highly toxic "even disregarding the radiation issues" not specifically that chemical toxicity is worse than radiological. So basically: If plutonium would cause physical harm if absorbed/ingested by a human regardless of radioactive properties, then the GP is correct.

  11. I always liked Sagans version better. by pecosdave · · Score: 2, Interesting

    The Cosmos Series had a very good explanation of floaters and sinkers and some predators etc... /huh huh huh floaters.

    --
    The preceding post was not a Slashvertisement.
  12. Re:Such stories are frustrating by sznupi · · Score: 1

    At least some of us might get a quite decent image (puns, et al) - many nearby systems should be close enough for some good interferometer with a way of canceling-out the starshine; even JWST might give something not bad, for nearest systems, especially with some starshade added, flying in front of it in unison.

    But yeah, people raised on too much on scifi travels will be disappointed either way...

    --
    One that hath name thou can not otter
  13. About 50 by Anonymous Coward · · Score: 0

    About 50. However, there is a large overlap and the production of the matter matters nearly as much as the mass, so you can have brown dwarfs at 20 jupiters and massive planets at 60 or more Jupiters.

  14. It all makes sense now by captainpanic · · Score: 2, Funny

    Note, if we get an efficient engine that can keep accelerating (no "idle flight" period), it would be 60-70 years for earth-based observers, but much shorter for the crew. The speed limit of 1c is relevant to surrounding universe, but from the spaceship crew standpoints, the engine power - acceleration - speed - distance - travel time relation behaves in mostly newtonian way. If they expend power needed to travel at 10c according to newtonian mechanics, it will take (in their perception) 1/10 the time of travel at 1c to get there.

    Ok... Now I understand why we haven't traveled to the stars yet.

    We must overestimate the power needed, so that we can underestimate the time required.

    This is opposite from all engineering projects on earth, where the final design is underpowered and delayed.

  15. Hot Jupiters by Anonymous Coward · · Score: 0

    Hot Jupiters. We have some that are in mercury-sized orbits.

    Where do you and the OP get the idea that you need COLD to form a Jupiter? All you need is mass.

  16. I am an author of the study by Theory+of+Everything · · Score: 5, Informative

    I am an author of the paper in which this discovery was reported. You can find a copy of the paper here.

    While the planet probably is near the habitable zone, this isn't the first time a giant planet has been found in the habitable zone of a star, and while it could have moons, there isn't any reason to speculate more about this planet than any of the others.

    However, this planet is important for two other reasons:
    1. It was the first planet discovered using a technique called "astrometry", which is measuring the positions of stars in the sky, as the move up/down and left/right in reaction to a planet orbiting it. This technique has the potential to find earthlike planets in the habitable zones of nearby stars.
    2. It is found in a binary system and the second star is close enough that its gravity would have impacted planet formation. The leading theory of planet formation, called "core accretion", requires millions of year for planets to form, as dust in a disk around the star collides together and clings electrostatically (similar to the way dustballs collect on a hardwood floor). Eventually the dustballs grow large enough to be considered rocks, those collide and grow bigger, etc. But the second star's gravity would cause the dust to be swept out of the system in just thousands of years, far too little time for core accretion to occur. Thus, we need a different mechanism to explain planet formation in this system. This isn't the only such binary, but it this study does offer more controlled statistics of how frequently such binaries host planets, and these facts combined show that some had to form in the binary itself---the chances of a binary interacting with another star (that originally hosted the planet), leading to an exchange where the binary picks up the star, are much too small to explain the high rate observed.

    Also, here is another press story covering the discovery (by the way, stars have multiple names---don't be confused that this article calls it "HR 7162" and the other one refers to "HD 176051"---they really are the same system). The third figure on the right hand panel is particularly useful.

    Any questions? I'll try to answer responses to this post.

    1. Re:I am an author of the study by Geoffrey.landis · · Score: 1

      Any questions? I'll try to answer responses to this post.

      How can so much about the planet be observed without knowing which star the planet orbits? I'd think that information would be critical before any of the other information could be inferred.

      --
      http://www.geoffreylandis.com
    2. Re:I am an author of the study by Philomage · · Score: 1

      I've always thought that a binary system would create eddies in the dust and that mass caught in the eddies would coalesce quite quickly (incidentally, becoming a mass big enough to draw in more mass at an increasingly faster rate). I haven't seen any of the planetary creation models, so how much do they consider this kind of eddying and coalescence? I would think the eddying would be greater in a binary or trinary system than a single star system.

    3. Re:I am an author of the study by Theory+of+Everything · · Score: 3, Interesting

      Any questions? I'll try to answer responses to this post.

      How can so much about the planet be observed without knowing which star the planet orbits? I'd think that information would be critical before any of the other information could be inferred.

      The planet was discovered by measuring variations in the separation of the two stars. Their separation changes very slowly as the stars orbit each other, and on top of that motion, we found a very small wobble in their separation that repeats every ~3 years. That 3 year effect is the reaction of one of the stars to the planet orbiting it. Since we are measuring the relative separations of the stars, there is no way to know which one is wobbling. For the science content, it turns out not to matter nearly as much as one might think.

    4. Re:I am an author of the study by Theory+of+Everything · · Score: 1

      I've always thought that a binary system would create eddies in the dust and that mass caught in the eddies would coalesce quite quickly (incidentally, becoming a mass big enough to draw in more mass at an increasingly faster rate).

      I haven't seen any of the planetary creation models, so how much do they consider this kind of eddying and coalescence? I would think the eddying would be greater in a binary or trinary system than a single star system.

      Yes, an alternative model of planet formation called "gravitational instability" or "gravitational collapse" predicts that planets form in this way. That method is predicted to form planets very rapidly, and while there is not universal agreement on the subject, it seems likely that this is enhanced in binary systems. In the study, we discuss that this alternative model is one way to solve the problem of how this planet (and similar other ones) formed. This finding offers significant support to that alternative theory.

      Note that we are not claiming that the "core accretion" model does not happen in nature. Rather, it cannot be the only method by which planets form.

    5. Re:I am an author of the study by Graymalkin · · Score: 1

      With current telescopes what's the distance limit that we can use astrometry with any hope of accuracy (how many parsecs out can this technique be used)? In a similar vein are you using a single viewing session with one (or a single set) of telescopes or are you making multiple observations at different points in the year to create a virtual optical array? Does this increase the astrometric measurements in a meaningful way?

      --
      I'm a loner Dottie, a Rebel.
    6. Re:I am an author of the study by Luminary+Crush · · Score: 1

      Would it be easier to detect the existence of large (small planet-sized) moons around a gas giant than earth-sized planets around a star? Would not the perturbation of the gas giant be easier to detect because the mass ratios are closer (large moon to gas giant vs earth-sized planet to star)?

      If so, detecting the gas giant in the habitable zone and then looking for evidence of large moons or companion bodies could allow detection of candidates for life.

      I assume this would entail detailed, direct observation of the gas giant, but I would imagine that will happen sooner than detailed, direct observation of an earth-sized body.

    7. Re:I am an author of the study by Shadowmist · · Score: 1

      As I understand it... the bulk of the large moons in our solarsystem are made of low density materials essentially they're mini-frozen Jupiters in themselves or water ice balls like Enceladus. Wouldn't the formation of an Earthlike planet be precluded so close to a Jovian mass... Something with a substantial rocky core like Earth's forming at the same distance as a Jovian would have become a Jovian itself and most likely would have merged with the parent body? The Inner planets as I understand it were Jovians that had the bulk of thier gas envelopes blown clear during our Sun's T'Tauri phase of super strong solar winds.

    8. Re:I am an author of the study by sznupi · · Score: 1

      Do you have an impression that double / multiple star systems were up to this point neglected in searches of planets? While "gravitational instability" model perhaps even suggests they are at least comparably likely to form planets?

      --
      One that hath name thou can not otter
    9. Re:I am an author of the study by bhiestand · · Score: 1

      Is it possible that another force (I'm thinking magnetism) could kick-start or accelerate the process? It's late and I'm exhausted at the moment, but I can't shake the notion that there could be enough spinning iron or some other material in orbit that could, in some configuration, speed things up.

      --
      SWM seeks new sig for a brief fling
    10. Re:I am an author of the study by Theory+of+Everything · · Score: 1

      Do you have an impression that double / multiple star systems were up to this point neglected in searches of planets? While "gravitational instability" model perhaps even suggests they are at least comparably likely to form planets?

      It's actually a bit harder to find planets in binary systems using most of the current techniques. For example, the Doppler method is much more challenging when there are two spectra present to disentangle. When making measurements of extremely high, cutting-edge precision, and such complications can drastically reduce that precision. Similar, the transit technique is more challenging because there is more light present and because those studies usually require Doppler follow-up anyways to avoid false-positive signals (which have other, non-planetary, origins).

      So binaries were not neglected due to choice or because astronomers dismissed them as being uninteresting for exoplanet studies, but rather because the measurement methods could not work sufficiently well for them.

      We developed our new astrometry technique specifically because other methods were having problems with binaries, and because we recognized that binaries were an interesting laboratory to investigate planet formation (a null result also would have been enlightening on this topic).

    11. Re:I am an author of the study by Theory+of+Everything · · Score: 1

      With current telescopes what's the distance limit that we can use astrometry with any hope of accuracy (how many parsecs out can this technique be used)? In a similar vein are you using a single viewing session with one (or a single set) of telescopes or are you making multiple observations at different points in the year to create a virtual optical array? Does this increase the astrometric measurements in a meaningful way?

      With current telescopes? Well, the telescopes we used to do this work have been decommissioned (and bulldozed!), so I guess they're not current anymore. HST and some large ground-based telescopes are doing astrometry about 5x less precise than our program. The Europeans are building an array in Chile that should be able to do comparable precisions as our study (though over larger and more versatile set of target stars). Let us assume by "current" we mean something operating with precision similar to our program (35 micro-arcseconds).

      A Jupiter around a Sunlike star at 10 parsecs would cause the star's position to vary by 1000 microarcseconds. An SNR of about 5-6 is needed to make a detection. Depending on the number of measurements made, this means the smallest signal detectable is about 200 micro-arcseconds, so this technique could work to around 50 parsecs (160 light-years). For truly "current" telescopes, HST or ground-based AO might work to 10 parsecs.

      NASA/JPL has demonstrated technology for the Space Interferometry Mission (SIM) using the same method as our study, and shown that 1 micro-arcsecond astrometry is possible (again, on a much larger and far more versatile set of target stars). This could find Earthlike planets in the habitable zones of Sunlike stars to 10-20 parsecs. However, NASA canceled this program 2 weeks ago.

      We used an array of 3 telescopes working together as an interferometer, creating a system with resolving power equal to that of a 100 meter telescope. We observed our target stars several nights per week, every week, for several years. To see the signal, repeated measurements are necessary---we are looking for motion of the stars with time, as the planet slowly sweeps out its orbit. The number of measurements on a given star (50-100 over the years) helps improve the measurement noise some, but not a lot.

    12. Re:I am an author of the study by Theory+of+Everything · · Score: 1

      Would it be easier to detect the existence of large (small planet-sized) moons around a gas giant than earth-sized planets around a star? Would not the perturbation of the gas giant be easier to detect because the mass ratios are closer (large moon to gas giant vs earth-sized planet to star)?

      If so, detecting the gas giant in the habitable zone and then looking for evidence of large moons or companion bodies could allow detection of candidates for life.

      I assume this would entail detailed, direct observation of the gas giant, but I would imagine that will happen sooner than detailed, direct observation of an earth-sized body.

      Not with this method, since we are seeing the reflex motion of the star, which wouldn't be very different at all if the thing orbiting it were a planet by itself or a planet with a moon.

      However, for the transit method of planet formation that the Kepler mission is doing, we see the planet move in front of its star, periodically blocking the light. If the timing isn't perfectly periodic, that may mean its arriving too soon sometime, and too late others. This could be due to a moon orbiting the planet. This is a fairly large effect for Kepler.

    13. Re:I am an author of the study by Theory+of+Everything · · Score: 1

      As I understand it... the bulk of the large moons in our solarsystem are made of low density materials essentially they're mini-frozen Jupiters in themselves or water ice balls like Enceladus. Wouldn't the formation of an Earthlike planet be precluded so close to a Jovian mass... Something with a substantial rocky core like Earth's forming at the same distance as a Jovian would have become a Jovian itself and most likely would have merged with the parent body? The Inner planets as I understand it were Jovians that had the bulk of thier gas envelopes blown clear during our Sun's T'Tauri phase of super strong solar winds.

      The major moons in our solar system have densities between those of the terrestrial worlds and those of the giants. I certainly would not consider them to be mini-Jupiters.

      Planet formation isn't as simple as our old ideas of "if it forms here, it will be a gas giant, if not, it will be terrestrial". Clearly there are a lot more details that we don't know yet.

    14. Re:I am an author of the study by Shadowmist · · Score: 1

      Your point is noted. I do however don't think that there is any planetary model that would allow an Earth to be formed as a moon of Jupiter. It'd be rather disappointing though... that constant bath of radiation would preclude any life forming on the surface of such a world. Europa is a promising candidate because of the shielding its icy surface would provide for an interior ocean of life.

  17. Orbits by Hatta · · Score: 4, Informative

    It's not known with certainty which component of the binary system the planet is in orbit around at this point as both stars in HD 176051B are relatively Sol-sized (1.07 and .71 solar masses).

    Orbits do not work that way. The planet is orbiting around the center of gravity of the binary star/planet system. Since this is a binary star, this very well might be a point in empty space.

    --
    Give me Classic Slashdot or give me death!
    1. Re:Orbits by Anonymous Coward · · Score: 0

      I am afraid you are mistaken. It is quite possible for planets to have a stable orbit (as stable as orbits get anyway) in the habitable zone of one of stars of a binary star.

    2. Re:Orbits by TheTurtlesMoves · · Score: 3, Informative

      Check out the 3 body problem. Turns out that the only way you get long life orbit is if its orbiting just one star close enough that gravity is more or less dominated by that single object. ie to good approximation, its orbiting just one star.

      For a "stable" barycenter orbit, it would have to be very far away from the stars relative to the stars own separation. IIRC even then stable orbits are problematic for the scales we are talking about.

      --
      The Grey Goo disaster happened 3 billion years ago. This rock is covered in self replicating machines!
    3. Re:Orbits by BeanThere · · Score: 1

      If only that point didn't move.

  18. Radiation belts? by Latent+Heat · · Score: 1

    My understanding is that the moons of Jupiter are not human-habitable with any current technology on account of fierce charged particle radiation from the strong magnetic fields. Do I have this right, or does this only apply to Io, which is in one of the radiation belts?

    1. Re:Radiation belts? by Theory+of+Everything · · Score: 1

      My understanding is that the moons of Jupiter are not human-habitable with any current technology on account of fierce charged particle radiation from the strong magnetic fields. Do I have this right, or does this only apply to Io, which is in one of the radiation belts?

      With sufficient shielding, this could probably be overcome. However, there are other reasons those moons might not be comfortable places for humans: wrong temperature, no liquid water on the surface, no atmospheres, etc. On this new planet, it doesn't seem likely we'll be measuring its magnetic field any time soon, so it's a bit early to speculate more.

    2. Re:Radiation belts? by sznupi · · Score: 1

      (question is how much we would care; those radiation numbers certainly look awfully high)

      Regarding magnetic field: due to interactions in the field of Jupiter, its radio emissions can apparently "outshine" the Sun; occasionally...
      Maybe somebody who's strongly into radio astronomy, and available to you, can comment if our radio telescopes have the potential of resolving such source?

      --
      One that hath name thou can not otter
    3. Re:Radiation belts? by Theory+of+Everything · · Score: 1

      (question is how much we would care; those radiation numbers certainly look awfully high)

      Regarding magnetic field: due to interactions in the field of Jupiter, its radio emissions can apparently "outshine" the Sun; occasionally...
      Maybe somebody who's strongly into radio astronomy, and available to you, can comment if our radio telescopes have the potential of resolving such source?

      We don't yet have radio telescopes powerful enough to detect the radio emission of a planet like Jupiter around another star. There has been some recent speculation that if the radio brightness increases as the planet is brought closer to its star, and if that scaling is optimistically strong, then maybe some next generation radio telescopes could do so for the closest-in giant planets (i.e. the hot Jupiters), though this is planet not one of those.

  19. Not so fast! by GodfatherofSoul · · Score: 1

    I'm sure a bunch of hater scientists will discover there was a Fern Gully planet found 2 decades before.

    --
    I swear to God...I swear to God! That is NOT how you treat your human!
    1. Re:Not so fast! by wed128 · · Score: 1

      Not to mention the Dances with Wolves planet, some time before that!

    2. Re:Not so fast! by neminem · · Score: 1

      I'm pretty sure we've already found that one; it's called "Earth". Same with the Pocahontas planet.

      I'm still waiting for the Manta's Gift planet, though.

  20. But does it... by Galestar · · Score: 0, Redundant

    have unobtanium?

    --
    AccountKiller
  21. Trying to find other habitable planets is futile.. by mark-t · · Score: 1, Troll

    This post is probably going to get modded as a troll... it's certanly got all the earmarks of it, but all I can say is that this is still my sincere belief on the matter. I see absolutely no point to the exercise to finding habitable exoplanets. At all.

    What good does it do to know that habitable exoplanets are out there? Can we send people there? And even if we did, in the enormous time that it takes them to reach their destination, would the descendants of the original crew even be the sort of people who might actually want to engage in such a mission? What if, when they get there, they find out it's a bust? We've sentenced generations of people to death in the blacknesss of space, with absolutely *NO* means of ever getting back within their lifetime. We could hypothetically also just send a probe, but again, the sheer magnitude of time that would elapse before a probe actually reached the destination could make it unlikely that any people are actually still listening for the probe to send back any data.

    As I see it, scouting around the galaxy for exoplanets that can possibly host life when we don't have the technology to send anything there within a time frame that is reasonable for the purposes of what would have to be just an experiment, is one of the hugest wastes of time and resources that I can imagine.

    Now I've heard the arguments that living only on this planet, we *do* have all of our eggs in one basket, and it wouldn't take very much to wipe us out. These arguments are not wholly lost on me, but I can't see sending people to a place so far away that meaningful communication is not just impossible because of limitations on technology, but impossible because of physical constraints on the operation of the universe itself, is going to help matters... the time scales involved are so insanely large that it's unlikely in the extreme that anyone on earth around the time of its predicted arrival would even know or care if the vessel actually reached its destination at the scheduled time. We could not have any comfort that we might endure beyond a global catastrophe because there would be no way to ever know. That said, of course... it's not impossible for people to receive comfort from believing in things that aren't necessarily true, but that's not very scientifically valid is it? It's hardly any sort of real solution to the problem that we are likely to all be wiped out if we stay here when we subject parts of our population to even greater risks just by propelling them off this rock at the greatest velocities that are physically achievable by technology that we have with not even the slightest hope of ever returning.

    Now that said, if we could find a way to extend productive and healthy human life to be at least a couple of orders of magnitude larger than how long we have it currently, well then, sending people to other stars might become a viable thing to do. Or, even more unlikely (IMO), if we find a way to break the speed limit that the universe has imposed on absolutely every single thing that exists, then I could see finding habitable exoplanets possibly being something of promise... and of hope. Until then, however, I'm afraid I really just don't see the point.

    Okay... I'm done. Mod away.

  22. Mj = Jupiter Mass ? by lolococo · · Score: 1

    Go figure ...

  23. Re:Trying to find other habitable planets is futil by Gotung · · Score: 2, Insightful

    The galaxy is really, really, really big. There are lot's and lot's of stars. Really. There are a whole slew of them.

    Finding as much interesting stuff as we possibly can now, will help tremendously when we finally have the technology to send probes in a reasonable time.

    And developing new techniques for searching for interesting stuff is important as well.

    If we listened to you, in 100 years or so when we can send something somewhere, we would just have to cross out fingers, close our eyes, and point somewhere in the sky when picking where to go.

  24. Re:Trying to find other habitable planets is futil by ColdWetDog · · Score: 2, Insightful

    What good does it do to know that habitable exoplanets are out there? Can we send people there? And even if we did ... (rest of depressing post)

    Tiger got to hunt
    Bird got to fly
    Man got to sit and wonder - why, why, why?

    Tiger got to sleep
    Bird got to land
    Man got to tell himself - he understand.

    (Kurt Vonnegut, Jr.)

    --
    Faster! Faster! Faster would be better!
  25. Check our own solar system for life first, hey? by Anonymous Coward · · Score: 0

    I think humans just like to fantasize about the possibility of life somewhere far away because they know we can't verify it in our lifetimes. Nobody wants to hypothesize about life on a planet that we could go and check within 10 - 20 years and disprove. The truth is wouldn't it be wise to check our own solar system for life first?

    I mean, we've glanced at our moon and Mars, the two most dead looking things in our solar system. But, we have a gas giant with moons, one with lots of water on it (Europa) in fact right here near Jupiter. Couldn't we, you know, fly over there and see if there are fish / whales / sea otters swimming around? Everyone sort of writes off our own solar system, but if you don't travel to and investigate our own planets and moons how can you know. Yet, you can suggest there is life light years away on another moon near a gas giant, where's the precedence? Why couldn't there also be that same life next to our own, if we're going to start writing fiction? Why should the massive distance matter? It just baffles me.

    If it is that likely that there is meaningful life that many light years away, then let's just assume our own solar system is teeming with life and start investigating. It's easier than travelling light years.

    I think the root of the problem is, if we start saying hey it's right here in our solar system let's go find it. Then, they don't find anything at all, everyone is depressed and gives up. But, if they say, he it's light years away, that's something to reach for in the long run. It keeps hope alive.

  26. What about Yavin? by cupofjoe · · Score: 1

    http://en.wikipedia.org/wiki/Yavin ...I mean, in the litany of famous gas-giants, this one certainly rates. Not much else could get between the rebels and the first Death Star.

    1. Re:What about Yavin? by Anonymous Coward · · Score: 0

      Agreed. This is the first one I thought of.

      Considering how underwhelming avatar was to me, I totally forgot it was a moon.