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Scientists Discover Biggest Star

Hugh Pickens writes "Scientists at the University of Sheffield have discovered the most massive stellar giant, R136a1 measured at 265 solar masses, using the European Southern Observatory's Very Large Telescope in Chile and data from the Hubble Space Telescope. It's in the Tarantula Nebula in the Large Magellanic Cloud, a small 'satellite' galaxy which orbits the Milky Way. Previously, the heaviest known stars were around 150 times the mass of the Sun, known as the 'Eddington Limit,' and this was believed to be close to the cosmic size limit because as stars get larger, the amount of energy created in their cores grows faster than the force of gravity which holds them together. 'Because of their proximity to the Eddington Limit they lose mass at a pretty high rate,' says Professor Paul Crowther, the chief researcher in the Sheffield team. Hyper-stars like R136a1 are believed to be formed from several young stars merging together, and are only found in the very heart of stellar clusters. R136a1 is believed to have a surface temperature of more than 40,000 degrees Celsius, and is 10 million times brighter than the Sun. Crowther adds that R136a1 is about as big as stars can get. 'Owing to the rarity of these monsters, I think it is unlikely that this new record will be broken any time soon.'"

202 comments

  1. You think that's big!?!?!? by Impy+the+Impiuos+Imp · · Score: 5, Funny

    "Owing to the rarity of these monsters, I think it is unlikely that this new record will be broken any time soon.""

    Owing to the size of the universe, I think it is likely that this new record will be broken sometime soon.

    Two theories, now let's sit back and see who's right!

    --
    (-1: Post disagrees with my already-settled worldview) is not a valid mod option.
    1. Re:You think that's big!?!?!? by Chris+Burke · · Score: 4, Insightful

      Two theories, now let's sit back and see who's right!

      I think he'll be right for human scales of "soon", and you'll be right for cosmological scales.

      --

      The enemies of Democracy are
    2. Re:You think that's big!?!?!? by elocinanna · · Score: 2, Interesting

      I think more to the point is the size of the bit of the universe we can observe and then process the results of observation for. Something this big is rare for us to see from Earth as it stands and so without an improvement in technology or increase in resources spent on star-gazing it'll remain to be an impressive feat to find another of this size.

      ..Of course if we talk of this without taking our earthly abilities into account it just turns into a game of looking for an extremely large needle in an infinite haystack.

    3. Re:You think that's big!?!?!? by Random+Data · · Score: 5, Insightful
      Two theories, now let's sit back and see who's right

      No theories, but two hypotheses. One of which is actually based on modelling and thought, the other on intuition that the Universe is a big place.

      You may be right, but because the Universe is such a big place I *don't* think it's likely to be broken soon, since it's bloody hard to look around. The Tarantula Nebula is nice because it's recent, dense and relatively close, which means this could be found. Of course, they're all relative terms. We've been looking at the Tarantula Nebula for at least 250 years, and we've only found this one now...

    4. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      "sometime soon"? Give a goddamn date and then we can sit back and see who's right.

    5. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      "soon" is meaningless due to relativity, especially when discussing exotic cosmic objects. Not only is very likely that record been "broken", its already happened - so I should say this breaks no records as we don't know what the record is. Whether we'll find out about it on the other hand...

      "The views expressed here are mine and do not reflect the official opinion of my employer or the organization through which the Internet was accessed."

    6. Re:You think that's big!?!?!? by Impy+the+Impiuos+Imp · · Score: 1

      I'll take that bet, too, if you consider 5-10 years as "soon". In the context of astronomical discoveries, that's a fairly decent description.

      And ZOMG, I got FP for the first time in my Slashdot career!

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      (-1: Post disagrees with my already-settled worldview) is not a valid mod option.
    7. Re:You think that's big!?!?!? by Sockatume · · Score: 3, Insightful

      We can't readily measure the size of stars across the whole universe, and you think that our likelihood of finding a star even closer to the Eddington limit is a slam-dunk? I think the guy who found this one has a pretty good idea how hard they are to come across.

      --
      No kidding!!! What do you say at this point?
    8. Re:You think that's big!?!?!? by Killer+Instinct · · Score: 2, Funny

      "In theory, practice and theory are the same. In practice, they are not."

      --
      #include bier;
    9. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      FP... it does not mean what you think it means.

    10. Re:You think that's big!?!?!? by v1k · · Score: 5, Funny

      >intuition that the Universe is a big place.

      Dude, the universe is a big place. You just won't believe how vastly, hugely, mind-bogglingly big it is. I mean, you may think it's a long way down the road to the drug store, but that's just peanuts to the universe.

    11. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 1, Funny

      thank you for that insightful commentary. Until now, I had assumed that the universe was no more than twice as big as the distance from my house to the drug store, since that seemed pretty big to me. Now, where do I get my peanuts?

    12. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      it is a reference to a radio play. Or book. Or movie. (depending on which version V1k was referencing. Probably book)

    13. Re:You think that's big!?!?!? by maxume · · Score: 1

      HAHAHAHAHA 42.

      --
      Nerd rage is the funniest rage.
    14. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      Take a left at Milky Way. The peanuts aren't too far down the road from there.

    15. Re:You think that's big!?!?!? by Psmylie · · Score: 5, Funny

      Now, where do I get my peanuts?

      Depends on how ambitious you're feeling. If you'd prefer not to venture out into the vastness of space, I'd suggest checking between and under the couch cushions.

      --

      psmylie's dictionary: Godzillion (noun) Any number large enough to destroy Tokyo

    16. Re:You think that's big!?!?!? by NotBornYesterday · · Score: 1

      That quote ... it does not mean what you think it means.

      --
      I prefer rogues to imbeciles because they sometimes take a rest.
    17. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      Fart Petition?

    18. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      Now, where do I get my peanuts?

      You don't have to get any. Ford gives them to you after you wake up aboard the Vogon ship.
      But good luck getting the Babel fish.

    19. Re:You think that's big!?!?!? by SETIGuy · · Score: 3, Interesting

      Owing to the size of the universe, I think it is likely that this new record will be broken sometime soon.

      The record is for the largest one found, not the largest one in the universe. These things are pretty difficult to find. They're all in dense clusters in active star forming regions. The cluster R136 is so dense that prior to the launch of HST we thought that there were fewer stars in it, but each of those stars would have been several hundred solar masses. HST was able to resolve those superstars into multiple smaller (50 solar mass) stars. Except for this one, apparently.

      We haven't found any equivalent star clusters in the Milkyway (yet). It's possible there aren't any. Maybe something about the composition or dynamics of Galactic gas prevents such large stars from forming. No other galaxy would be close enough that we could resolve cluster into individual stars. The SMC doesn't have active star formation. So we're stuck with the LMC as a target for finding a larger star. There's no other cluster in the LMC like R136, so to break this record we'd probably need to find a larger star in the same cluster. Or we would need to find out that R136a1 is a multiple star system containing 2 or more smaller stars rather than one star of 265 solar masses.

      As far as how significant this is... I'm sure it will drive star formation theorists nuts trying to build stars that big in a cluster environment. But as a find, in and of itself, they looked for a really huge star in what is well known as the only place you're going to possibly find a really huge star. It seems kind of like "discovering" a route from your front door to the bus stop when you know where both of them are. Given how many people are interested in star forming regions, I'm kind of wondering why nobody did it earlier. I may have to read the paper to see if some interesting or difficult technique was necessary.

    20. Re:You think that's big!?!?!? by Nutria · · Score: 1, Insightful

      One of which is actually based on modelling and thought

      Except that the Eddington Limit was also based on modeling and thought, but was then smashed by reality.

      2.5 years ago, astronomers with a spreadsheet "discovered" that the Milky Way is really 2x thicker than previously accepted.

      While I'm glad that Science allows scientists to alter their theories and beliefs, ISTM that too many astronomers/cosmologists think they know far more than they really know.

      --
      "I don't know, therefore Aliens" Wafflebox1
    21. Re:You think that's big!?!?!? by bunratty · · Score: 2, Funny

      You've just given me flashbacks to my time in the total perspective vortex, you insensitive clod!

      --
      What a fool believes, he sees, no wise man has the power to reason away.
    22. Re:You think that's big!?!?!? by oldhack · · Score: 1

      I am not getting it. Just how big is this universe thing?

      --
      Fuck systemd. Fuck Redhat. Fuck Soylent, too. Wait, scratch the last one.
    23. Re:You think that's big!?!?!? by severoon · · Score: 1
      From TFA:

      Owing to the rarity of these monsters, I think it is unlikely that this new record will be broken any time soon.

      Yea, the only way we'd stand a good chance of finding a bigger star than this would be...well, let's just say there'd have to be thousands of stars for that to even be possible.

      --
      but have you considered the following argument: shut up.
    24. Re:You think that's big!?!?!? by sexconker · · Score: 0, Troll

      "In theory, practice and theory are the same. In practice, they are not."

      I hate this quote.
      In theory and in practice, theory and practice are separate and different.

    25. Re:You think that's big!?!?!? by shaitand · · Score: 1

      "And ZOMG, I got FP for the first time in my Slashdot career!"

      Bitch

    26. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      You don't have sex with another person very often do you?

    27. Re:You think that's big!?!?!? by weicco · · Score: 1

      Have you noticed that the distance from your house to the nearest drug store is constant but the distance back from the drug store changes vastly depending the prescription? Weird shit. Once it took me a week to even remember where I lived!

      --
      You don't know what you don't know.
    28. Re:You think that's big!?!?!? by PopeRatzo · · Score: 1

      without an improvement in technology

      Can you give me an example of an epoch of human history when there was not an "improvement in technology"?

      --
      You are welcome on my lawn.
    29. Re:You think that's big!?!?!? by Killer+Instinct · · Score: 1

      Thank you for sharing, we are all enlightened. Here's your sign, move along.

      --
      #include bier;
    30. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      You know what you do when you assume...

      ...you make a reasonable prediction based on past experience.

    31. Re:You think that's big!?!?!? by blair1q · · Score: 1

      You makee mistakee.

      It's somewhat certain that there are stars larger than this one, even if they're wayyyyyyy out on the long tail of the distribution, which itself drops off like a cliff somewhere beyond this one due to the nonlinearity of the processes occurring in larger stars (they tend to explode-implode into your darker dwarves and holes).

      But it's also almost certain that we won't detect one of them for a long time, since, as you nearly pointed out, astronomy budgets are somewhat wee compared to the size of the universe.

      So you confuse existence with discovery. Something more likely than anything else we've been discussing, really.

    32. Re:You think that's big!?!?!? by sycodon · · Score: 1

      Crowther adds that R136a1 is about as big as stars can get.

      Right.

      That's what Eddintgon said

      --
      When Fascism comes to America, it will call itself Anti-Fascism, and tell you to give up your guns.
    33. Re:You think that's big!?!?!? by stewardwildcat · · Score: 1

      While you are completely correct, it is harder and harder to see individual stars as you observe galaxies farther away. The farthest we can clearly observe bright, single stars is the Virgo Cluster which is only 50 million light years away. So until we get much larger telescopes we have to rely on the local universe to provide us with record breakers or we are sunk for the time being.

    34. Re:You think that's big!?!?!? by madpansy · · Score: 1

      and you think that our likelihood of finding a star even closer to the Eddington limit is a slam-dunk?

      The summary mentioned that this newly discovered star, observed at 265 solar masses, is much larger than the Eddinton limit, which is around 150 solar masses.

    35. Re:You think that's big!?!?!? by stewardwildcat · · Score: 1

      13.7 Billion light years to the edge of your visible universe.

    36. Re:You think that's big!?!?!? by Zcar · · Score: 2, Insightful

      Yep. Is there a bigger star out there? Almost certainly. Is there a bigger star out there where we have to ability to observe it? This is where it gets difficult.

    37. Re:You think that's big!?!?!? by ceraphis · · Score: 1

      Subscribe to Slashdot and you'll get all the Flux Paradigms you want.

    38. Re:You think that's big!?!?!? by ceraphis · · Score: 2, Funny

      Pah, no luck needed. The infinite improbability drive guarantees getting the babel fish. And the peanuts.

    39. Re:You think that's big!?!?!? by ceraphis · · Score: 1

      They were advised by Blizzard Valve and 3Drealms. It'll be done when it's done.

    40. Re:You think that's big!?!?!? by Mysticalfruit · · Score: 1

      I'd also have to imagine with that much mass and considering the amount of energy it's outputting that it's life span for a star would be relatively short.

      --
      Yes Francis, the world has gone crazy.
    41. Re:You think that's big!?!?!? by uvajed_ekil · · Score: 1

      Dude, the universe is a big place.

      Nah, it can't be that big, or else how could the multiverse host infinite universes?

      --
      This is a hacked account, for which the owner can not be held responsible.
    42. Re:You think that's big!?!?!? by Chowderbags · · Score: 1

      ...a game of looking for an extremely large needle in an infinite haystack.

      I think I saw that porno once. It was almost as hot as this star.

    43. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      The dark ages.

    44. Re:You think that's big!?!?!? by PopeRatzo · · Score: 1

      The dark ages.

      Silly AC. Yes, even in the "dark ages" mankind advanced technologically.

      As anyone who has studied world or European history during the past half-century will tell you, the "dark ages" were anything but. It was actually a time of great advances in many human pursuits, especially in certain parts of the world. Ireland, for example, was a center of research and learning during what is mis-named by the ignorant the "dark ages". Also South Asia, also parts of the Middle East.

         

      --
      You are welcome on my lawn.
    45. Re:You think that's big!?!?!? by Abstrackt · · Score: 1

      "Owing to the rarity of these monsters, I think it is unlikely that this new record will be broken any time soon.""

      Owing to the size of the universe, I think it is likely that this new record will be broken sometime soon.

      Two theories, now let's sit back and see who's right!

      Science would be a lot more fun if scientists solved disputes with death matches.

      --
      They say a little knowledge is a dangerous thing, but it's not one half so bad as a lot of ignorance. - Terry Pratchett
    46. Re:You think that's big!?!?!? by Albert+Sandberg · · Score: 1

      how many library of congress is that?

    47. Re:You think that's big!?!?!? by lgw · · Score: 2, Informative

      Except that the Eddington Limit was also based on modeling and thought, but was then smashed by reality.

      Hardly "smashed" by reality - this is how real science works! Real science involves falsifiable hypotheses. If the hypothesis is good, you learn something useful even by finding exceptions. "Based on our best models this is as big as it gets - but wait, here's something interesting."

      With good science, you admit that exceptions are interestng, and while your model usually makes accurate predictions, a fundamental assumption might just be wrong. Investigating the corner cases where usually-accurate models fail is the work of good science. With junk science, you tweak your model (retroactvely, if you can get away with it) to explain the new data too, and dismiss the exceptions as meaningless (or worse, just hide or change the inconvenient data).

      This particular star is likely not an interesting exception: the Eddington limit is just the luminosity beyond which a star will rapidly shed mass. This star was probably formed through stellar collisions, and is likely rapidly shedding mass. There are other objects which seem stable above the Eddington limit, however.

      --
      Socialism: a lie told by totalitarians and believed by fools.
    48. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      Nice example of a massively-sun-sized trolling. Here is your bridge, get under it.

    49. Re:You think that's big!?!?!? by fiannaFailMan · · Score: 2, Insightful

      >intuition that the Universe is a big place.

      Dude, the universe is a big place. You just won't believe how vastly, hugely, mind-bogglingly big it is. I mean, you may think it's a long way down the road to the drug store, but that's just peanuts to the universe.

      "Dude?" "Drug store?" Please don't tell me they translated the Hitchhiker's Guide into American English!

      --
      Drill baby drill - on Mars
    50. Re:You think that's big!?!?!? by Chris+Burke · · Score: 1

      Yea, the only way we'd stand a good chance of finding a bigger star than this would be...well, let's just say there'd have to be thousands of stars for that to even be possible.

      The odds of such a star existing is very, very different than the odds of us finding it. The circumstances where you'll find one aren't just anywhere. There are certainly plenty such places in the universe, but not so many where we could actually see them and resolve the individual stars, which was a challenge even in this case.

      --

      The enemies of Democracy are
    51. Re:You think that's big!?!?!? by shermo · · Score: 1

      "We think it's unlikely there will be any stars bigger than the Eddington limit"

      "Ok we found one significantly bigger than the Eddington limit. Now we really think it's unlikely we'll find stars bigger than this one, really."

      --
      Insanity: voting in the same two parties over and over again and expecting different results
    52. Re:You think that's big!?!?!? by Nutria · · Score: 1

      With junk science, you tweak your model

      Isn't that what all modelers do on a regular basis?

      to explain the new data too, and dismiss the exceptions as meaningless

      I have a premonition...

      This particular star is likely not an interesting exception

      Did you just call yourself a junk scientist?

      --
      "I don't know, therefore Aliens" Wafflebox1
    53. Re:You think that's big!?!?!? by lgw · · Score: 1

      Well, all science deals with models of reality, but not all models are computer simulations - one didn't used to need to make that distinction. Sure, many "modelers" tweak their model on a regular basis, but then there's a lot of embarassingly bad science going around these days, and when the internals of the computer models are well-kept secrets, it's just sad.

      Just a few years back the proceedings from a string theory conference would be more philosophical ramblings than even something as close to science as "model tweaking", and the same problem was showing up in journals too (though Tipler still had to self-publish his really crazy stuff, so there were some standards). I can only hope future generations look back at this and laugh, rather than noting the defunding of the SSC as the beginning of the end of America's reign in physics research.

      And an "exception" to a model as described in some news story may not be an exception to the actual model at all, as seems to be the case here. Sumarizing for headlines is quite lossy compression when it comes to theory. But there are real and interesting exceptions - this just isn't one of them.

      --
      Socialism: a lie told by totalitarians and believed by fools.
    54. Re:You think that's big!?!?!? by dylan_- · · Score: 1

      Well, all science deals with models of reality, but not all models are computer simulations -

      What kind of scientific models are you thinking of that aren't mathematical models?

      --
      Igor Presnyakov stole my hat
    55. Re:You think that's big!?!?!? by lgw · · Score: 1

      Well, all science deals with models of reality, but not all models are computer simulations -

      What kind of scientific models are you thinking of that aren't mathematical models?

      Well, there is all this "anthropic princple" BS, but obviously that wasn't what I was talking about above. And perhaps I unfairly blame overreliance on computer modeling, since it's useful for visualization in just about every field. To put it a different way: a good scientific model can be falsified by measurements or experimental data, and a model that can be expressed in a few equations with few tunable paramters is more likely to clear that bar. If you have a computer model with a host of tunable parameters, such that any new data can be incorporated simply by tuning, you don't really have a falsifiable hypothesis. But then, I guess that's not just a computer model problem - if you have a string theory style abstract mathematical model that can describe any imaginable universe by tuning a few parameters, you're in the same boat.

      --
      Socialism: a lie told by totalitarians and believed by fools.
    56. Re:You think that's big!?!?!? by Anonymous Coward · · Score: 0

      Aww, all I found was twenty dollars. But I wanted a peanut!

    57. Re:You think that's big!?!?!? by Impy+the+Impiuos+Imp · · Score: 1

      I wonder, did anyone actually graph inventions through the Greek/Roman era, through the "Dark Ages", to Renaissance, to now? Was there a dip in the rate of inventions in the "Dark Ages"? Per capita, from Europe (as opposed to Persia or China or somewhere.)

      Inquiring minds want to know!

      --
      (-1: Post disagrees with my already-settled worldview) is not a valid mod option.
    58. Re:You think that's big!?!?!? by Keerok · · Score: 1

      seriously, thats pretty funny :P Stuff in headlines does have a way of being measured with Units of LoC. ps it would be 987e892 kg, or there abouts

  2. Pretty cool but... by elocinanna · · Score: 4, Funny

    Anyone could find something if it's that big! Wake me up when they find the smallest one! :p

    1. Re:Pretty cool but... by Anonymous Coward · · Score: 2, Funny

      Here's a list of all the smallest known stars.

    2. Re:Pretty cool but... by Anonymous Coward · · Score: 0

      Have you checked your pants lately? That's a good contender.

    3. Re:Pretty cool but... by 2obvious4u · · Score: 1

      That wasn't punny...

    4. Re:Pretty cool but... by An+ominous+Cow+art · · Score: 3, Funny

      Is this the joke thread? Ok, here's mine...

      Twinkle, twinkle, really freaking big star...

    5. Re:Pretty cool but... by Anonymous Coward · · Score: 0

      Here's a list of all the smallest known stars
      You left out the brown dwarf.

      (too soon?)

    6. Re:Pretty cool but... by mcgrew · · Score: 1

      Wake me up when they find the smallest one!

      Look in your boyfriend's pants, ma'am.

    7. Re:Pretty cool but... by c++0xFF · · Score: 1

      The only way we'll find a larger star is if you mom auditions for American Idol.

  3. I guess it's time to update the earth to star by assemblerex · · Score: 1

    comparison animations, as we are now more inconsequential than ever!

    1. Re:I guess it's time to update the earth to star by RivenAleem · · Score: 2, Interesting

      Just you wait until some committee somewhere out there decides that the sun is too small and inconsequential to be classed as a real star. If it happened to Pluto...

    2. Re:I guess it's time to update the earth to star by Digital+Vomit · · Score: 1

      comparison animations, as we are now more inconsequential than ever!

      Sentence fragments are really

      --
      Modern copyright is theft of culture from everyone and it retards the progress of the useful arts and sciences.
    3. Re:I guess it's time to update the earth to star by jonamous++ · · Score: 1

      Read the subject, then the body. The first part of his sentence is the subject. The second part of it is the body of the comment.....

    4. Re:I guess it's time to update the earth to star by Digital+Vomit · · Score: 1

      I guess it's time to update the earth to star Read the subject, then the body. The first part of his sentence is the subject. The second part of it is the body of the comment.....

      Man, this internet thing is hard!

      --
      Modern copyright is theft of culture from everyone and it retards the progress of the useful arts and sciences.
    5. Re:I guess it's time to update the earth to star by jonamous++ · · Score: 1

      It gets me sometimes too. Like in the above example I heard a whooshing sound but didn't realize the joke was flying above my head.

  4. R136a1 or Rieshai by jack2000 · · Score: 1

    Maybe they should have named it Rieshai instead of using numbers.

    1. Re:R136a1 or Rieshai by Sique · · Score: 1

      Which would be (rather bad) German and could be translated as "wet meadow shark" (even though the term "Ries" for a wet, grassy plain is not often used in contemporary German).

      --
      .sig: Sique *sigh*
    2. Re:R136a1 or Rieshai by Anonymous Coward · · Score: 0

      Wait, Germany has meadow sharks? Why was I not informed?

    3. Re:R136a1 or Rieshai by Mindcontrolled · · Score: 1

      Linguistics nerd alert! Where do you get that meaning of "Ries"? That must be a local thing. Grimm's dictionary does not document any use of "Ries" for meadow, wet or not. It might be a local pars pro toto, as "Ries" used to be a name for cane or rush, which tends to grow on such meadows.

      --
      Ubi solitudinem faciunt, pacem appellant.
  5. Unhealthy Universe? by Hoi+Polloi · · Score: 4, Funny

    Clearly obesity is not just a problem on earth.

    --
    It is by the juice of the coffee bean that thoughts acquire speed, the teeth acquire stains. The stains become a warning
    1. Re:Unhealthy Universe? by Anonymous Coward · · Score: 0

      Smoking and speeding also seem to be endemic.

      Perhaps we should require suns to switch to snus and wear helmets.

    2. Re:Unhealthy Universe? by sconeu · · Score: 1

      I was waiting for a CowboyNeal joke on this...

      --
      General Relativity: Space-time tells matter where to go; Matter tells space-time what shape to be.
    3. Re:Unhealthy Universe? by ITBurnout · · Score: 1

      Not only is it obese, it's got gas.

  6. Unhealthy indeed... by leonardofelin · · Score: 1

    I'll need more sunscreen.

  7. how many library of congress is that? by Anonymous Coward · · Score: 0

    or actually, how does this compare to VY canis majoris?

  8. Mass vs Radius by TheMidnight · · Score: 4, Insightful

    One thing the article didn't mention was the radius of the new star. It's obviously larger than the sun, but is it the "largest" star found or simply the most massive? It seems with that kind of mass it might be denser than your average supergiant and have less volume, and therefore less radius.

    1. Re:Mass vs Radius by AstroMatt · · Score: 2, Informative

      Stars on the main sequence get less dense the hotter/brighter they are. When the evolve off the main sequence, they get bigger still. It's likely this has the largest radius, too. Very interesting formation mechanism ... stellar collisions!

    2. Re:Mass vs Radius by meringuoid · · Score: 1
      One thing the article didn't mention was the radius of the new star. It's obviously larger than the sun, but is it the "largest" star found or simply the most massive? It seems with that kind of mass it might be denser than your average supergiant and have less volume, and therefore less radius.

      It's blue, therefore it's hot, therefore it's dense, therefore it's (comparatively) small. VY Canis Majoris would be much larger, even if not so massive - and cooler, and therefore red. Indeed, notice the diagram in the article, showing this star as compared to the Sun. The Sun is visible on the diagram. This would not be the case with VY Canis Majoris!

      It's all gas law really, just like in high school physics. pV = nRT. When a star contracts, it heats up; when it expands, it cools. As a supergiant's core switches on and off as it works its thermonuclear way up the periodic table, it may inflate and deflate over and over again.

      --
      Real Daleks don't climb stairs - they level the building.
    3. Re:Mass vs Radius by delt0r · · Score: 1

      You are wrong because you have completely neglected the heat source. More massive stars are hotter because they burn more fuel. The volume to surface area ratio means the cores are hotter and larger compared to a less massive star, that means more fusion. So as stars get more massive, they get hotter and less dense and hence have a larger radius.

      --
      If information wants to be free, why does my internet connection cost so much?
    4. Re:Mass vs Radius by olsmeister · · Score: 2, Informative

      Red giant stars would have a much larger radius. The radius of R136a1 is estimated at something like 30 times that of the sun. It is thought that our own sun, when reaching the end of its lifetime, may expand past the orbit of the earth, or 93,000,000/432,000: about 215 times it's original radius.

      Here is the link to the original paper.

    5. Re:Mass vs Radius by meringuoid · · Score: 1
      Ah, but core temperature isn't what we're interested in here. We're interested in the surface temperature. What are the dynamics of a star's atmosphere - of the outer layers of gas not participating in nuclear fusion? Well, there's gas pressure which tends to make the atmosphere expand and cool, and gravity which tends to make the atmosphere contract and heat up. As the atmosphere expands and cools, gas pressure decreases, and as the atmosphere contracts and warms, thermal pressure increases, and eventually an equilibrium is struck where the gas pressure outwards equals the gravitational force inwards.

      The core heat source is actually secondary to this. More massive stars are hotter because they are more massive - the sheer mass of gas that collapsed from a nebula to form such a star provides huge amounts of energy by gravitational accretion. Then, because of being so hot to begin with, they burn fuel faster than their smaller, cooler cousins, and that keeps them hot.

      So the largest stars are the ones where the equilibrium is found at a point where the atmosphere is large, sparse and cool, and hence red. This isn't such a star. In a super-hot star like this the radiation pressure comes to predominate over gas pressure, and that has a tendency to blow any surrounding gas clean away. It's too heavy, and, as you say, too hot, and very unstable. So it can't form a well-behaved convective envelope around itself and become a red hypergiant. It remains a very massive, very hot, and very luminous star, but it never troubles the list of the largest stars known.

      --
      Real Daleks don't climb stairs - they level the building.
    6. Re:Mass vs Radius by delt0r · · Score: 1

      Indeed when i said hotter--I meant more Luminous, as in more energy is radiated. However Average density is what defines the radius, and for a star like ours that's at the hydrogen burning phase, it does get larger and less dense with more mass (with a hotter surface IIRC with a CN cycle). Later in its life when burring heaver elements they swell to much larger sizes and become red giants.

      Also the heat of collapse does not change the equilibrium. It does change the amount of mass in the star (part of the gas gets blown away once the fusion starts).

      However, its been years since i ran the numbers.

      --
      If information wants to be free, why does my internet connection cost so much?
  9. not unlikely to be broken by wjh31 · · Score: 1

    On the contrary, the record is probably being broken currently, or maybe even was broken millions/billions of years ago, but the light has yet to reach us, our technology is unable to detect it, or we arnt looking in the right direction.

    1. Re:not unlikely to be broken by Nadaka · · Score: 1

      The thing about records is...

      They are not really records until they are recorded.

    2. Re:not unlikely to be broken by rossdee · · Score: 1

      Recorded by who?

    3. Re:not unlikely to be broken by necro81 · · Score: 1

      There's bound to be some sort of koan in there, along the lines of the tree falling in the forest:

      If a really freakin' huge star is created in the universe and no one is around to observe it, does it break a record?

    4. Re:not unlikely to be broken by Nadaka · · Score: 1

      The record keeper.

    5. Re:not unlikely to be broken by osu-neko · · Score: 2, Insightful

      If a really freakin' huge star is created in the universe and no one is around to observe it, does it break a record?

      That one's easy, as there are no unrecorded records, by definition. The real question is, lacking any observation, does it even exist, or does it just probably exist, or "exist" in an undetermined state until observed? And what counts as "observation"?

      --
      "Convictions are more dangerous enemies of truth than lies."
    6. Re:not unlikely to be broken by necro81 · · Score: 1

      Damn you, Schrödinger!

  10. Temperature on the surface of Sol by metamechanical · · Score: 3, Informative

    For anyone curious, as I was, what the surface temperature of our star is: 5500 degrees C

    My source was NASA's world book page (then again, it goes on to state that our solar system has nine planets, so trust NASA at your own risk)

    --
    If I had a nickel for every time I had a nickel, I'd be richcursive!
    1. Re:Temperature on the surface of Sol by Locke2005 · · Score: 2, Funny

      Huge props to the guy that managed to stick a thermometer in it!

      --
      I've abandoned my search for truth; now I'm just looking for some useful delusions.
    2. Re:Temperature on the surface of Sol by Muad'Dave · · Score: 4, Informative

      For anyone curious, as I was, what the surface temperature of our star is: 5500 degrees C

      Which you can derive from noting the Sun's yellow color (approximately 570–590 nm) and applying Planck's Law or Wein's Displacement Law in reverse. Note that this pic shows the 5500 degree C peak aligns well with 500-600 nm.

      From the Wein's Displacement article:

      " * The surface temperature (or more correctly, the effective temperature) of the Sun is 5778 K. Using Wien's law, this temperature corresponds to a peak emission at a wavelength of 2.89777 million nm K/ 5778 K = 502 nm = about 5000 Å. This wavelength is fairly in the middle of the most sensitive part of land animal visual spectrum acuity. Even nocturnal and twilight-hunting animals must sense light from the waning day and from the moon, which is reflected sunlight with this same wavelength distribution. Also, the average wavelength of starlight maximal power is in this region, due to the sun being in the middle of a common temperature range of stars.

      [See for example the article color, because of the spread resulting in white light. Due to the Rayleigh scattering of blue light by the atmosphere this white light is separated somewhat, resulting in a blue sky and a yellow sun]."

      [Emphasis mine]

      See also:

      http://hypertextbook.com/facts/2002/TahirAhmed.shtml

      --
      Tiller's Rule: Never use a word in written form that you've only heard and never read. You will end up looking foolish.
    3. Re:Temperature on the surface of Sol by BJ_Covert_Action · · Score: 1

      It does have 9 planets. Vulcan's real you insensitive clod!

    4. Re:Temperature on the surface of Sol by Amiralul · · Score: 1

      For anyone curious, as I was, what the surface temperature of our star is: 5500 degrees C

      Ha! My inductively coupled plasma has 6000 degrees celsius!

    5. Re:Temperature on the surface of Sol by Amiralul · · Score: 1

      Pluto was nothing like the "other" planets. I'm glad it's not considered an actual planet anymore. Just because you're spinning around the Sun, doesn't make you a planet, you know...

    6. Re:Temperature on the surface of Sol by Muad'Dave · · Score: 1

      Ha! My inductively coupled plasma has 6000 degrees celsius!

      <worfVoice>Then your "inductively coupled plasma" is weak!</worfVoice> lol

      This one claims a temperature of 25000 F (13871 C), and this one claims 15000 C.

      15000 C puts the peak spectral wavelength at about 190 nm, which is solidly in the near UV spectrum. Guard against 'sun' burn while using it! I've been 'sun' burned a few too many times arc welding. I tend to forget to cover the vee at the top of my shirt.

      --
      Tiller's Rule: Never use a word in written form that you've only heard and never read. You will end up looking foolish.
    7. Re:Temperature on the surface of Sol by Quirkz · · Score: 1

      For anyone curious, as I was, what the surface temperature of our star is: 5500 degrees C

      Which you can derive from noting the Sun's yellow color (approximately 570–590 nm) and applying Planck's Law or Wein's Displacement Law in reverse.

      So, uh, according to these laws, what color is 40,000 degrees Celsius? Your linked chart didn't seem to go that high.

    8. Re:Temperature on the surface of Sol by Muad'Dave · · Score: 1

      That corresponds to a wavelength of 72nm, which is way past purple, just past near UV and into the extreme UV part of the spectrum. Real sunburn, electron ejection, cats-living-with-dogs territory.

      http://en.wikipedia.org/wiki/File:Electromagnetic-Spectrum.png

      --
      Tiller's Rule: Never use a word in written form that you've only heard and never read. You will end up looking foolish.
    9. Re:Temperature on the surface of Sol by Quirkz · · Score: 1
      Thank you.

      Wow, Ultraviolet Sun? It sounds like a science fiction story from the 50's.

      It'd be about beings that live not on a planet, but on a small, cool star that, in comparison to the ultraviolet sun, might as well be solid ground. The UV sun is their star, because it's so much brighter and hotter than their own world.

      Completely nonsensical, of course, and also copyright by Shampoo, 2010.

    10. Re:Temperature on the surface of Sol by Muad'Dave · · Score: 1

      Remember that those equations give you the wavelength of peak intensity - there would likely be some of what we call visible light in that spectrum. There would be a lot more X- and gamma rays from that star than from the sun, through. Can you say mutation-a-go-go?

      Using the percentile table here and the spectral energy density function mentioned here, I calculate that a 40000 C star has less than of 1% its radiation in wavelengths that we consider visible. Additionally, the vast majority of that visible light would be at the violet end of the spectrum - talk about blue skies! 90% of its radiation would be in wavelengths shorter than 291 nm (UV), 99% in wavelengths shorter than 710nm (deep red), and 99.9% in wavelengths shorter than 1600nm (IR). Oddly, in space you wouldn't feel warmth from the star (little IR), but would get a heck of a sunburn (lots of UV+). Conversely only about 1% of the spectrum is in visible light and longer wavelengths (800-700nm and up).

      You can create graphs of the spectra by evaluating this equation over the desired wavelength range and temperature of interest (I'd suggest scaling them so that all of the irradiance values are a percentage of the max value for that object). You'll see that the spectrum of your uber star is very narrow compared to the Sun or a typical 288K planet in absolute wavelength terms, but that the spectral curves are identical when viewed with the X axis as a logarithmic scale.

      --
      Tiller's Rule: Never use a word in written form that you've only heard and never read. You will end up looking foolish.
  11. I was already impressed by VY Cannis Majoris... by Picass0 · · Score: 1

    ... a star so large if you swapped it with our sun it's surface would extend past Saturn's orbit.

  12. Anonymous Coward by Anonymous Coward · · Score: 5, Informative

    I puzzled over this for a bit too, but this newly discovered star is the most massive discovered. The largest known star in terms of size is still VY Canis Majoris at ~2000 solar radii, but only ~20 times the mass of the Sun.

    1. Re:Anonymous Coward by Chris+Burke · · Score: 3, Interesting

      Well yeah, the first line of the summary says "most massive", which in astronomy is usually (usually) what "biggest" means.

      Though it is admittedly ambiguous. I was watching Jeopardy (a taped episode a friend of mine was in and *won*) and one of the answers was "It's the biggest planet after Jupiter and Saturn", and the correct question was "Neptune?" (the 3rd most massive) but the contestant questioned "Uranus?" (3rd largest diameter). The judges ended up accepting it due to the ambiguity of the question.

      And I know that I personally consider the Jeopardy judges to be the ultimate authority on when something is ambiguous and multiple interpretations are valid!

      --

      The enemies of Democracy are
    2. Re:Anonymous Coward by Anonymous Coward · · Score: 0

      The correct question is "What is Uranus/Neptune?" ...

    3. Re:Anonymous Coward by Chris+Burke · · Score: 1

      I edited for brevity. Though I think it would be funny if simply giving the "answer" with an upturned inflection was sufficient.

      --

      The enemies of Democracy are
    4. Re:Anonymous Coward by vrt3 · · Score: 1

      The judges ended up accepting it due to the ambiguity of the question.

      Don't you mean the ambiguity of the answer?

      --
      This sig under construction. Please check back later.
  13. Yo momma so fat ... by jbeaupre · · Score: 4, Funny

    she breaks the Eddington limit! (sorry, couldn't help myself)

    --
    The world is made by those who show up for the job.
    1. Re:Yo momma so fat ... by tooleb · · Score: 1

      I had the same thought....

  14. Link to research paper (arxiv) by Octoploid · · Score: 5, Informative

    Here is the link to the research paper: http://arxiv.org/abs/1007.3284

  15. VY Canis Majoris by Spacelem · · Score: 3, Interesting

    The article states that R136a1 is 265 solar masses, however it doesn't say how big it is.

    VY Canis Majoris is 2,100 times the size of the sun, and 230,000 times the size of Earth. It is so huge, that if it occupied the centre of our solar system, its boundaries would be Saturn's orbit.

    If R136a1 is the heaviest star, then it must be considerably more dense than VY Canis Majoris, but I find the latter to be far more impressive.

    1. Re:VY Canis Majoris by Anonymous Coward · · Score: 0

      If a star is so big that it goes out past Saturn's orbit, its radius is 2100 times our Sun's radius. That makes it 2100^3 times the volume of our Sun. In other words, VY Canis Majoris is 10 billion times the size of our Sun!

      dom

    2. Re:VY Canis Majoris by Anonymous Coward · · Score: 0

      Don't worry, if you just wait around long enough I'm sure that R136a1 will swell up to a much larger size. And shortly thereafter it will shrink rapidly. And then expand very, very, very rapidly....

    3. Re:VY Canis Majoris by stewardwildcat · · Score: 3, Informative

      You are correct! I am an astronomer and want to straighten out a few things. When it comes to stars, MASS is what matters. Mass governs the size, lifetime, luminosity, and temperature of the star. To form a star gas clouds in the galaxy slowly collapse under their own gravity and form dense clumps, these clumps continue to collapse sometimes forming a single or multiple stars. In the centers of the largest star forming regions, these clumps are very dense and are close to each other which increases the probability that they will bump into each other and combine. This is one theory of how we can form the most massive stars, where several smaller, say 50-100 solar mass stars get squished together to form a so called 'hyper star' of several hundred solar masses. Once the star is formed it is on what we call the 'Main Sequence' where it will fuse hydrogen into helium in its core. At this time the star will have the hottest surface temperature of its life as well as the smallest physical size for its evolution. The reason a 'smaller' sized star can be so bright is the fact that luminosity (L) is related to the star's surface area (A) times the surface temperature (T) to the 4th power (L=A*T^4). Because this star is so hot, it can be 10 million times brighter than our sun but is maybe 10-100 times the physical size (radius). To continue evolving the star, as it ages the star will "puff up" and cool becoming a red hypergiant in this case. This is after it has used up all the hydrogen in its core. The star is headed for death but seems to keep roughly the same luminosity as it cools down and expands. If it cools from 80,000 Kelvin to 3,000 Kelvin then it must expand to 500,000 times its original surface area or 700 time larger in radius. This is why stars like VY CMaj and Alpha Ori (Betelgeuse) are so astronomically huge. They do not have to be extremely massive to become incredibly large in radius. VY CMaj is only 25 times the mass of our sun and is mind-bogglingly HUGE. Think of what a star 10 times more massive would look like when its on its death bed. If you live in the southern hemisphere when this new star dies, you will certainly see the supernova with your naked eye. So while in size this new star seems to be small in comparison to some nearby giants, when it is compared side by side its beyond anything we have seen before.

    4. Re:VY Canis Majoris by plut4rch · · Score: 1

      It's estimated to be around 30 times the radius of our sun, I think.

      --
      An intriguing solution to a problem that should never have existed in the first place...
    5. Re:VY Canis Majoris by instagib · · Score: 1

      That's what she hoped...

    6. Re:VY Canis Majoris by toddestan · · Score: 1

      I don't know who put this animated gif together:
      http://s273.photobucket.com/albums/jj210/RUPERT_THE_MAYOR_OF_CRAZYTOWN/?action=view&current=wjyvqw.gif&newest=1

      But it helps with trying to visualize just how large some of these stars are.

    7. Re:VY Canis Majoris by Anonymous Coward · · Score: 0

      Yeah, mass is just relative to the amount of Matter the object consists off, where as size is relative to the amount of Volume the object is. R136a1 is 265 Solar Masses, but only 35 times the diameter of our Sun. In terms of Mass, R136a1 wins. However, in terms of Volume, R136a1 is only 35 times the Diameter of our Sun. Our Sun is approximately 865,000 Miles in Diameter. R136a1 is approximately 30,275,000 miles in Diameter, pretty large. If it were to replace our Sun, it would be touching the Boundaries of Mercury's Orbit, which is approximately 35,000,000 miles. Earth is approximately 93,000,000 miles away from the Sun. To give you an idea of our Voluminous VY Canis Majoris is, it is 1,800,000,000 miles across. 1,800,000,000 > 30,275,000 by a long shot. Saturn's Orbit is 1,350,000,000 away from the Sun. So, if R136a1's outer edges would singe Mercury if it were in the place of our sun, VY Canis Majoris in it's place would be hiding Mercury, Venus, Earth, Mars, Asteroid Belt, Jupiter and Saturn in itself, with room to spare.

    8. Re:VY Canis Majoris by Spacelem · · Score: 1

      When it comes to stars, MASS is what matters. Mass governs the size, lifetime, luminosity, and temperature of the star.

      Ah! Fair enough, I didn't realise how important the mass was to a star. When you put it in those terms, R136a1 suddenly becomes much more impressive.

    9. Re:VY Canis Majoris by Spacelem · · Score: 1

      Actually that animation was how I first found out about VY Canis Majoris. It's quite difficult to picture something "2100 X" the size of something else at that scale, because it's far bigger than anything we can really comprehend. However, I've seen it put quite elegantly somewhere:

      Imagine that Earth is a ball with a 1cm diameter, then the sun is a ball with a 1.09m diameter, and VY Canis Majoris is a ball with a 2.3km diameter. By rescaling to these sizes, I can just about handle the size differences. Sometimes a little perspective is good.

  16. Scientists are late. by 140Mandak262Jamuna · · Score: 1

    These scientists are quite late to the party. Tamilians had discovered the Biggest Star, The Super Star, Rajnikant way back in 1975.

    --
    sed -e 's/Chuck Norris/Rajnikant/g' joke > fact
    1. Re:Scientists are late. by Anonymous Coward · · Score: 0

      With a super star that close, they must be some really hot tamilians!

  17. So these stars are Orkans? by Chas · · Score: 1

    "Unlike humans, these stars are born heavy and lose weight as they age,"

    If I get burned to death by Johnathan Winters I'm going to be PISSED!

    --


    Chas - The one, the only.
    THANK GOD!!!
  18. peck by Anonymous Coward · · Score: 0

    I always though that the biggest star was Prince :/

  19. What bugs me about stories about space by dimethylxanthine · · Score: 0

    is that discoveries like that require extensive use of one's imagination to visualise what the biggest star, the longest gravitational jet or the exoplanets that have been "imaged directly" actually look like... An "artist's impression" is to astrophysics as artificial flavouring is to food.

  20. Re:The Biggest Open Source Starr by Anonymous Coward · · Score: 0

    I lol'd

  21. Oblig.. by Anonymous Coward · · Score: 0

    We should never need a star more than 265 solar masses.

  22. Why isn't it... by camperdave · · Score: 1

    256 solar masses? I thought everything over 10 solar masses collapses into itself, forming a black hole. What's going on with this star?

    --
    When our name is on the back of your car, we're behind you all the way!
    1. Re:Why isn't it... by Anonymous Coward · · Score: 0

      They don't do it immediately. They burn for a while, and then when they have exhausted their fuel they collapse. If they are massive enough they can collapse to black holes. In order to do that they need to keep more than about 1.4 solar masses, after any matter ejection that occurs as part of the collapse process.

    2. Re:Why isn't it... by Anonymous Coward · · Score: 0

      There are several methods of star death depending on star mass and composition. For stars in the 130-2xx solar mass range (the upper bound isn't clear), the common result is something called a pair-instability supernova. As the star ages (quite rapidly for such a large star), it heats up. When gamma ray production in the core (which is temperature dependent) hits a certain point, the gamma rays start to spontaneously create electrons and positrons. Since these particles travel much slower than gamma rays, more of the energy is trapped in the core, which causes it to heat up, which produces more gamma rays... you see where I'm going with this. The net result is that the core temperature spikes, everything fuses to iron instantly, and the star blows up without leaving a black hole behind.

      Stars between 50 and 130 masses collapse directly into black holes at the end of their natural lifespan without exploding.

      Stars like this one, above 2xx solar masses (again, not sure where that bound is and it's probably dependent on composition, spin rate, etc.) are going to do something a bit different - their cores get *so* hot that the energy actually rips apart all the heavier elements that the star created through fusion. This uses up energy, cooling and contracting the core catastrophically, which results in a good ol' fashioned rebound supernova (well, hypernova, really) and a black hole remnant just like stars in the 20-50-ish solar mass range.

    3. Re:Why isn't it... by Anonymous Coward · · Score: 0

      The mass limits you're thinking about refer to the ultimate state of a star, not its immediate state. Stars over a certain mass are doomed to become black holes once they've exhausted their fusion fuel and can no longer resist the forces of gravity. Less massive stars will not become black holes at the end of their lives. But in any case, very massive stars can exist because the outward pressure from fusion is enough to resist the inward pressure of gravity.

      As for the actual limits, if the end-of-lifetime mass (after shedding outer layers, etc.) is below 1.4 solar masses, it becomes a white dwarf. If it's above that, it instead collapses into a neutron star... or if the remaining mass is above 4 solar masses, collapses all the way down to a black hole.

    4. Re:Why isn't it... by NotBornYesterday · · Score: 1

      The same thing keeping any star from collapsing: fusion. Black holes form when a star of sufficient mass (which is where the Tolman–Oppenheimer–Volkoff limit of 10 solar masses comes in) can't support itself through nuclear reaction in its core. See also supernovae.

      --
      I prefer rogues to imbeciles because they sometimes take a rest.
    5. Re:Why isn't it... by Locke2005 · · Score: 1

      Just because it hasn't collapsed into itself yet doesn't mean it isn't going to eventually. This is a very young star formed by merging several other together. Once it's fusion engine slows down, it should collapse. It's not like these things happen overnight!

      --
      I've abandoned my search for truth; now I'm just looking for some useful delusions.
  23. Can we watch it die? by Nadaka · · Score: 1

    The more massive the star, the shorter its life as it burns through its fuel more quickly.

    Stars smaller than the sun are believed to endure for hundreds of billions or even trillions of years.

    Stars of near the suns size last for billions to tens of billions of years.

    Large stars are believed to last for tens or hundreds of millions of years.

    The largest previously known stars at up to a hundred times the suns mass are believed to live for only a few hundred thousand or million years.

    How long will this star last? Millennia? Centuries? Decades?

    1. Re:Can we watch it die? by imakemusic · · Score: 1

      I'm no expert by any means but here are some numbers I pulled out of...Google. By extrapolating from what this guy says I get an answer of about only 750,000 years and judging by what else I've read that number is probably very low. Not that long on the cosmic scale but a little longer than you or I will be around for.

      --
      Brain surgery - it's not rocket science!
  24. The "Eddington Limit" is NOT based on science by Anonymous Coward · · Score: 0

    It is merely a revenue generator.

  25. That's a big Twinkie by Picass0 · · Score: 1

    TSIA

    1. Re:That's a big Twinkie by fiannaFailMan · · Score: 1

      TSIA

      I hate acronym abuse. Why can't people just speak fucking English? I mean, not even Google can decipher this post! Technology Services Industry Association? Twinkies? What the fuck are you waffling about?

      Sheesh!

      --
      Drill baby drill - on Mars
  26. Ten million times brighter than the Sun? by fuego451 · · Score: 2, Interesting

    How do they measure that? As an amateur astronomer, I understand relative magnitude but...wow. I'm guessing they use some other method? Also, would this star be considered a super-massive blue giant or...?

    1. Re:Ten million times brighter than the Sun? by Kaz+Kylheku · · Score: 4, Interesting

      I'm guessing that what it probably means is that this star is estimated at having ten million times the power output compared to the Sun. Therefore, at some fixed reference distance, it would deliver ten million times more watts of illumination per square meter. This doesn't mean that the surface brightness is ten million times greater than that of the Sun, because some of the brightness comes from the greater size of the star. If you make a lamp with one hundred light bulbs, they are not individually brighter than a single light bulb, but as an aggregate, they provide more illumination, and can be more easily seen from farther away.

    2. Re:Ten million times brighter than the Sun? by stewardwildcat · · Score: 1

      Spectroscopy, modeling, and relative photometry. Many of the brightest stars in R136 have been well studied and by comparing brightness at the same distance you can measure the luminosity. That said, you might like to know what has happened to most of the previously discovered most massive stars. With the advent of larger and space telescopes, the HUGE stars were found to be very very tight binaries that were not resolved as individual stars previously.

    3. Re:Ten million times brighter than the Sun? by stewardwildcat · · Score: 1

      If I have 1 100W bulb and compare it to 2 100W bulbs, a single patch of surface area will not be intrinsically brighter but the object with two bulbs is twice as bright. I posted about this elsewhere on this page already, but luminosity is equal to the surface area (A) times the Temperature(T) to the 4th power. L=A*T^4. Every lightbulb has the same temperature but as you add lightbulbs together the emitting area goes up. If you took a star like our sun, kept the surface temperature the same but made it a million times bigger in size, the luminosity would go up 1 million times.

  27. Yo momma's so fat by Anonymous Coward · · Score: 0

    she's measured in solar masses.

  28. Your momma jokes.... by mace9984 · · Score: 1

    Ready and ... Start!

  29. New name for R136a1 by Anonymous Coward · · Score: 0

    Since R136a1 is a rather boring name, based on the physical description I propose the name "Mother-in-Law of All Stars".

  30. what does 265 solar masses mean? by oddTodd123 · · Score: 2, Funny

    I need that in units I can comprehend:

    The mass of the sun is 1.99x10^30kg. The average mass of a book is 340g. There are 21,814,555 books cataloged by the Library of Congress. So, 265 solar masses * 1.99x10^30kg/solar mass * 1000g/kg / 340g/book / 21,814,555 books/LoC = 7.1x10^25LoC. Therefore, the new star is equivalent in mass to 71YLoC (yotta Libraries Of Congress). Wow, that's a big star!

    1. Re:what does 265 solar masses mean? by Anonymous Coward · · Score: 0

      7.1x10^25 libraries is easier for you to comprehend than 265 solar masses?

      What is wrong with you?

    2. Re:what does 265 solar masses mean? by Anonymous Coward · · Score: 2, Funny

      And since the radius is about 30 times greater than the Sun's, R136a1's radius must be about 12964909.92 miles, which we can convert to 2111196448775450 square miles of surface area. That's roughly equal to 1759330373979.54 Rhode Islands! You're right, that star is HUGE!

  31. Uhoh by Anonymous Coward · · Score: 0

    Céline Dion is really pissed that she was just over taken

  32. Oh noes, 265! by RegTooLate · · Score: 2, Funny

    256 solar masses should be enough for anyone.

  33. "Unlike humans ..." by Kaz+Kylheku · · Score: 3, Insightful

    From article: "Unlike humans, these stars are born heavy and lose weight as they age," Crowther said.

    This is obviously wrong. Some humans are plump when young, and turn into skeletons as they age.
    In fact, this is commonly observed among those humans who, ironically, are called ``stars''.

    1. Re:"Unlike humans ..." by hesaigo999ca · · Score: 1

      i don't know how to rate this, funny, offtopic, troll....there is just too many levels to your comment.. O_O

    2. Re:"Unlike humans ..." by shaitand · · Score: 1

      The gp didn't refer to plumpness, he referred to weight. Those old skeletons still weigh more than infants.

    3. Re:"Unlike humans ..." by shaitand · · Score: 1

      Sorry, gp should have been "the article"

    4. Re:"Unlike humans ..." by alexo · · Score: 1

      Some humans are plump when young, and turn into skeletons as they age.

      Most humans eventually turn into skeletons (unless e.g. cremated)

  34. Original Journal Article by catchblue22 · · Score: 2, Informative

    Here is a posting on Science Magazine's ScienceNow, and here is the original journal article originally published in the Monthly Notices of the Royal Astronomy Society. I think it is always better, when possible to refer to original sources when talking about scientific issues. Scientific discussions can become muddled when translated by journalists.

    --
    This and no other is the root from which a tyrant springs; when first he appears as a protector - Plato (423 to 327 BC)
  35. Eddington by hesaigo999ca · · Score: 1

    Eddington I guess was a hog for headlines, why would he need to say there is a limit to anything, on what grounds did he base it on, did he get core samples of our sun, was he anywhere near the sun to see if maybe there might be some form of material missed in his calculations to know how the sun keeps its light (fire) going....

    I find too many space scientists are using their theories and saying that this is fact. I just hope now we can have an end to this, and go on thinking the universe is limitless like the church tells us it is....

    1. Re:Eddington by Lithdren · · Score: 1

      TLDR version of your comment:

      LOL SCIENCE IS HARD. They got it wrong, that means I'm right!

      Nobody says its a fact except the idiot journalists who write about it, and the idiots like you who believe the journalists. Just an FYI.

    2. Re:Eddington by east+coast · · Score: 1

      I go half and half with you and Lithdren on this one:

      I have heard scientists come out and make wide and absolute proclamations that really don't seem to be based on much more than known observances. There is just so much we don't really know yet.

      At the same time, the evening news, that runs 4 hours, seems to be too busy reporting on the latest celebrity and sport star gossip to give any scientific press release more than 30 seconds. So much is lost in this sound bite society.

      I do wonder about where the church mentions that the universe is limitless. I've never heard this.

      --
      Dedicated Cthulhu Cultist since 4523 BC.
    3. Re:Eddington by JSBiff · · Score: 1

      I may be wrong, but I don't believe the article even suggests the Eddington limit is wrong, even now. The Eddington limit seems to say that when a star exceeds a certain mass, the amount of energy radiated from the star becomes so great that the star will begin gradually losing mass (absent some other source of additional mass being added to the star, such as the star merging with another star), until it reaches the Eddington limit, then it might attain a sort of equilibrium.

      From my reading of the article, this has not been demonstrated to be wrong. They've just found a very young star which is much more massive than typical, but that doesn't mean the Eddington limit is wrong - it would only be wrong if the star is not losing mass.

    4. Re:Eddington by hesaigo999ca · · Score: 1

      >this has not been demonstrated to be wrong
      All I am saying is we say these things with supposed certainty, when none of these scientists have even come close to the sun to be able to figure out what it consists of, and if there is an unknown element that helps fuel its light/fire, that we still are not knowing...and of course when I mention
      hey this guy obviously is wrong because here is a contradiction to what he was saying, and we should review his whole theory, because it is just a theory...with a fine tooth comb, everyone jumps on the bashing band wagon....

    5. Re:Eddington by hesaigo999ca · · Score: 1

      the universe is limitless because the church knows nothing about it, so because of its lack of knowledge, the universe is like god and god is limitless so therefor so is his universe we live in, but I believe in science so I don't buy this either...

    6. Re:Eddington by hesaigo999ca · · Score: 1

      All I am saying is we say these things with supposed certainty, when none of these scientists have even come close to the sun to be able to figure out what it consists of, and if there is an unknown element that helps fuel its light/fire, that we still are not knowing...and of course when I mention
      hey this guy obviously is wrong because here is a contradiction to what he was saying, and we should review his whole theory, because it is just a theory...with a fine tooth comb, everyone jumps on the bashing band wagon....

  36. Meh. by PPH · · Score: 1

    Marlon Brando. Old news.

    --
    Have gnu, will travel.
  37. Amusing by shaitand · · Score: 0, Troll

    "Crowther adds that R136a1 is about as big as stars can get."

    This week, last week we thought they could only get to about 60% of this size.

    You'd think the scientist would be a bit more cautious before making a leap like this after a previous widely accepted theory was crushed. Of course tomorrow someone will be assuring us all that scientific theories are really more like facts than current, subject to change, understanding.

    Of course theories are not mere guesses but they are often given as much too much weight in the scientific world as they are given too little in the civilian.

    Additionally, there is the bogus idea that a revised theory should still be considered a theory. Instead a revised theory is now no more than a hypothesis, requiring fresh predictions (to be tested against new observation not previous data) and verification and requiring the fresh application of Occam's Razor (since a revised theory is also usually going to have additional complexity to patch up the previous theory).

    1. Re:Amusing by stewardwildcat · · Score: 1

      Additionally, there is the bogus idea that a revised theory should still be considered a theory. Instead a revised theory is now no more than a hypothesis, requiring fresh predictions (to be tested against new observation not previous data) and verification and requiring the fresh application of Occam's Razor (since a revised theory is also usually going to have additional complexity to patch up the previous theory).

      While I cannot completely disagree with your argument, theories are just that, a working hypothesis. We have a model that describes everything that happens in the universe around us. We call this model a theory. It does an amazing job predicting 99.999% of everything we see. Then someone makes a discovery that contradicts some of the assumptions and outcomes of the theory. We go back, look at the physics, and adjust/revise, the theory so it can explain all of the observations. Its not that the theory is broken or is wrong, it could not describe EVERYTHING. Every theory must explain existing data as a start and then make predictions about the data we will take in the future. A great way to test a theory is to see if it can model existing data. The data don't change because you changed your theory but if you need to make a new prediction then you need new data to test that piece. A good example of this is Newton's Laws of Gravity. NO ONE can argue that gravity exists and that Newton's Laws work for almost everything. Well they didn't work for Mercury's orbit. When they compared the predictions of Mercury's orbit from Newton's Laws, they found that the model was off by 43 arcseconds every centrury. Does that mean Newton's laws don't work here on Earth? No, it means we needed a new model of how gravity worked in more extreme situations. This is where Einstein's Theory of General Relativity comes in. It explained the precession right away and we have used Relativity since then to explain motions around black holes and other extreme objects. Newton's Laws still work perfectly fine with in the errors of measurement for everything else.

  38. Scientsist Discover Biggest Star... by tekrat · · Score: 1

    Scientsist Discover Biggest Star : Kirstie Alley.

    --
    If telephones are outlawed, then only outlaws will have telephones.
    1. Re:Scientsist Discover Biggest Star... by mark72005 · · Score: 1

      Damn you Trebek!

  39. Biggest Star by mark72005 · · Score: 1

    I thought the answer would be "Jones".

  40. is it really that massive? by phlegmofdiscontent · · Score: 1

    I've read numerous articles in the past dealing with supermassive stars and as often as not, the largest stars turn out to be binaries, i.e. what they thought was a 300 solar mass star was simply two 150 solar mass stars. However, I read the paper on arxiv (http://arxiv.org/PS_cache/arxiv/pdf/1007/1007.3284v1.pdf) and it appears that the scientists have ruled that out. The thinking is that if it was actually two unresolved stars revolving around each other, their stellar winds would collide and produce x-rays, which are not evident.

    However, they do rely heavily on models to come up with the theoretical mass. Without an orbiting companion, it's currently impossible to measure the mass reliably except for depending on those models. Refined models may result in different masses.

    Another thing to consider is this. The Eddington limit refers to a star in equilibrium. However, such a large star is not in equilibrium. In the paper, they estimate its original mass to be about 320 solar masses, with 265 being the current mass. Obviously, since the star exceeds the Eddington limit, it is shedding its outer layers as expected. In this case, it has shed a whopping 55 solar massses since its birth...

  41. "Very Large Telescope" by karlandtanya · · Score: 1

    Beautiful.
    An accurate and descriptive term.
    Anything else would detract from the truth--something simply is what it is.

    We must get sales and marketing involved for the next one, though!
    We need a snappy name--something that really pops--for several of them working together, perhaps arranged in some sort of an array?

    --
    "Reality is that which, when you stop believing in it, it doesn't go away." - Philip K. Dick
    1. Re:"Very Large Telescope" by sneakyimp · · Score: 1

      I Agree. R136a1 is hardly a good name for one of the biggest.

      My girlfriend suggested Prometheus for the big one.

      Maybe 'the four horsemen' ?

    2. Re:"Very Large Telescope" by Anonymous Coward · · Score: 0

      I thought R136a1 was the coolant they used.
      Something that big must need a hell of an A/C.

  42. Summary error. Limit to star masses ~60solar by Anonymous Coward · · Score: 0

    Summary error. Limit to star masses ~60solar. Because the collapse of such a star to start internal fusion reaction would require such density as to immediately cause the star to go nova, ejecting the still-accreting star. This was figured to be bollocks in the 90's AT LEAST because in 92 I investigated an area less than 10AU across that had to have at least 150 solar masses amongst two stars (60 and 90) and another case where 220 solar masses were shared amongst no more than three ignited stars, the largest one being 120 solar masses for most likely setup.

    I know because I did an undergrad dissertation on supermassive stellar objects, which I reckoned everyone else would be yibbering on about supermassive black holes. I figured I'd look into supermassive STARS so I wouldn't be competing with others' efforts. Didn't work because it went to a prof who

    a) liked supermassive black holes in galaxies
    b) thought stars >60 solar masses were impossible and just cranks believed it

    Nearly got him crying when trying to get him to justify the mark he gave... >-)

  43. That's a puppy... by Anonymous Coward · · Score: 0

    That's a puppy...There's one that is assumed to be just a gas cloud it's so big, except it's an eclipsing binary, so that's a HEAVY gas cloud and small enough that a star will go around it often enough we can see the light curve change.

    It would extend three times that diameter (no less than 3 billion km).

    But because of that damn cool.

    Mind you, may find that is an extended atmosphere of a supermassive star that is shucking out gurt big lumps of atmosphere and not really a star per se at all.

    Bummer...

  44. Much ado over Pluto (OT) by khallow · · Score: 3, Insightful

    then again, it goes on to state that our solar system has nine planets, so trust NASA at your own risk

    Argh, this nonsense again. The IAU dropped the ball and we remain without an adequate definition of what a planet is. "Clearing the neighborhood" remains undefined and there are ways to define "neighborhood", as a large loci in space-time around the trajectory of the object in question, so that Pluto, and perhaps even Ceres and some of the dwarf planet candidates, clear their neighborhoods. The point here is that while a considerable number of astronomers intend a particular definition of "neighborhood" (as a spherical shell around the Sun), that definition has not been adopted nor, I might add, does it seem all that useful.

    Semantically, it's also a mess since we have "minor planets" and now "dwarf planets" which are not "planets". Also, it just confuses the issue for the billions of people who were taught for decades that Pluto was a planet. I find the redefinition of "planet" to be inconsiderate of their needs and as a result rather frivilous abuse of IAU's power. Just because we had a similar screw up back when Ceres was demoted as a planet, doesn't mean that we need to repeat this error.

    Finally, this definition only applies to the Solar System. We'd have enormous difficult applying this definition anywhere else. It would be hard and time consuming to verify the dynamics of other star systems in enough detail to distinguish between planets and dwarf planets using such a definition. And those systems may have orbital dynamics that are far different from the nearly circular orbits of planets in the Solar System.

    Personally, I have no problems with eight, nine, or hundreds of planets. But I think it reasonable that the definition of planet have a scientific basis. That bit is the common view I share with the people who came up with the current definition. But I think it's been an embarrassment to come up with the current weak and unuseful definition and then attempt to sell it as being scientific (remember the old definition happens to be much more well-defined and hence, scientific than the new one, people were just concerned about the growing number of objects that would be considered planets).

    Personally, I find it more credible that we're just seeing a continuation (in intellectually mutated form) of the old, irrational opposition to Pluto's original naming. Its first two letters, "P" and "L" happen to be, either by coincidence or artifice, the initials of Percival Lowell, the man who had established and funded the observatory that discovered Pluto.

    1. Re:Much ado over Pluto (OT) by osu-neko · · Score: 1

      o.O

      Thanks for the wonderful example of the irrationality that surrounds this particular debate.

      --
      "Convictions are more dangerous enemies of truth than lies."
    2. Re:Much ado over Pluto (OT) by khallow · · Score: 1

      Thanks for the wonderful example of the irrationality that surrounds this particular debate.

      For background, I'm a mathematician. Defining things precisely is one of the things I do. I also have a somewhat compulsive behavior. So yes, the IAU redefinition really ticks me off in an irrational corner of my mind. But it also was a rather cavalier thing to do to the public especially when coupled with the subsequent condescending lectures on the philosophy of science (which were wholly irrelevant to the action). As I see it, here's the argument for the current IAU definition: "We had to change the definition of 'planet' so that school kids wouldn't need to memorize a zillion different names." That's acceptable, but they should have carried through with a competent definition afterward.

    3. Re:Much ado over Pluto (OT) by Chris+Burke · · Score: 1

      "Clearing the neighborhood" remains undefined and there are ways to define "neighborhood", as a large loci in space-time around the trajectory of the object in question, so that Pluto, and perhaps even Ceres and some of the dwarf planet candidates, clear their neighborhoods.

      You have a fair point that the definition of "neighborhood" is vague, but all sensible attempts at least refer to the entire orbit and not just the immediate vicinity of the planet. By that standard, vagueness notwithstanding, it is obvious that Pluto and Ceres have not cleared their neighborhood and the eight planets have.

      All the planets have masses which are at least several orders of magnitude larger than the rest of the mass in their orbit combined. Pluto is a small fraction of the rest of the mass in its orbit, less than 0.1. Ceres has a higher ratio than that, but it's still well under 1.

      There's a huge gap in orbit-clearing ability that clearly distinguishes Pluto from Mars, and you can say it's possible to define your way around this clear and obvious distinction but that doesn't make the distinction go away.

      Pluto is not a planet. It's a large Kupier Belt Object, but not one so large that it isn't just another asteroid in the belt. It was a mistake to ever call it a planet, and I'm sorry for everyone who grew up learning about the 9 planets and can't get used to the idea that the only reason we ever called it that is because we didn't know any better. Our telescopes sucked then compared to now; we were lucky to see it at all. Oh well, things change.

      --

      The enemies of Democracy are
    4. Re:Much ado over Pluto (OT) by khallow · · Score: 1

      You have a fair point that the definition of "neighborhood" is vague, but all sensible attempts at least refer to the entire orbit and not just the immediate vicinity of the planet. By that standard, vagueness notwithstanding, it is obvious that Pluto and Ceres have not cleared their neighborhood and the eight planets have.

      First, keep in mind that the orbit is the trajectory of the planet. The 3-dimensional paths we trace out are a convenient fiction and every Solar System body deviates to some degree from this path.

      Aside possibly from an occasional visit by Eris, nothing larger than Pluto appears within 11 AU of Pluto. That's huge for an "immediate neighborhood", especially given that Pluto's closest approach to the Sun is 29 AU. Those numbers are comparable to the planets. Ceres probably has similar ratios as well.

      The proposed definition used a heuristic that happened to conveniently delineate most existing planets (save Pluto) from the new and old objects that could be considered planets. That's fine. What's not fine is both failing to complete the definition and wrapping the decision in sanctimonious terms. For example,

      Pluto is not a planet. It's a large Kupier Belt Object, but not one so large that it isn't just another asteroid in the belt. It was a mistake to ever call it a planet, and I'm sorry for everyone who grew up learning about the 9 planets and can't get used to the idea that the only reason we ever called it that is because we didn't know any better. Our telescopes sucked then compared to now; we were lucky to see it at all. Oh well, things change.

      Just because the IAU settled on one particular heuristic approach for deciding what a planet is, which so happens to weed out Pluto, it is now a "mistake" to have ever called Pluto a planet. Can't you even see the problem with your words?

      Here's another heuristic choice for definition. An object is considered a planet, if it is not a Moon (that is, gravitationally bound to a nearby object and the center of gravity of the local system is within that other object) and the mass, averaged over time, gravitationally bound to the Sun but not to the object and within a sphere a third of the closest distance to the Sun, is less than 1% of the mass of the local system to which the object is gravitationally bound. Pluto is likely a planet under that definition while more distant Kuiper belt objects may not be (they might not be in orbital resonance with Neptune). Ceres probably would not be a planet.

      As a heuristic definition it has pluses and minuses compared to the probable IAU definition. It has a natural definition of neighborhood unlike the IAU definition. However, the mass content of that neighborhood for distant objects is unknown, meaning you can have for long periods of time "probable planets" after they are discovered, but before the mass content of their neighborhoods is determined.

      The point here is that I have a more rigorous and scientific definition for planets than the IAU generated. But it results in a slightly different set of objects as planets. This is why your assertion above is so abominable to me. You are claiming a subjective choice was objective. And then you trot out a cliche about change, implying resistance to the IAU definition is solely by sticks-in-the-mud.

    5. Re:Much ado over Pluto (OT) by Chris+Burke · · Score: 1

      First, keep in mind that the orbit is the trajectory of the planet. The 3-dimensional paths we trace out are a convenient fiction and every Solar System body deviates to some degree from this path.

      Okay, that's what you meant. It sounded like you were talking about some 4-D volume some distance from the object, and some fixed amount of time. I misunderstood.

      But if we're talking about considering the whole orbit and a reasonable distance...

      Aside possibly from an occasional visit by Eris, nothing larger than Pluto appears within 11 AU of Pluto. That's huge for an "immediate neighborhood", especially given that Pluto's closest approach to the Sun is 29 AU. Those numbers are comparable to the planets. Ceres probably has similar ratios as well.

      So it's the biggest Kuiper Belt Object known. So what? There are several objects approaching its size in similar orbits known. Those plus all the smaller objects total over 10 times Pluto's mass. It's "neighborhood" looks nothing like the neighborhoods of the other planets. They've all cleared their orbits to the point where they dominate by at least 4 orders of magnitude. And while most of them have other small objects in their orbits, they're ones that have been gravitationally captured by the planet, either orbiting the planet or clustered around La Grange points. Aforementioned mass ratio means Pluto isn't close to dominating its orbit with its gravity. It's this gravitational dominance that clearly sets apart the 8 planets from Pluto and similar objects.

      Just because the IAU settled on one particular heuristic approach for deciding what a planet is, which so happens to weed out Pluto, it is now a "mistake" to have ever called Pluto a planet. Can't you even see the problem with your words?

      Just because primitive instruments meant that Pluto was the only object of its asteroid belt to be seen and assumed to be largely alone in its orbit like the other planets, the decision to call it a planet wasn't made out of ignorance? Not in a pejorative sense, but the literal meaning of "lacking knowledge"?

      If the main asteroid belt had been discovered more or less all at once, then I doubt we would have ever called Ceres a planet. We did call it a planet, but it's not a planet, it's just the biggest rock that coalesced from the remnants of what could have been a planet but probably got ripped apart by Jupiter before it could congeal. It seems silly to call it a planet when it's surrounded by rubble of a comparable mass. And Ceres accounts for 1/3rd of the asteroid belt mass, a much greater ratio than Pluto. But because of the great distance Pluto orbits at, it took much longer for us to realize it was not a lone planet with a few objects clinging around, but part of an asteroid belt similar to the inner one.

      We only called Pluto a planet because we didn't realize that, and so many people are complaining only because we just realized this recently so most of us grew up looking at diagrams that showed Pluto as the 9th planet. Those same diagrams show the asteroid belt, and of course we have no qualms about not calling Ceres a planet because it's obviously just a part of the belt, though big and interesting. In another generation the textbooks will show a second asteroid belt, and it'll seem quite logical that Pluto isn't classified as a planet, since it is just another component of the belt that is of scientific and historical interest.

      Here's another heuristic choice for definition.

      Okay, I realize that this whole exercise is about the human desire for names and classifications, and not a rule of the universe. I recognize that this means the real distinction is vague, and attempts to precisely define the criterion involve some amount of arbitrariness. Pointing that out is completely valid criticism.

      On the other hand, this is a heuristic that is somewhat comparable to the criterion by which we first named Ceres and Pluto planets, and also comparable to the reason why we

      --

      The enemies of Democracy are
    6. Re:Much ado over Pluto (OT) by khallow · · Score: 1

      You want Pluto to be a planet because it was one for 70 years, even though our impression of Pluto's role in the solar system has changed greatly since that time.

      No, I can live with Pluto being or not being a planet. What bothered me was the frivolous and sloppy manner of making the new definition. To be blunt here, I see little scientific value in changing a 70 year old official definition of planet. We don't become more stupid or less just because we change our minds about what characteristics acquire the label of planet. Nor do I agree that the "role" of Pluto has changed greatly since its discovery. The only significant change is that we now have discovered objects that we had already suspected were there.

      Having said that, the heuristic of gravitational domination, is really the killer argument for your point of view. I'll say more of this at the end.

      I see two things that would have made the debate irrelevant for me. First, if the definition had been completed with the "neighborhood" element nailed down. And second, if IAU had made a decision that involved the majority of its members and had deliberated over a period of time.

      Again, the IAU definition is fundamentally subjective. Yet it still does a better job of accounting for current knowledge of the solar system.

      Definitions do not account for knowledge. The purpose of a good definition is to enhance communication by putting a label on important or frequently discussed patterns. It's at this point that I must agree that the notion of gravitational dominance is an important pattern in not just Solar System dynamics, but also dynamics of other relatively mature star systems. That needs to have a label. Calling such objects "planets" is a reasonable notion. Else we'd have to invent a possibly clumsy term to cover that (say "gravitationally dominant object").

      My point of view on such things is as a mathematician. Semantics is always a choice. And as long as the choice of definition doesn't result in loss of ability to communicate (say because you have no way to describe the notion of a "planet"), excessive overhead (your label for planet takes ten minutes to pronounce), or is overly difficult to translate into another semantic structure (my definition of planet has subtle overtones that makes it difficult to render accurately in your language), then it's a legitimate choice equivalent to any other of similar efficiency and usefulness.

    7. Re:Much ado over Pluto (OT) by Chris+Burke · · Score: 1

      To be blunt here, I see little scientific value in changing a 70 year old official definition of planet. We don't become more stupid or less just because we change our minds about what characteristics acquire the label of planet. Nor do I agree that the "role" of Pluto has changed greatly since its discovery. The only significant change is that we now have discovered objects that we had already suspected were there.

      The thing is, once you set aside that no formal definition of "planet" existed, we really aren't changing the definition of a planet, or the characteristics which acquire that label. They're essentially the same characteristics by which we say all of the 8 planets are planets. The same characteristics by which we first said Ceres was a planet, but then decided it wasn't when we learned more about it's neighborhood. Planets were expected to be the dominant objects in their orbits, and when it turned out Ceres wasn't, we stopped calling it a planet.

      And Pluto's role has absolutely changed as our knowledge has increased. It was discovered in 1930 in the search for a 9th planet suspected to be the cause of perturbations in Uranus' orbit not explained by Neptune, and when found was presumed to be that planet. Over the next decades there were hypothesis of there being or having been a population objects past Neptune's orbit, though few such hypothesis looked anything like the actual Kuiper Belt. Also many (including Kuiper) hypothesized that Pluto, thought to be as massive as Earth, would have long since tossed all of those smaller objects out of its orbit (i.e. like a planet does) and so the belt had disappeared long ago in the solar system's development.

      It wasn't until over 40 years later in the late 70s that we could actually measure Pluto's mass and realize just how small it was, and that it couldn't be the planet that caused the disturbance of Uranus (and which later measurement showed wasn't actually disturbed). It wasn't until the early 90s, less than 20 years ago, that we actually began finding other objects in the Kuiper Belt and began discovering its actual characteristics and the consequences to Pluto's role in its orbit as just the biggest asteroid in an asteroid belt, like Ceres, not the dominant object of its orbit, like every other planet.

      So what changed is not the characteristics that get called a planet. What changed is:
      1) the characteristics of Pluto as we understand them -- from earth-size and dominating its orbit, to a large asteroid in the midst of a belt.
      2) the formalization of the classical definition of planet, such that we can't continue calling something that is clearly completely unlike every other planet a planet just because it's comfortable.

      Like I said before, the only reason we ever called Pluto a planet is because we thought it had the characteristics that we attribute to the other planets. If you had proposed the IAU definition of planet back in the 1930s, everyone would have thought that Pluto met them. It does not. Regardless of the IAU definition, had we known in the 1930s about the Kuiper Belt, we would not have called Pluto a planet. Because it isn't one.

      "Planet" used to mean roughly what it does today. Only when we knew that Pluto didn't fit at all, but still called it a planet, did the word get reduced to meaning "things which were historically called planets for whatever reason". I think there is great scientific value in making it mean something again. And there's an orders-of-magnitude distinction between that meaning and all the objects like Pluto that don't fit, so I think it is clearly indicating something meaningful.

      I see two things that would have made the debate irrelevant for me. First, if the definition had been completed with the "neighborhood" element nailed down.

      Having "neighborhood" be vaguely defined is actually a feature. Any precise definition would necessarily be an arbitrary one, and prevent reasoned analysis of individua

      --

      The enemies of Democracy are
    8. Re:Much ado over Pluto (OT) by khallow · · Score: 1

      If you had proposed the IAU definition of planet back in the 1930s, everyone would have thought that Pluto met them.

      No, because they knew (or at least would know in a few years, I don't know when the orbit of Pluto was nailed down well enough) that Pluto crossed the orbit of Neptune and that it was a lot less massive than Neptune. The same heuristic argument that was made in 2006 could have been made in or shortly after 1930 and it would have the same result.

      Having "neighborhood" be vaguely defined is actually a feature. Any precise definition would necessarily be an arbitrary one, and prevent reasoned analysis of individual cases that might be near the boundary. What if we found a system with a planet in a completely cleared orbit with just moons and trojans, but flanked by asteroid belts that just happened to come too close for the precise definition?

      Nonsense. The definition only applies to the Solar System. The IAU said so. If you recall, this was one of my original complaints about the definition!

      And I don't see the advantages of creating an interminable argument over whether something is or isn't a planet (say, Pluto for example) simply because the original definition blew off defining a key term. For example, the heuristic I mentioned back a couple of posts happens to be a way to define a neighborhood of Pluto in a way that would be consistent with the IAU definition and Pluto as planet. The neighborhood just so happens to be defined to not contain Neptune. To summarize, if it weren't for the fact that the IAU explicitly says subsequent to the definition of "planet" that Pluto isn't a planet, then we wouldn't know whether the IAU defined Pluto as a planet! That's how ill-defined terms cripple a definition.

    9. Re:Much ado over Pluto (OT) by Chris+Burke · · Score: 1

      No, because they knew (or at least would know in a few years, I don't know when the orbit of Pluto was nailed down well enough) that Pluto crossed the orbit of Neptune and that it was a lot less massive than Neptune. The same heuristic argument that was made in 2006 could have been made in or shortly after 1930 and it would have the same result.

      Pluto's orbit doesn't cross Neptune's orbit. It gets closer to the Sun than Neptune at one point in its orbit, but the orbits aren't actually close to each other because at that point Pluto is also well above the ecliptic. The IAU definition does not say orbits are not allowed to cross in any case, and it certainly doesn't say the planet must have a constant closer/farther relationship with other planets. Neptune has nothing to do with Pluto's definition as a dwarf planet.

      Pluto is excluded because Pluto's own orbit has many asteroids in it that total up to many times Pluto's mass. It has not cleared its neighborhood, ergo it is not a planet.

      They thought Pluto had roughly the mass of earth. They thought it was the only significant object in its orbit. They would have called it a planet by the IAU definition. They would have been -- were -- wrong.

      Very salient information about Pluto has been acquired since it was first called a planet. Information that had it been known in 1930 would have prevented Pluto from ever being called a planet. It's the same story as with Ceres.

      But no complaints about Ceres' status. How odd.

      Nonsense. The definition only applies to the Solar System. The IAU said so. If you recall, this was one of my original complaints about the definition!

      Yes, they didn't want to presume to define "planet" for ever system in the universe when our knowledge of other solar systems is so primitive. Yet, at the same time, one can craft the definition such that is amenable to extension to other systems. As we study other systems, we may learn that our definition isn't applicable at all and must be wildly revised. Or, because of their foresight, they can simply state that the definition does apply to all solar systems and there we go.

      You're complaining about one of the wisest things they did.

      And I don't see the advantages of creating an interminable argument over whether something is or isn't a planet (say, Pluto for example) simply because the original definition blew off defining a key term.

      Because that's how you deal with the reality of the universe, that it frequently defies the human desire for strict classification. You don't draw an arbitrary line with infinite precision where no such line exists. That would be arbitrary and unscientific. Yes, it's true -- real science often involves accepting ambiguity.

      However, there is no argument over whether or not Pluto is a planet amongst those who accept the IAU definition. The definition is completely unambiguous when it comes to every known object in our solar system. The only argument comes from those who want to draw a precise line so that Pluto is a planet.

      For example, the heuristic I mentioned back a couple of posts happens to be a way to define a neighborhood of Pluto in a way that would be consistent with the IAU definition and Pluto as planet. The neighborhood just so happens to be defined to not contain Neptune.

      As I said before, your heuristic requires drawing a very arbitrary line right in the middle of a huge gray area where there are many objects that are within a few percent of making or not making the cut. Your definition would also have included Haumea, Makemake, and Eris as planets as well as Ceres. You could jiggle your definition a tiny bit to exclude Haumea and Makemake maybe, but you can't include Pluto without including Eris and Ceres. But why exactly there? Why don't Haumea and Makemake or other slightly smaller objects not make the cut? There's absolutely no reason for such a precise line to be drawn through a freaking asteroid belt

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      The enemies of Democracy are
    10. Re:Much ado over Pluto (OT) by khallow · · Score: 1

      Pluto's orbit doesn't cross Neptune's orbit.

      I wasn't speaking of physically crossing. I meant in that it gets closer to the Sun than Neptune does.

      Whereas the IAU definition has a four order of magnitude difference between the least of the things called planets and the greatest of things called dwarf planets. There is a clear and obvious gap between objects that are capable of clearing out their orbits, and those that aren't.

      The gap is two orders of magnitude smaller than you claim. Earth is two orders of magnitude greater than the Moon, not four.

  45. What about dark matter stars? by Omnifarious · · Score: 1

    It seems to me that this Eddington limit idea depends on all the matter that's gravitationally bound to the star's atmosphere participate in the fusion reactions at the core of the star. What about matter that doesn't participate in those kinds of reactions? Wouldn't a preponderance of dark matter allow a star to form that's much bigger than the Eddington limit since the dark matter wouldn't be participating in energy releasing fusion reactions?

    And why isn't it possible that this star is one such?

    1. Re:What about dark matter stars? by physburn · · Score: 1
      The weight of the dark matter would increase the pressure on the star's core, increasing the burn speed of the baryons in the star, if dark matter can self annihilate though it will create enegery of its own is helping to support the star. So it very much depends on the properties of dark matter as to weather it would help a star bet the Eddington limit.

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      Dark Matter Feed @ Feed Distiller

  46. Is it Lindsay Lohan? by sethmeisterg · · Score: 1

    It's gotta be, right?

  47. Binary star? by jmv · · Score: 1

    I'm curious, does anyone know how/if they can tell it's not a binary star system, i.e. two stars that are each below the Eddington limit?

  48. What kind of name is that? by Eclipse-now · · Score: 1

    R136a1!!?? Are you kidding me? Why not Biff? Biff is a nice name.

  49. That's no star... by tedgyz · · Score: 1

    ...it's a space station.

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    "No matter where you go, there you are." -- Buckaroo Banzai