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Powerful Supernova May Be Related To Death Spasms of First Stars

necro81 writes "The New York Times is reporting on a discovery from a team of UC Berkley researchers, who may have discovered the brightest stellar explosion ever observed. Observations of the cataclysmic explosion of a 100- to 200-solar-mass star began last September, based on data from the Chandra X-ray Observatory. The researchers believe that the explosion is similar to the death spasms of the first stars in the universe. The super-massive star's collapse is believed to have been so energetic as to create unstable electron-positron pairs that tore the star apart before it could collapse into a black hole — seeding the universe with heavier elements."

43 of 136 comments (clear)

  1. Kinda OT, but I thought I'd say... by Red+Flayer · · Score: 5, Funny

    Great summary. Lots of informative links, accurate and intriguing summary of the article(s). No gratuitous inflammatory question.

    Someone pinch me, I think I'm dreaming.

    --
    "Trolls they were, but filled with the evil will of their master: a fell race..." -- J.R.R. Tolkien on Olog-hai
    1. Re:Kinda OT, but I thought I'd say... by Anonymous Coward · · Score: 3, Funny

      Look, though! there's an off-topic post!!!

    2. Re:Kinda OT, but I thought I'd say... by BlackSnake112 · · Score: 2, Informative

      "University of Texas graduate student Robert Quimby first observed the supernova on Sept. 18, 2006 in the galaxy NGC 1260, located in the constellation Perseus. Filippenko's team immediately began observing it with its dedicated supernova search and monitor telescope at Lick, the Katzman Automatic Imaging Telescope." They did, if you RTFA

  2. Oddity by tomstdenis · · Score: 3, Interesting

    They talk at the end about a star 7500 LY away that might "go supernova soon." It should probably be pointed out that it could have already gone supernova 6000 years ago and we'd not know about it.

    I guess they should say "might see if it went supernova soon."

    Tom

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    1. Re:Oddity by Nos. · · Score: 4, Insightful

      I think this is getting a bit pedantic. Sure, the light takes 7500 years to get here, thus it could have gone supernova quite some time ago, and the astronomers know this. It doesn't mean we have to speak about everything having occurred in the past... its all relative.

    2. Re:Oddity by JesseL · · Score: 4, Insightful

      Your post is based on the flawed premise that there exists some kind of objective time.

      --
      "Prefiero morir de pie que vivir siempre arrodillado!"
    3. Re:Oddity by ls+-la · · Score: 3, Informative

      I guess they should say "might see if it went supernova soon."
      We know information cannot travel faster than the speed of light (or if you prefer, cannot reach outside the light-cone of the event). So if an event "happens" 7500 light years away, did it really happen before the light reaches us? In some sense, an event has not happened until we are inside its light-cone.
      Perhaps it "happens" when its light-cone intersects ours? The question with this interpretation is, where does our light-cone start?

      Time is relative, and over distances of at least the order of a light second (186,000+ miles), it is difficult to think about correctly.

    4. Re:Oddity by Orange+Crush · · Score: 5, Informative

      There is no such thing as synchronicity in this universe. Cause travels at the speed of light (or slower), gravity and relative velocity alter time and quantum states are ambiguous until observed. That star has a high probability of already having gone supernova, but this is meaningless in our frame of reference until the event is observable.

    5. Re:Oddity by profplump · · Score: 2, Insightful

      That's only true if you assume that two distant points share the same timescale -- a relativist might argue that "now, far away" is the same moment in time as "here, long ago", at least baring the discovery of macro-scale faster-than-light causation. That is to say, while an observer near the supernova might have seen the explosion long ago, his "long ago" and your "now" may be the same moment, not just two different perspectives of the same event that happened long ago with respect to all observers.

      Beside that, even if there is a universal timescale unrelated to the speed of light, from our perspective it is happening "now", and since we don't often communicate with anyone more than a few thousand miles away it's silly to express things in any other timescale.

    6. Re:Oddity by linzeal · · Score: 2, Informative

      Also known as, Minkowski Space.

  3. Eta Carinae by tiluki · · Score: 5, Interesting
    What is more impressive about this story is the footnote of similar activity recently exhibited by Eta Carinae - a much closer star to us (well, 7500 light years). To quote the BBC article http://news.bbc.co.uk/1/hi/sci/tech/6633609.stm:

    Dave Pooley, at the University of California at Berkeley, said if Eta Carinae were to explode "it would be so bright that you would see it during the day, and you could even read a book by its light at night". Eta Carinae's death could be "the most spectacular star show in history." Is it just me, or does that sound a little bit too close...
    1. Re:Eta Carinae by Jugalator · · Score: 4, Informative
      It's not too bad unless we'd be unlucky and have a gamma radiation burst from it heading towards us.
      From here:

      The potential danger comes from the fact that explosions of massive stars generally emit jets of intense gamma radiation, among the most powerful and harmful forces in the universe. If Eta Carinae did explode and a jet was pointed in the general direction of the solar system, Livio said, Earth could be endangered. But because the gamma-ray jets tend to be relatively narrow, like the beam of a lighthouse, the odds are that the jet would miss Earth.

      So it's not too bad, it would probably just miss us.

      :-/

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    2. Re:Eta Carinae by vrmlguy · · Score: 4, Informative

      First, Eta Carinae is not visible to anyone north of 27 N, so in the US only people in or south of Miami will see it. In Africa, you basically have to be in a country that doesn't touch the Mediterranean Sea; while in Asia every country touching the Indian Ocean will see it, but not China or Japan. Among English-speaking countries, only Austrailia will have a great view, but the ozone layer will protect them (and the rest of the Southern Hemisphere) from direct radiation. "Scientists at NASA and Kansas University have determined that the supernova would need to be within 26 light years from Earth to significantly damage the ozone layer and allow cancer-causing ultraviolet radiation to saturate the Earth's surface. An encounter with a supernova that close only happens at a rate of about once in 670 million years(...) The new calculations are based largely on advances in atmospheric modeling, analysis of gamma rays produced by a supernova in 1987 called SN1987a, and a better understanding of galactic supernova locations and rates. A supernova is an explosion of a star at least twice as massive as our Sun." Since Eta Carinae is 300 times that distance, its blast wound need to be 90,000 times as energetic to be dangerous. A hypernova is about 100 times more powerful than a supernova, so there's plenty of margin of safety there.

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    3. Re:Eta Carinae by secPM_MS · · Score: 2, Interesting
      Eta Carinae is a Luminous Blue Variable, a very massive star (~ 80 to 120 Msolar) that is quite unstable. Last century it ejected ~ 10 solar masses of material. It is also a binary star, with a companion estimated to be ~ 80 solar masses or so. The orbit is significantly inclined from our point of view, so the spin axis is not pointed at all towards us, which is very fortunate indeed. I seem to remember one article a year or so ago that estimated that Eta Carinae was spinning at ~ 90 % of its breakup speed. This is very fast indeed, and if true, would mean that it would be a potential gamma ray burst source when it goes supernovae. Note that it would have to shed its atmosphere first and become a Wolf Rayet star before the GRB could punch through the stellar atmosphere.

      Pair creation supernovae were predicted decades ago. The conditions for their formation are a bit strict and they do not appear to be very common at this point. Black hole creation is probably must more common. If we have seen one now, it is a good reinforcement of old theoretical work.

    4. Re:Eta Carinae by georgewilliamherbert · · Score: 2, Informative

      Pair creation supernovae were predicted decades ago. The conditions for their formation are a bit strict and they do not appear to be very common at this point. Black hole creation is probably must more common.

      If you neglect angular momentum (i.e., for only moderately rotating stars), the current predictions are that pair creation supernovae are the normal mechanism for stars with a low metalicity and immediately pre-supernova mass from about 140 to about 260 solar masses. If you look at the webpage in the summary http://astro.berkeley.edu/~soffner/imgsf8.html it shows the metalicity / mass behavior estimates. Also see http://www.ucolick.org/~alex/firststars/, particularly the diagram at the bottom. It shows the no angular momentum low metalicity stellar behavior: 8-25 Solar Masses, you get a neutron star. 25-50ish, you get a neutron star that then reabsorbs enough of the source star's mass via fallback to become a black hole. 50-100, you get a direct collapse to a black hole. From 100 to 130 solar masses, the pair production mechanism kicks in and pulses a few times, ejecting mass, and then it falls below 100 SM from the ejections and should collapse to a black hole on the next pulse. From 130 or 140 up to about 250 or 260 (depends on whose paper/numbers), pair production doesn't pulse, it goes bang, and the explosion generates enough energy to gravitationally unbind the whole star (blow it completely apart, no or little remnant). Above the 250/260 point, they predict that pair production happens but it just direct collapses essentially the whole star to a black hole, not fusions off to explosion as in the slightly smaller ones.
  4. Re:we should we believe the astrophysicists now? by Vendetta · · Score: 5, Insightful

    So you're saying it's a bad thing to revise theories based on new information or observations? There is a reason they are called "theories".

  5. Boom? by Jugalator · · Score: 3, Funny

    Big badaboom!

    --
    Beware: In C++, your friends can see your privates!
  6. Re:Time-lapse video? by ls+-la · · Score: 5, Informative

    As far as I can tell from the articles, most of the observation was through means other than the optical spectrum pictures you're looking for (e.g. x-ray and IR pictures, spectroscopy, etc.). In fact, this supernova was so far away (240 million light years) that I'm not sure they could see it through optical telescopes. Most of a supernova's radiation (especially in something this violent) is emitted in the gamma ray range.

  7. Re:we should we believe the astrophysicists now? by PFI_Optix · · Score: 4, Insightful

    It's the revisions that make it science.

    Some scientists--and physicists can be especially guilty of this in my experience--place too much faith in their own knowledge and accept the current findings of science as absulute fact. They forget that science is fluid, always changing as new information enters the equation and each answer spawns new questions. Call it arrogance if you want; I think it's something less than that.

    In any case, what's the alternative? "God did it"? That may very well be true, but it doesn't answer the question of "how did it happen?"...which is what science seeks to explain.

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  8. Here's the NASA page. by u-bend · · Score: 5, Informative
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    u-bend
    1. Re:Here's the NASA page. by john83 · · Score: 2, Informative

      Here's the paper about it.

      From the abstract:
      We report our discovery and early observations of the peculiar Type IIn supernova SN 2006gy... It is not yet clear what powers the enormous luminosity ... but we argue that any known mechanism ... requires a very massive progenitor star... SN 2006gy is the first supernova for which we have good reason to suspect a pair-instability explosion... SN 2006gy also suggests that the most massive stars can create brilliant supernovae instead of dying ignominious deaths through direct collapse to a black hole. If such a fate is common among the most massive stars, then supernovae from Population III stars in the early universe will be more numerous than previously believed.

      Interesting stuff!
      --
      Strange women lying in ponds distributing swords is no basis for a system of government.
  9. Re:we should we believe the astrophysicists now? by Red+Flayer · · Score: 4, Informative

    Just goes to show you the arrogance of physicists- they claim answers and grandiose Standard Theories, but are frequently revising them because they mis things like accelerating expansion and 150SM supernova.
    Right. So we should not put blind faith in any theory, because it's open to being falsified. That's basic scientific method stuff.

    Isn't this what academic research is (in theory) all about? The search for better understanding, enabling us to revise our theories of how the universe (or some small subset of it) works?

    Find the simplest theory that fits all the observations. New data may mean you need a new theory, or that you need to revise your current theory. I don't understand the problem you have, unless it's just with the arrogance of some theorists who claim to have found the answer to Life, the Universe, and Everything. I say, let them be arrogant -- when they are disproved, they'll fall harder for it.
    --
    "Trolls they were, but filled with the evil will of their master: a fell race..." -- J.R.R. Tolkien on Olog-hai
  10. Re:we should we believe the astrophysicists now? by Ambitwistor · · Score: 5, Insightful

    Why shouldn't we believe "the astrophysicists"? Did they lie to you? Gore your ox? Steal your candy? Pee in your breakfast cereal?

    After 70 years of computer simulations and observations they failed to predict this new kind of supernova.

    Yeah, so? There are infinitely many things that are true which scientists have yet to predict. Why are you under the impression that scientists are supposed to know everything? Even if they did know all the physics involved, you can still only make finitely many predictions in finite time.

    Its interesting to read speculations about degenerate lepton gases, but arent they just hand-waving again?

    "Again"? When were they "hand-waving" before? About what?

    Just goes to show you the arrogance of physicists- they claim answers and grandiose Standard Theories, but are frequently revising them because they mis things like accelerating expansion and 150SM supernova.

    That's a feature, not a bug. It's how science works! Physicists claim answers because they have answers. That doesn't mean they have ALL the answers, or they're always right. This is no different in astrophysics than in any other field of physics, or any other science, or in any other field of study, period. People know some things, they can predict some things, and sometimes they miss something or get something wrong. That doesn't mean that nobody knows anything or that experts have nothing useful to say.

    (By the way, accelerating expansion was in Einstein's theory from the start, but he took it out because there wasn't any evidence for it at the time.)

    I seriously don't understand your point of view, unless (as is likely) it's just flamebait. Every time something new is discovered, do you seriously run around disparaging whole fields of science just because the new thing wasn't predicted ahead of time? Or do you just have some bug up your nose about astrophysicists? It's not like they were even wrong about normal supernovae, they just didn't predict this new kind.

  11. Re:we should we believe the astrophysicists now? by DrJay · · Score: 2, Insightful

    Actually, my understanding was that astronomers are suggesting that this may be the first observed case of a type of supernova called pair-instability. The actual prediction of pair-instability supernovae was made decades ago - it's more that observations are catching up with predictions.

    So, you seem to have gotten this exactly backwards.

    As a bit of reading should also make clear, the reason that observations of this type of supernova are rare is that the conditions that favored the formation of stars capable of exploding this way have become rare as the universe has aged. They are expected to be far more common in the early universe, and it's hoped that the next generation of space telescope will be capable of viewing them (as it will see further, and thus earlier, into the universe).

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  12. E.L.E by TheSciBoy · · Score: 4, Interesting
    What I found interesting was that Eta Carinae apparently behaves the same way as the other star, which begs the question: could we survive the supernova? The explosions of stars certainly are powerful enough to destroy such delicate lives as ours if they are close enough. Question is, is Eta Carinae close enough?

    Now that's an Extinction Level Event.

    "Ooh! Aaah!" dead

    --
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    1. Re:E.L.E by OldSoldier · · Score: 2, Interesting

      Yes and no. Astronomers have been wondering about Eta Carinae for awhile. It appears that it can produce "gamma ray bursts" that are powerful enough to wipe out life even here, 7500 light years away, but current thinking is that GRBs are focused events, gamma rays streaming along the magnetic axis of the exploding star and fortunately Eta Carinae's axes are not pointed in our direction.

      I'm not endorsing this link http://people.roma2.infn.it/~aldo/dar01.pdf but it does corroborate what I've heard on TV science shows.

    2. Re:E.L.E by Frozen+Void · · Score: 2, Informative

      Its not so clear.
      1.It depends on how much matter is dispersed between us and the supernova(plasma,dust,stars,etc)
      2.The estimate of mass and star composition are correct.
      3.The mechanism of supernova production is well understood.(not really:the electron-positron pair supernova is new)
      4.GRB angle.

      http://en.wikipedia.org/wiki/SN_2006gy
      Similarity to Eta Carinae

      Eta Carinae ( Carinae or Car) is a highly luminous hypergiant star located approximately 7,500 light years from Earth in the Milky Way galaxy. It is estimated to be similar in size to the star which became SN2006gy. Dave Pooley, one of the discoverers of SN2006gy, says that if Eta Carinae exploded in a similar fashion, it would be bright enough that one could read by its light. However, Pooley estimates the likelihood of the star exploding in the near future as small, with a minimal risk to life on Earth.[4]

  13. Re:Actually, it's T E X A S by MontyApollo · · Score: 3, Informative

    From the article:

    The discovery was made by Robert Quimby, a University of Texas graduate student, who was using a small robotic telescope at McDonald Observatory near Fort Davis, Tex., to troll for supernovas
  14. That's no Supernova by MHz-Man · · Score: 3, Funny

    It was a precursor bomb! Looks like someone's copying the Shofixti's tactics.

  15. Re:Time-lapse video? by $RANDOMLUSER · · Score: 5, Informative

    Indeed. The best images are from the Chandra X-ray observatory. They have some animations here.

    --
    No folly is more costly than the folly of intolerant idealism. - Winston Churchill
  16. Re:Time-lapse video? by p_trekkie · · Score: 3, Informative

    Most of a supernova's radiation (especially in something this violent) is emitted in the gamma ray range.


    Actually, most of the radiation comes out as neutrinos. Only 1% comes out in forms we can detect at all...
  17. Re:we should we believe the astrophysicists now? by Hoi+Polloi · · Score: 4, Insightful

    How is trying to explain something based on the best current evidence arrogance? Are you saying people shouldn't ever believe anything or they should just ignore new info? Sorry but science is a continual learning process and unlike religion is constantly adjusting to new information and better explanations.

    --
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  18. Re:we should we believe the astrophysicists now? by stewardwildcat · · Score: 5, Insightful

    As an astrophysicist I feel I should comment. First of all, 70 years of computer simulations later.... we are just beginning to be able to model a supernova with high enough resolution that we can "kind of" fit the observations without contrived scaling factors. This is also only being done in two dimensions and for the first few microseconds of a supernova. Models that hardly include all the physics involved are too much for the modern computational machine. Everytime we run a new model that includes more physics, they fit the data better and better. It is this way we discover what physics matters in the actual explosion. Since we cannot COMPLETELY model anything in real life on a computer all simulations are hand-wavy. Second, developing theories is very important. You use all of the available data and create a theory that can be tested and describes the current state of what you are studying. The real test of a theory is if it stands up to scrutiny. IF the "standard model" was so vague that no meaningful tests could be performed to prove the theory incorrect then it is a bad theory. Scientists prove things wrong, that is out job. We find situations where the current models do not describe the observations. That is scientific progress. We adjust our theories and learn about new physics. If gravity wasnt tested we would still be using Newtonian Gravity rather than General Relativity, which is still being worked on today (Gravity Probe B). Lastly, Astronomers have never observed a 150-200 Msolar supernova before. This is the first time we are able to look at what might have happened when the first stars formed. If we had seen a whole lot of these and had a perfect unified model then we wouldnt have to do science or discover things anymore. This is an exciting time as we have the most advanced instruments built by humans peering into the early universe discivering where we came from. I am always excited about new results, whether they be proven wrong or not, because we are always one step closer to understanding the world in which we live.

  19. Re:heavy elements by stewardwildcat · · Score: 2, Informative

    http://en.wikipedia.org/wiki/Nucleosynthesis its called nucleosynthesis. The reaction chains that fuse in the sun are called nuclear reaction networks. There is a lot of information available on this but Wikipedia gives a nice overview./

  20. Re:heavy elements by navyjeff · · Score: 2, Informative
    I would start with a chart of nuclides and a chart of the current model of subatomic particles to investigate the chain of fusions and fission.

    I hope you like physics, though. The chart of nuclides can be a bit confusing at first.

  21. Re:Time-lapse video? by Tablizer · · Score: 2, Funny

    Is there a time-lapse video of this somewhere? The article I read only had an artist's rendering. Or when they say "observed" are they just talking about measurements?

    Be veeery careful when asking for images on slashdot of anything that explodes, bursts, or has holes in it.

  22. Eta Carinae by phrostie · · Score: 2

    in the space.com article on this they mention that our own MilkyWay has a star about to go SuperMasive Nova at any time called Eta Carinae. Eta Carinae is about 7000 light years away so they say we are safe, but the Nova from last September eventually became brighter than it's own galaxy. So what i )BÇm wondering is even if we are safe from debris from this soon-to-be nova, what about an EMP from it?

  23. Re:Time-lapse video? by p_trekkie · · Score: 2, Informative

    Type I versus Type II

    A fundamental difference between Type I and Type II supernovae is the source of energy for the radiation emitted near the peak of the light curve. The progenitors of Type II supernovae are stars with extended envelopes that can attain a degree of transparency with a relatively small amount of expansion. Most of the energy powering the emission at peak light is derived from the shock wave that heats and ejects the envelope.[57]

    The progenitors of Type I supernovae, on the other hand, are compact objects, much smaller (but more massive) than the Sun, that must expand (and therefore cool) enormously before becoming transparent. Heat from the explosion is dissipated in the expansion and is not available for light production. The radiation emitted by Type I supernovae is thus entirely attributable to the decay of radionuclides produced in the explosion; principally nickel-56 (with a half-life of 6.1 days) and its daughter cobalt-56 (with a half-life of 77 days). Gamma rays emitted during this nuclear decay are absorbed by the ejected material, heating it to incandescence.

    As the material ejected by a Type II supernova expands and cools, radioactive decay eventually takes over as the main energy source for light emission in this case also. A bright Type Ia supernova may expel 0.5-1.0 solar masses of nickel-56,[58] while a Type Ib, Ic or Type II supernova probably ejects closer to 0.1 solar mass of nickel-56.
    Thanks in advance for advancing my understanding. Apologies if there is anything akin to an apples/oranges misunderstanding at the base of my query...

    The answer lies in whether you count neutrinos as radiation or not. What I should have stated in my original post was that the vast majority of the energy released in supernoave comes out in the form of neutrinos, which we have a really really hard time detecting...

    Wikipedia is correct as to the source of photons that we detect. I counted neutrinos as a form of radiation in my earlier statement (since in my mind, that's what they effectively are), but neutrinos are not photons. Hence, there is no discrepancy. Basically, when we take the energy difference between the potential energy of a star before and after a Type II SNa (like this one) and check that against the energy we see from photons, we are only seeing 1% of the energy that should be coming out in all forms of light. The rest of the energy is believed to escape in the form of neutrinos.
  24. Re:Time-lapse video? by imsabbel · · Score: 3, Informative

    Also:
    "
    The core implodes at velocities reaching 70,000 km/s (0.23c),[40] resulting in a rapid increase in temperature and density. Through photodissociation, gamma rays decompose the iron into helium nuclei and free neutrons. The conditions also cause electrons and protons to merge through inverse beta decay, producing neutrons and electron neutrinos. About 1046 joules of gravitational energy are converted into a ten-second burst of neutrinos.[41] These carry away energy from the core and accelerate the collapse, while some neutrinos are absorbed by the star's outer layers and begin the supernova explosion.[42]

    The inner core eventually reaches a density comparable to that of an atomic nucleus, where the collapse is halted. The infalling matter then rebounds, producing a shock wave that propagates outward. This expanding shock can stall in the outer core as energy is lost through the dissociation of heavy elements. However, through a process that is not clearly understood, the shock reabsorbs 1044 Joules[a] (1 foe) of energy, producing an explosion.[43]"

    You might have stumbled upon this part of the article while getting to the part you quoted. 10^44 joule ->explosion, 10^46 joule -> neutrino burst.
    ->only 1% is visible.

    --
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  25. 200 solar mass possible? by Dasher42 · · Score: 2

    Do we know that 200 solar mass stars can exist within the Eddington limit? To summarize, higher mass will increase the energy output of the star's fusion reactions, and there's a point where this can more than counter the force of gravity. How would a star exceed this? Are collisions or mass accretion from another object likely?

  26. Old News... by rthille · · Score: 3, Funny


    Slashdot, 240 million years behind the times.

    (I should probably post this anonymously :-)

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  27. Re:Time-lapse video? by MollyB · · Score: 2, Interesting

    Many thanks to you & the OP. You (both) are very tactful, as I skimmed right past the relevant Wiki section you noted so graciously. I'll try to do more exhaustive research before jumping in with questions next time.

  28. RIP Planet Krypton by Anonymous Coward · · Score: 2, Funny

    The New York Times is reporting on a discovery from a team of UC Berkley researchers, who may have discovered the brightest stellar explosion ever observed. causing the tragic end of the vibrant Kryptonian civilization.

    seeding the universe with heavier elements. Hmm...didn't they recently discover Kryptonite. Co-incidence?