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Bizarre Star Could Host a Neutron Star In Its Core

ananyo writes "Astronomers say that they have discovered the first example of a long-sought cosmic oddity: a bloated, dying star with a surprise in its core — an ultradense neutron star. Such entities, known as Thorne-Zytkow objects, are theoretically possible but would alter scientists' understanding of how stars can be powered. Since Thorne-Zytkow objects were first proposed in 1975, researchers have occasionally offered up candidates, but none have been confirmed."

40 of 73 comments (clear)

  1. Boo :-( by Baby+Duck · · Score: 4, Funny

    A star IN a star? Now I can't make fun of Sunshine anymore.

    --

    "Love heals scars love left." -- Henry Rollins

    1. Re:Boo :-( by Anonymous Coward · · Score: 1

      "scientists' understanding of how stars can be powered". I thought it was cocaine.

    2. Re:Boo :-( by send2erik · · Score: 1

      Kind of Brangelina

    3. Re:Boo :-( by JavaLord · · Score: 1

      Kind of Brangelina

      Yes, the only question, like with Brangelina is which star is inside which.

  2. Yo dawg, I herd yo like stars by Anonymous Coward · · Score: 5, Funny

    So I put a star in yo star so you can collapse into a black hole if your combined solar mass exceeds the Oppenheimer-Volkoff limit.

    1. Re:Yo dawg, I herd yo like stars by fisted · · Score: 1

      combined solar mass

      Ehhhhhhhm.

  3. Yo dawg by trmj · · Score: 4, Funny

    I heard... you know what? It's too easy.

    --
    Work sucked, until it became unemployment, when it became slightly more tolerable. -Tet
  4. That's inexplicable, but not inexplicable enough! by ackthpt · · Score: 4, Funny

    Such entities, known as Thorne-Zytkow objects, are theoretically possible but would alter scientists' understanding of how stars can be powered.

    How apt this phrase is now: There is a theory which states that if ever anyone discovers exactly what the Universe is for and why it is here, it will instantly disappear and be replaced by something even more bizarre and inexplicable.

    --

    A feeling of having made the same mistake before: Deja Foobar
  5. scan of the original article by Trepidity · · Score: 5, Informative

    "Stars with degenerate neutron cores", Astrophysical Journal, 1977.

    Courtesy of the SAO/NASA Astrophysics Data System, an open-access digital library that other fields could do well to emulate...

    1. Re:scan of the original article by Anonymous Coward · · Score: 1

      Unfortunately page 3 of the original F.A. lays out exactly why this probably never happens: The formation of neutron stars blows shit up - there's no other way analogous to how a white dwarf forms from the settling of nuclear ash. So now you have to get a new envelope onto the neutron star.

      The only scenario they propose that I might buy is if the neutron star outright collides with a companion and wears the companion's corpse like a skin suit. There's no other way you're gonna (i) get matter in place fast enough to heat it up and get pressure support against that massive gravity field and (ii) keep that heat from being radiated away immediately.

      I have a hard time believing that any accretion disk scenario would work. Ignoring the matter of where the angular momentum goes, assume that supercritical accretion gets to the point that mass piles on until the radiation-driven outflow is stifled long enough to get pressure support against the neutron star's gravity. Okay, you've now balanced cold and probably dense matter (remember, you just trapped a very hot but very tenuous outflow) on top of hot light matter... The Rayleigh-Taylor overturning will probably be spectacular.

      But, eh, it'd be freakin awesome if they found one.

    2. Re:scan of the original article by Anonymous Coward · · Score: 1

      From what I read about a decade ago a common envelope event could be a plausible scenario leading (sometimes) to the merger of a (super)giant and a neutron star and a formation of a Thorne-Zytkow object.

      In that case, the angular momentum goes into the common envelope as heat.

    3. Re:scan of the original article by Sockatume · · Score: 1

      It's not quite an "open-access digital library": they scan and host old material from some journals with their permission, but a good deal of the material they index is still paywalled.

      --
      No kidding!!! What do you say at this point?
    4. Re:scan of the original article by Sockatume · · Score: 1

      Analogy: Google Books for astrophys papers.

      --
      No kidding!!! What do you say at this point?
  6. Where is this claim? by hubie · · Score: 3, Interesting

    I read TFA and I don't see where this comes from: but would alter scientists' understanding of how stars can be powered

    It sounds like Thorne and Zytkow proposed the scenario and predicted what one would observe, followed up by people like the guy quoted in the brief article (Podsiadlowski), and these astronomers are putting forth a candidate based upon their observations being similar to what the theory suggests. I'm missing the part that alters the understanding. Podsiadlowski, by the way, has been thinking about these objects for a very long time.

    1. Re:Where is this claim? by czert · · Score: 1

      I thought this was a peculiar statement. Either the theory predicts such objects or it doesn't. If it does, then there's no need to change them once their prediction is found to be right...

  7. Some more explaination by Michael+Woodhams · · Score: 5, Informative

    While I've not heard of a Thorne-Zytkow object before, I can apply my general astronomical knowledge to explain a bit further.

    The idea of an internally inert condensed object at the centre of a star is very standard: red giants have a white dwarf at their core, indeed this is how white dwarfs are formed. The weirdness is in having a neutron star instead of a white dwarf core.

    The condensed object is supported by degeneracy pressure (electron degeneracy pressure for a white dwarf, neutron degeneracy pressure for a neutron star.) (Degeneracy pressure is a quantum mechanical effect. It is only appreciable at very high densities, and is not dependent on temperature.) The surface of the condensed object will be very hot, because nuclear burning is going on nearby and it is insulated from the coldness of space by the envelope of the star (i.e. the bits of star which are not the condensed object.) The density of gas just above the surface of the core will also be large, due to the high surface gravity plus the pressure of the weight of the envelope.

    High temperature and high density leads to nuclear burning (combining light nuclei into heavier ones, releasing energy.) The nuclear reactions are generally very strongly dependent on temperature (e.g. one important reaction has a rate approximately proportional to temperature to the 17th power) so the burning happens in a thin layer. The 'burnt' material settles on the core, slowly enlarging it.

    The gravitational attraction of the core pulling the envelope inward is largely balanced by gas pressure and radiation pressure. While stars like our sun are dominated by gas pressure, in this case radiation pressure will dominate. As the radiation escapes outward, mass is able to migrate inwards, to the thin burning layer. An equilibrium is reached between the burning/energy production rate and the mass inflow rate.

    Because they are dominated by radiation pressure, it doesn't take much extra push for something at the surface of a red giant star to escape, so these stars have strong stellar winds and high mass loss rate to winds. So the envelope gets eaten from the bottom by burning and deposition onto the growing white dwarf, and from the top by mass loss. Eventually there is no envelope left and a bare white dwarf is exposed. (The final transition is quite spectacular and is called a planetary nebula.)

    Heat transport in red giants is dominated by convection rather than radiation. (I think this is a general property of being dominated by radiation pressure, but I may be mistaken.) This allows material which has been close to the burning zone to mix through the star. Various secondary nuclear reactions occur there (e.g. s-process nucleosynthesis), so the products of this are mixed to the surface, where they can be observed in the spectrum. (I'm not sure whether partly-burnt material from the main burning shell can get mixed out or not.)

    Evidently (according to the article) in Thorne-Zytkow objects these reactions are different from in a normal red giant and so mix different products to the surface. The star of the article has a spectrum rich in predicted reaction products of a Thorne-Zytkow object.

    While white dwarf naturally grow inside stars, the process that generates neutron stars (supernovae) removes the stellar envelope, so finding a neutron star inside an envelope requires some rare post-supernova event to supply the neutron star with stellar-mass quantities of fresh gas.

    --
    Quattuor res in hoc mundo sanctae sunt: libri, liberi, libertas et liberalitas.
    1. Re: Some more explaination by Anonymous Coward · · Score: 1

      And this is why I like reading Slashdot.

    2. Re:Some more explaination by DirePickle · · Score: 2

      THIS is why I still come to Slashdot. Thank you!

    3. Re:Some more explaination by able1234au · · Score: 2

      requires some rare post-supernova event to supply the neutron star with stellar-mass quantities of fresh gas.

      Such as a binary star where one goes supernova and somehow the binary is not destroyed? Perhaps a binary with a long period? Though imagine that the binary pair would be destroyed or ejected. What is another example that might do this?

    4. Re:Some more explaination by ridgecritter · · Score: 1

      Thanks for this. No mod points to give you, but I see they're not needed.

    5. Re:Some more explaination by Anonymous Coward · · Score: 3, Interesting

      Whether a binary system survives a supernova event is a bit complex topic, actually.

      First, the explosion is not likely to destroy the companion star, even on a fairly close orbit. Stars are really massive objects, and can readily absorb the fraction of supernova energy that happens to hit them. Second, if too much mass is ejected from the system in the explosion, the neutron star and its companion will become gravitationally unbound and drift off separately into space. Assuming a circular orbit and a perfectly symmetrical collapse of the exploding supergiant's core, this will happen if more than half of the total mass is ejected from the system. Now, there are good reasons to believe that the collapse is often slightly asymmetrical, and given the amount of energy released in the explosion, a 'slight' asymmetry might give the remaining neutron star enough 'kick' to propel it out of the host galaxy, let alone of a binary system.

      That all said, there are objects such as Cygnus X-1 that are composed of a regular star and a degenerate object that is believed to be a supernova remnant (in case of Cygnus X-1, a black hole rather than a neutron star, but the principles are the same), so it appears that at least some supernova events do not disrupt binary systems. In that case, when the companion becomes a (super)giant itself later, if it is close enough to the neutron star to fill its Roche lobe (as in Cygnus X-1) and at some point the mass transfer onto the neutron star becomes fast enough, a common envelope will form around the binary system. Common envelope causes much drag and shrinkage of the orbit; in some cases it is believed to cause both objects inside it to merge.

      Of course, much of that is rather speculative, mainly because the common envelope stage is short-lived and thus difficult to observe.

    6. Re:Some more explaination by NoImNotNineVolt · · Score: 2

      I'm no astrophysicist, but the respectable Randall Munroe suggests that "However big you think supernovae are, they're bigger than that."

      According to this What If, you'd get more photons hitting your eye from a supernova seen from as far away as the Sun is from the Earth than the detonation of a hydrogen bomb pressed against your eyeball... by nine orders of magnitude. So while stars are really massive objects, supernovae are apparently unimaginably energetic phenomena.

      --
      Chuuch. Preach. Tabernacle.
  8. "a surprise in its core" by Anonymous Coward · · Score: 4, Funny

    Who else was thinking "nougat"?

    1. Re:"a surprise in its core" by PPH · · Score: 2

      I'd mod you up, but my keyboard is covered with powdered sugar.

      --
      Have gnu, will travel.
    2. Re:"a surprise in its core" by camperdave · · Score: 1

      Who else was thinking "nougat"?

      /me, but I prefer cherry blossoms, or brandy beans.

      --
      When our name is on the back of your car, we're behind you all the way!
  9. Re:Thank god it's not plucking phil by gargleblast · · Score: 1

    Who could this be? Let's see, something about defecation - Oh yes! Hello again, Shithouse Astronomer!

  10. Take THAT, science! by Swampash · · Score: 4, Funny

    Another nail in the coffin of so-called "knowledge". How can you trust a belief system that CHANGES all the time?

    1. Re:Take THAT, science! by AbsGeekNZ · · Score: 1

      Wanted to mod this funny....but unsure if post is serrious? I was thinking of https://en.wikipedia.org/wiki/Poe's_law but this is more of the reverse situation where I am unsure if the original post is serrious....

      On a related note what is the name of the law for this situation? I'm sure slashdot can help me out with this.

    2. Re:Take THAT, science! by Swampash · · Score: 1

      it was a joke :)

  11. Neutron Star Decay by TrollstonButterbeans · · Score: 2

    So let's say you have a neutron star.

    How does it decay? Blackholes have hawking radiation, neutron stars don't need to decay that way of course but they must eventually decay

    If a neutron star emits enough energy to pass below the limit that keeps the pressure as neutrons --- and neutrons have a half-life of 14 minutes outside an atom --- do the neutrons decay into a proton (hydrogen) and an electron and become hydrogen and then start fusing again into helium?

    --
    Priest: "Universe from nothing, no laws of physics, sped up time"+ huge discrepancies. Creationism? No. Big Bang Theory
    1. Re:Neutron Star Decay by IndustrialComplex · · Score: 2

      Why "must" it decay?

      Neutron stars basically just cool off/slow down over time due to rather normal mechanisms of radiation. There's some other stuff going on, but very old neutron stars are basically just lumps of cold very old neutrons.

      --
      Out of modpoints but really liked a post? 1BDkF6TtmmeZ3yqXbz9yhdYVqRYnwFoXDj
    2. Re:Neutron Star Decay by Sockatume · · Score: 1

      There's no reason to suppose they "must eventually decay". I expect that all that happens is that you have a vanishingly low concentration of protons and electrons near the surface (due to buoyancy) that turn over back into neutrons by the inverse process.

      --
      No kidding!!! What do you say at this point?
    3. Re:Neutron Star Decay by Maritz · · Score: 1

      very old neutron stars are basically just lumps of cold very old neutrons.

      Probably more accurate to say 'will be' rather than 'are'. I don't think the Universe is anywhere near old enough to have cold neutron stars.

      A few interesting points about neutron stars here.

      --
      I do not want your cheap brainburning drugs. They are useless for work. And I am a working man today.
  12. Still guesswork by Anonymous Coward · · Score: 1

    Not conclusive evidence for a Thorn-Zytkow object. FTFA:

    "The star is enriched in lithium, rubidium and molybdenum. Elevated amounts of these elements are thought to arise as by-products of Thorne-Zytkow objects, which have to burn through unusual nuclear fusion pathways."

    "The object is an excellent candidate, although it is perhaps not an open-and-shut case,” says Podsiadlowski. There is not quite as much of the three enriched elements as expected, he says."

    1. Re:Still guesswork by HolyCrapSCOsux · · Score: 1
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      0xB315AA8D852DCD3F3DCA578FD2E0BF88
  13. Neutron & Proton decay by emil · · Score: 1

    Protons are stable to a period greater than 2.1 * 10^29 years (also listed as 10^36 years in the article). Free protons will/might fall apart after that time.

    Free neutrons have a very short period of stability (about 15 minutes). Within dense confinement, one would wager them to be on the order of proton decay.

  14. Forget it by justthinkit · · Score: 1

    What you are proposing would be healthy for the physics community, so it will never happen. It is imperative that physics appear to be all knowing, especially when you talk about worm holes and the Big Bang and what will happen in 10^^100 years. We know exactly what is going on, right up until everything changes as one flawed theory is replaced by another with new flaws.

    I think the other two replies are reacting to the notion that physics doesn't need to be taught, but rather just let everyone "have a go". Personally I don't think that is what you meant.

    I find physics at once childish and elitist, and wish it was more humble. For example, with regard to the ether. We thought it was there, then we "proved" it was not...but today it is generally held that there is "vacuum energy" (and/or dark energy). Clearly there is an ether, and it is "made of" energy, not matter. And it is at an energy level vastly higher than 2.7K, so we need to create theories that are comfortable with this. I've done my part.

    --
    I come here for the love
    1. Re:Forget it by justthinkit · · Score: 1

      I appreciate your thoughts. Fair comment that TV does not equal real life. Too bad that 99.9% are getting the TV message though.

      I'm curious why you differentiate ether & vacuum energy. Why can't one be the other? A medium for transmitting (ether), is also the force that pushes the Universe apart?

      --
      I come here for the love
  15. Apologies for the length, but... by justthinkit · · Score: 1

    Usually I assume if someone is interested enough in the topic, especially something history related, they might have at least checked the Wikipedia article on it first. If for someone reason you don't trust/like Wikipedia for an executive summary, that article links to plenty of primary and secondary sources, so there is not much need for me to try to track down online versions of stuff on my bookshelf.

    My questions about the sources of your blanket statements was to point out that YOU were not backing up YOUR statements.

    But as previously stated, the properties attributed the aether changed as experiments and new findings invalidated older properties. Sometimes it was different people, but in a few cases it was the same person updating their previous theory.

    Einstein never made any mistakes with his theories?

    String Theory doesn't change its tune every month?

    There is nothing wrong with changing a theory that doesn't work. In fact, that is my position -- physics today is in the doldrums because the major theories have major problems. Those trying to provide something better/different need to be heard if we are ever going to make further progress in physics.

    The aether went from a fluid to a solid to a really stiff fluid,

    Talk of solids and fluids reflects the lack of scientific knowledge that was present a hundred years ago. There is no child today that would propose that. But there are plenty of scientists that have maintained that there must be an ether. In other words, there seems to be something about an ether that could explain stuff, at least in the minds of Newton, Poincare, De Pretto and Samuel Tolver Preston. Personally, I think they were on to something.

    My theory says the ether is ultra high energy (which is what physicists calculate space should be composed off anyway...they just haven't managed to detect it yet), and "mechanically" as you keep saying, my "particles" are 20 orders of magnitude smaller than those of the atomic scale. Solids and fluids are at one end of a very very long scale, and my "springs" are precisely at the opposite end.

    Off the top of your head, what test would you use to detect something 20 orders of magnitude smaller than a proton, and having an energy sixty to one hundred orders of magnitude higher than the background energy of space that we presently measure?

    it went from negative compressibility to incompressible. Early experiments discounted the idea of the aether drag, but then precision interferometer experiments necessitated reintroduction of aether drag. The properties were not because we measured the aether, but because experiments kept eliminating properties that made it work, and the theories had to be updated.

    I am all for eliminating what can not be. That is how science makes progress. I just think that the last thing we have eliminated is the ether itself. We need to do more eliminating, if we can, but we also need to compose theories and models where an ether is part of the model...and see if such models can produce the results we see in the world.

    Sometimes we need to carry models along for quite some time, in tandem with conflicting models. For example, the static versus expanding universe. Einstein thought it was static. We didn't kick him to the curb for this. Looking back, it didn't really matter whether we thought it was expanding or not. What mattered was that we found a way to prove it was expanding, and we have gone with that. In the future it may yet prove to not be expanding, or be expanding faster than we thought, or, or, or.

    It doesn't pay to be too smug about a physics theory.

    The position of the majority of the physics community on the ether has determined our direction since the time it was ruled out. And right now we have ended up with

    --
    I come here for the love
    1. Re:Apologies for the length, but... by justthinkit · · Score: 1
      Thanks for the reply. I am about out of time on this discussion as well -- insulating the crawl space takes precedence for the rest of the morning at least.

      You end up with two ways to go, to either work toward completeness, that a theory must be as accurate and complete as possible, at potentially but not necessarily the cost of complexity, or you work toward finding approximations that are simpler and more practical, at the cost of only working within specific bounds and situations.

      Totally agree with this. Physics is pushing the "more accuracy" frontier pretty hard these days but at least one drawback of this is...ahem LHC ahem...cost. I think the Higgs particle/field is on the wrong path, so to me the LHC has yet to, and might never, prove itself worth the billions spent.

      And chemistry has been built on that simple basis ever since.

      You should look into modern physical chemistry... if you think learning about propagators is complicated, then you won't find modern chemistry simple, at least the parts trying to be predictive and starting to allow designer chemicals and materials to be made in silica.

      I think you are confusing engineering and science. Engineering is always tough, science only sometimes (i.e. until a good theory is conceived. After a good theory has been developed, the science flows like water).

      And I wasn't sure if the idea of speed of light changing 0.25 mph in the last century or so was meant as something based on reported measurements (the speed of light wasn't measured that accurately until the 70s).

      That result was part of my calculations section, based on my theory. So it is a predictive calculation I have made.

      And speaking to the first line of your latest reply:

      I don't know on which end communication is breaking down,

      I think we just have a fundamental difference of opinion when it comes to (1) the potential value of factoring an ether into present & future physics theories, and (2) whether that very ether can also be a lot of other things (like dark energy/vacuum energy).

      I wouldn't sweat it if I were you. Personally, I am quite comfortable with us disagreeing.

      but I don't have the saintly patience to try until that is figured out, but a couple big picture points:

      I hope you don't take this the wrong way, but I read "saintly patience" as condescending. Instead I look at this or any other exchange as a chance for someone, or both, to learn something. If we can't imagine we have something to learn from an exchange, then we will come across as know-it-all (while we miss out).

      By the way, I wouldn't mind knowing who I am talking with. Drop me an email to at least let me know that. I promise I won't spam you (besides email filters handle that sort of thing pretty well).

      --
      I come here for the love