64 comments

  • jahnu 3 days ago ago

    One thing worth noting is our popular notion of what a star seems to be is quite different from what astronomers have.

    One example, Canis Majoris has a radius of about 1420 solar radii. But its mass is roughly 17±8 times the mass of the Sun and therefore an average density of 5.33 to 8.38 mg/m3. “It is over 100.000 times less dense than Earth’s atmosphere at sea level.”

    https://en.wikipedia.org/wiki/VY_Canis_Majoris

    https://nineplanets.org/vy-canis-majoris/

    • Sharlin 3 days ago ago

      The surface radius of a star is defined based on optical thickness. If you were there, the star would in fact look like a fairly well-defined opaque spheroid with the reported radius. The density of the photosphere plasma is near zero, but there’s a lot of it.

      • brabel 3 days ago ago

        Why doesn’t the stuff just falls in towards the center? It just floats there??

        • zygentoma 3 days ago ago

          Radiation pressure! There is so much heat (= photons) radiating outwards, that it counteracts the gravitational pull.

          • stouset 3 days ago ago

            What’s particularly interesting to me is that for stars the size of our sun, regular old gas pressure dominates. The sun’s atmosphere is held up essentially just from the temperature (and therefore high kinetic energy) of the plasma.

            Only once you get to 10+ solar masses does radiation (light) pressure begin to become significant, and at 50+ solar masses is when it dominates and the atmosphere is held up by the momentum of light.

          • sega_sai 3 days ago ago

            In most star photospheres the role of radiation pressure is negligible. They are supported by the pressure gradients. The exception is very hot stars.

          • brabel 3 days ago ago

            Wow I knew that stars have that radiation pressure but had no idea it caused mass to get so crazy far away from the ignited area of the star!

            • Sharlin 3 days ago ago

              These giant stars burn so very very bright. And correspondingly only live a few tens of millions years at most.

        • kulahan 3 days ago ago

          To add on to the other response, think of it like the star “leaking” into space. It’ll be defined as a pretty radically different size at some point in the future, even as it’s still undergoing fusion.

    • usrnm 3 days ago ago

      My layman definition of what a star is is "it's somewhere in the sky and it gives off light". The word "density" wouldn't even come to my mind

      • kulahan 3 days ago ago

        Thanks to blackbody radiation, every human skydiver briefly becomes a star by this definition! ;)

        It needs a core generating energy through fusion, which has density requirements, for what it’s worth.

    • FranOntanaya 3 days ago ago

      I always wonder when do they stop considering the outer layers part of the star and not relatively dense solar wind soup. Nobody says Earth has 7000km radius, even tho there's traces of exosphere past 500km.

      • antognini 3 days ago ago

        The outer boundary is the point where a photon has a ~50% chance of escaping without encountering another particle.

        • encrypted_bird 3 days ago ago

          Do you have a source? I'd love to read more. :)

          • zamadatix 3 days ago ago

            Amateur stargazer's understanding:

            Depending what kind of reading material you're looking for (e.g. high level details or mathematically/jargon dense papers) look for things discussing "Rosseland optical depth" and "grey atmosphere approximation".

            At a high level, the common convention is to define the radius by finding where the optical depth is 2/3 when using Rosselands clever way of calculating a weighted mean of the opacity from that layer in the star to space across different wavelengths of light. 2/3 being a clever derivation from Eddington where, in an idealized model of a star, that's when the actual temperature of the star should equal its blackbody equivalent temperature.

            Pedantically, this distance to the point of equality is an ever so slightly different value than the "distance from the center where there is a 50% chance a photon traveling directly outward will escape the star without another interaction" rule of thumb (in the same idealized grey model). Practically, that the difference is so small is why it's a fantastic rule of thumb explanation.

          • antognini 2 days ago ago

            I'd recommend Carroll & Ostlie's Introduction to Modern Astrophysics, though it requires some basic calculus and physics.

      • chabska 3 days ago ago

        The radius is based on visual observation. We have good theories and models about what's happening inside the star. We are quite sure that it's mostly empty space inside the radius. But that's not a good enough reason to say that the star's radius is anything other than what we see through our telescope.

        • zamadatix 2 days ago ago

          Importantly, this works for stars relatively close to us (the farthest I can find is 16,000 light years for one hyper giant) but the majority of the stars catalogued in even our own galaxy have only been assigned a radius via taking the temperature (via color) and luminosity.

      • 3 days ago ago
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    • margalabargala 3 days ago ago

      > therefore an average density of 5.33 to 8.38 mg/m3

      That's nuts. How on earth does fusion happen at that density? Is there a denser core that actually fuses, and the outer fluffy bits just glow from the inner heat?

      • adrianN 3 days ago ago

        Averages are quite misleading. The core is obviously a lot denser. Our sun has an average energy output per cubic meter that is comparable to a compost heap.

        • margalabargala 3 days ago ago

          Sure, but now I'm left wondering what the size of the body doing fusion is. If most of the star is glorified glowing atmosphere, I want to know the mass and radius of the fusing bits.

          • peri-cl 3 days ago ago

            There's dedicated Wikipedia articles responsive to this,

            https://en.wikipedia.org/wiki/Solar_core

          • idiotsecant 3 days ago ago

            Depends on the class of the star. Our sun? About 1/4 radius and in is fusion reaction. But it gets weird in other stars. In red giants the fusion zone is a very small shell around a dead core. Maybe something like earths orbit in radius, but very very thin.

        • throwaway89864 3 days ago ago

          Astra says this claim is misleading. Sun's average energy output per cubic meter is three orders of magnitude smaller than that of a compost heap. The fusion core is comparable though.

          • Retric 3 days ago ago

            The energy density of specific compost heaps varies by several orders of magnitude it’s not a single number. Volume, moisture content, internal temperature, external temperature, materials being composted, etc all play a significant role.

            • mordechai9000 3 days ago ago

              Stellar fusion could also be a factor in a sufficiently large compost heap.

          • malfist 3 days ago ago

            Of course it's misleading, thats the point GP was trying to make. Averages belie truth in large, diverse systems with extremes

    • lrasinen 3 days ago ago

      Average density for non-uniform objects is pretty useless, since the cubic volume scaling makes a mess of things.

      As an example, I pulled the stats for an electric locomotive. 19x3x4.4 meters, mass 90 metric tonnes. That's an average density of about 1/3rd of water.

      • Rygian 3 days ago ago

        So a locomotive floats. Interesting.

        • TeMPOraL 2 days ago ago

          Locomotive itself? Probably not. If you turned its abstract bounding box into real box - thin, negligible mass, enough strength not to break up - and evacuated the air inside, then yes, the box with locomotive in it should float.

    • dpriddle 3 days ago ago

      Yes and no. It’s fluffy on the outside, but at the core it’s likely denser than our sun.

    • ramraj07 3 days ago ago

      The largest supermassive blackholes have an average density less than earth's atm as well.

    • dylan604 3 days ago ago

      I love astronomy simply for things like "17±8 times the mass". That's ~50% acceptable variance. I wish I could apply that logic to my creditors.

      • e_l 2 days ago ago

        Yeah, Physics (and particularly astronomy/cosmology) often have huge variances, some of which are even greater.

        An example being the number of stars in the (observable) universe which ranges from 10^22 to 10^24 stars...a variance of 100x (or ~10,000%)!!! https://www.esa.int/Science_Exploration/Space_Science/How_ma...

      • kulahan 3 days ago ago

        I worked for a financial org with over a trillion in assets, and they had a 100% acceptable variance on project length predictions. Made for a laid-back atmosphere at work but boy. How they ever swung that is beyond me.

        “We predict a year, so it’ll take anywhere between 8 seconds and 24 months!” AND IT WORKED???

    • peri-cl 3 days ago ago

      These objects (black hole stars) seem to be far larger than that,

      https://en.wikipedia.org/wiki/Quasi-star#Formation_and_prope... (Caption: "Size comparison of a hypothetical quasi-star to some of the largest known stars")

  • benji-york 3 days ago ago

    Any decent human being would have called these Black Hole Suns.

    • vardump 3 days ago ago

      I just twisted my mouth sides upwards with my fingers to form a smile in agreement.

    • pixelpoet 3 days ago ago

      Sadly, those won't come.

    • ramraj07 3 days ago ago

      By all indications Chris Cornell likely tried to paint some poignantly depressing mindset with that lyric, so its doubly ironic the universe is choke full of it. Or at least was.

  • ck2 3 days ago ago
    • brabel 3 days ago ago

      They are great but you forgot Anton! He definitely belongs with them in my opinion, he is a wonderful person after all :)

      Link: https://youtu.be/gUobqtANMfE?si=NVG26d6Aoc2XNEWg

      • Hikikomori 3 days ago ago

        Was also a fan of Anton but professor Dave recently made a video about him.

        https://youtu.be/dst-C0IDQRU

        • kulahan 2 days ago ago

          I’m not really down to watch a 90 minute video on the dramas of astrophysics, so I’m not sure what it says, but interestingly Sabine Hossenfelder took an extremely minor swipe at him not too long ago. Guess the dude is at least legit-enough for that? Haha

          • Hikikomori 2 days ago ago

            Dave does a lot debunk videos but this is just a clickbait title as it's an interview with Anton.

            • andrewflnr 2 days ago ago

              Clickbait which you made worse? Come on man, don't do that.

              • Hikikomori 2 days ago ago

                Continuing the joke on Antons titles, lighten up.

            • kulahan 2 days ago ago

              Roger, that makes sense. I… might actually watch this now LOL

      • blop 3 days ago ago

        Anton is definitely wonderful! He explains everything very well with no drama and BS. High information density and yet very clear!

  • JumpCrisscross 3 days ago ago

    Is there an experiment that could resolve this? Literally resolve these objects better, or otherwise distinguish between these hypotheses?

    Is there anything behind these objects they could lens?

    • vardump 3 days ago ago

      I wonder if our universe is the experiment to resolve this.

      • itsalwaysgood 3 days ago ago

        We don't have a good fuel source or reason for expansion. We also don't know where all the theorized white holes could be.

        To me it's an interesting coincidence, thought description of these objects baffles me.

        Unless the universe is recursively within itself: the black hole stars have black holes within them that also exit at the big bang. But then so do all other smaller big bangs we see: exact same exit point and coincidentally, the same moment in time.

        Oh, and there is a beautiful symmetry here: only one white hole exists.

        One beginning, many endings. It's armchair philosophy but fun to imagine.

    • wraith_ilands 3 days ago ago

      [flagged]

  • debo_ 3 days ago ago

    Soundgarden was apparently prophetic with their hit song "Black Hole Sun."

    • TimeBearingDown 3 days ago ago

      May Chris Cornell rest in peace. He should have seen this.

  • joebig 3 days ago ago

    Wouldn't objects this ancient (following in the wake of the big bang, essentially) be redshifted anyway, on account of cosmological expansion?

    • Tuna-Fish 3 days ago ago

      Yes, and we are already accounting for it. The objects as seen by us are actually very deep in infrared, when you correct for the redshift to match the key absorbtion lines of hydrogen, they still remain very red.

      • joebig 2 days ago ago

        Appreciated. May I ask regarding the determination of the magnitude of correction to apply? Is it a case-to-case basis? In other words, is it very sensitive to the distance assumped for the LRDs?

        • Tuna-Fish 2 days ago ago

          The light curve is not smooth, there is a clear spectrum caused by absorption lines. You find the pattern in the lines that you know to be hydrogen, and measure how much redder it is than it would be without redshift.

  • itsalwaysgood 3 days ago ago

    Perhaps they are somehow related to the elusive white hole: exit points of black holes.

    Fuel for a Big Bang, if you can imagine. A universe within itself.

    The article says they're sucking up gas though so I don't know. The arrow of time is weird. It would feel elegant to me, but I'm way out of my league.

    The imagined scenario only works if you picture all black holes 'twisting time' towards its beginning.

    Sort of like recursion, or a tesseract, where there's one beginning and many endings.

  • a day ago ago
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  • NeoByte 2 days ago ago

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