Comment by sixo
11 hours ago
Can someone knowledgeable weigh in: is the "dark object" here believed to be a localized blob of dark matter? A dark star or black hole? Or is "dark" being used generally to mean "not bright enough to see at this distance"?
In this context, “dark object” really does mean a localized blob of dark matter, not a black hole or a dim, normal-matter object.
The research team detected it only through its gravitational lensing effect — the way it slightly distorted the light from a more distant galaxy. There’s no emission at any wavelength (optical, infrared, or radio), and its gravitational signature matches a million-solar-mass clump of invisible mass rather than a compact point source like a black hole.
They specifically interpret it as a dark matter subhalo — one of the small, dense lumps that simulations of “cold dark matter” predict should pepper the universe’s larger halos. It’s too massive to be a single star, far too diffuse to be a stellar remnant, and not luminous enough to be a faint galaxy.
So “dark” here isn’t just shorthand for “too dim to see at this distance” — it’s used in the literal physical sense: matter that doesn’t emit or absorb light at all, detectable only via gravity.
Eventually, all the dark matter clumps into rings around galaxies, but since this one is so distant, ~10B light years, so we are seeing that clump as it was that long ago before it difused into it's ring shape we can see in the galaxies around us.
Why does dark matter form halos/rings around galaxies. Why isn't it attracted to the centre of the galaxy like 'normal' matter?
It is attracted to the center of the galaxy.
Normal matter also makes halos or rings around the center of the galaxy. That's how gravity works. And since dark matter interacts less, it stays more spread.
4 replies →
I believe that you have the order of operations misunderstood.
I probably don't know that much more than you about the subject, but from what I understand, the prevailing model suggests that these Halos formed early in the formation of the universe when spacetime had varying "pockets" of density that naturally led to these halos - the formation of the galactic disk therein was actually supported by the halo existing first, because baryonic matter (aka non-dark matter, the stuff that makes up planets, stars, etc) was still too energetic from the formation of the universe to become gravitationally bound to itself.
2 replies →
Dark in the context of astrophysics means specifically that the object/matter does not interact directly with electromagnetic radiation (eg absorb an optical/microwave/radio photon). So it is probably dark matter, but probably unlikely to be a black hole because we can typically detect a black hole's effects in an indirect manner :P
From the paper, it could be the dark-matter halo of an otherwise too faint dwarf galaxy. They state that a “more definitive statement on what type of object [it] is will require deep optical/infrared observations to detect any potential EM emission”.
Definitionally, yes. It’s inert but lenses light around it.
The paper is more about the technical achievement of detecting it, IIUC. It’s not the first dark matter inference we’ve had, and doesn’t really tell us anything new about the stuff.
It challenges warm dark matter and ultralight dark matter theories because they'd be less likely to clump into something so small. Similarly MOND would have trouble explaining a completely isolated chunk of it at this size (any baryonic matter trapped in a region this small would almost certainly emit enough light to detect).
I’m admittedly a few years out of date in this, but weren’t those already kinda ruled out? I’ve never met anyone who took MOND seriously - it looks like it’s a pet project of a small number of people who cite each other, and people in different subfields have always been saying it doesn’t work for them (diffuse galaxies, etc.).
I know the current models favor cold DM, I thought the hot DM model was abandoned already when it became clear that clusters of any size exist?
I'm an amateur but I feel confident enough to answer -- hopefully not a mistake!
They're explicitly looking for "Dark Matter", which doesn't "interact" with normal ("baryonic") matter or electromagnetic radiation (e.g. light). So it's not a black hole for sure, as those are composed of regular ol' matter.
RE:"dark star", that's really up in the air, I'd say! AFAICT the only academic reference to that term is for normal stars influenced by dark matter[1], but kinda the whole problem here is that we don't know much about what dark matter is composed of or into. Certainly it's not going to be a star in the traditional sense as it can't emit light, but I'm not aware of any reason this object can't end up being a giant sphere.
FWIW, Wikipedia says "One of the most massive stars known is Eta Carinae, with 100–200 [solar masses]", whereas this object "has a mass that is a million times greater than that of our Sun". If we're going to use metaphors, I think "dark dwarf galaxy" might be more appropriate?
[1] https://arxiv.org/pdf/1004.1258
(I’m an astrophysics undergrad.) Black holes aren’t composed of anything, they’re just defined by their charge, spin and mass equivalent.
Dust clouds have those mass ranges. It’s not a galaxy-scale mass by any measure.
This thread has a lot of CS people being confident about physics.
I was always surprised that when we talk about BHs mass, charge, and spin that we really mean U(1) (electromagnetic) gauge charge and not charges from global symmetries. (If BHs had global charge, you could at least say that this or that black hole was made out of N baryons, or whatever.)
But it's really so---according to GR, black holes don't have global charges. So even if you see a star made out of baryons collapse into a black hole, once the BH settles down into a steady state you can't say it's "really" got baryons inside: the baryon number gets destroyed.
(Of course, a different model of gravity that preserves unitarity might upset this understanding.)
2 replies →
Welcome to Hacker News.
I mean, I included a disclaimer... But regardless, you appear to be wrong on both counts (or at least contradicting Wikipedia):
1. "The presence of a black hole can be inferred through its interaction with OTHER MATTER and with electromagnetic radiation such as visible light." https://en.wikipedia.org/wiki/Black_hole
2. "A dwarf galaxy is a small galaxy composed of ABOUT 1000 up to several billion stars" https://en.wikipedia.org/wiki/Dwarf_galaxy
Darn astrophysics majors being confident about astronomy! ;)
which doesn't "interact" with normal ("baryonic") matter
I think you mean it doesn't interact electromagnetically with either matter or radiation. It does interact with normal matter via gravity -- that's pretty much the strongest (only?) argument for its existence.
I'm not aware of any reason this object can't end up being a giant sphere
AIUI, most theories posit that solid spheres of dark matter are very unlikely because matter accretion is governed by electromagnetism in addition to gravity, and dark matter is not supposed to obey the former. Most models assume that dark matter is organized in gaseous clouds (halos); strictly speaking that's still a giant sphere, just not in the same way that Jupiter or the Sun or even the Oort Cloud is.
100-200 solar masses is not one of the largest known. There are many that are 1000s of times more massive than the sun.
This confused me too from all those solar object size comparisons I’ve seen. Turns out there are stars that are 1000s of times bigger than the sun, but they aren’t the same density.
I'm unaware of any stars in the 1000 Msun range. Wikipedia puts 291 Msun of R136a1 at the largest. After that, 195 M of R136a2 is the next. A star at 100 Msun would be in the most massive stars known.
https://en.wikipedia.org/wiki/List_of_most_massive_stars#Lis...
1 reply →
[dead]
Or a cloaked ship?
If so it's a big one, 1M solar masses.
That’s just how warp drives happen to appear from the outside.
EXCESSION
... and its heading right for us :P
They found a statistical anomaly that they're trying to atrribute to new physics, using some novel maths. So a tiny speck of evidence towards a new theory of matter (i know nothing about astro, just my supposition)