- #1
- 19,011
- 14,564
Just noticed this article. Wonder if anyone here has further info. Sounds very interesting.
http://www.bbc.com/news/science-environment-43543195
http://www.bbc.com/news/science-environment-43543195
https://phys.org/news/2018-03-dark-galaxy.htmlThe research, published in the March 29th issue of the journal Nature, amassed data from the Gemini North and W. M. Keck Observatories, both on Maunakea, Hawai'i, the Hubble Space Telescope, and other telescopes around the world.
https://phys.org/news/2016-08-scientists-dark-milky-massive-galaxy.htmlScientists discover a 'dark' Milky Way: Massive galaxy consists almost entirely of dark matter
I'm seeing this too. If I were to guess, the link is correct but Nature hasn't physically released the paper on their website yet. Probably a website glitch that prevented the paper from being displayed at the same time the press embargo lifted. It'll probably be visible within a day or so, unless there was some publication problem that made Nature want to pull the article at the last minute before release.fresh_42 said:Here's what I've found:
https://phys.org/news/2018-03-dark-galaxy.html
Unfortunately the link to the paper: https://www.nature.com/articles/doi:10.1038/nature25676
seems to be broken. But as it happened to me on two different sources (https://www.sciencealert.com/galaxy-ncg1052-df2-no-dark-matter-ultra-diffuse-dragonfly-array being the other one), it might be a local problem. However, I think nature is behind a paywall anyway.
Also interesting in this context is an example of the opposite:
https://phys.org/news/2016-08-scientists-dark-milky-massive-galaxy.html
I do find this interesting, and I would be willing to bet it was the result of some particularly violent events in the galaxy's past which separated matter and dark matter.phinds said:Just noticed this article. Wonder if anyone here has further info. Sounds very interesting.
http://www.bbc.com/news/science-environment-43543195
kimbyd said:The process would have had to have been the normal matter being removed from a dark matter halo through some process.
The article can be found here: https://www.nature.com/articles/nature25767fresh_42 said:Unfortunately the link to the paper: https://www.nature.com/articles/doi:10.1038/nature25676
seems to be broken. But as it happened to me on two different sources (https://www.sciencealert.com/galaxy-ncg1052-df2-no-dark-matter-ultra-diffuse-dragonfly-array being the other one), it might be a local problem. However, I think nature is behind a paywall anyway.
It is indeed behind a paywall.Abstract said:Studies of galaxy surveys in the context of the cold dark matter paradigm have shown that the mass of the dark matter halo and the total stellar mass are coupled through a function that varies smoothly with mass. Their average ratio Mhalo/Mstars has a minimum of about 30 for galaxies with stellar masses near that of the Milky Way (approximately 5 × 1010 solar masses) and increases both towards lower masses and towards higher masses. The scatter in this relation is not well known; it is generally thought to be less than a factor of two for massive galaxies but much larger for dwarf galaxies. Here we report the radial velocities of ten luminous globular-cluster-like objects in the ultra-diffuse galaxy NGC1052–DF2, which has a stellar mass of approximately 2 × 108 solar masses. We infer that its velocity dispersion is less than 10.5 kilometres per second with 90 per cent confidence, and we determine from this that its total mass within a radius of 7.6 kiloparsecs is less than 3.4 × 108 solar masses. This implies that the ratio Mhalo/Mstars is of order unity (and consistent with zero), a factor of at least 400 lower than expected. NGC1052–DF2 demonstrates that dark matter is not always coupled with baryonic matter on galactic scales.
The cluster collision was the one idea I had. This has the nice property of the fact that it can leave some normal matter in a location far from dark matter, and the colllision itself acts to compress the normal matter, potentially kicking off star formation (the formation of bright stars could remove the rest of the gas and dust from the galaxy).Grinkle said:Can you give some example hypothetical processes to show the distinction you have in mind? One uses the same process to separate yolk from white as white from yolk, is why I can't picture it.
kimbyd said:The cluster collision
I don't know if anybody has tried to model this. I wasn't able to find anything obvious from my small amount of searching.Grinkle said:I don't know how to search for such a paper - I wonder if anyone has tried to model gravitational events that would remove gas from hypothetical rings of dark matter and see if they can get a result that leaves the gas both isolated and in a state that can subsequently form a galaxy that won't spin itself apart.
I'll bet someone does now, though. ;-)kimbyd said:I don't know if anybody has tried to model this.
Sensible on its face, at least.In any event, I'd be willing to bet that such situations are quite rare in practice. But a cluster collision does, at least on the surface, have two properties that make it nice for the problem:
1) The colliding gas is compressed as a result of the collision.
2) The colliding gas is separated (at least partially) from both the dark matter and stars.
If their scientific history were the same as ours, they would instead be faced with explaining why their galaxy was void of dark matter. They would first observe dark matter in terms of missing mass due to galaxies moving too fast in a nearby cluster. Then by looking at rotational curves of other galaxies. Eventually they would of course try to measure the dark matter density of their own galaxy and conclude it iz zero. As you said, some would likely look for anthropic arguments while others would try to explain it in other ways.Demystifier said:How would scientists living in the galaxy without dark matter explain that all other galaxies have dark matter?
My first guess is that they would try to make up an antropomorphic explanation, according to which only galaxies without dark matter support intelligent life.
Note that EM radiation does not interact with DM, after all that's why DM is dark.anorlunda said:What a fun find.
This is not my field, but here's a novice question. Is there any scenario where radiation pressure could be large enough to separate ordinary matter from DM?
Demystifier said:Note that EM radiation does not interact with DM, after all that's why DM is dark.
Yeah, but it would tend to spread it out in all directions, not move it off in a cluster.anorlunda said:Yes, that's the origin of my novice question. Radiation pressure would push ordinary matter away but it would not interact with the DM. Therefore radiation pressure if strong enough, should tend to separate the OM from the DM.
Demystifier said:How would scientists living in the galaxy without dark matter explain that all other galaxies have dark matter?
My first guess is that they would try to make up an anthropic explanation, according to which only galaxies without dark matter support intelligent life.
My first guess is that they would use the particular facts that were well known in their galactic neighborhood -- say, the presence of an equivalent of M31. Galaxy collisions and the size & nature of M31 have been known here longer than DM has been known.Demystifier said:How would scientists living in the galaxy without dark matter explain that all other galaxies have dark matter?
My first guess is that they would try to make up an anthropic explanation, according to which only galaxies without dark matter support intelligent life.
Maybe not banned, but it appeal to the participants of this thread to stop speculations about an imaginary civilization in another galaxy. I've read the post which started this as a critic on the anthroposophical principle, which is certainly worth a discussion, but not here. It is even highly speculative with regard to the fact, that we have absolutely no idea what dark matter actually is, and less its possible cosmological interactions - except for one.JMz said:speculations that would, of course, get banned from their version of PF ;-).
That's difficult to do, I think. Stars experience very little dynamical friction. The effect you'd be looking for here is a galaxy moving through a cloud of gas that is so large that the extremely tiny amount of dynamical friction they do experience is enough to separate them from the dark matter. I don't have a clear handle on the magnitude of dynamical friction for stars, however, so I don't know what would be required to observe this effect. It may be utterly infeasible.JMz said:But if, instead, the galaxy already has stars, is it possible to separate the stars from the DM by dynamical friction with the stars of the galaxy it's hypothetically passing through?
Actually, I was asking about star/star interactions, in the absence of all gas. Yes, friction is small, but I don't think we've hypothesized a pre-collision size for the galaxy, so it could be a small fraction of something large.kimbyd said:That's difficult to do, I think. Stars experience very little dynamical friction. The effect you'd be looking for here is a galaxy moving through a cloud of gas that is so large that the extremely tiny amount of dynamical friction they do experience is enough to separate them from the dark matter. I don't have a clear handle on the magnitude of dynamical friction for stars, however, so I don't know what would be required to observe this effect. It may be utterly infeasible.
I took @Demystifier's suggestion as being tongue-in-cheek, and my comment about "their" PF was in the same spirit.fresh_42 said:Maybe not banned, but it appeal to the participants of this thread to stop speculations about an imaginary civilization in another galaxy. I've read the post which started this as a critic on the anthroposophical principle, which is certainly worth a discussion, but not here. It is even highly speculative with regard to the fact, that we have absolutely no idea what dark matter actually is, and less its possible cosmological interactions - except for one.
Star-star interactions have effectively zero friction. Direct collisions are far too rare to be a significant friction component. Gravitational-only interactions are something that dark matter also experiences, and won't be capable of separating stars from dark matter.JMz said:Actually, I was asking about star/star interactions, in the absence of all gas. Yes, friction is small, but I don't think we've hypothesized a pre-collision size for the galaxy, so it could be a small fraction of something large.
I'm referring to https://en.wikipedia.org/wiki/Dynamical_friction, a la Chandrasekhar. My intuition -- and this is really the heart of my question -- is that DM will experience far less of it than stars, due to stars being "lumpier". That is, star/star interactions will be less frequent but, when they do occur, very much larger; DM interactions with stars or with DM will be frequent but tiny, exactly as if the star were moving through gas. The former would be capable of large angular change for a small fraction of the stars, the latter would not. (Just a form of the central limit theorem, or at least the law of large numbers.)kimbyd said:Star-star interactions have effectively zero friction. Direct collisions are far too rare to be a significant friction component. Gravitational-only interactions are something that dark matter also experiences, and won't be capable of separating stars from dark matter.
I did not follow the point about MOND. As for the Quanta quote, that seems to be an error in reasoning, right?mitchell porter said:"In MOND, violation of Newton's laws occurs at extremely small accelerations" (wikipedia). Some comenters are treating this as a falsification of MOND because it's a very low mass galaxy, so the gravitational force should be in the MONDian regime.
However, in MOND, the presence of gravitational fields from neighboring massive objects can impose a Newtonian or quasi-Newtonian regime on a light object. Ironically, this is something dark matter theorists want too, in order to explain the lack of dark matter in NGC1052-DF2 - "the larger gravitational field from adjacent galaxies could have pulled dark matter away from it" (Quanta).
It would make no sense at all to believe that gravity acts one way for normal matter and another way for dark matter.Grinkle said:To whoever may know - is there any evidence that dark matter has the same G (gravitational constant) as visible matter? I think the reasoning in this thread all assumes that it does, I'm wondering if that is a default assumption or if there some way to draw that conclusion from cosmological observations.
I am admittedly over my head in asking this question - I intend to be asking if the ratio of inertia to gravitational attraction for dark matter is the same as for visible matter, or if we have any evidence to say one way or the other. I think we just assume that it does, and that drives our calculation of halo's etc of dark matter.
They could be right .Demystifier said:only galaxies without dark matter support intelligent life.
I don't buy for an instant that MOND can explain the variation in observed dark matter between different galaxies. At least not in anything approaching a reasonable manner (that is, no parameters that are tuned per-galaxy). MOND is basically dead now anyway. Has been for a long time.JMz said:I did not follow the point about MOND. As for the Quanta quote, that seems to be an error in reasoning, right?
Questioning that ratio is the appropriate way to ask about this assumption.Grinkle said:asking if the ratio of inertia to gravitational attraction for dark matter is the same as for visible matter, or if we have any evidence to say one way or the other. I think we just assume that it does, and that drives our calculation of halo's etc of dark matter.