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#1
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How can that be?
As I mentioned in another thread, the disk of the satellite galaxies of
Andromeda is extremely thin: http://arxiv.org/abs/1301.0446 A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy From the abstract: "The structure is vast: at least 400 kpc in diameter, but also extremely thin, with a perpendicular scatter 14.1 kpc (99% confidence)." Well, that is a factor of around 30... At only 150Kpc the rotation period is 5 billion years. Since the supposed "age of the Universe" this disk can at most have done 2.74 revolutions. But Andromeda did not exist right after the supposed big bang so it must be quite less than that. How can it be so flat? Isn't it that flat disks flatten themselves by rotating? This is clearly not the case he there isn't enough time to do a lot of rotations. Or I am miscalculating something? This huge structure must be more ancient than 2.75 rotations. Much more. Maybe 20, 30 rotations to flatten itself, at least! |
#2
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How can that be?
On Monday, August 18, 2014 8:18:34 AM UTC-4, jacob navia wrote:
Or I am miscalculating something? This huge structure must be more ancient than 2.75 rotations. Much more. Maybe 20, 30 rotations to flatten itself, at least! One thing you are obviously missing is the possibility that the planar morphology is NOT due to rotational flattening. Perhaps other models like the capture/breakup model are needed? [Mod. note: reformatted -- mjh] |
#3
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How can that be?
In article , jacob navia
writes: Well, that is a factor of around 30... At only 150Kpc the rotation period is 5 billion years. Since the supposed "age of the Universe" this disk can at most have done 2.74 revolutions. But Andromeda did not exist right after the supposed big bang so it must be quite less than that. Leave out "supposed" and people will take you more seriously. How can it be so flat? Isn't it that flat disks flatten themselves by rotating? This is clearly not the case he there isn't enough time to do a lot of rotations. Probably. In which case your time-scale argument is irrelevant. Or I am miscalculating something? This huge structure must be more ancient than 2.75 rotations. Much more. Maybe 20, 30 rotations to flatten itself, at least! So why are you invoking the time-scale argument again? There was some discussion recently that it was unbelievable that voids could exist because it would take galaxies too long to clear out of them. But that is not how voids form. Rather, galaxies themselves formed elsewhere. Probably something similar applies here. |
#4
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How can that be?
Jacob said:
"Isn't it that flat disks flatten themselves by rotating? This is clearly not the case he there isn't enough time to do a lot of rotations. thin, with a perpendicular scatter 14.1 kpc (99% confidence)." Well, that is a factor of around 30... At only 150Kpc the rotation period is 5 billion years. Since the supposed "age of the Universe" this disk can at most have done 2.74 revolutions. But Andromeda did not exist right after the supposed big bang so it must be quite less than that. How can it be so flat? " Brad said: Isn't it that flat disks flatten themselves by rotating? This is clearly not the case he there isn't enough time to do a lot of rotations Prog. Theor. Phys. (1983) 70 (5): 1276-1282. doi: 10.1143/PTP.70.1276 Try this as a partial explanation for your question. In addition review other articles written by H Sato [Mod. note: please try to quote previous articles using the standard quoting character , and restrict lines to 80 characters. I have fixed the second of these but not the first in this posting -- mjh] |
#5
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How can that be?
As I mentioned in another thread, the disk of the satellite galaxies of
Andromeda is extremely thin: http://arxiv.org/abs/1301.0446 A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy From the abstract: "The structure is vast: at least 400 kpc in diameter, but also extremely thin, with a perpendicular scatter 14.1 kpc (99% confidence)." Well, that is a factor of around 30... At only 150Kpc the rotation period is 5 billion years. Since the supposed "age of the Universe" this disk can at most have done 2.74 revolutions. But Andromeda did not exist right after the supposed big bang so it must be quite less than that. How can it be so flat? Isn't it that flat disks flatten themselves by rotating? This is clearly not the case he there isn't enough time to do a lot of rotations. Or I am miscalculating something? This huge structure must be more ancient than 2.75 rotations. Much more. Maybe 20, 30 rotations to flatten itself, at least! Galaxy formation theories are still incomplete. IMO the problem is the Dark Matter paradigm. But, here are alternatives. Humitaka Sato coauthored several papers expanding on earlier work by Israel and generalizing the ideas of metric junctions between Schwatrzschild, deSitter spaces in matter dominated universe to explain the newly discovered Voids. See: Prog. Theor. Phys. (1983) 70 (5): 1276-1282. doi: 10.1143/PTP.70.1276 See: Prog. Theor. Phys. (1984) 71 (5): 938-945. doi: 10.1143/PTP.71.938 See: Prog. Theor. Phys. (1986) 76 (6): 1250-1259. doi: 10.1143/PTP.76.1250 He found that the growth of voids resulted in first a thin matter shell that denied ' crossover' of matter that kept voids comparatively devoid of matter that resulted in a "snowplow" effect that concentrated matter. It seems reasonable to add this process to the formation of matter structures so that he Flatness would be a result of constraints brought about by this division of the Universe into 2 distinct spacetime regimes. Brad [Mod. note: reformatted -- mjh] |
#6
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How can that be?
On 8/18/14, 7:18 AM, jacob navia wrote:
This huge structure must be more ancient than 2.75 rotations. Much more. Maybe 20, 30 rotations to flatten itself, at least! At several hundred z's, Galactic formation dimensions were much smaller with faster rotation imprinting the present visual display at z=0. |
#7
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How can that be?
Le 20/08/2014 15:43, brad a écrit :
Prog. Theor. Phys. (1983) 70 (5): 1276-1282. doi: 10.1143/PTP.70.1276 Try this as a partial explanation for your question. In addition review other articles written by H Sato No, that doesn't apply. That theory is speaking about the huge voids that happen to appear in the "foam" that seems to be the universe at larger scales. Thos voids are made of galaxies since *their absence* characterizes them. Galaxies group in filaments (or "rivers") of galaxies and are obviously much smaller than the filaments they build, that are made of several clusters of galaxies at their intersections. This web is like a condensation of matter in a foam. Galaxies are very small at this scales. Galactic structures can't be affected by forces acting at intra-cluster of bigger objects. And the scientist you cite is describing VOIDS as a consequence of some equations about the universe as a whole, nothing less. Not Andromeda's disk. With all due respect, I have the feeling that applying those very general equations to galactic scales is a mistake of several orders of magnitude. The temperature-constant expansion the scientist is speaking about tries to explain how this foam came to look like it looks today, not how the same expansion would yield a flat disk, a completely different outcome, at much smaller scales. But anyway it was a completely strange idea, this kind of "pressure" that would make the galaxies concentrate at the borders. A condensation process is, for instance, rain. When it rains, the condensation is directed and carried into rivers, i.e. *paths in the gravitational field*, that carry the product of the condensation away. It rains galaxies out there. And voids (like mountains) are avoided by the condensation product that is directed into rivers, that flow into clusters of galaxies. This was a powerful idea. Will those ponds of galaxies eventually overflow and fill some of the voids? After some unimaginable time? It was a nice article, thanks for your answer. |
#8
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How can that be?
In article ,
jacob navia writes: Isn't it that flat disks flatten themselves by rotating? If you are imagining mass that is originally in the center and then spreads out by centrifugal force, I don't know a single astronomical example of that. (I won't swear I'm not missing something.) More common is initially spherical collapse, where the collapse along one axis proceeds fairly rapidly and collapse in the perpendicular plane is greatly slowed by angular momentum or a magnetic field or both. Magnetic fields are likely to be important for star formation but probably not for galaxy formation, but I don't think either one is certain. -- Help keep our newsgroup healthy; please don't feed the trolls. Steve Willner Phone 617-495-7123 Cambridge, MA 02138 USA |
#9
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How can that be?
Le 22/08/2014 19:01, Steve Willner a écrit :
More common is initially spherical collapse, where the collapse along one axis proceeds fairly rapidly and collapse in the perpendicular plane is greatly slowed by angular momentum or a magnetic field or both. Magnetic fields are likely to be important for star formation but probably not for galaxy formation, but I don't think either one is certain. That sounds very plausible. The collapse along one axis proceeds fairly rapidly and kinetic energy is gained by the collapsing material in the direction of the collapsing axis. Obviously it will overshoot the central plane and at the other side, the same forces will make it stop and then reverse and fall in the other direction, where it will overshoot again (but less) the central disk. This will take a HUGE amount of time! We are speaking here about GALAXIES, and even for dwarf galaxies their movements are VERY slow. One revolution of that disk is 5GY. How much time a single damped oscillation will take is anyone guess, but several oscillations are SURELY required in my humble opinion. Relember: the galaxies are aligned with a form factor of around 30. 400 kpc diameter, 14 kpc thin. This structure is incredibly OLD, at least 50 GY or more. You have to align precisely all this galaxies in this rotating disk. And that takes an incredibly amount of time! |
#10
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How can that be?
On 8/26/2014 7:13 AM, jacob navia wrote:
We are speaking here about GALAXIES, and even for dwarf galaxies their movements are VERY slow. One revolution of that disk is 5GY. How much time a single damped oscillation will take is anyone guess, but several oscillations are SURELY required in my humble opinion. Relember: the galaxies are aligned with a form factor of around 30. 400 kpc diameter, 14 kpc thin. This structure is incredibly OLD, at least 50 GY or more. You have to align precisely all this galaxies in this rotating disk. And that takes an incredibly amount of time! So you're ignoring the possibility that they were closer together before the universe expanded this much, and therefore such a collapse would happen faster? [Mod. note: quoted text trimmed -- mjh] |
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