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And our galaxy is a spiral galaxy, in contrast to elliptical galaxies.sophiecentaur said:Why should they be devoid? These so-called spiral arms in our galaxy
And our galaxy is a spiral galaxy, in contrast to elliptical galaxies.sophiecentaur said:Why should they be devoid? These so-called spiral arms in our galaxy
The lack of arms says nothing about the orbits of the stars around a central attractor. An armless galaxy will presumably not have the appropriate density of stars to interact with each other and to have resonances to form waves. The arms are merely 'virtual' patterns of star density they are not spokes on a wheel.snorkack said:And our galaxy is a spiral galaxy, in contrast to elliptical galaxies.
It is the lenticular galaxies which are said to be like spirals, only without arms.sophiecentaur said:The lack of arms says nothing about the orbits of the stars around a central attractor. An armless galaxy will presumably not have the appropriate density of stars to interact with each other and to have resonances to form waves.
I found this link which discusses spiral, lenticular and elliptical galaxies in terms of their angular momentum and 'bulge factor'. It has references from the 1990s and later. Well done if you can read every word!snorkack said:It is the lenticular galaxies which are said to be like spirals, only without arms.
It is interesting that the elliptical galaxies do seem to rotate, without an obvious difference.sophiecentaur said:I found this link which discusses spiral, lenticular and elliptical galaxies in terms of their angular momentum and 'bulge factor'. It has references from the 1990s and later. Well done if you can read every word!
They have to orbit, but they do not have to orbit at similar rates.sophiecentaur said:The stars in other galaxies also orbit at similar rates - they would have to or collapse into the centre PDQ.
Their orbit period will relate to the mass distribution of the galaxy and the position of the star in question.snorkack said:they do not have to orbit at similar rates.
Is this surprising ? The Oort Cloud is spherical so a comet could (ignoring effects that I / we don't know about) have any orbital plane. The fact that the Oort Cloud is spherical must be to do with its great distance out from the Sun and planets and a lack of the influence of at disc. Comets originate in the cloud and are ejected from time to time as the interactions with the rest of the cloud produce just the right conditions. We will only see bodies which happen to get close enough but I imagine there could be loads of them with orbits way beyond Pluto and some could even end up in deep(er) space.snorkack said:When you look at comets, it turns out that their inclinations are not limited to the 7 degrees of the 7 planets.
If it didn't, it would fall inwards. Same rules apply with gravity and orbits.snorkack said:Does Oort cloud rotate?
No I think snork's clarification is valid:sophiecentaur said:If it didn't, it would fall inwards. Same rules apply with gravity and orbits.
I don't see why the Oort Cloud as a whole has to have a net preferred rotation. I can see why it might, but if it didn't, it wouldn't, as you say, fall inwards.snorkack said:That is, when you make a statistic of long period comets, is the number of retrograde comets within the limits of coincidence equal to that of prograde comets, or is there any perceptibly preferred direction?
Perhaps the net polar component of the angular momentum of the cloud is in the same direction as the rest of the SS but could it be that outside influences (from no preferred direction) could have injected am, not about the common axis? The Oort objects are very far away and far apart so some different rules or timescale could apply.DaveC426913 said:No I think snork's clarification is valid:
I don't see why the Oort Cloud as a whole has to have a net preferred rotation. I can see why it might, but if it didn't, it wouldn't, as you say, fall inwards.
Why must there be a significant net rotation at all? (I don't mean zero; I mean not statistically significant.)sophiecentaur said:Perhaps the net polar component of the angular momentum of the cloud is in the same direction as the rest of the SS but could it be that outside influences (from no preferred direction) could have injected am, not about the common axis?
Good point. I was sort of assuming that the original nebula would have a uniform net AM. But if OoC is far enough out then could its behaviour be isolated from the SS is some way? Obviously there's a strong enough attraction to keep it near the Sun and SS but the large gap between them that the subtle changes in energy that produced the planets and the asteroid belt etc. may be too weak at that great distance. I sort of hinted at this, further up.DaveC426913 said:Why must there be a significant net rotation at all? (I don't mean zero; I mean not statistically significant.)
Imo, there would not be much to select either group to interact with the SS. Why not relate to to relative numbers of each? That Noddy theory at least agrees with observation.DaveC426913 said:I'm just not sure which group would get disturbed faster: pro-grade bodies or retrograde bodies.
Well, except that they do, occasionally.sophiecentaur said:Imo, there would not be much to select either group to interact with the SS.
That term is unfamiliar to me. I find references to a real event, but I don't know how it translates into a metaphor.sophiecentaur said:That Noddy theory...
It was my noddy theoryDaveC426913 said:That term is unfamiliar to me.
Exactly. At such a distance - well on the edge of the first order gravitational effects of the SS (only enough to keep the cloud in place but not to form a disc)- the other effects due to the larger planets would be even less but perhaps enough to affect the direction of things observed / select coming out of the Ooc.DaveC426913 said:Well, except that they do, occasionally.
Incidentally, while it is very easy to piece together an argument that most galaxies should have angular momentum, the scaling relations discussed in the linked paper, which are very regular, are harder to explain and require a much more involved model than the bare bones ones offered up in this thread.sophiecentaur said:I found this link which discusses spiral, lenticular and elliptical galaxies in terms of their angular momentum and 'bulge factor'. It has references from the 1990s and later. Well done if you can read every word!
Imo, it's important to understand that spiral arms are not like spokes on a wheel and they don't rotate 'in step' with the individual stars' orbits. The stars in other galaxies also orbit at similar rates - they would have to or collapse into the centre PDQ.
That sums up what we would be after. The 'why' question is never very fruitful. All we can say we know is that there is unlikely, ever, for the component parts of a nebula to have net zero angular momentum. So you have your input spin from the very beginning and it is all about the statistics of many body interactions.Mendrys said:This is new and describes other processes that contribute to the spin of a galaxy.