B Why don't galaxies obey gravity?

[Wallsy]

Hi all,my second question is this.Why don't galaxies obey gravity? In our solar system the closer to our sun the planet is the faster it rotates.So the outer planet takes much longer for a solar year.
When we look at galaxies this gravitational law doesn't apply.The outside stars spin at the same rate as the inside stars.
My question is why?

 

[davenn]

In our solar system the closer to our sun the planet is the faster it rotates.So the outer planet takes much longer for a solar year...When we look at galaxies this gravitational law doesn't apply.The outside stars spin at the same rate as the inside stars.

where did you get that idea from ?, please show a link

also you cannot compare the simple planetary orbital velocities around their parent star, with the more complex orbital systems of star around their parent galaxy
they are very different

there is plenty of info on the net that disproves it

here's just one ...

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

 

[phinds]

Hi all,my second question is this.Why don't galaxies obey gravity? In our solar system the closer to our sun the planet is the faster it rotates.So the outer planet takes much longer for a solar year.
When we look at galaxies this gravitational law doesn't apply.The outside stars spin at the same rate as the inside stars.
My question is why?

Dark Matter, and of course they DO obey gravity, it's just that there is a different distribution of matter in the galaxy than in the solar system.

 

[rootone]

My question is why?

Because it only makes sense if some kind of invisible matter exists. which has mass like normal matter, but does not interact with it other than through gravity.
There are numerous experiments ongoing to detect what it might be, best guess at present is some kind of supersymmetric particle.
You may well say as others have, well maybe our understanding of gravity is incorrect.
So far though speculation of modified gravity has been fruitless, nobody has produced a theory which explains GR, yet also includes a 'dark' component.

 

[Wallsy]

My mind says our understanding of gravity is spot on.Our understanding of galaxies isn't.Thinking outside the box-Maybe black holes aren't sucking in planets and stars but spitting them out?Creating stars?

 

[rootone]

My mind says our understanding of gravity is spot on.Our understanding of galaxies isn't.Thinking outside the box-Maybe black holes aren't sucking in planets and stars but spitting them out?Creating stars?

You will not get far with alternative cosmnology here unless you have data

 

[phinds]

My mind says our understanding of gravity is spot on.Our understanding of galaxies isn't.Thinking outside the box-Maybe black holes aren't sucking in planets and stars but spitting them out?Creating stars?

This is nonsense. Thinking outside the box only works well when you first understand what's IN the box.

 

[Janus]

My mind says our understanding of gravity is spot on.Our understanding of galaxies isn't.Thinking outside the box-Maybe black holes aren't sucking in planets and stars but spitting them out?Creating stars?

1. The dark matter hypothesis is based on the idea that our understanding of gravity is correct and thus, if the matter we can see doesn't have enough mass to produce the gravity needed to hold galaxies from flying apart, then there is matter that we can't see that is providing that extra mass and gravity.

2. Black holes spitting out stars would be contrary to our understanding of gravity and thus this suggestion conflicts with your first sentence.

3. How would black holes producing stars explain the observations we have made about galaxies?

 

[Mike Holland]

I have just been re-reading "Stars in the Making" by Cecelia Payne-Gaposchkin. I first read it in my teens, about 1960. The book is way out of date, and her claims may no longer be correct, but she says that the visible matter in the spiral arms and core of the galaxy accounts for only 1-10% of the mass of the galaxy, and that the balance is in the globular star clusters and high-speed stars that form a (mostly invisible to us) sphere. I.e. our galaxy is spherical with just a tiny sliver across the middle where the gas, new-born bright stars and spiral arms are.

All the write-ups on stellar motion in the galaxy refer to the distribution of the visible matter. They seem to ignore most of the matter of the galaxy. If we take into account that the stars are in a great sphere of matter rather than a disc, then we would get a much flatter velocity curve. If the sphere was of uniform density (which of course it isn't), then the gravity would fall off as the inverse of the radius instead of its square! Do we really need dark matter to explain the observed curves?

 

[phinds]

I have just been re-reading "Stars in the Making" by Cecelia Payne-Gaposchkin. I first read it in my teens, about 1960. The book is way out of date, and her claims may no longer be correct, but she says that the visible matter in the spiral arms and core of the galaxy accounts for only 1-10% of the mass of the galaxy, and that the balance is in the globular star clusters and high-speed stars that form a (mostly invisible to us) sphere. I.e. our galaxy is spherical with just a tiny sliver across the middle where the gas, new-born bright stars and spiral arms are.

All the write-ups on stellar motion in the galaxy refer to the distribution of the visible matter. They seem to ignore most of the matter of the galaxy. If we take into account that the stars are in a great sphere of matter rather than a disc, then we would get a much flatter velocity curve. If the sphere was of uniform density (which of course it isn't), then the gravity would fall off as the inverse of the radius instead of its square! Do we really need dark matter to explain the observed curves?

Mike, do you seriously think that something this obvious has been overlooked by thousands (probably 10's of thousands) of scientists?

 

[stoomart]

1. The dark matter hypothesis is based on the idea that our understanding of gravity is correct and thus, if the matter we can see doesn't have enough mass to produce the gravity needed to hold galaxies from flying apart, then there is matter that we can't see that is providing that extra mass and gravity.

Is there a macroscopic concept of "binding energy" for galaxies, along the same lines as atoms having more mass than the sum of their constituents, or mass defect?

 

[Janus]

Is there a macroscopic concept of "binding energy" for galaxies, along the same lines as atoms having more mass than the sum of their constituents, or mass defect?

The binding energy is due to the forces holding the atom together. The force holding the galaxies together is gravity (we have no evidence of any other significant binding forces.) Gravity is the weakest of the known forces. So if you are asking whether or not the binding energy of the gravity itself is enough to generate a mass defect large enough to make up for the "missing mass", then no, not by a long shot.

If you are thinking of a different "binding energy", what force would provide it? Why have we never noticed it? And any force capable of producing a large enough mass defect to make up for the missing mass would have to be so strong that in of itself it would capable of holding the galaxy together many times over, rather than having to rely on the mass defect it produced. (in fact it would be so strong that we would be wondering why galaxies don't collapse in on themselves rather than why they don't fly apart.)

 

[stoomart]

The binding energy is due to the forces holding the atom together. The force holding the galaxies together is gravity (we have no evidence of any other significant binding forces.) Gravity is the weakest of the known forces. So if you are asking whether or not the binding energy of the gravity itself is enough to generate a mass defect large enough to make up for the "missing mass", then no, not by a long shot.

If you are thinking of a different "binding energy", what force would provide it? Why have we never noticed it? And any force capable of producing a large enough mass defect to make up for the missing mass would have to be so strong that in of itself it would capable of holding the galaxy together many times over, rather than having to rely on the mass defect it produced. (in fact it would be so strong that we would be wondering why galaxies don't collapse in on themselves rather than why they don't fly apart.)

My understanding is gravity is a non-factor at the quantum scale because it is simply too weak, hence why we have nuclear forces; I suspect a similar case at galactic scales, but I don't want to start coming up with personal theories. This excerpt from the wiki article in my last post is what got me thinking about this:

The nuclear force must be stronger than the electric repulsion at short distances, but weaker far away, or else different nuclei might tend to clump together. Therefore, it has short-range characteristics. An analogy to the nuclear force is the force between two small magnets: magnets are very difficult to separate when stuck together, but once pulled a short distance apart, the force between them drops almost to zero.​

 

[Mike Holland]

Phinds, here is a quote from Wikipedia -
"When mass profiles of galaxies are calculated from the distribution of stars in spirals and mass-to-light ratios in the stellar disks, they do not match with the masses derived from the observed rotation curves and the law of gravity."
Whoever wrote that had no concept of the sphere of matter surrounding our galaxy (and presumably other galaxies). I have not found a single write-up on the rotation curves and dark matter that refers to the 90% of the mass outside the plane of the spirals. Or was Cecelia's estimate totally wrong?

 

[Janus]

My understanding is gravity is a non-factor at the quantum scale because it is simply too weak, hence why we have nuclear forces; I suspect a similar case at galactic scales, but I don't want to start coming up with personal theories. This excerpt from the wiki article in my last post is what got me thinking about this:

The nuclear force must be stronger than the electric repulsion at short distances, but weaker far away, or else different nuclei might tend to clump together. Therefore, it has short-range characteristics. An analogy to the nuclear force is the force between two small magnets: magnets are very difficult to separate when stuck together, but once pulled a short distance apart, the force between them drops almost to zero.​

But again, we have no reason to suspect any type of short range force on the galactic scale to provide this binding energy. But let's use the nuclear binding energy model. For a uranium atom, the total mass defect amounts to less than 1% of the total mass, of the atom. But with galaxies, the missing mass isn't equal to just a tiny fraction of the mass of the visible matter, but more than it. So what makes more sense? To hypothesize some unknown short range force that is capable of making up that much mass in the form of binding energy ( which, by the way, would not solve the rotation curve problem. It isn't just how fast the stars orbit, it is also how those orbital speeds change as you move outward from the center. Assuming a short range force at the galactic center would mean that there is where the mass defect mass would be, and the orbital speeds would behave like those of our solar system.). or that there is some form of matter that is not detectable by electromagnetic radiation that is providing that extra mass (considering that we already know of 1 particle that fits this bill, the neutrino)?

 

[Janus]

Phinds, here is a quote from Wikipedia -
"When mass profiles of galaxies are calculated from the distribution of stars in spirals and mass-to-light ratios in the stellar disks, they do not match with the masses derived from the observed rotation curves and the law of gravity."
Whoever wrote that had no concept of the sphere of matter surrounding our galaxy (and presumably other galaxies). I have not found a single write-up on the rotation curves and dark matter that refers to the 90% of the mass outside the plane of the spirals. Or was Cecelia's estimate totally wrong?

The point isn't that the mass providing the observed rotation curves isn't spread out in a sphere surrounding the center of the Galaxy,( if fact , DM is based on this assumption, it is that this mass could be made of regular baryonic matter, and remain undetectable at with any wavelength of the electromagnetic spectrum. If that mass where made up of ordinary matter, we would see it.

 

[Mike Holland]

I don't know how one would determine the spread of dark matter vertical to the plane of the galaxy by observing the movement of stars in the plane of the galaxy. But there is an awful lot of matter that is spread out in a sphere, about 90% according to Cecelia, and this matter would certainly flatten the velocity/distance curves to some degree.

Is Cecelia;'s estimate still valid, or have more recent X-ray surveys etc given a different view of the matter distribution of the spiral galaxy and surrounding stars and clusters? I have read dozens of books on Astronomy, and subscribe to New Scientist, but have never seen any other mention that the spiral arms and visible stars are just a small part of our galaxy. The halo of globular clusters is commonly mentioned, but never its contribution to the total mass of the galaxy.

 

[UsableThought]

I have read dozens of books on Astronomy, and subscribe to New Scientist, but have never seen any other mention that the spiral arms and visible stars are just a small part of our galaxy. The halo of globular clusters is commonly mentioned, but never its contribution to the total mass of the galaxy.

Although I'm a big fan of books as opposed to online reading, I often Google for specific questions, given that web searches are both far broader & far more specific than is possible with hard-copy books and magazines. I think that would be helpful in your case also.

Indeed, a search for +'Globular cluster' +'dark energy' +'halo' pulls up what seem to be quite relevant hits; for example here is a 2015 study titled "Dark Matter Halos in Galaxies and Globular Cluster Populations. II: Metallicity and Morphology":

https://arxiv.org/abs/1504.03199

The study starts off like this:

A remarkably simple empirical correlation has emerged between two global properties of galaxies that belong to early phases of galaxy formation: these two quantities are $M_h$ (the total halo mass of a galaxy including all visible and dark matter in its potential well); and $M_GCS$ (the total mass in its globular cluster system).​

Of course a study like this is narrowly technical; but even at a glance it seems to speak to the point of whether scientists interested in dark matter had somehow forgotten about either globular clusters or the galactic halo.

 

[Mike Holland]

Thanks, UseableThought. I will study those links.

 

[Janus]

I don't know how one would determine the spread of dark matter vertical to the plane of the galaxy by observing the movement of stars in the plane of the galaxy. But there is an awful lot of matter that is spread out in a sphere, about 90% according to Cecelia, and this matter would certainly flatten the velocity/distance curves to some degree.

Is Cecelia;'s estimate still valid, or have more recent X-ray surveys etc given a different view of the matter distribution of the spiral galaxy and surrounding stars and clusters? I have read dozens of books on Astronomy, and subscribe to New Scientist, but have never seen any other mention that the spiral arms and visible stars are just a small part of our galaxy. The halo of globular clusters is commonly mentioned, but never its contribution to the total mass of the galaxy.

In this link, they estimate the mass of the stellar halo as being between 1e8 and 1e9 solar masses:
http://burro.astr.cwru.edu/Academics/Astr222/Galaxy/Structure/halo.html
Fairly recently, a study has calculated the total galactic mass out to 600,000 ly as being between 6e12 and 7.5e12 solar masses.
http://www.skyandtelescope.com/astronomy-news/new-mass-estimate-milky-way/
Even we take the high end mass estimate for the halo and the low end estimate for the total, the halo would represent just 1/600 of this total galactic mass.(DM included.)

The estimated luminous mass for the galaxy is ~9e10 solar masses, of which the stellar halo would contribute ~1.11% to the total.

 

[stefan r]

The halo of globular clusters is commonly mentioned, but never its contribution to the total mass of the galaxy.

This paper might be helpful. They are claiming that globular clusters and supermassive black holes in a galaxy have similar mass. If we take Andromeda as an example the galaxy has mass 1.5x10¹² and the SMBH is 1.4x10⁸ solar mass. Less than 10^-4 contribution to mass would make the globular cluster mass much less than the error in the measurement of galaxy mass. For example here they list the ratio of Milky Way to Andromeda as between 0.37 and 0.77.
Compare to insects in a forest. The butterflies and fireflies are very noticeable, interesting, and biologically important. You would not bother weighing them if you tried to measure the weight of the biomass in a hectare using a primitive scale.

Edit: or what Janus said while I was out to lunch. Notice the difference between his link and wikipedia. All of the globular cluster mass disappeared a few hundred times with a new measurement.

 

[OnlyMe]

Hi all,my second question is this.Why don't galaxies obey gravity? In our solar system the closer to our sun the planet is the faster it rotates.So the outer planet takes much longer for a solar year.
When we look at galaxies this gravitational law doesn't apply.The outside stars spin at the same rate as the inside stars.
My question is why?

Apologizing in advance for a long, drawn out and perhaps at times redundant and confusing, attempt to question a potential previously unaddressed contribution to the issue being raised in the OP... And without attempting to suggest this is an answer.., or even valid issue, treat the following more as a question of whether frame dragging itself has any persistent affect on spacetime, that might contribute to the observed dynamics at issue in the OP.

Without comment on the unchallenged accuracy of the above statement (I am sure a confusing qualifier), even accepting that stars distant from the center of a galaxy, orbit the galactic center at velocities which seem too exceed orbital velocities predicted from a strictly Newtonian view of gravity, even an initial evaluation within the context of general relativity, a question that has puzzled me from some time has been, how might the frame dragging effect of a mature gravitational system affect the observed orbital velocities, when the system as a whole is being evaluated/observed from a frame of reference external to the, in this case galaxy? Is the affect of frame dragging on spacetime itself persistent?

The issue being we observe the orbital velocities of stars relative to a galactic center from outside the involved gravitational system. At the same time we have very little mature information about just what the affect of frame dragging in all of its manefestaions would have on the dynamics of the curvature of spacetime associated with the galaxy as a whole.

From a frame of reference outside the galactic gravitational system, we cannot distinguish the difference between what portion of a specific star's orbital velocity is the result of a frame dragging effect of the involved spacetime, which would be unobservable from within the galactic system and how much is actually equivalent to the gravitational dynamics we observe and understand when we plot out the orbits of planets in a solar system.. where the frame dragging effect on spacetime is either relatively insignificant or unobservable.

.. How much of the observed velocities of stars near the outer reaches of a galaxy is due to the fact that spacetime itself is also rotating with the galaxy. Keep in mind that while we have with the Gravity Probe B experiment (and others) verified frame dragging associated with the angular momentum of both the Earth and the sun, there is also an as yet (directly) unverified predicted linear frame dragging and that, we as yet have no understanding that demonstrates whether either or both aspects of the frame dragging effect have persistent affects on spacetime.

If spacetime itself orbits a galaxy, any affect it has on the velocity of a star's orbit, when observed from a frame of reference outside of the galactic gravitational system, would be indistinguishable from a planet's orbital velocity absent the contribution which might be attributed to the orbiting spacetime. And if spacetime itself orbits the galaxy, at least some portion of its orbital velocity would have no influence on the gravitational dynamics governing the orbits of any massive object within the galactic system. Basically we have two frames of reference; one external to the galactic system where any orbital dynamics/velocity of the involved spacetime as a whole is observable and one from within the galactic system where any orbital dynamics of spacetime as a whole, would be unobservable and have no affect on the gravitational interaction between the involved gravitational masses.., within the galactic system?

 

[stefan r]

the gravitational dynamics we observe and understand when we plot out the orbits of planets in a solar system.. where the frame dragging effect on spacetime is either relatively insignificant or unobservable.

A 1 stellar mass black hole's gravity will effect an object at 1 au distance the same as the sun effects earth. The LARES satellite was launched in order to observe the Earth's frame dragging.

 

[OnlyMe]

A 1 stellar mass black hole's gravity will effect an object at 1 au distance the same as the sun effects earth. The LARES satellite was launched in order to observe the Earth's frame dragging.

I understand what you are talking about. I followed the GP-B experiment very closely. What I was intending to suggest or question was whether frame dragging effect has a persistent dynamic effect on spacetime itself... This would probably be more significant where linear frame dragging is involved. Essentially questioning whether the fact that massive objects have been orbiting the galactic center of mass for long enough that spacetime itself would acquire some associated angular momentum. from within the galactic system the acquired orbital like momentum of the involved spacetime would be transparent to unobservable. While from outside the galactic system an observer would see orbital velocities that include a velocity as predicted by both Newtonian mechanics and/or general relativity and an added angular momentum or orbital velocity associated with the involved galactic spacetime.

While frame dragging as demonstrated by the GP-B experiment is a measure of the affect on massive objects. It suggests an underlying affect on spacetime itself. Frame dragging associated with the rotation of a massive gravitationally significant object is accepted as having been proven to exist and suggests that the predicted linear form of frame dragging, which has not been observed, should also exist. The question then becomes, does frame dragging in either or both forms have a persistent affect on spacetime. Meaning does the effect of frame dragging on spacetime, cause spacetime to acquire over time some angular (or obital) momentum of its own? If this does happen it would be observable by an outside observer as orbital velocities greater than would be predicted, based on our generally localized experience of gravity.

 

[ddjj77]

I thought that gravity doesn't exist, and what we call gravity is the distortion of space by matter.

 

[rootone]

I thought that gravity doesn't exist, and what we call gravity is the distortion of space by matter.

So it exists!

 

[phinds]

I thought that gravity doesn't exist, and what we call gravity is the distortion of space by matter.

Yes, and the distortion of space-time is called ... wait for it ... "gravity".

 

[mfb]

Just to add some numbers:
In our solar system, 99.9% of the total mass is in the center, the Sun. Everything orbits the Sun.
In our galaxy, the central black hole has 0.001% of the total mass of the galaxy. There are some stars directly orbiting it at very fast speeds, but clearly the overall situation is completely different. Most stars orbit "the rest of the galaxy". The mass inside their orbit depends on the radius, so we get a different distance to orbital velocity relation.

 

[OnlyMe]

Just to add some numbers:
In our solar system, 99.9% of the total mass is in the center, the Sun. Everything orbits the Sun.
In our galaxy, the central black hole has 0.001% of the total mass of the galaxy. There are some stars directly orbiting it at very fast speeds, but clearly the overall situation is completely different. Most stars orbit "the rest of the galaxy". The mass inside their orbit depends on the radius, so we get a different distance to orbital velocity relation.

mfb, this is a good point, both to the original OP's question, where it leads to introduction of Dark Matter (or sometimes less popular ideas) to explain the orbital velocities observed for objects near the outer edges of galactic systems.., and to my question about the possibility that there might be a persistent affect on the spacetime associated with a galaxy and the frame dragging effect...

Under most conditions it does not matter whether the mass, say inside the orbit of our solar system, is spread out or consolidated into a single object, when we predict the gravitational influence of that mass. Add frame dragging and again if one treats the total mass as a single object nothing changes, because all of the associated frame dragging would be associated with the axial spin of a hypothetical object at the center of mass.., and that effect would drop off at the same rate as the influence of gravitation itself. The issue is different when, the total mass is spread out, as is the case, you pointed out above, because when the mass is spread out there would also be a linear frame dragging effect associate with the orbital motion of each individual massive object involved. And the question remains is the frame dragging effect that a massive object has on the dynamics of spacetime persistent? Maybe even cumulative over time?

From inside the glaxtic system an object that is essentially coasting with the resulting orbital motion of the involved spacetime, would fall into the galactic center of mass. Any orbiting object would have to have an orbital velocity in addition to the orbital component of the involved spacetime, to maintain any kind of stable galactic orbit... And from inside the galactic orbital component of the involved spacetime would be transparent or unobservable, while to an outside observer the orbital velocity of an object orbiting the galactic center would consist of both the object's intrinsic orbital velocity and the orbital component of the involved spacetime itself.

I am not attempting to present this as an answer to the question raised in the OP. The generally accepted presence of Dark Matter, is the explanation for otherwise unexplained orbital velocities. Still, ever since the early days of the published results of the GP-B experiment, I have wondered whether frame dragging might have a persistent affect on the dynamics of spacetime, which might at least in part affect the orbital velocities in question and perhaps a few other problematic and as yet unexplained observations.

I am unsure that anyone really has an answer. Still I wonder.

 

[mfb]

Frame dragging is completely negligible on the scale of galaxies.

 

[BenAS]

Frame dragging is completely negligible on the scale of galaxies.

I'm not sure if I should start a new thread, being this is a "b" level thread. I'm curios as to how this is calculated, on a about "I" level is about all I will be able to understand.

 

[mfb]

Frame-dragging scales with (gravitational constant)*(angular momentum)/(2*(radius)³*(speed of light)²). For a satellite in low Earth orbit, you get 10^-14/s - this leads to a frame-dragging effect of about 1/100,000 of a degree per year, measurable only with extremely sensitive satellites. For our galaxy, you get 10^-25/s, 11 orders of magnitude weaker.

 

[stefan r]

to an outside observer the orbital velocity of an object orbiting the galactic center would consist of both the object's intrinsic orbital velocity and the orbital component of the involved spacetime itself.

The observed deviation is the opposite. Particles in the outer galaxy are moving too fast.

 

[OnlyMe]

The observed deviation is the opposite. Particles in the outer galaxy are moving too fast.

Moving too fast yes, as seen from an outside observer. Opposite to what I was saying no.

If the spacetime associated with a galaxy is itself orbiting the galaxy, to an outside observer a particle (or massive object) would appear to have an orbital velocity that is the product of the "orbital" velocity of the involved spacetime and the orbital velocity that would be predicted based on either Newtonian dynamics or general relativity.., because from inside a galaxy, any orbital velocity of the spacetime within the galaxy, would be observable only within the context of its frame dragging affect... and even then almost certainly were dealing with two body interacts.

The point or question is/was, if the spacetime within a galaxy does orbit the galaxy, from within the galaxy it would be dynamically flat and unobservable. It would not add to the basic gravitational interaction of objects inside the galaxy (except as it involves frame dragging). Nor would it create any centrifugal like effect. An object moving moving with the dynamic motion of spacetime, would be essentially at rest realize to the dynamics of that spacetime. That is from within the fish bowl so to speak. Staying within the fish bowl analogy, spacetime would be the water in the bowl and a star in the galaxy a fish. The fish cannot know there is any current in the water without a frame of reference outside the flow of the current... a swimmer caught in a riptide does not know or feel that they are being swept out to sea and they don't experience it more difficult to swim in any direction, a scent an outside frame of reference.

Might a portion of the too fast orbital velocity distant from a galactic center be in part due to the current (the orbit of spacetime) and in part due to the actual orbital velocity of the object?

Frame-dragging scales with (gravitational constant)*(angular momentum)/(2*(radius)³*(speed of light)²). For a satellite in low Earth orbit, you get 10^-14/s - this leads to a frame-dragging effect of about 1/100,000 of a degree per year, measurable only with extremely sensitive satellites. For our galaxy, you get 10^-25/s, 11 orders of magnitude weaker.

I don't believe your above comment can be applied to the question. It is a two body solution to a massively multi body problem. If you were addressing the interaction between two galaxies it would be a close approximation, as close as we can get at present. But the mass in a galaxy is spread out and for most individual stars or solar systems within the galaxy the curvature of spacetime is affected by a distribution of mass both inside and outside its galactic orbit. It also seems to address only that aspect of frame dragging associated with the axial rotation of a gravitationally significant object, again not well suited to attempting to understand the frame dragging affects of multi body systems. Additionally, my original question relied more on how the predicted linear form of frame dragging might affect the dynamics of spacetime and whether there might be some persistent or even cumulative dynamic affect on spa time associated with the linear frame dragging, of all of the objects in a galaxy over time. (Time here being billions of years.)

And again I am unsure anyone has an answer to the question at present. We have only just begun to dip our toes into the weak field implications of frame dragging associated with gravitationally significant rotating objects. Even there our current experimental data is based on the Earth and the sun both of which have significant gravitational and magnetic fields. Do we need to repeat experiments where the the planet or moon our test satellite orbits has no magnetic field?

 

[mfb]

@OnlyMe: It is an order of magnitude estimate, a factor 2 more or less doesn't matter.

Can we please keep 10^-20 effects of general relativity out of a [B]-level thread? It is beyond the scope, and it is utterly negligible anyway.

 

[BenAS]

@OnlyMe: It is an order of magnitude estimate, a factor 2 more or less doesn't matter.

Can we please keep 10^-20 effects of general relativity out of a [B]-level thread? It is beyond the scope, and it is utterly negligible anyway.

So I think what he's asking about (I've been thinking about it also, which is why I asked about the math. Thanks btw) is wether or not spacetime can "rotate" around a galaxy. This would be in addition to the frame dragging. I figure people smarter than me (Not a high bar) have considered this. It seems it could change the expected orbital velocity of stars.

 

[OnlyMe]

So I think what he's asking about (I've been thinking about it also, which is why I asked about the math. Thanks btw) is wether or not spacetime can "rotate" around a galaxy. This would be in addition to the frame dragging. I figure people smarter than me (Not a high bar) have considered this. It seems it could change the expected orbital velocity of stars.

mfb is right in pointing out that my question and discussion is beyond the scope of a B level thread. Perhaps even an A level discussion.