Any system of randomly moving particles will likely have a small residual angular momentum. As the system collapses (e.g., under its own gravity, such as when a galaxy or a solar system forms), conservation of angular momentum causes it to rotate faster. Associated with this rotation is the plane in which the rotation takes place. Due to mutual interactions of the particles in the system (especially when gas and dust are present so the interactions are not purely gravitational), motion that is perpendicular to the plane of rotation tends to be dampened; the overall rotation, however, remains constant because once again, angular momentum is conserved. As a result, over a long period of time the system tends to flatten out.
For a more detailed explanation, see, for instance, http://physics.stackexchange.com/questions/25950/why-are-some-galaxies-flat
Any system of randomly moving particles will likely have a small residual angular momentum. As the system collapses (e.g., under its own gravity, such as when a galaxy or a solar system forms), conservation of angular momentum causes it to rotate faster. Associated with this rotation is the plane in which the rotation takes place. Due to mutual interactions of the particles in the system (especially when gas and dust are present so the interactions are not purely gravitational), motion that is perpendicular to the plane of rotation tends to be dampened; the overall rotation, however, remains constant because once again, angular momentum is conserved. As a result, over a long period of time the system tends to flatten out.
For a more detailed explanation, see, for instance, http://physics.stackexchange.com/questions/25950/why-are-some-galaxies-flat
Charles, I don't think Sanjit's question was about the large-scale alignment. Perhaps I misunderstood but I think he was simply wondering about why planets in the solar system all orbit in roughly the same plane, or why stars in the Milky Way all orbit in roughly the same plane, not how the rotation planes of distant galaxies may statistically align.
Still, gravitational collapse within an amorphous gas cloud commonly produces protoplanetary disks - It seems that inertial rotation must be fundamental to the process of collapsing particles...
The "statistical" argument is that if you have a large loose collection of co-orbiting matter with a net angular momentum around its common centre of gravity, then over a large period of time that angular momentum will tend to be shared and smeared and averaged out amongst the orbiting material by collisions and gravitational flybys. It's a "road traffic" problem - if any matter is moving through the cloud too fast, or too slow, or in the wrong rotation plane (or in the opposite direction!), then it'll have an increased rate of collisions and gravitational interactions that will keep changing its orbit. The lowest rate of orbit-changing collisions and flybys happens when everything is rotating in step with its neighbours (or as close as can be achieved bearing in mind orbital mechanics), so that tends (statistically) to be the end result. Ish.
If the disc is a thick disc then it'll tend to collapse to form a thinner disc, because there's no obvious forces to keep it "fat" to counteract gravitational effects perpendicular to the plane. Anything that orbits slightly out of the plane, but sharing a common centre of gravity with the rest of the material will have to cross the plane twice per orbit, again with a greater chance of having it's orbit changed by a collision or gravitational flyby each time that it crosses.
However, much further away from the centre of the solar system, we reckon that there's something called the Oort Cloud, at a distance of maybe 2000 to 5000 times the distance of the Earth from the Sun. This is reckoned to be pretty much spherical, with its bodies orbiting pretty much any which way - however, the cloud must be sufficiently rarefied, with the rate of collisions and gravitational interactions so small, that it's never had the need to establish a more orderly "one way system". Come back in a zillion zillion zillion years, and perhaps you might find that the Oort cloud has settled down into a co-rotating disk, too.
We assume that the Oort Cloud exists because of the occasional icy comets that come into the solar system at crazy angles that take them reasonably close to the Sun. We know that at least some of these are orbiting (like Halleys), but we also know that they seem to only be able to make a limited number of passes before evaporating, so somewhere out there there should be a reserve of icy objects orbiting far from the Sun that occasionally throws something our way after an interaction, so that the supply of fresh orbiting comets is kept "topped up" (otherwise there probably wouldn't be enough of them left by now for us to notice).
There is a report of a study of rotation in >15,000 spiral galaxies in the Sloan Digital Sky Survey (SDSS) data (mostly in the Northern hemisphere) that found a 7% excess of 'counter-clockwise' rotation (I think this also implies some preference in orientation). See http://physicsworld.com/cws/article/news/2011/jul/25/was-the-universe-born-spinning.
However, a subsequent study of the SDSS data evaluating the rotation of >125,000 spiral galaxies found that their rotational preference depends on their position within the sky - potentially indicating a universal spin orientation! See http://astrobites.org/2012/07/24/is-god-right-handed-spiral-galaxies-rotation-and-isotropy/ - it provides links to several other studies with somewhat similar findings. I cringe at the title, however...
James, the Shamir study is very interesting. Thanks for the link. In my own meager observations, I also saw a higher degree of right-handed rotation. The question is why this is so.
Yes - No one can definitively answer that question yet, but the simplest conjecture would be that the initial universe was spinning. I also wonder if a spinning universe might very directly explain some initial preference for the condensation of matter rather than antimatter...
As I understand, the motions of all rotating objects is determined by the net influence of gravitational and centrifugal effects. Even objects at the periphery of galactic disks are affected not only by centrifugal effects resulting from their rotational velocities, but their gravitational bindings with billions of comparably massive neighboring objects.
Unfortunately, most evaluations consider only their gravitational attraction to a collective center of mass, which seems surprisingly insufficient to prevent their expulsion from the disk. This leads to the misconception that some undetected mass must be contributing to the gravitational potential of the 'virtual' central point mass - to prevent expulsion resulting from high velocity centrifugal effects...
As for the idea that:
"In our galaxy, the position of our Solar system is in a fortunate location about 3/5 ths of the way from the center to the outside. This is the quiet zone where material is neither moving toward the center, nor moving toward the perimeter, so the number of collisions between objects of differing sizes is greatly reduced, because the difference between rotational velocities of objects about the galactic center is diminished."
The rotational velocity of objects at the same radius from a central mass would vary _only_ if the masses were significantly different _and_ were significant in relation to the mass of the idealized central object (m1+m2 for each planetary orbital was significantly different from the other). In all cases of disk objects, it's considered that each orbital's mass can be disregarded in evaluating gravitational effects since it is so much smaller than the idealized collective mass (improperly) represented by m1.
However, galaxy disks are not independently orbiting planetary systems - actually, locally bound components of the disk interact, rotating collectively, at nearly identical speeds.
Yes - at least to the extent that I can follow. I guess it takes engineering or information analysis experience to recognize that galactic scale (and greater) objects are compound structures that can't be properly represented as simplistic two-body mass distributions!
I really don't do math, but as I understand, the fundamental issue in classical treatments of galaxy gravitation is that, in a network of interacting bodies, the gravitational force imparted by each body to a subject body is determined not only by its distinct mass, but also by (the inverse square of) its distinct separation distance from the subject!
As I understand, galactic evaluations commonly represent a vast distribution of bodies by a simple aggregation of its mass and a single separation distance (r). There is no attempt to approximate the non-linear effect of varying separation distances. As a result, the estimated mass required to produce observed rotational velocities - at a separation distance equal to the subject's radial distance - is far greater than if a significant portion of the distributed mass was evaluated at its actual separation distance from the subject - requiring a summation of at least many individual vectors - as you imply.
I hope this explanation & my perhaps inappropriate terminology can be properly understood. You might also find it (more) interesting to consider a complex method of radially partitioning the disk evaluation in an attempt to more closely approximate actual separation distances: see http://dx.doi.org/10.1088/1674-4527/11/12/005 or http://arxiv.org/abs/1104.3236 - referenced in my informal profile essay. It is good to hear from someone with a similar perspective!