Galactic Traffic Patterns 81
eldavojohn writes "Using Hubble, researchers have noticed traffic patterns of stars within our own galaxy. From the article, 'Researchers analyzed 47 Tucanae, the second largest cluster in the Milky Way's galactic neighborhood, and determined the cluster sorts out stars according to their masses. Due to the associated gravitational pull, heavier stars slow down and sink to the cluster's core, while lighter stars pick up speed and zip out to the cluster's periphery.' There is speculation that these movements of stars — although tiny — can have significant implications and possibly result in mass segregation."
Re:Something at the centre? (Score:4, Interesting)
Does this have universal implications? (Score:3, Interesting)
And, if that's so, what would "THE core" be like. Hmmm, black hole not of one star but of entire galaxies?
Which begs the question, is there enough gravitational pull at a hypothetical core of all cores to hold the universe together like a giant counter weight on a pendulum, with fluctuations between expansions and collapses? (Never mind if 'Sha Ka Ree' is really there if it has the mass of 1 million Milky Ways, heh.)
IANA astronomer, astrophysicist, etc. Just curious because from what I read, as go moons, so go solar systems, so go galaxies, so goes the universe.
Re:I fail to see ... (Score:5, Interesting)
Here, we're looking at stars of different sizes and masses. There aren't some stars made mostly from silicates and iron oxides, while other stars are hollow plastic shells with slightly compressed air cores, or anything like that. A big red giant star may weigh 5x the mass of our sun, but be hundreds or thousands of times more voluminous, so the density as a whole object is actually much lower than a sun sized star.
Also, rocks sink in water. In a pool of mercury. both typical rocks and typical beachballs float. In vaccuum, near a gravitational source, everything that has mass is accelerated at the same rate, and densities really don't matter. Density affets falling objects if there's a drag, like there is falling through air. The space between stars is generally a near perfect vaccuum.
It's significant, because simple, standard physics explanations of sorting by density, type of material, or mass don't entirely explain this. Instead, there are probably other factors such as transfer of momentum between whole groups of stars, perhaps also to gas clouds or something, and maybe even modifying factors such as light pressure or angular momentum-linear momentum exchanges which are in turn affected by such unexpected things as the stars involved's relative surface areas or diameters.
The article talks about slingshot effects. Small stars can be slingshotted a lot faster by the same force that will only moderately accelerate large ones. This in turn means their orbit around the galactic core may even become a parabola or hyperbola, so that any given encounter sometimes becomes their last pass through the cluster. Larger stars get sped up and slowed down, but seldom by all that much, so they tend to keep returning to the cluster.
Sorting out which of these factors, and possibly others, are important and which are trivial is why the people studying this actually have to learn some math.