Quote:
Originally Posted by peeter
I was reading the wiki page on dark matter, and have trouble visualizing how galaxies keep their shape if most of the stars rotate at the same rate. If I try to imagine this (ie: without any sort of math modelling of the gravity interactions involved) I picture everything just merging into a big amorphous disk instead of shapes like spirals.
Does anybody know of a nice animation or visualization of long term effects of a gravity model of a spiral galaxy? Ideally I'd like to see how the rotation would look over time with and without the dark matter distribution.
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The spiral pattern is not a result of stars holding their places relative to
each other in spiral arms as they orbit around and around and around
the center of the galaxy.
Instead, the spiral pattern is in large part due to a wave of compression
which causes gas clouds in a small region to become slightly more dense
than usual, which causes stars to form in them. Some of those stars
are massive, blue, luminous and short-lived. They light up the regions
in which they formed for just a few million years, then die. Those few
luminous stars define the spiral arms in many galaxies. Because they
only live for 5-20 million years, while it takes 200 million years to complete
one orbit around the center of the galaxy, the pattern they make doesn't
really rotate with the longer-lived stars.
If you were to ride in a helicopter far above New York City, you'd
see patterns of red brake lights in the streets below. Those patterns
would appear to move over time. However, the pattern is not due
to a small number of cars which always have their brake lights on,
and which slowly cruise down the street at a constant speed.
Instead, one car hits the brakes, which causes the one behind it
to hit the brakes, which causes the one behind IT to hit the brakes,
and so on. The pattern of red lights is really not tied to any
particular cars.
This is a very big subject. If you really want to understand it,
try reading books or articles on "spiral density waves in galaxies".