by apodman » Fri Nov 28, 2008 7:21 am
For the layman:
As far as I know, when a small galaxy travels near a large galaxy, it can have one of four basic outcomes (each one the effect of gravity):
(1) The small galaxy's path, shape, and composition may be affected to some degree by the passage. The large galaxy's path, shape, and composition may be affected to a lesser degree. Their passage is relatively fast and separated, and after the passage they go off separately into space.
(2) The small galaxy's path, shape, and composition may be affected to some degree. The large galaxy's path, shape, and composition may be affected to a lesser degree. Their passage is at a relatively moderate speed with moderate separation, and the small galaxy goes into a roughly elliptical orbit around the large galaxy that may be stable for one to thousands of passes.
(3) The small galaxy's path, shape, and composition are affected greatly. The large galaxy's path, shape, and composition are affected more as the smaller galaxy spirals closer. Their passage is at a relatively slow speed with small separation; the small galaxy spirals into the larger galaxy and merges into it as it does so.
(4) The small galaxy's path, shape, and composition are affected greatly. The large galaxy's path, shape, and composition are affected more as the smaller galaxy passes through. Their passage is at a relatively high speed with small separation; the small galaxy passes through the larger galaxy and exchanges material as it does so.
In the case of today's APOD, I think we might be somewhere between (2) and (3).
For two galaxies of more equal size or more than two galaxies, the possible outcomes become more numerous, more complicated, and favor more large-scale deformation. Galaxies may pass through each other multiple times before they merge completely.
Galaxies exist in galaxy clusters. Each galaxy, except as perturbed by the gravity of other galaxies that pass by, pursues an independent elliptical path focused at the center of the galaxy cluster. Each elliptical path has a different size (and therefore a different orbital period and speed), has a different eccentricity (is more elongated or more circular), and is set at a different angle in a different plane, though they all are bound by their common gravity to the same center. As a result, galaxies can pass each other at all angles, each resulting in a unique outcome.
If that's too simplistic or not entirely correct, somebody please expand upon this.
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And what's with Judy's tooth?
For the layman:
As far as I know, when a small galaxy travels near a large galaxy, it can have one of four basic outcomes (each one the effect of gravity):
(1) The small galaxy's path, shape, and composition may be affected to some degree by the passage. The large galaxy's path, shape, and composition may be affected to a lesser degree. Their passage is relatively [b]fast and separated[/b], and after the passage they go off separately into space.
(2) The small galaxy's path, shape, and composition may be affected to some degree. The large galaxy's path, shape, and composition may be affected to a lesser degree. Their passage is at a relatively [b]moderate speed with moderate separation[/b], and the small galaxy goes into a roughly elliptical orbit around the large galaxy that may be stable for one to thousands of passes.
(3) The small galaxy's path, shape, and composition are affected greatly. The large galaxy's path, shape, and composition are affected more as the smaller galaxy spirals closer. Their passage is at a relatively [b]slow speed with small separation[/b]; the small galaxy spirals into the larger galaxy and merges into it as it does so.
(4) The small galaxy's path, shape, and composition are affected greatly. The large galaxy's path, shape, and composition are affected more as the smaller galaxy passes through. Their passage is at a relatively [b]high speed with small separation[/b]; the small galaxy passes through the larger galaxy and exchanges material as it does so.
In the case of today's APOD, I think we might be somewhere between (2) and (3).
For two galaxies of more equal size or more than two galaxies, the possible outcomes become more numerous, more complicated, and favor more large-scale deformation. Galaxies may pass through each other multiple times before they merge completely.
Galaxies exist in galaxy clusters. Each galaxy, except as perturbed by the gravity of other galaxies that pass by, pursues an independent elliptical path focused at the center of the galaxy cluster. Each elliptical path has a different size (and therefore a different orbital period and speed), has a different eccentricity (is more elongated or more circular), and is set at a different angle in a different plane, though they all are bound by their common gravity to the same center. As a result, galaxies can pass each other at all angles, each resulting in a unique outcome.
If that's too simplistic or not entirely correct, somebody please expand upon this.
---
And what's with Judy's tooth?