What Causes Galactic Plains?

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Discussion Overview

The discussion revolves around the formation of galactic plains and their potential similarities to planetary plains. Participants explore the underlying causes of these structures in the context of astrophysical processes.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants suggest that galactic plains may form due to collisions between galaxies.
  • Others propose that both galaxies and star systems are planar because they originate from large rotating clouds of gas and dust, which retain angular momentum as they condense.
  • One participant discusses the gravitational interactions among planets, suggesting that these interactions could lead to a common orbital plane over time, likening it to a "viscosity" effect in the system.
  • A participant raises questions about the tilt of the ecliptic relative to the galactic plane and the orbits of extrasolar planets, speculating that these orbits may generally align with the galactic plane, with variations due to localized turbulence.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the causes of galactic and planetary plains, and the discussion remains unresolved with no consensus reached.

Contextual Notes

Participants note the complexity of gravitational interactions and the potential for energy loss and angular momentum cancellation in the formation of common orbital planes, but do not resolve the specifics of these processes.

M.C.
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What causes Galactic Plains to form? Is it the same reason there is a planetary plain?
 
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http://www.kingsu.ab.ca/~brian/astro/course/lectures/winter/chp11.htm

i think mosty due to collision between galaxies
 
Last edited by a moderator:
so what causes the planetary plain?
 
Originally posted by M.C.
so what causes the planetary plain?

I want to understand your question better

first of all, the plane of the Earth's orbit is not quite the same as the plane of jupiter's orbit
or the plane of another planet
or the plane of the moon's orbit

all these planes are slightly tilted with respect to each other and do not exactly coincide

but I think you are asking why do they so NEARLY coincide
mostly they are tilted only a few degrees from each other

what evened them out?
if you started with a central star and 100 planets orbiting every which way around it
so the orbit-planes of the 100 planets are initially all tilted randomly by as much as 90 degrees from each other or even more
then what would cause those 100 planets to gradually
work out an approximate common orbit plane?

wolram mentioned collisions
and there is gravitational interaction which can ressemble a soft-core collision and happen repeatedly over millions of years
maybe it gives a kind of "viscosity" to a system of 100 planets
so that eventually their angular momentums boil down and settle down to one basic orientation that they all more or less agree on
(because otherwise they keep bumping and perturbing each other)

a lot of energy must get lost and a lot of angular momentum (in opposed directions) must get canceled out and it must be a long process (wouldnt necessarily be pleasant to witness either)
but something like viscosity keeps dragging on them and bugging them until they work out an approximate common plane

Let us try to get Phobos or Integral or some such astronomy honcho to pronounce the word on this
 
My guess would be that galaxies are planar for the same reason as star systems - they formed out of large rotating clouds of gas and dust. As the gas condenses, it retains its angular momentum and "settles down" to a plane. It's similar to the oblateness of the Earth due to its rotation, but taken to an extreme due to the gaseous nature of the cloud and the speed of rotation (Earth's surface rotates at about 1 kps; gas at 1AU goes around at about 30kps). I believe we are going around the center of the galaxy at about 200 kps, so despite the massive size it would still flatten out on a timescale of billions of years.

As a side note, how tilted is the ecliptic with respect to the galactic plane? What about for the orbits of extrasolar planets? I suspect that planetary orbits would be, for the most part, similar to the galactic plane, differences being due to localized turbulence in the original gas cloud as it was condensing.
 
Last edited:
Ok, I understand it now. Thanks for the information guys:smile:
 

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