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thomasxin t1_j81gnu6 wrote

Reply to comment by Player_KK in Why is the Oort cloud spherical? by Outliver

Gravity does interact over long distances over long periods of time though, is there a mechanism that acts against that compared to smaller accretion disks? What prevents an elliptical galaxy collapsing into a spiral, and how do we know that won't happen even if given a trillion years?

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Cheshire-Kate t1_j81i8j2 wrote

If the only thing acting on stars is gravity, then they will stay in their elliptical orbits undisturbed and the overall shape of the galaxy won't change.

It's only once you start adding drag and friction into the mix from gas clouds and nebulas that the forces necessary to collapse the shape into a disc are present. With those gases, a galaxy will eventually collapse into a disc, but without them, there's no reason for them to do so.

Most elliptical galaxies are very old, and no longer have any new star formation. This means far less drag and friction, meaning no forces to flatten the orbits of stars within the galaxy, meaning it will remain an elliptical galaxy forever

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willun t1_j81up2b wrote

Would the dark matter provide drag? I wonder what the movements of dark matter would be in galaxies like that. I assume for the Milky Way it just rotates in line with the movement of stars (or more accurately, the stars move in line with the dark matter)

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gladfelter t1_j82x2uy wrote

The electrical field of an atom is many orders of magnitude larger than the radius of a theoretical WIMP. So interactions and friction would be orders of magnitude less for dark matter.

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willun t1_j82xgoa wrote

Not drag from friction, but gravity is what i meant. The same effect that causes the moon to face earth.

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SkoomaDentist t1_j864qop wrote

> Would the dark matter provide drag?

The way it was explained to me, dark matter only interacts via gravity, including on itself.

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UnarmedSnail t1_j82y5ly wrote

I suspect elliptical galaxies are the merger of galaxies where the collision canceled out both galaxies rotational energy.

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