What spatial scales does dark matter become significant?

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The discussion centers on the spatial scales at which dark matter becomes significant and its effects on general relativity (GR). It is established that dark matter does not cause GR to break down; rather, it introduces additional mass that must be accounted for. The critical volume of space necessary to observe dark matter effects is primarily associated with large structures, such as galaxies, while smaller entities like star clusters may not exhibit these effects. Accurate measurements of celestial body motions are essential for determining the influence of dark matter.

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Albertgauss
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Hello,

How much volume or mass of space does one need to see appreciable effects of dark matter where general relatively seems to break down? What is the critical volume of space at this time where people can see the effects of dark matter and where they cannot? Is there a spatial scale smaller than galaxies--or even sub-sections of galaxies--where the effects of dark matter first manifest themselves as departures from general relativity?
 
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Albertgauss said:
How much volume or mass of space does one need to see appreciable effects of dark matter
Small galaxies and similar structures. Star clusters are usually too small, but there are exceptions.
Albertgauss said:
where general relatively seems to break down?
It doesn't.
 
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Albertgauss said:
How much volume or mass of space does one need to see appreciable effects of dark matter where general relatively seems to break down?
If dark matter exists then GR is not breaking down. There is just extra mass that needs to be taken into account.
Albertgauss said:
What is the critical volume of space at this time where people can see the effects of dark matter and where they cannot?
I think that would technically depend on how accurately you can measure the motions of bodies in space. Dark matter is often considered important when studying large sections of galaxies and anything larger. I am not aware of any precise number for the scales at which dark matter should be considered.
 
Okay, sounds good. I just wanted to get a basic idea. Yes, yes about GR not breaking down, I realize I worded that wrong.
 

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