What spatial scales does dark matter become significant?

In summary, the effects of dark matter can be seen in small galaxies and similar structures, but not in star clusters. General relativity does not break down due to the existence of dark matter, but rather extra mass must be taken into account. The critical volume of space where the effects of dark matter are observable depends on the accuracy of measuring the motions of bodies in space, with dark matter being considered important in large sections of galaxies and anything larger. There is no specific scale at which dark matter should be considered, as it varies depending on the context.
  • #1
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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  • #2
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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  • #3
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.
 
  • #4
Okay, sounds good. I just wanted to get a basic idea. Yes, yes about GR not breaking down, I realize I worded that wrong.
 

1. What is dark matter and why is it important?

Dark matter is a hypothetical form of matter that is thought to make up about 85% of the total matter in the universe. It does not interact with light and is therefore invisible, making it difficult to detect. However, its gravitational effects can be observed, making it a crucial component in understanding the structure and evolution of the universe.

2. What spatial scales does dark matter become significant?

Dark matter becomes significant at the largest spatial scales, such as galaxy clusters and superclusters. It is also present on smaller scales, such as within individual galaxies, but its effects are most pronounced on a larger scale.

3. How do scientists study dark matter on different spatial scales?

Scientists use a variety of techniques to study dark matter on different spatial scales. These include gravitational lensing, which measures the bending of light around massive objects like galaxy clusters, and simulations that model the distribution of dark matter in the universe.

4. Can dark matter be observed directly?

No, dark matter cannot be observed directly because it does not interact with light. However, scientists are working on ways to indirectly detect dark matter, such as through its interactions with other particles or through its gravitational effects on visible matter.

5. How does the presence of dark matter affect the formation of galaxies?

Dark matter plays a crucial role in the formation of galaxies. Its gravitational pull helps to draw in and hold together gas and other matter, allowing galaxies to form and grow. The distribution of dark matter also influences the overall structure and shape of galaxies.

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