Dark Matter in Galaxies/Star Clusters

[Rorkster2]

Has dark matter been observed to exist in quantities that correlate with the apparent observed mass or overal volume of gallexy/ star clusters? I'm wondering if dark matter is distributed in relative even amounts based on given characteristics or if it is thought to be random/unknown.

 

[Drakkith]

We cannot observe dark matter directly, only indirectly. The observations of "missing mass" and other oddities is exactly what we use to determine where dark matter is and what it is doing. We have no idea how to measure quantities of it other than the mass of it in a volume of space.

Edit: Hmm, I'm not sure that answers your question. I believe the distribution is relatively even if we look at very large volumes of space, such as mega-parsec distances, but on the local scale it is very different. Much of the dark matter in the milky way is believed to be in a spherical "halo" around the outskirts of the galaxy.

 

[Bobbywhy]

Rorkster2, You may find information about your question, supplied by marcus on 20 August here in this fourm:

Astrophysical and cosmological probes of dark matter
Matts Roos
17 Aug 2012
http://arxiv.org/abs/1208.3662v1

Cheers,
Bobbywhy

 

[Chalnoth]

Has dark matter been observed to exist in quantities that correlate with the apparent observed mass or overal volume of gallexy/ star clusters? I'm wondering if dark matter is distributed in relative even amounts based on given characteristics or if it is thought to be random/unknown.

The ratio of normal matter to dark matter varies quite dramatically from galaxy to galaxy. Smaller galaxies tend to have a much greater relative abundance of dark matter than larger galaxies, in large part because when smaller galaxies form, their gravitational potential wells aren't strong enough to hold in the material from the violent formation of the first stars. So most of the normal matter gets blown away, leaving just a little bit of behind, while the dark matter remains unaffected.

 

[sardar]

I can say that the existence of dark matter in galaxies and star clusters has been observed through various observational techniques such as gravitational lensing and the rotation curves of galaxies. However, the exact nature and distribution of dark matter is still a topic of ongoing research and debate.

While it is generally believed that dark matter is present in quantities that correlate with the observed mass and volume of galaxies and star clusters, the exact distribution of dark matter within these structures is not fully understood. It is thought that dark matter is distributed in a "halo" around galaxies and clusters, but the exact shape and density of this halo is still being studied.

Furthermore, there is evidence that the distribution of dark matter may not be completely even, with some regions having higher concentrations of dark matter than others. This could be due to various factors such as the merging of galaxies or the gravitational pull of nearby structures.

Overall, while we have observed the presence of dark matter in galaxies and star clusters, there is still much to learn about its distribution and characteristics. Further research and observations are needed to fully understand the role of dark matter in shaping the structure and evolution of these cosmic objects.