Re: Dark matter
- From: Ernest Major <{$to$}@meden.demon.co.uk>
- Date: Mon, 17 Sep 2007 17:27:19 +0100
In message <1190045107.868790.128830@xxxxxxxxxxxxxxxxxxxxxxxxxxxx>, Bill Hudson <oldgeek61-951@xxxxxxxxx> writes
On Sep 17, 7:24 am, Ye Old One <use...@xxxxxxxxx> wrote:One of the observations that supports the existence of dark matter is that galaxies in clusters and stars in (the outer regions of) galaxies would not be bound if the visible matter was all that was there (and our theories of gravity and mechanics are correct). Globular clusters are much denser systems than galaxies and clusters, so, if dark matter is (much) less strongly clumped than visible baryonic matter the effect of dark matter on orbits within globular clusters could be less than the error bars on the observations.On Mon, 17 Sep 2007 01:17:39 -0700, spintronic
<spintro...@xxxxxxxxxxx> enriched this group when s/he wrote:
>On 16 Sep, 19:29, Lee Oswald Ving <leeov...@xxxxxxxxx> wrote:
>> > spintronic <spintro...@xxxxxxxxxxx> wrote in
>> >news:1189941467.586354.45840@xxxxxxxxxxxxxxxxxxxxxxxxxxx:
>> >> Question!
>> >> Could you tell me why dark matter is homogenous in *all* galaxies,
>> >> yet missing in globular clusters?
>> And while we're at it - why do you believe this?
>Because it's true!
Cite?
--
Bob.
I don't know that it is true. Since dark matter was only recently
detected in galaxies, it could be that they have not refined the
technique enough to detect it in clusters. As far as I know (but I
certainly could be wrong) dark matter is detected (indirectly) only in
galaxy clusters, not individual galaxies. So far, DM is detectable
only by the gravitational lensing of more distant objects, so you'd
need a lot of it. Clusters need not apply at this point.
From observations of stellar motions we can at best only put a lower bound on the excess density of dark matter in globular clusters.
--
alias Ernest Major
.
- References:
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