On Sun, Oct 05, 2008 at 04:28:26PM -0400, Shane Mage wrote:

> >I see that astronomers can "see" planets circling far away stars by
> >observing the wobble of the star cause by the planet's gravity...
> 
> That is a deduction which will or will not stand up to a modest  
> increase in the resolving power of our telescopes.  But if a  
> sufficient increase in telescopic resolution shows no planet, leaving  
> that "wobble" unexplained, what should one think of an astronomer who  
> reacted by saying "that planet is really there, all right--we just  
> don't see it because it is made of dark matter?"

Dark matter has absolutely nothing to do with extra-solar planets
and the reasons they can't be seen with optical telescopes.

Dark matter is the non-radiating stuff that is operating on orders of
magnitude larger objects, like galactic clusters.  Galaxies and
clusters are behaving in gravitational ways that indicate there is
probably a lot of mass there, but none of it seems to be emitting any 
radiation.

This is different than the normal (baryonic) matter which does emit
radiation, but we simply are too far or it is too faint to see (such
as brown dwarf stars and extra-solar planets).  That matter is
virtually irrelevant when considering the large gravitational
structure in galaxies and clusters.


Matt

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