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Comment Re:Not Dark Matter (Score 2, Informative) 97

Ok, fair point - there are a lot of little, dense things like brown dwarfs and planets that we can't currently observe. However, these can only be a tiny component of the "dark" stuff that we don't see. If brown dwarfs or planets comprised a significant chunk of the dark matter, it would be detected by gravitational microlensing events, and those observations suggest that dense baryonic objects (such as stars, brown dwarves, etc.) aren't a big (which is to say, dynamically important) component of the galactic halo.

Also, with respect to dust, it's actually quite easy to detect it in the interstellar medium, in both emission and absorption. It doesn't ALWAYS emit radiation, and doesn't do it spontaneously, but when dust is bombarded by light from nearby stars, it tends to re-emit in the infrared and radio. So it's incredibly easy to detect it in both of those bands, and use it to learn things about galaxies. It blocks optical light, of course, so you can see it in nearby (and not so nearby) gas-rich galaxies.

I see by the link below your name that you're from Berkeley, or at least probably have some berkeley ties. You should go talk to Chris McKee in the astronomy department if you think dust is more of a pain than it's worth - he'll set you straight!

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