C
CalliArcale
Guest
Since this is clearly a topic of great interest, I figured I'd start a new thread.<br /><br />Dark matter is, of course, material which cannot be detected by its electromagnetic radiation or reflection. It is quite literally dark. The only way to detect it is by its effect: gravitational influence on other objects.<br /><br />It is certain that dark matter does exist; consider absorption nebulae such as the Horsehead Nebula, visible primarily because of its profile. And of course there are limits to current technology. More and more brown dwarfs are being detected as the ability to find such objects in infrared improves. As it is impossible to really know what we haven't discovered, it is reasonable to assume there are at least a few more of these sorts of things, and probably quite a lot.<br /><br />Some interestings questions are:<br /><br />Just how much dark matter is there?<br /><br />If you can't see it, how can you detect it?<br /><br />Even if you're detecting it gravitationally, how much does this really tell you about the dark matter?<br /><br />[Edited because I finally noticed a grammatical error in the title. D'oh!] <div class="Discussion_UserSignature"> <p> </p><p><font color="#666699"><em>"People assume that time is a strict progression of cause to effect, but actually from a non-linear, non-subjective viewpoint it's more like a big ball of wibbly wobbly . . . timey wimey . . . stuff."</em> -- The Tenth Doctor, "Blink"</font></p> </div>