it's actually a pretty complicated question that's taken a long, long time to discern with any real accuracy.<br /><br />First, the fact that we are in a galaxy that is primarily a plane is easy to determine, merely look at the overall distribution of stars.<br /><br />With good optics, and thurough surveys, its easy to determine that we can look further in one direction along the disk, than the others, thus indicating we are near an edge. We can look further in that direction, because we get to the edge, and have no more material to block our view. In the opposite directions, we have to wade through lots of stuff.<br /><br />By observing the motions of stars relative to eachother, and the motions of globular clusters, we can begin to discern a center of the galaxy.<br /><br />Most disk galaxies are spirals, and spiral arms have various properties (O and B class stars, denser hyrodgen contents, etc) and by mapping out the locations of these properties, we can map out the spiral arms (quite imprecisely I might add). <div class="Discussion_UserSignature"> <p align="center"><font color="#c0c0c0"><br /></font></p><p align="center"><font color="#999999"><em><font size="1">--------</font></em></font><font color="#999999"><em><font size="1">--------</font></em></font><font color="#999999"><em><font size="1">----</font></em></font><font color="#666699">SaiphMOD@gmail.com </font><font color="#999999"><em><font size="1">-------------------</font></em></font></p><p><font color="#999999"><em><font size="1">"This is my Timey Wimey Detector. Goes "bing" when there's stuff. It also fries eggs at 30 paces, wether you want it to or not actually. I've learned to stay away from hens: It's not pretty when they blow" -- </font></em></font><font size="1" color="#999999">The Tenth Doctor, "Blink"</font></p> </div>