the distinction between generations as I'm familiar with it is:<br /><br />1st: Pure hydrogen helium stars, the primordial first stars. We've found a couple of stars very close to this.<br /><br />2nd: Low, low metal content, basically the first stars formed after the primordial giants died. These tend to be the older stars in globular clusters (among other places).<br /><br />3rd: "modern" stars, with significant metal contents. Massive O & B stars actually require a significant metal content in order for their particular brand of fusion to work (the CNO cycle uses C, N, and O atoms as catalysts). <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>