Star mass is the primary determination. Stars larger than 10 solar masses (our star is one solar mass, by definition) will turn into neutron stars. Stars larger than ....shoot... 30? Solar masses will turn into black holes.<br /><br />The limit isn't a really hard one, as variations in the supernovae can shed more (or less) mass from the core, and it is the final core mass that determines the fate. If a very large star sheds most of it's mass, it may drop it below the maximum threshold for a neutron star (3.5 solar masses...though all observed neutron stars are rarely larger than 2.5 solar masses, we don't know why).<br /><br />But, if the final core mass is less than 1.4 solar masses, it's a white dwarf. Less than 3.5, it's a neutron star. Greater than 3.5, it's a black hole. if the mass of the white dwarf, or neutron star increases (say by capturing material from a companion star) they can be upgraded to black holes. <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>