Metal clusters featuring closed supershells or aromatic character usually exhibit remarkably enhanced stability in their cluster series. However;
not all stable clusters are subject to these fundamental constraints. Here;
by employing photoelectron imaging spectroscopy and ab initio calculations;
we present experimental and theoretical evidence on the existence of unexpectedly stable open-shell clusters;
which are more stable than their closed-shell and aromatic counterparts. The stabilization of these open-shell Al-Mg clusters is proposed to originate from the S-P molecular orbital coupling;
leading to highly stable species with increased HOMO-LUMO gaps;
akin to s-p hybridization in an organic carbon atom that is beneficial to form stable species. Introduction of the coupling effect highlighted here not only shows the limitations of the conventional closed-shell model and aromaticity but also provides the possibility to design valuable building blocks. © 2014 American Chemical Society;