Everybody who has been paying any amount of attention to the hunt for habitable extrasolar planets (AKA exoplanets) has probably heard the term “Goldilocks Zone” in regards to planet location. The Goldilocks Zone refers to a thin band around a star where water can exist in liquid form. Too close, the water boils away; too far and it freezes solid.
However, scientists here at ASU have found that the distance from a star is not the only factor governing potential habitability. The composition of the star itself plays a role as well. Patrick Young and others contend that the abundant elements carbon, oxygen, sodium, magnesium, & silicon are particularly important. Higher concentrations of these elements can cool down a star and slow its growth. This would keep the Goldilocks Zone steady for longer, which means that any planets inside that zone will have longer to develop the proper conditions for life.
It’ll be interesting to see where this research goes from here. Maybe I can asked Dr. Young if I could volunteer! *gasp*