We show that the presently available data on the Gamow-Teller (GT) str
ength in mid-fp-shell nuclei are proportional to the product of the nu
mbers of valence protons and neutron holes in the full fp-shell. This
observation leads to important insights into the mechanism for GT quen
ching and to a simple parametrization of the Gamow-Teller strengths im
portant for electron capture by fp-shell nuclei in the early stage of
supernovae.