  The flux of 7Be and 8B neutrinos from the Sun and the production of 7Li via
primordial nucleosynthesis depend on the rate of the 3He(alpha,gamma)7Be
reaction. In extension of a previous study showing cross section data at 127 -
167 keV center of mass energy, the present work reports on a measurement of the
3He(alpha,gamma)7Be cross section at 106 keV performed at Italy's Gran Sasso
underground laboratory by the activation method. This energy is closer to the
solar Gamow energy than ever reached before. The result is sigma = 0.567 +-
0.029(stat) +- 0.016(syst) nbarn. The data are compared with previous
activation studies at high energy, and a recommended S(0) value for all
3He(alpha,gamma)7Be activation studies, including the present work, is given.
