We consider the possibility that neutrinos (but no other light fermion
s) are coupled very weakly to an extremely light scalar boson. We firs
t analyze the simple problem of one generation of neutrino and show th
at, for ranges of parameters that are allowed by existing data, such a
system can have serious consequences for the evolution of stars and c
ould impact precision laboratory measurements. We discuss the extensio
n to more generations and show that the general conclusion remains via
ble. Finally, we note that, should such a scalar field be present, exp
eriments give information about effective masses, not the masses that
arise in unified held theories.