Two groups have independently reported the possible detection of extra
galactic deuterium in the absorption spectrum of the same high-redshif
t, low-metallicity QSO. Although the high value for the inferred deute
rium abundance poses no problems for cosmology (i.e. big bang nucleosy
nthesis), it is in apparent conflict with Solar system observations of
deuterium and helium-3. This latter inconsistency is explained and ma
de quantitative, and it is shown that, unless the inferred D/H ratio i
s too high by a factor of 3, these data challenge our understanding of
the stellar and Galactic evolution of helium-3. This conflict is reso
lved if the observed absorption feature is, in fact, due to a hydrogen
interloper rather than to high-z, low-Z deuterium.