  Estimates of the deuterium abundance in quasar absorbers are reviewed,
including a brief account of incorrect claims published by the author and a
brief review of the problem of hydrogen contamination. It is concluded that the
primordial abundance may be universal with a value $(D/H)_P\approx 10^{-4}$,
within about a factor of two, corresponding to $\Omega_B h_{0.7}^2\approx 0.02$
or $\eta_{10}\approx 2.7$ in the Standard Big Bang. This agrees with current
limits on primordial helium, $Y_P\le 0.243$, which are shown to be surprisingly
insensitive to models of stellar enrichment. It also agrees with a tabulated
sum of the total density of baryons in observed components. Much lower
primordial deuterium ($\approx 2\times 10^{-5}$) is also possible but disagrees
with currently estimated helium abundances; the larger baryon density in this
case fits better with current models of the Lyman-$\alpha$ forest but requires
the bulk of the baryons to be in some currently uncounted form.
