We derive here two new estimators of admixture proportions based on a
coalescent approach that explicitly takes into account molecular infor
mation as well as gene frequencies. These estimators can be applied to
any type of molecular data (such as DNA sequences, restriction fragme
nt length polymorphisms [RFLPs], dr microsatellite data) for which the
extent of molecular diversity is related to coalescent times. Monte C
arlo simulation studies are used to analyze the behavior of our estima
tors. We show that one of them (m(Y)) appears suitable for estimating
admixture from molecular data because of its absence of bias and relat
ively low variance. We then compare it to two conventional estimators
that are based on gene frequencies. m(Y) proves to be less biased than
conventional estimators over a wide range of situations and especiall
y for microsatellite data. However, its variance is larger than that o
f conventional estimators when parental populations are not very diffe
rentiated. The variance of m(Y) becomes smaller than that of conventio
nal estimators only if parental populations have been kept separated f
or about N generations and if the mutation rate is high. Simulations a
lso show that several loci should always be studied to achieve a drast
ic reduction of variance and that, for microsatellite data, the mean s
quare error of m(Y) rapidly becomes smaller than that of conventional
estimators if enough loci are surveyed. We apply our new estimator to
the case of admired wolflike Canid populations tested for microsatelli
te data.