  The metallicity distribution in the Fornax cluster was studied with the XIS
instrument onboard the Suzaku satellite. K-shell lines of O and Mg were
resolved clearly, and the abundances of O, Mg, Si, S and Fe were measured with
good accuracy. The region within a 4' radius of NGC 1399 shows approximately
solar abundances of Fe, Si and S, while the O/Fe and Mg/Fe abundance ratios are
about 0.4--0.5 and 0.7 in solar units. In the outer region spanning radii
between 6' and 23', the Fe and Si abundances drop to 0.4--0.5 solar and show no
significant gradient within this region. The abundance ratios, O/Fe and Mg/Fe,
are consistent with those in the central region. We also measured the Fe
abundance around NGC 1404 to be approximately solar, and the O, Ne and Mg
abundances to be 0.5--0.7 times the Fe level. The significant relative
enhancement of Fe within 130 kpc of NGC 1399 and in NGC 1404 indicates an
origin in SN Ia, in contrast to the species O, Ne, and Mg which reflect the
stellar metallicity. The mass-to-light ratios for O and Fe within 130 kpc of
NGC 1399 are over an order of magnitude lower than those in rich clusters,
reflecting the metal enrichment history of this poor cluster.
