In order to realizea rtificial photosynthetic devices for splitting water to H 2 and O 2 (2 H 2 O + hn!2H 2 + O 2 ), it is desirable to use awider wavelength range of light that extends to alower energy region of the solar spectrum. Here we report at riruthenium photosensitizer [Ru 3 (dmbpy) 6 (m-HAT)] 6+ (dmbpy = 4,4'-dimethyl-2,2'-bipyridine,H AT = 1, 4,5,8,9,12-hexaazatriphenylene) + , [4] with bpy = 2,2'-bipyridine and ppy = 2-phenylpyridinate), and acatalyst (e.g., colloidal Pt, [5] Pt II , [6] Rh II [7] and Co II [8] complexes). As shown in Scheme 1, either an oxidative or reductive quenching process triggers the lightdriven electron transfer (ET) processes.I ns pite of the great advancement so far in this area, little efforts have been made to develop PSs capable of driving ET events by making use of awider wavelength range of the solar spectrum. Forinstance, one of the well-known PSs,[ Ru(bpy) 3 ] 2+ ,c an absorb light in the 280-600 nm range,w hich covers only 19.1 %o ft he total solar irradiance on the basis of the integrated photon flux. [9] However,the integrated photon flux can be almost doubled if the 280-800 nm domain (39.6 %ofthe total solar irradiance) could be fully used by the PS when driving H 2 evolution. In this context, Hanan et al. employed qpy (4,4':2,2'':4'',4'''-quarterpyridine) instead of bpy,and showed that [Ru(qpy) 3 ] 2+ (see Figure 1A)i sc apable of absorbing longer wavelength light and can actually drive photochemical H 2 evolution even