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The relation between the lithium abundance, A_Li, and photospheric activityof solar-type Pleiads is investigated for the first time via acquisition andanalysis of B and V-band data. Predictions of activity levels of target starswere made according to the A_Li/(B-V) relation and then compared with new CCDphotometric measurements. Six sources behaved according to the predictionswhile one star (HII 676), with low predicted activity, exhibited the largestvariability of the study; another star (HII 3197), with high predictedactivity, was surprisingly quiet. Two stars displayed non-periodic fadings,this being symptomatic of orbiting disk-like structures with irregular densitydistributions. Although the observation windows were not ideal for rotationalperiod detection, some periodograms provided possible values; the light-curveobtained for HII 1532 is consistent with that previously recorded.Comment: 8 Pages, 9 Figures, accepted in A&

Li abundance/surface activity connections in solar-type Pleiades