  We built the first-ever statistically significant sample of ~ 80,000
background quasar - foreground cluster pairs to study the cool, metal-rich gas
in the outskirts (> R500) of z ~ 0.5 clusters with a median mass of ~ 10^14.2
M_sun. The sample was obtained by cross-matching the SDSS cluster catalog of
Wen & Han (2015) and SDSS quasar catalog of Lyke et al. (2020). The median
impact parameter (rho_cl) of the clusters from the quasar sightlines is 2.4 Mpc
(median rho_cl/R500 = 3.6). A strong MgII, along with marginal FeII, absorption
is detected in the mean and median stacked spectra of the quasars with total
MgII rest-frame equivalent width (W^(2796+2803)) of 0.034 pm 0.005 A (7simga)
and 0.010 pm 0.003 A (3sigma), respectively. The W^(2796+2803) shows a
declining trend with increasing rho_cl and rho_cl/R500, but does not show any
significant trend with mass (M500) or redshift (zcl) within the small M500 and
zcl ranges probed here. The MgII absorption signal and the trends persist even
if we exclude the quasar-cluster pairs where the background quasars may be
probing the circum-galactic medium (CGM) of bright galaxies with impact
parameters < 300 kpc. The MgII (and FeII) absorption reported here is the first
detection of its kind. It indicates the presence of a cool, metal-rich gas
reservoir surrounding galaxy clusters out to several R500. We suggest that the
metal-rich gas in the cluster outskirts arise from stripped materials and that
gas stripping may be important out to large clustocentric distances (> 3R500 ).
