  Following the recent identification of discrete ROSAT and radio sources
associated with the virial shocks of MCXC clusters and groups, we examine if
the early eROSITA-DE data release (EDR) shows virial-shock X-ray sources within
its $140$ deg$^2$ field. EDR catalog sources are stacked and radially binned
around EDR catalog clusters and groups. The properties of the excess
virial-shock sources are inferred statistically by comparing the virial-shock
region to the field. An excess of X-ray sources is found narrowly localized at
the $2.0<r/R_{500}<2.25$ normalized radii, just inside the anticipated virial
shocks, of the resolved 532 clusters, for samples of both extended ($3\sigma$
for 534 sources) or bright ($3.5\sigma$ for 5820 sources; $4\sigma$ excluding
the low cluster-mass quartile) sources. The excess sources are on average
extended ($\sim 100$ kpc), luminous ($L_X\simeq 10^{43-44}$ erg s$^{-1}$), and
hot ($\sim$keV), consistent with infalling gaseous halos crossing the virial
shock. The results agree with the stacked ROSAT-MCXC signal, showing the higher
$L_X$ anticipated at EDR redshifts and a possible dependence upon host mass.
Localized virial-shock spikes in the distributions of discrete radio, X-ray,
and probably also $\gamma$-ray sources are new powerful probes of accretion
from the cosmic web, with strong constraints anticipated with future all-sky
catalogs such as by eROSITA.
