  In this paper we report two new super Li-rich K giants: KIC 2305930 and KIC
12645107 with Li abundances exceeding that of ISM (A(Li) $\geq$ 3.2 dex).
Importantly, both the giants have been classified as core He-burning red clump
stars based on asteroseismic data from Kepler mission. Also, both the stars are
found to be low mass (M $\approx$ 1.0 M$_{\odot}$) which, together with an
evidence of their evolutionary status of being red clump imply that the stars
have gone through both the luminosity bump and He-flash during their RGB
evolution. Stars' large Li abundance and evolutionary phase suggest that Li
enrichment occurred very recently probably at the tip of RGB either during
He-flash, an immediate preceding event on RGB, or by some kind of external
event such as merger of RGB star with white dwarf. The findings will provide
critical constraints to theoretical models for understanding of Li enhancement
origin in RGB stars.
