In this paper , we report the discovery of two new super Li-rich K giants : HD 24960 and TYC 1751-1713-1 .
Based on high resolution ( R \approx 60 , 000 ) spectroscopy , we have derived Li abundance of A ( Li ) \approx 4.0 dex for both stars .
Other elemental abundances are normal of typical K giants .
Low ratios of [ C/N ] \leq - 0.25 and ^ { 12 } C / ^ { 13 } C \leq 10 suggest that the stars are in upper RGB phase .
Further , based on Gaia astrometry and secondary calibrations using Kepler asteroseismic and LAMOST spectroscopic data , we argue that both stars belong to red clump ( RC ) phase with core He-burning .
Results add to half a dozen already known red clump Li-rich K giants , and support the growing evidence that the origin of Li excess in RC giants seems to be associated with either He-flash at the tip of the red giant branch ( RGB ) or recent planet/ brown dwarf merger events closer to the RGB tip .