  IC 4665 is one of only a dozen young open clusters with a ``lithium depletion
boundary" (LDB) age. Using an astrometrically and spectroscopically filtered
sample of cluster members, we show that both the positions of its low mass
stars in Gaia absolute colour-magnitude diagrams and the lithium depletion seen
among its K- and early M-stars are discordant with the reported LDB age of (32
+4/-5) Myr. Re-analysis of archival spectra suggests that the LDB of IC 4665
has not been detected and that the published LDB age should be interpreted as a
lower limit. Empirical comparisons with similar datasets from other young
clusters with better-established LDB ages indicate that IC 4665 is bracketed in
age by the clusters IC 2602 and IC 2391 at (55 +/- 3) Myr.
