Abstract. Recently King et al. (1999) discovered Nova 1999 in IC1613 with 0.8 m KAIT of Lick Observatory. The new object is located at α = 104^m48^s.97, δ = +2°05′28″.8 (J2000.0). On the IR frames taken on Oct. 15 1998 at the National Mexican Astronomical Observatory at "San Pedro Martir" the Nova 1999 has (J-K) = 1.14 and K = 14.69 m. Its presence on the images taken one year before the discovery and its brightness questioned its classification as a nova. The light curve based on 92 archive KAIT images was constructed and remarkably resembles that of Mira-type variable. The obtained period is 508 ± 10 days. The star is over-luminous with respect to the PL relation derived by Feast et al. (1989) for LMC Miras. At longer periods (P > 400 days) many LMC Miras show such kind of behavior and the relation appears to break down. It is possible that the situation in IC1613 is similar.

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