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We report observations of the eclipsing classical nova V368 Aql (Nova Aql1936 No. 2). These data reveal that the orbital period previously published byDiaz & Bruch is an alias of the true orbital period. A total of 14 eclipses (12complete and 2 partial) over 25 nights of observation have established that theorbital period of V368 Aql is 0.6905093(1) d (16.57 hr), which is roughly twicethe previously published period. With its revised orbital period, V368 Aql nowjoins other nova systems with periods in excess of 0.5 day that dominate thelong end of the orbital period distribution of cataclysmic variables.

The Orbital Period of V368 Aquilae (Nova Aquilae 1936 No. 2)