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We present CCD UBVI observations obtained in the field of the previouslyunstudied northern open clusters NGC 133 and NGC 1348. We argue that NGC 133 isa heavily contaminated cluster, for which we identify 13 candidate members downto $V$=14.50 mag on the basis of the position in the two-color Diagram .Membership has been checked against proper motions from Tycho~2, wheneveravailable. The cluster turns out to have a reddening E$(B-V)=0.60\pm0.10$ mag,to be $630\pm150$ pc distant from the Sun, and to have an age less than 10Myrs. NGC 1348 is a more reddened cluster (E$(B-V)=0.85\pm0.15$ mag) for whichwe isolate 20 members. The cluster lies at a distance of $1.9\pm0.5$ kpc awayfrom the Sun, and has an age greater than 50 Myrs.Comment: 9 pages, 13 eps figures, in press in A&

A photometric study of the two poorly known northern open clusters NGC 133 and NGC 1348