The Robotic Optical Transient Search Experiment I(ROTSE-I) experiment has g
enerated CCD photometry for the entire northern sky in two epochs nightly s
ince 1998 March. These sky patrol data are a powerful resource for studies
of astrophysical transients. As a demonstration project, we present first r
esults of a search for periodic variable stars derived from ROTSE-I observa
tions. Variable identification, period determination, and type classificati
on are conducted via automatic algorithms. In a set of nine ROTSE-I sky pat
rol fields covering roughly 2000 deg(2), we identify 1781 periodic variable
stars with mean magnitudes between m(v) = 10.0 and m(v) = 15.5. About 90%
of these objects are newly identified as variable. Examples of many familia
r types are presented. All classifications for this study have been manuall
y confirmed. The selection criteria for this analysis have been conservativ
ely defined and are known to be biased against some variable classes. This
preliminary study includes only 5.6% of the total ROTSE-I sky coverage, sug
gesting that the full ROTSE-I variable catalog will include more than 32,00
0 periodic variable stars.