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WDS 03286+2523 BRT 133, is a double-star system that has been underobservation since 1896. In this study, we present new measurements of theposition angle and separation of the system, utilizing data obtained from a webtelescope with a Charged Couple Device (CCD) camera, Gaia EDR3, and historicalrecords. We determined that the position angle and separation are 222.4{\deg}and 5.35", respectively, indicating a slight increase from the previous valuesof 222{\deg} and 5.34" measured in 2004. We also employed the parallax and theratio of proper motion metric (rPM) values of the system to assess itsbinarity. This analysis showed that the system may be gravitationally bound andwith a long orbital period.

Measurement of the Double Star System WDS 03286+2523 BRT 133 with a Web Telescope