Photometry Result of an Eclipsing Binary Star V798Her in the Globular Cluster NGC 6341

We present the photometric study of an eclipsing binary star V798Her in the globular cluster NGC 6341. The observations were obtained in Johnson's B, V & R filters using 0.8m Tarleton telescope and a CCD photometer. The observed light curves after determination of light elements show that V798Her is a W UMa contact binary system with a period of 0.2951110 days. This binary system will be further analyzed using Wilson Devinney model 2015 version.