In the past, church belfries, due to their higher layout, often served as reference points in surveying. With the development of satellite based positioning methods and the establishment of the D96/TM coordinate system, they slowly lost their significance. Nevertheless, unlike ground trigonometric points, they have remained largely intact. As such, they enable transformation parameters determination between the old and the new coordinate system. Therefore, we need to determine their positions in the new coordinate system. We described the determination of the church belfries position using terrestrial laser scanning, on the example of both belfries of the Trnovo church. The process involves determining coordinates of the tie points for georeferencing the point clouds. This requires the determination of the geodetic datum by a combination of GNSS measurement and geometric levelling, and the classical geodetic survey of the geodetic network with free-network adjustment and further use of the S-transformation. Based on the georeferenced point clouds, we determined the position of the trigonometric point by sphere parameters adjustment. The data is filtered using the RANSAC algorithm so that we only have points that belong to the sphere in the adjustment process. The results were compared with the positions determined based on the classical geodetic survey.