Abstract
We present a new lightcurve measurement and a shape and spin axis model for main-belt asteroid 2764 Moeller. The model was achieved with the lightcurve inversion process, using combined dense photometric data acquired from two apparitions, between 2018 and 2022 and sparse data from Catalina Sky Survey (693, 703, G97) and Asteroid Terrestrial-impact Last Alert System (ATLAS, T05-T08). Analysis of the resulting data found a sidereal period P = 5.953424 ± 0.000001 h and two mirrored pole solutions at (l = 310°, b = 41°) and (l = 133°, b = 39°) with an uncertainty of ± 20 degrees.