Photometric Analyses for Two Koronis Family Asteroids

We present photometric analyses of two Koronis family asteroids: (2742) Gibson and (993) Moultona based on data is collected from telescope observations worldwide and then processed at Union College. More specifically, we derived the synodic rotational period of (2742) Gibson at 20.60 ± 0.01 hours, which had no previously reported period. For (993) Moultona we obtained 5.2702 ± 0.0003 hours. Our results are in agreement with previously published observations of (993) Moultona, at 5.2702 ± 0.0004 hours (Crowley et al., 2023).