Collaborative photometric observations of two main-belt asteroids were conducted from five observatories in order to determine their synodic rotation periods. For 3157 Novikov we found a period of 9.952 ± 0.001 h with an amplitude of 0.31 ± 0.04 mag, for 7485 Changchun we found a period of 10.234 ± 0.001 h with an amplitude of 0.39 ± 0.02 mag.
Marchini, A., Papini, R., Banfi, M., Salvaggio, F., Bachini, M., Galdies, C., et al. (2019). Rotation Period Determination for 3157 Novikov and 7485 Changchun. THE MINOR PLANET BULLETIN, 46(2), 211-212.
Rotation Period Determination for 3157 Novikov and 7485 Changchun
Alessandro Marchini
Writing – Original Draft Preparation
;
2019-01-01
Abstract
Collaborative photometric observations of two main-belt asteroids were conducted from five observatories in order to determine their synodic rotation periods. For 3157 Novikov we found a period of 9.952 ± 0.001 h with an amplitude of 0.31 ± 0.04 mag, for 7485 Changchun we found a period of 10.234 ± 0.001 h with an amplitude of 0.39 ± 0.02 mag.
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https://hdl.handle.net/11365/1083831