Photometric observations of the main-belt asteroid 2484 Parenago performed by the authors in Italy in 2014 September revealed the bimodal light curve phased to 3.433 ± 0.001 hours as the most likely solution representing the synodic rotation rate for this asteroid.
Marchini, A., Papini, R., Salvaggio, F. (2015). Rotation Period Determination for 2484 Parenago. THE MINOR PLANET BULLETIN, 42(1), 40-40.
Rotation Period Determination for 2484 Parenago
Alessandro Marchini
Writing – Original Draft Preparation
;
2015-01-01
Abstract
Photometric observations of the main-belt asteroid 2484 Parenago performed by the authors in Italy in 2014 September revealed the bimodal light curve phased to 3.433 ± 0.001 hours as the most likely solution representing the synodic rotation rate for this asteroid.
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https://hdl.handle.net/11365/1083721