Photometric observations of the main-belt asteroids 5318 Dientzenhofer and 9083 Ramboehm were made in 2016 March and 2015 December, respectively. Analysis of the data found a bimodal lightcurve with a synodic rotation period of 8.062 ± 0.002 h for 5318 Dientzenhofer. A trimodal lightcurve with synodic period of 10.199 ± 0.004 h for 9083 Ramboehm was found to be the most likely solution.
Salvaggio, F., Marchini, A., Papini, R. (2016). Lightcurve and Rotation Period Determination for 5318 Dientzenhofer and 9083 Ramboehm. THE MINOR PLANET BULLETIN, 43(4), 348-349.
Lightcurve and Rotation Period Determination for 5318 Dientzenhofer and 9083 Ramboehm
Marchini, A.Investigation
;
2016-01-01
Abstract
Photometric observations of the main-belt asteroids 5318 Dientzenhofer and 9083 Ramboehm were made in 2016 March and 2015 December, respectively. Analysis of the data found a bimodal lightcurve with a synodic rotation period of 8.062 ± 0.002 h for 5318 Dientzenhofer. A trimodal lightcurve with synodic period of 10.199 ± 0.004 h for 9083 Ramboehm was found to be the most likely solution.
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https://hdl.handle.net/11365/1082133