Photometric observations of the main-belt asteroids 2496 Fernandus, 2727 Paton, and 69971 Tanzi were made by the authors from 2019 January 3 to April 5. Analysis found bimodal lightcurves for each one. The most likely synodic periods are: 2496 Fernandus, 2.807 ± 0.001 h; 2727 Paton, 5.324 ± 0.001 h; and 69971 Tanzi, 32.540 ± 0.009 h.
Salvaggio, F., Marchini, A., Papini, R., Banfi, M. (2019). Lightcurve and Rotation Period Determination for 2496 Fernandus, 2727 Paton, and 69971 Tanzi. THE MINOR PLANET BULLETIN, 46(3), 340-341.
Lightcurve and Rotation Period Determination for 2496 Fernandus, 2727 Paton, and 69971 Tanzi
Marchini, Alessandro
Membro del Collaboration Group
;
2019-01-01
Abstract
Photometric observations of the main-belt asteroids 2496 Fernandus, 2727 Paton, and 69971 Tanzi were made by the authors from 2019 January 3 to April 5. Analysis found bimodal lightcurves for each one. The most likely synodic periods are: 2496 Fernandus, 2.807 ± 0.001 h; 2727 Paton, 5.324 ± 0.001 h; and 69971 Tanzi, 32.540 ± 0.009 h.
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Utilizza questo identificativo per citare o creare un link a questo documento:
https://hdl.handle.net/11365/1165378