Photometric observations of five asteroids were made in order to acquire lightcurves for shape/spin axis modeling. The synodic period and lightcurve amplitude were found for 102 Miriam: 23.63 ± 0.01 h, 0.14 mag; 635 Vundtia: 11.784 ± 0.004 h, 0.20 mag; 1342 Brabantia: 4.175 ± 0.001 h, 0.13 mag; 2346 Lilio: 3.0290 ± 0.0005 h, 0.18 mag; (153201) 2000 WO107: 5.026 ± 0.001 h, 1.14 mag.
Collaborative Asteroid Photometry from UAI: 2020 October-December
Aceti Pietro;
2021-01-01
Abstract
Photometric observations of five asteroids were made in order to acquire lightcurves for shape/spin axis modeling. The synodic period and lightcurve amplitude were found for 102 Miriam: 23.63 ± 0.01 h, 0.14 mag; 635 Vundtia: 11.784 ± 0.004 h, 0.20 mag; 1342 Brabantia: 4.175 ± 0.001 h, 0.13 mag; 2346 Lilio: 3.0290 ± 0.0005 h, 0.18 mag; (153201) 2000 WO107: 5.026 ± 0.001 h, 1.14 mag.File in questo prodotto:
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