rotation period |
rot_per |
6.21 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Result based on fragmentary lightcurve(s), may be completely wrong. Published Reference List: [Ortiz, J.L.; Gutierrez, P.J.; Casanova, V.; Sota, A. (2003) Astron. Astrophys. 407, 1149-1155.] [Ivanova, V.; Borisov, G.; Bel'skaya, I. (2005) Abstr. IAU Symp. 229, p. 54.] |