The possible dual nature of the asteroid (12499) 1998 FR47
G. Borisov, N. Todorovic, E. Vchkova-Bebekovska, A. Kostov, G., Apostolovska

TL;DR
This study analyzes the rotation, shape, and potential binary nature of asteroid (12499) 1998 FR47, revealing complex lightcurve patterns, possible binary characteristics, and its dynamical behavior near Mars resonances.
Contribution
It provides detailed lightcurve analysis, suggests the asteroid may be a non-synchronized binary, and explores its dynamical evolution within the asteroid belt.
Findings
Rotation period of ~6.17 hours
Possible binary system with periods ~3.08 or ~4.12 hours
Asteroid's orbit is near the 7:4 resonance with Mars
Abstract
We present the R-band lightcurves of the Flora family asteroid (12499) 1998 FR47, obtained in 2022 at two different astronomical sites: Bulgarian National Astronomical Observatory Rozhen (MPC Code 071) and Astronomical Station Vidojevica (MPC Code C89). The quadramodal lightcurves reveal a rotation period of 6.172+/-0.003 h and an amplitude of about 0.44 mag. Using the lightcurve inversion method, with the combination of our dense lightcurves and the sparse data from Gaia DR3, we found the sidereal period, an indication of a retrograde rotation of (12499) and its low-convex resolution shape. Nonetheless, the unusual shape of the quadramodal lightcurve and its additional analysis reveals two possible periods, 3.0834+/-0.0085 h and 4.1245+/-0.0151 h, making the suspect that the asteroid might be a non-synchronised wide binary system. Spectral analysis of the asteroid using data from the…
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