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Optical observations of NEA 3200 Phaethon (1983 TB) during the 2017 apparition SCI
  • 김명진;이희재;이상민;김동흔;F. Yoshida;P. Bartczak;G. Dudziski;박진태;최영준;문홍규;임홍서;최진;최은정;윤요라;A. Serebryanskiy;M. Krugov;I. Reva;K. E. Ergashev;O. Burkhonov;S. A. Ehgamberdiev;Y. Turayev;Z.Y. Lin;T. Arai;K. Ohtsuka;T. Ito;S. Urakawa;M. Ishiguro
  • 2018-11-14
  • ASTRONOMY & ASTROPHYSICS 619 : A123-1~A123-8
Context. The near-Earth asteroid 3200 Phaethon (1983 TB) is an attractive object not only from a scientific viewpoint but also because of JAXA’s DESTINY+ target. The rotational lightcurve and spin properties were investigated based on the data obtained in the ground-based observation campaign of Phaethon. Aims. We aim to refine the lightcurves and shape model of Phaethon using all available lightcurve datasets obtained via optical observation, as well as our time-series observation data from the 2017 apparition. Methods. Using eight 12-m telescopes and an optical imager, we acquired the optical lightcurves and derived the spin parameters of Phaethon. We applied the lightcurve inversion method and SAGE algorithm to deduce the convex and non-convex shape model and pole orientations. Results. We analysed the optical lightcurve of Phaethon and derived a synodic and a sidereal rotational periods of 3.6039 h, with an axis ratio of a?b = 1.07. The ecliptic longitude (λp) and latitude (βp) of the pole orientation were determined as (308°, ?52°) and (322°, ?40°) via two independent methods. A non-convex model from the SAGE method, which exhibits a concavity feature, is also presented.