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Study of photometric phase curve with new brightness model:refining phase function system parameters of asteroid(107)Camilla
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作者 Yi-Bo Wang Xiao-Bin Wang Ao Wang 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2016年第9期117-122,共6页
We characterize the morphology of the photometric phase curve model of an asteroid with a three- parameter magnitude phase function H - G1 - G2 system by considering the effect of brightness variation arising from a t... We characterize the morphology of the photometric phase curve model of an asteroid with a three- parameter magnitude phase function H - G1 - G2 system by considering the effect of brightness variation arising from a triaxial ellipsoid representing the asteroid's shape. Applying this new model and a Markov Chain Monte Carlo method, we refine the photometric phase curve of asteroid (107) Camilla and obtain its absolute magnitude H = 7.026-0.054^+0.052 mag, and phase function parameters G1=0.489-0.044^+0.043 and G2 = 0.259-0.023^+0.023.Meanwhile, we also determine (107) Camilla's orientation of pole (74.1°-4.5°^+4.3°,50.2°-5.0°^+5.4°). with rotational period of 4.843928-0.000001^+0.000001 h, and axial ratios a/b : 1.409-0.020^+0.020 And b/c =1.249-0.060^+0.063. Furthermore, according to the values of phase function parameters G1 and G2, we infer that asteroid (107) Camilla is an X-type asteroid. 展开更多
关键词 minor planets asteroids general phase curve -- minor planets asteroids individual (107)camilla -- techniques PHOTOMETRIC
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