论文标题
小行星(3200)Phaethon:极化,光度和光谱观测的结果
Asteroid (3200) Phaethon: results of polarimetric, photometric, and spectral observations
论文作者
论文摘要
We present results of polarimetric, photometric, and spectral observations of the near-Earth asteroid (3200) Phaethon carried out at the 6-m BTA telescope of the Special Astrophysical Observatory and the 2.6-m and 1.25-m telescopes of the Crimean Astrophysical Observatory over a wide range of phase angles during its close approach to the Earth at the end of 2017 (19-135 deg) and in 2020在α= 52.2度。使用我们的文献数据中的其他可用性,我们发现在相角124度下,V频段中Phaethon的最大线性极化度为45%。使用依赖性(偏光斜率 - 阿尔贝托),我们发现小行星phaethon的几何反照率为0.06。该值落入由不同方法确定的小行星的反照率值范围。小行星的平均颜色指数U-B = 0.207和B-V = 0.639分别以HeliePentric和GeePentric距离得出1.077 AU和0.102 AU。根据获得的绝对幅度和几何反照率,估计Phaethon的有效直径,等于6.8 km。使用由富含Mg的硅酸盐(90%)和无定形碳(10%)组成的共轭随机高斯颗粒的SH-Matrix模型获得了观察到的偏光数据的最佳拟合。
We present results of polarimetric, photometric, and spectral observations of the near-Earth asteroid (3200) Phaethon carried out at the 6-m BTA telescope of the Special Astrophysical Observatory and the 2.6-m and 1.25-m telescopes of the Crimean Astrophysical Observatory over a wide range of phase angles during its close approach to the Earth at the end of 2017 (19-135 deg) and in 2020 at α= 52.2 deg. Using our and other available in literature data, we found that the maximum degree of linear polarization of Phaethon in the V band is 45% at the phase angle 124 deg. Using the dependence (polarimetric slope-albedo) we have found the geometric albedo of asteroid Phaethon to be 0.06. This value falls into the lower range of albedo values for asteroids determined by different methods. The mean color indices U-B=0.207 and B-V=0.639 of the asteroid are derived at heliocentric and geocentric distances 1.077 au and 0.102 au, respectively. The effective diameter of Phaethon is estimated from obtained absolute magnitude and geometrical albedo, it is equal to 6.8 km. The best fit to the observed polarimetric data was obtained with the Sh-matrix model of conjugated random Gaussian particles composed of Mg-rich silicate (90%) and amorphous carbon (10%).