文章基本信息

标题：Split Active Asteroid P/2016 J1 (PANSTARRS)
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作者：Man-To Hui (許文韜) ; David Jewitt ; Xinnan Du (杜辛楠) 等
期刊名称：The Astronomical journal
印刷版ISSN：0004-6256
电子版ISSN：1538-3881
出版年度：2017
卷号：153
期号：4
DOI：10.3847/1538-3881/aa6039
语种：English
出版社：American Institute of Physics
摘要：We present a photometric and astrometric study of the split active asteroid P/2016 J1 (PANSTARRS). The two components (hereafter J1-A and J1-B) separated either ~1500 days (2012 May to June) or 2300 days (2010 April) prior to the current epoch, with a separation speed V sep = 0.70 ± 0.02 m s−1 for the former scenario and 0.83 ± 0.06 m s−1 for the latter. Keck photometry reveals that the two fragments have similar, Sun-like colors that are comparable to the colors of primitive C- and G-type asteroids. With a nominal comet-like albedo, p R = 0.04, the effective, dust-contaminated cross sections are estimated to be 2.4 km2 for J1-A and 0.5 km2 for J1-B. We estimate that the nucleus radii lie in the range 140 R N 900 m for J1-A and 40 R N 400 m for J1-B. A syndyne–synchrone simulation shows that both components have been active for 3–6 months, by ejecting dust grains at speeds ~0.5 m s−1 with rates ~1 kg s−1 for J1-A and 0.1 kg s−1 for J1-B. In its present orbit, the rotational spin-up and devolatilization times of 2016 J1 are very small compared to the age of the solar system, raising the question of why this object still exists. We suggest that ice that was formerly buried within this asteroid became exposed at the surface, perhaps via a small impact, and that sublimation torques then rapidly drove it to breakup. Further disintegration events are anticipated owing to the rotational instability.
关键词：methods: data analysis;minor planets; asteroids: general;minor planets; asteroids: individual (P/2016 J1)