A Dormant Captured Oort Cloud Comet Awakens: (18916) 2000 OG44

Colin Orion Chandler, William J. Oldroyd, Chadwick A. Trujillo, Dmitrii E. Vavilov and William A. Burris
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Abstract

We report the discovery of activity emanating from (18916) 2000 OG44 (alternately designated 1977 SD), a minor planet previously reported to be both an extinct comet and an asteroid on a cometary orbit. We observed 2000 OG44 with a thin tail oriented towards the coincident antisolar and antimotion vectors (as projected on the sky) in images we acquired on UT 2023 July 24 and 26 with the Apache Point Observatory 3.5 m Astrophysical Research Consortium telescope (New Mexico, USA). We also include observations made in Arizona with the Vatican Advanced Technology Telescope at the Mount Graham International Observatory and the Lowell Observatory Lowell Discovery Telescope near Happy Jack. We performed dynamical simulations that reveal 2000 OG44 most likely originated in the Oort cloud, arriving within the last 4 Myr. We find 2000 OG44, which crosses the orbits of both Jupiter and Mars, is at present on an orbit consistent with a Jupiter-family comet. We carried out thermodynamical modeling that informed our broader diagnosis that the observed activity is most likely due to volatile sublimation.
一颗休眠被捕获的奥尔特云彗星苏醒:(18916)2000 OG44
我们报告了从(18916)2000 OG44(或称为1977 SD)发出的活动的发现,这是一颗小行星,以前报道过既是一颗灭绝的彗星,也是一颗在彗星轨道上运行的小行星。在7月24日和26日的UT 2023上,我们用阿帕奇点天文台3.5米天体物理研究联盟望远镜(美国新墨西哥州)拍摄的图像中,我们用一条指向重合的反太阳和反运动矢量的细尾巴观测了2000 OG44。我们还包括在亚利桑那州用格雷厄姆山国际天文台的梵蒂冈先进技术望远镜和快乐杰克附近的洛厄尔天文台洛厄尔发现望远镜进行的观测。我们进行了动力学模拟,结果显示2000og44极有可能起源于奥尔特云,在过去的4myr内到达。我们发现2000 OG44,它穿过木星和火星的轨道,目前的轨道与木星家族的彗星一致。我们进行了热力学建模,这为我们更广泛的诊断提供了信息,即观测到的活动最有可能是由于挥发性升华。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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