Discovery of Jupiter Family Comet 2011 UG104 Through AI Enhanced Citizen Science

Jarod A. DeSpain, C. O. Chandler, Nima Sedaghat, William J. Oldroyd, C. Trujillo, William A. Burris, Henry H. Hsieh, Jay K. Kueny, Kennedy A. Farrell, Mark Jesus Mendoza Magbanua, Scott S. Sheppard, Michele T. Mazzucato, Milton K. D. Bosch, Tiffany Shaw-Diaz, Virgilio Gonano, Al Lamperti, José A. da Silva Campos, Brian L. Goodwin, Ivan A. Terentev, Charles J. A. Dukes
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Abstract

We report the discovery of cometary activity from minor planet 2011 UG104, which we classify as a Jupiter Family Comet (JFC). This discovery was aided by our Artificial Intelligence (AI) classification system: TailNet. JFC's, short-period comets with eccentric Jupiter-crossing orbits, originate from the Kuiper Belt and thus give us unique insight into the composition and distribution of volatiles in the outer solar system, past and present. Our AI assistant TailNet first classified 2011 UG104 as active, which was affirmed by Citizen Scientists on our NASA Partner Program Active Asteroids. Through further archival image searches our science team found evidence of activity on 2011 UG104 on three separate observations from 2021 February to 2021 April (81.°8 < f < 95.°0). 
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通过人工智能增强公民科学发现木星家族彗星 2011 UG104
我们报告发现了小行星 2011 UG104 的彗星活动,并将其归类为木星家族彗星(JFC)。这一发现得益于我们的人工智能(AI)分类系统:TailNet。木星家族彗星是一种偏心木星交叉轨道的短周期彗星,源自柯伊伯带,因此能让我们对外太阳系过去和现在的挥发物组成和分布情况有独特的见解。我们的人工智能助手TailNet首先将2011 UG104归类为活跃小行星,这一点得到了NASA合作伙伴计划 "活跃小行星 "中的公民科学家的肯定。通过进一步的档案图像搜索,我们的科学团队在 2021 年 2 月至 2021 年 4 月(81.°8 < f < 95.°0)的三次单独观测中发现了 2011 UG104 活动的证据。
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