Detection of the Activity of 468861 (2013 LU28)
文献类型:期刊论文
作者 | Xu XM(徐小萌)3,4,5![]() ![]() ![]() |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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出版日期 | 2025-03-01 |
卷号 | 25期号:3 |
关键词 | Kuiper Belt objects: individual (2013 LU28) techniques: photometric minor planets, asteroids: individual (2013 LU28) |
ISSN号 | 1674-4527 |
DOI | 10.1088/1674-4527/adbea2 |
产权排序 | 第3完成单位 |
文献子类 | Article |
英文摘要 | The perihelion of long-period comets places them near the Sun so they may exhibit activity. Before 2013 LU28 reached its perihelion, we performed a continuous observation to detect possible activity. Using the Lijiang 2.4 m telescope with a Johnson R filter, we measured the brightness of 2013 LU28 from 2024 January 3 to April 13. The instrumental magnitudes were subsequently transformed into the Pan-STARRS r system. Due to the noticeable descending trend in the absolute magnitude, we verified the cometary activity and constrained some photometric properties of 2013 LU28. Consequently, the increased cross-sectional area had a rate of 42.8 km(2) day(-1), and the corresponding mass-loss rate was 2.64 kg s(-1) with the assumption of a dust-particle size a=10 mu m and the density rho = 400 kg m(-3). We estimated the nucleus radius as 0.11 less than or similar to r(n) less than or similar to 0.21 km for CO sublimation and 0.20 less than or similar to r(n) less than or similar to 0.71 km for CO2 sublimation and the grain size of 2013 LU28 was a(c) similar or equal to 117.95 mu m for CO and a(c) similar or equal to 7.57 mu m for CO2. The long-term observations provided in this paper will offer significant value for investigating the mechanisms driving the activity of 2013 LU28. |
学科主题 | 天文学 ; 太阳与太阳系 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | COMET ; PHOTOMETRY |
资助项目 | Center for Astronomical Mega-Science, Chinese Academy of Sciences; CAS; People's Government of Yunnan Province - Civil Aerospace pre-research project[D020302]; National Natural Science Foundation of China[U12150009]; National Natural Science Foundation of China[12150009]; CAS Light of West China Program; China Manned Space Project |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001455964600001 |
出版者 | IOP Publishing Ltd |
资助机构 | Center for Astronomical Mega-Science, Chinese Academy of Sciences ; CAS ; People's Government of Yunnan Province - Civil Aerospace pre-research project[D020302] ; National Natural Science Foundation of China[U12150009, 12150009] ; CAS Light of West China Program ; China Manned Space Project |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/28243] ![]() |
专题 | 云南天文台_丽江天文观测站(南方基地) |
作者单位 | 1.University of Chinese Academy of Sciences, Beijing 100049, China 2.State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau 999078, China; 3.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China; 4.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China; 5.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China; |
推荐引用方式 GB/T 7714 | Xu XM,Zhang XL,Wu, Yun-Zhao,et al. Detection of the Activity of 468861 (2013 LU28)[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2025,25(3). |
APA | 徐小萌,张西亮,Wu, Yun-Zhao,&范相钰.(2025).Detection of the Activity of 468861 (2013 LU28).RESEARCH IN ASTRONOMY AND ASTROPHYSICS,25(3). |
MLA | 徐小萌,et al."Detection of the Activity of 468861 (2013 LU28)".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 25.3(2025). |
入库方式: OAI收割
来源:云南天文台
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