Cometary observations in light-polluted environments: a case study of interstellar comet 2I/Borisov

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Josep M. Trigo-Rodríguez, Damya Souami, Maria Gritsevich, Marcin Wesołowski, Gennady Borisov
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Abstract

Comets and asteroids have long captured human curiosity, and until recently, all documented examples belonged to our Solar System. That changed with the discovery of the first known interstellar object, 1I/2017 U1 (‘Oumuamua), in 2017. Two years later, on August 30, 2019, Gennady Borisov discovered a second interstellar object, 2019 Q4, which was officially designated 2I/Borisov. From its initial images, the object’s diffuse appearance hinted at its cometary nature. To better understand the photometric evolution of comet 2I/Borisov as it traveled through the inner Solar System, we compiled observations using medium-sized telescopes. This data is crucial for gaining insights into its size and composition, as well as how such objects, after millions of years in interstellar space, behave when exposed to the Sun’s radiation. Given that 2I/Borisov is the first interstellar comet ever observed, constraining its behavior is of great scientific interest. In this paper, we present photometric data gathered from observatories in Crimea and Catalonia, highlighting the importance of systematic photometric studies of interstellar objects using meter-class telescopes. Our observations showed a steady increase in the comet’s brightness as it approached perihelion, likely due to the slow sublimation of ices. Over the five-month pre-perihelion observation period, we did not detect any significant changes in magnitude. The analysis of observations reveals a steady increase in comet 2I/Borisov brightness as it approached perihelion, likely due to the sublimation of ices, with no observable outbursts during the five-month pre-perihelion period. Additionally, we discuss the challenges in ground-based observation of comets posed by light pollution today, particularly in urban areas, where visual observations are severely limited. Using sample surface brightness measurements, we demonstrate the impact of light pollution and outline the importance of systematic photometric studies for interstellar objects.

光污染环境下的彗星观测:星际彗星2I/Borisov的案例研究
彗星和小行星长期以来一直吸引着人类的好奇心,直到最近,所有记录在案的例子都属于我们的太阳系。随着2017年发现第一个已知的星际物体1I/2017 U1 (' Oumuamua),这种情况发生了变化。两年后的2019年8月30日,根纳季·鲍里索夫发现了第二个星际物体2019 Q4,正式命名为2I/鲍里索夫。从最初的图像来看,这个物体的扩散外观暗示了它的彗星性质。为了更好地了解彗星2I/Borisov在穿越太阳系内部时的光度演变,我们使用中型望远镜收集了观测结果。这些数据对于了解它的大小和组成,以及这些物体在星际空间中经过数百万年的暴露在太阳辐射下的行为是至关重要的。考虑到2I/Borisov彗星是有史以来观测到的第一颗星际彗星,限制它的行为具有很大的科学意义。在本文中,我们展示了从克里米亚和加泰罗尼亚的天文台收集的光度数据,强调了使用米级望远镜对星际物体进行系统光度研究的重要性。我们的观测显示,当彗星接近近日点时,它的亮度稳步增加,这可能是由于冰的缓慢升华。在近日点前5个月的观测期间,我们没有发现任何显著的星等变化。对观测结果的分析显示,随着2I/Borisov彗星接近近日点,它的亮度稳步增加,可能是由于冰的升华,在近日点前的五个月里没有观测到爆发。此外,我们还讨论了目前光污染给地面观测彗星带来的挑战,特别是在视觉观测严重受限的城市地区。利用样品表面亮度测量,我们展示了光污染的影响,并概述了对星际物体进行系统光度研究的重要性。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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