用肉眼观察木星的白天可见度

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
Ki-Won Lee, Byeong-Hee Mihn, Sang Hyuk Kim, Young Sook Ahn
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引用次数: 0

摘要

本研究检视韩国在日光下观测木星的历史记录,以估计在日光下无光学辅助观测天体的经验极限星等。我们利用《朝鲜王朝实录》、《成正院日记》、《东宫日记》等资料,确定了朝鲜王朝(1392 ~ 1910年)的40个白天观测木星的事例。利用天文算法和现代星历,我们计算了日出、凌日和日落时间,以确定观测时间,确定事件是发生在白天还是黄昏。此外,我们还确定了每次记录事件期间木星的方位和大小,以验证观测到的现象的方向和亮度。我们的分析得出了以下主要发现:(1)木星的白天目击记录集中在16和17世纪,对应于太阳活动极小期的延长。这些观测发生在光天化日之下,而不是黄昏时分。(3)白日观测天体的极限星等至少为-2.1等。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Daylight Visibility of Jupiter with the Naked Eye

Daylight Visibility of Jupiter with the Naked Eye

This study examines Korean historical records of daylight sightings of Jupiter to estimate the empirical limiting magnitude for observing celestial bodies without optical aid during daylight. Using sources such as Joseonwangjo-Sillok (The Veritable Records of the Joseon Dynasty), Seungjeongwon-Ilgi (The Daily Records of the Royal Secretariat of the Joseon Dynasty), and Donggung-Ilgi (The Daily Records of the Royal Education Bureau for the Crown Prince of the Joseon Dynasty), we identified 40 instances of daylight observations of Jupiter during the Joseon dynasty (1392–1910). Employing astronomical algorithms and modern ephemeris, we calculated sunrise, solar transit, and sunset times to identify the observation hour, confirming whether the events occurred during daytime or twilight. Additionally, we determined the azimuth and magnitude of Jupiter during each recorded event to verify the direction and brightness of the observed phenomenon. Our analysis yielded the following key findings: (1) The records of daylight sightings of Jupiter are concentrated in the 16th and 17th centuries, corresponding to prolonged periods of solar activity minima. (2) These observations occurred during broad daylight rather than twilight. (3) The limiting magnitude for unaided daylight observations of a celestial body is at least –2.1.

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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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