天琴座流星雨:一个历史的视角

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
M.J. Martínez Usó , F.J. Marco Castillo , J.A. López Ortí
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引用次数: 0

摘要

四月天琴座流星雨是历史上有记录以来最古老的连续流星雨,可以追溯到公元前687年。在20世纪之前,历史资料只提供了两年的强烈活动和多达9个可能的额外事件的报告。目前,流星雨的活跃度较低,但在20世纪,它有过明显的发作,似乎以12年或60年的时间间隔重复发生。更早的爆发也可能以与这一时期一致的频率发生。在其他流星雨中也有爆发的活动。经典的解释是它们与母彗星离地球很近有关,在20世纪的最后几年被证明是错误的,这在四月天琴座彗星的例子中也很清楚,它的母彗星是C/1861 G1(撒切尔),轨道周期约为400年。我们之前的研究使我们在过去的2000年里编制了一个可能的四月天琴座彗星的额外列表。本文有两个目的。首先,我们列出了可能的天琴座星,这将大大增加迄今为止考虑的历史观测的数量。其次,研究历史资料是否与有关Lyrids的主要理论和最新研究相吻合。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Lyrids meteor shower: A historical perspective

The April Lyrid meteor shower is the oldest meteor shower ever recorded continuously throughout history, dating as far back as 687 BC. Before the 20th century, historical sources only provided reports of two years of strong activity and up to nine possible additional events. Currently, the shower has low activity, but it has had significant episodes that, during the 20th century, seem to repeat at time intervals that are multiples of 12yr or 60 yr. Earlier outbursts may have also occurred with a frequency consistent with this period. Outbursts of activity are also known in other meteor showers. The classical explanation that they are correlated to the close proximity of the parent comet to the Earth was proven wrong in the last years of the 20th century and this is also clear in the case of the April Lyrids, whose parent comet is C/1861 G1 (Thatcher), with an orbital period of about 400 yr. Our previous research has led us to compile an additional list of possible April Lyrids in the last 2000 years. This paper has two objectives. First, to present the list of possible Lyrids that we have compiled that would significantly increase the number of historical observations considered to date. Secondly, to study if the historical data fit well with the main theories and recent studies concerning the Lyrids.

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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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