近地彗星 7P/Pons-Winnecke 的演变状态

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Solar System Research Pub Date : 2024-07-12 DOI:10.1134/s003809462470028x
A. O. Novichonok, A. A. Shmal’ts, S. V. Nazarov, A. S. Pozanenko, E. V. Novichonok, M. A. Tereshina, V. A. Voropaev
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摘要

摘要7P/Pons-Winnecke 是一颗近地短周期彗星,活动水平中等。在本文中,我们分析了在 2021 年对这颗彗星的一次有利观测中进行的观测,结果表明它是一颗过渡性老化彗星。当彗星接近太阳时,在 RON = 1.76 ± 0.1 AU 的距离上开始升华,并持续约 13 个月,这显然是由残余的水冰储备造成的。即使在近日点,彗星的尘埃产生率也不高(150 千克/秒),彗核区域 1.4% 的活跃部分足以提供这种质量损失。这颗彗星的测光年龄为 PAGE = 54.4 彗年;结合 ASEC(1;1) = 5.5m 的光曲线振幅,这一年龄相当于一颗过渡性中年彗星的状态。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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The Evolutionary State of Near-Earth Comet 7P/Pons–Winnecke

Abstract

7P/Pons–Winnecke is a near-Earth short-period comet of a moderate activity level. In this paper, we present the analysis of observations performed during a favorable apparition of the comet in 2021, indicating its status as a transitional ageing comet. The sublimation starts when the comet is close to the Sun, at a distance of RON = 1.76 ± 0.1 AU, and continues for ~13 months, which is apparently caused by residual reserves of water ice. The dust production rate of the comet is not high even at perihelion (<150 kg/s), and the 1.4-percent active portion of the nucleus area is sufficient to provide this mass loss. The photometric age of the comet is PAGE = 54.4 comet years; being combined with a light curve amplitude of ASEC(1;1) = 5.5m, this age corresponds to the state of a transitional middle-aged comet.

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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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