29P/Schwassmann-Wachmann 1 号彗星异常爆发活动的解释:关于大型卫星存在的假设

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Yu. D. Medvedev, S. R. Pavlov
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引用次数: 0

摘要

摘要 我们用卫星在其轨道的边缘接触彗核表面来解释 29P/Schwassmann-Wachmann 1 号彗星的异常爆发活动。假设卫星在偏心轨道上运动,大量尘埃在与彗核尘埃层碰撞后被抛射出来,这些尘埃对光线的反射导致亮度的周期性爆发(BAA 2023)。根据卫星穿透尘埃层的深度,会出现不同强度的彗星亮度爆发。通过位置观测对彗星轨道进行改进,可以根据光心偏移确定物质喷射的优先方向,我们将其解释为最大卫星在围心的速度矢量方向。我们对卫星与彗核尘埃层接触引起的尘埃粒子喷射和随后的运动进行了数值模拟,模拟结果解释了在彗星上观测到的结构的形成:尘埃喷流及其镜面对称性,以及从彗核表面喷射物质的区域范围。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Explanation of the Anomalous Outburst Activity of Comet 29P/Schwassmann–Wachmann 1: The Hypothesis about the Existence of Large Satellites

Explanation of the Anomalous Outburst Activity of Comet 29P/Schwassmann–Wachmann 1: The Hypothesis about the Existence of Large Satellites

Explanation of the Anomalous Outburst Activity of Comet 29P/Schwassmann–Wachmann 1: The Hypothesis about the Existence of Large Satellites

We explain the anomalous outburst activity of comet 29P/Schwassmann–Wachmann 1 by the existence of satellites touching the surface of the comet nucleus at the pericenters of their orbits. It is assumed that the satellites move in eccentric orbits and a large amount of dust, the reflection of light from which causes periodic outbursts in brightness (BAA 2023), is ejected as a result of their collisions with the dust layer of the nucleus. Depending on the depth of penetration of the satellites into the dust layer, outbursts in comet brightness of various intensities occur. An improvement of the comet orbit by invoking positional observations allows the preferred direction of the ejection of material to be determined from the photocenter offset, which we interpret as the direction of the velocity vector of the largest satellite at the pericenter. The results of our numerical simulations of the ejection and subsequent motion of dust particles caused by the contact of the satellite with the dust layer of the comet nucleus explain the formation of the structures observed in the comet: the dust jets and their mirror symmetry as well as the extent of the region of material ejection from the surface of the comet nucleus.

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来源期刊
CiteScore
1.70
自引率
22.20%
发文量
0
审稿时长
6-12 weeks
期刊介绍: Astronomy Letters is an international peer reviewed journal that publishes the results of original research on all aspects of modern astronomy and astrophysics including high energy astrophysics, cosmology, space astronomy, theoretical astrophysics, radio astronomy, extragalactic astronomy, stellar astronomy, and investigation of the Solar system.
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