The Process of Formation of a Single Star System for Gravitational Compression of a Gas-dust Cloud in Outer Space

A. Belyaev
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引用次数: 1

Abstract

In this paper it is shown that in the process of formation of a single star system favorable conditions are created for the appearance of the planetary system due to the collision of the oppositely moving condensed dust zones from the newly born star and falling onto it from the periphery. A hypothetical version of the possible structure of the core of a single star born in a rarefied gas-dust cloud, explaining the cause of the mismatch of the axis of rotation of the star and the dipole magnetic field, is proposed. An assumption is made about the causes of the appearance of a directed orbital motion of planets that are not related to external perturbations of the initial gas-dust cloud.
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外太空气体尘埃云重力压缩下单星系统的形成过程
本文指出,在单星系统的形成过程中,由于新生恒星的反向运动的凝聚尘埃带和从外围落向行星系统的碰撞,为行星系统的出现创造了有利条件。在稀薄的气尘云中诞生的一颗恒星的核心可能结构的一个假设版本,解释了恒星旋转轴和偶极磁场不匹配的原因,被提出。对行星定向轨道运动出现的原因作了一个假设,这与初始气体尘埃云的外部扰动无关。
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