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首页> 外文期刊>Astronomy and astrophysics >The role of Mab as a source for the μ ring of Uranus
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The role of Mab as a source for the μ ring of Uranus

机译:Mab作为天王星μ环的来源的作用

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Context. We previously analysed how the solar radiation force combined with the planetary oblateness changes the orbital evolution of a sample of dust particles located at the secondary ring system of Uranus. Both effects combined with the gravitational perturbations of the close satellites lead to the depletion of these dust particles through collisions on the surfaces of these satellites on a timescale of hundreds of years. Aims. In this work we investigate if the impacts of interplanetary dust particles (IDPs) onto Mab’s?surface can produce sufficient particles to replenish the μ?ring population. Methods. We first analysed through numerical simulations the evolution of a sample of particles ejected from the surface of Mab and computed the lifetime of the grains when the effects of the solar radiation pressure and the planetary oblateness are taken into account. Then we estimated the mass production rate due to the impacts of IDPs following a previously established algorithm, and used this value to determine the time necessary to accumulate an amount of particles comparable with the mass of the μ?ring. Results. Based on an estimate of the flux of interplanetary particles and on the surface properties of Mab it is expected that the satellite supplies material to the ring at a rate of??~3?g/s. Meanwhile, our?numerical model showed that the ejected particles are removed from the system through collisions with the satellite, and the mean lifetime of the grains may vary from?320 to?1500?years, depending on the radius of the?particle. Conclusions. The time necessary to accumulate the mass of the μ?ring via ejection from Mab is much shorter than the mean lifetime of the particles, and a stationary regime is not reached. If?the ring is kept in a steady state, other effects such as the electromagnetic force and/or the existence of additional bodies may play a significant role in the dust balance, but the current lack of information about the environment renders modelling these effects unfeasible.
机译:上下文。我们之前曾分析过太阳辐射力与行星扁率的结合如何改变位于天王星次级环系统的尘埃颗粒样品的轨道演变。这两种效应与近身卫星的引力扰动相结合,导致在数百年的时间尺度上,这些尘埃颗粒通过在这些卫星表面上的碰撞而耗竭。目的在这项工作中,我们研究了行星际尘埃粒子(IDP)对Mab表面的影响是否可以产生足够的尘埃来补充μring种群。方法。我们首先通过数值模拟分析了从Mab表面喷出的颗粒样品的演化过程,并在考虑了太阳辐射压力和行星扁率的影响下计算了颗粒的寿命。然后,我们按照先前建立的算法估算了由于IDP的影响而产生的批量生产速度,并使用该值来确定积累与微环质量相当的颗粒数量所需的时间。结果。基于对行星际粒子通量的估计以及基于Mab的表面性质,可以预期卫星以??〜3?g / s的速度向环提供材料。同时,我们的数值模型表明,通过与卫星的碰撞将喷射出的粒子从系统中去除,根据粒子的半径,粒子的平均寿命可能在320至1500年之间变化。结论。通过从Mab喷射来累积微环质量所需的时间比粒子的平均寿命短得多,并且没有达到固定状态。如果环保持稳定状态,则其他影响(例如电磁力和/或其他物体的存在)可能在粉尘平衡中起重要作用,但是当前缺乏有关环境的信息,因此无法对这些效果进行建模。

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