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Studying Close Approaches for a Cloud of Particles Considering Atmospheric Drag

机译:研究考虑大气阻力的粒子云的接近方法

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The present paper has the goal of studying close approaches between a planet and a group of particles. The mathematical model includes the presence of the atmosphere of the planet. This cloud is assumed to be created by the passage of the spacecraft in the atmosphere of the planet, which can cause the explosion of the spacecraft. The system is assumed to be formed by the Sun, the planet, and the spacecraft that explodes and becomes a cloud of particles. The Sun and the planet are assumed to be in circular orbits and the motion is planar. The equations of motion are the ones given by the circular planar restricted three-body problem combined with the forces given by the atmospheric drag. In the numerical simulations, the planet Jupiter is the celestial body used for the close approaches. The initial positions and velocities of the spacecraft and the particles are specified at the periapsis, because it is assumed that this is the point where the explosion occurs.
机译:本文的目的是研究行星和一组粒子之间的接近方法。数学模型包括行星大气的存在。假定该云是由航天器在行星大气中通过而产生的,这可能导致航天器爆炸。假定该系统由太阳,行星和宇宙飞船组成,它们爆炸并变成粒子云。假定太阳和行星处于圆形轨道,并且运动是平面的。运动方程是由圆形平面约束三体问题给出的方程,再加上大气阻力给出的方程。在数值模拟中,木星是用于近距离进近的天体。航天器和粒子的初始位置和速度是在围手术期指定的,因为假定这是爆炸发生的地点。

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