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Alpha Centauri System and Meteorites Origin

机译:半人马座α系统和陨石起源

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We propose a mathematical model for determining the probability of meteorite origin, impacting the earth. Our method is based on axioms similar to both the complex networks and emergent gravity. As a consequence, we are able to derive a link between complex networks and Newton’s gravity law, and as a possible application of our model we discuss several aspects of the Bacubirito meteorite. In particular, we analyze the possibility that the origin of this meteorite may be alpha Centauri system. Moreover, we find that in order for the Bacubirito meteorite to come from alpha Cen and be injected into our Solar System, its velocity must be reduced one order of magnitude of its ejected scape velocity from alpha Cen. There are several ways how this could happened, for example through collision with the Oort cloud objects (located outside the boundary of our Solar System), and/or through collisions within the Solar meteorites belt (located between Mars and Jupiter). We also argue that it may be interesting to study the Bacubirito meteorite from the perspective of the recently discovered Oumuamua object.
机译:我们提出了一个数学模型来确定陨石起源,撞击地球的可能性。我们的方法基于类似于复杂网络和新兴引力的公理。因此,我们能够得出复杂网络与牛顿引力定律之间的联系,并且作为我们模型的可能应用,我们讨论了杆菌属陨石的几个方面。特别是,我们分析了这种陨石的起源可能是半人马座星系的可能性。此外,我们发现,为了使芽孢杆菌陨石来自αCen并被注入到我们的太阳系中,必须将其速度降低到其从αCen射出的逸出速度的一个数量级。发生这种情况的方式有多种,例如通过与奥尔特云物体碰撞(位于太阳系边界之外)和/或通过太阳陨石带内碰撞(位于火星与木星之间)。我们还认为,从最近发现的Oumuamua物体的角度研究Bacubirito陨石可能是有趣的。

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