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Waiting to make an impact: a probable excess of near-Earth asteroids in 2018 LA-like orbits

机译:等待产生影响:2018年类似LA轨道的近地小行星可能过剩

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Context. The discovery and tracking of 2018 LA marks only the third instance in history that the parent body of a fireball has been identified before its eventual disintegration in our atmosphere. The subsequent recovery of meteorites from 2018 LA was only the second time materials from outer space that reached the ground could be linked with certitude to a particular minor body. However, meteoroids like 2018 LA and its forerunners, 2008 TC_(3)and 2014 AA, are perhaps fragments of larger members of the near-Earth object (NEO) population. As the processes leading to the production of such fragments are unlikely to spawn just one meteoroid per event, it is important to identify putative siblings and plausible candidates from which the observed meteoroids might have originated. Aims. Here, we study the pre-impact orbital evolution of 2018 LA to place this meteoroid within the dynamical context of other NEOs that follow similar trajectories. Methods. Our statistical analyses are based on the results of direct N -body calculations that use the latest orbit determinations and include perturbations by the eight major planets, the Moon, the barycentre of the Pluto–Charon system, and the three largest asteroids. A state-of-the-art NEO orbit model was used to interpret our findings and a randomization test was applied to estimate their statistical significance. Results. We find a statistically significant excess of NEOs in 2018 LA-like orbits; among these objects, we find one impactor, 2018 LA, and the fourth closest known passer-by, 2018 UA. A possible connection with the χ -Scorpiids meteor shower is also discussed. The largest known NEO with an orbit similar to that of 2018 LA is the potentially hazardous asteroid (454100) 2013 BO_(73)and we speculate that they both originate from a common precursor via a collisional cascade. Conclusions. Future spectroscopic observations of 454100 and other NEOs in similar orbits may confirm or deny a possible physical relationship with 2018 LA.
机译:上下文。对2018 LA的发现和追踪仅标志着火球的母体在其最终在我们的大气中解体之前已经被识别出的历史上的第三次实例。随后从2018 LA回收陨石,这只是第二次将外层空间到达地面的材料与特定的次要物体联系起来。但是,像2018 LA及其先驱者,2008 TC_(3)和2014 AA之类的流星体,可能是近地天体(NEO)种群较大成员的碎片。由于导致此类碎片产生的过程不太可能在每个事件中仅产生一个流星体,因此,重要的是要识别出观察到的流星体可能来自的假定兄弟姐妹和可能的候选者。目的在这里,我们研究了2018 LA的撞击前轨道演变,以将该流星体置于遵循类似轨迹的其他NEO的动力学环境中。方法。我们的统计分析是基于使用最新轨道确定的直接N体计算的结果,其中包括八个主要行星,月球,冥王星-Charon系统的重心以及三个最大的小行星的扰动。使用最新的NEO轨道模型来解释我们的发现,并应用随机检验来估计其统计意义。结果。我们发现,在2018年类似LA的轨道上,近地天体存在统计学上的显着增加;在这些对象中,我们找到了一个撞击物,即2018 LA,以及排名第四的最接近的行人,即2018 UA。还讨论了与χ-蝎子流星雨的可能联系。已知最大的,与2018 LA相似的NEO轨道是潜在危险的小行星(454100)2013 BO_(73),我们推测它们都是通过碰撞级联起源于共同的前体。结论。未来在类似轨道上对454100和其他近地天体的光谱观察可能证实或否认与2018 LA的可能物理关系。

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