论文标题

2019年8月对木星的影响的破碎模型

Fragmentation modelling of the August 2019 impact on Jupiter

论文作者

Sankar, Ramanakumar, Palotai, Csaba, Hueso, Ricardo, Delcroix, Marc, Chappel, Ethan, Sanchez-Lavega, Agustin

论文摘要

2019年8月7日,在木星上观察到了持久的影响闪光灯。分析了此事件的视频以获得光曲线并确定能量释放和初始质量。我们发现,影响器的总能源为96-151美元的TNT $ kilotons,相当于最初的质量在$ 190-260 $吨之间,直径在4-10美元之间。我们开发了一个碎片模型,以模拟物体的大气破裂并重现灯光曲线。我们对三种不同的材料进行建模:彗星,石质和金属,速度为$ 60 $,$ 65 $和70美元/s/s/s $ km/s,以确定撞击物体的材料构成。较慢的箱子最适合强,金属物体,而较快的情况则需要较弱的材料。

On 7th August 2019, an impact flash lasting $\sim1$s was observed on Jupiter. The video of this event was analysed to obtain the lightcurve and determine the energy release and initial mass. We find that the impactor released a total energy of $96-151$ kilotons of TNT, corresponding to an initial mass between $190-260$ metric tonnes with a diameter between $4-10$m. We developed a fragmentation model to simulate the atmospheric breakup of the object and reproduce the lightcurve. We model three different materials: cometary, stony and metallic at speeds of $60$, $65 $ and $70$ km/s to determine the material makeup of the impacting object. The slower cases are best fit by a strong, metallic object while the faster cases require a weaker material.

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