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“双形态卫星”受“双小行星重定向测试”撞击后抛射物的光变曲线和颜色。

Light curves and colours of the ejecta from Dimorphos after the DART impact.

机构信息

SETI Institute, Carl Sagan Center, Mountain View, CA, USA.

Unistellar, Marseille, France.

出版信息

Nature. 2023 Apr;616(7957):461-464. doi: 10.1038/s41586-023-05852-9. Epub 2023 Mar 1.

Abstract

On 26 September 2022, the Double Asteroid Redirection Test (DART) spacecraft struck Dimorphos, a satellite of the asteroid 65803 Didymos. Because it is a binary system, it is possible to determine how much the orbit of the satellite changed, as part of a test of what is necessary to deflect an asteroid that might threaten Earth with an impact. In nominal cases, pre-impact predictions of the orbital period reduction ranged from roughly 8.8 to 17 min (refs. ). Here we report optical observations of Dimorphos before, during and after the impact, from a network of citizen scientists' telescopes across the world. We find a maximum brightening of 2.29 ± 0.14 mag on impact. Didymos fades back to its pre-impact brightness over the course of 23.7 ± 0.7 days. We estimate lower limits on the mass contained in the ejecta, which was 0.3-0.5% Dimorphos's mass depending on the dust size. We also observe a reddening of the ejecta on impact.

摘要

2022 年 9 月 26 日,双小行星重定向测试(DART)航天器撞击了小行星 65803 双星系统的卫星迪迪莫斯(Dimorphos)。因为它是一个双星系统,所以可以确定卫星轨道改变了多少,这是测试用何种手段使可能与地球发生撞击的小行星偏离其轨道的一部分。在名义情况下,撞击前对轨道周期缩短的预测范围约为 8.8 到 17 分钟(参考文献)。在这里,我们报告了撞击前后来自全球公民科学家望远镜网络的对迪迪莫斯的观测结果。我们发现撞击时最大亮度增加了 2.29 ± 0.14 星等。迪迪莫斯在 23.7 ± 0.7 天的时间内恢复到撞击前的亮度。我们估计了抛射物中包含的质量下限,根据尘埃大小,抛射物质量占迪迪莫斯质量的 0.3-0.5%。我们还观察到撞击时抛射物的红化现象。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/15cc/10115630/59d167d69b98/41586_2023_5852_Fig1_HTML.jpg

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