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首页> 外文期刊>Astronomy and astrophysics >2P/Encke, the Taurid complex NEOs and the Maribo and Sutter’s Mill meteorites
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2P/Encke, the Taurid complex NEOs and the Maribo and Sutter’s Mill meteorites

机译:2P / Encke,Taurid复杂NEO和Maribo和Sutter的Mill陨石

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Aims. 2P/Encke is a short period comet that was discovered in 1786 and has been extensively observed and studied for more than 200 years. The Taurid meteoroid stream has long been linked with 2P/Encke owing to a good match of their orbital elements, even though the comet’s activity is not strong enough to explain the number of observed meteors. Various small near-Earth objects (NEOs) have been discovered with orbits that can be linked to 2P/Encke and the Taurid meteoroid stream. Maribo and Sutter’s Mill are CM type carbonaceous chondrite that fell in Denmark on January 17, 2009 and April 22, 2012, respectively. Their pre-atmospheric orbits place them in the middle of the Taurid meteoroid stream, which raises the intriguing possibility that comet 2P/Encke could be the parent body of CM chondrites. Methods. To investigate whether a relationship between comet 2P/Encke, the Taurid complex associated NEOs, and CM chondrites exists, we performed photometric and spectroscopic studies of these objects in the visible wavelength range. We observed 2P/Encke and 10 NEOs on August 2, 2011 with the FORS instrument at the 8.2 m Very Large Telescope on Cerro Paranal (Chile). Results. Images in the R filter, used to investigate the possible presence of cometary activity around the nucleus of 2P/Encke and the NEOs, show that no resolved coma is present. None of the FORS spectra show the 700 nm absorption feature due to hydrated minerals that is seen in the CM chondrite meteorites. All objects show featureless spectra with moderate reddening slopes at λ 800 nm, which is not seen in 2P/Encke, which suggests that they are not related. Conclusions. Despite similar orbits, we find no spectroscopic evidence for a link between 2P/Encke, the Taurid complex NEOs and the Maribo and Sutter’s Mill meteorites. However, we cannot rule out a connection to the meteorites either, as the spectral differences may be caused by secondary alteration of the surfaces of the NEOs.
机译:目的2P / Encke是一种短期彗星,于1786年被发现,经过200多年的广泛观察和研究。尽管彗星的活动强度不足以解释观测到的流星数量,但由于金牛座流星体流的轨道元素很匹配,因此它与2P / Encke长期保持联系。已经发现各种轨道附近的小型近地天体(NEO),这些天体可以与2P / Encke和Taurid流星体流联系起来。 Maribo和Sutter's Mill是CM型碳质球粒陨石,分别于2009年1月17日和2012年4月22日在丹麦落下。它们的大气前轨道将它们置于金牛座流星体的中部,这增加了2P / Encke彗星可能成为CM球粒陨石母体的可能性。方法。为了研究2P / Encke彗星,与Taurid配合物相关的NEO和CM球粒陨石之间是否存在关系,我们在可见波长范围内对这些物体进行了光度和光谱研究。我们于2011年8月2日在塞罗帕拉纳尔(智利)的8.2 m超大型望远镜上使用FORS仪器观测到2P / Encke和10个NEO。结果。 R滤镜中的图像用来调查2P / Encke和NEO核周围可能存在的彗星活动,显示没有昏迷。由于在CM球陨石陨石中发现了水合矿物,因此FORS光谱均未显示700 nm的吸收特征。所有物体均显示无特征的光谱,在λ800 nm处有适度的红变斜率,这在2P / Encke中未发现,这表明它们无关。结论。尽管轨道相似,但我们没有发现2P / Encke,Taurid复杂NEO与Maribo和Sutter的Mill陨石之间存在联系的光谱证据。但是,我们也不能排除与陨石的联系,因为光谱差异可能是由NEO表面的二次变化引起的。

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