...
首页> 外文期刊>Astronomy and astrophysics >Decay of COSAC and Ptolemy mass spectra at comet 67P/Churyumov-Gerasimenko
【24h】

Decay of COSAC and Ptolemy mass spectra at comet 67P/Churyumov-Gerasimenko

机译:COSAC和PTOLEMY MASS SPECTA的腐烂67p / churyumov-gerasimenko

获取原文
   

获取外文期刊封面封底 >>

       

摘要

Context. The Rosetta lander Philae successfully landed on the nucleus of comet 67P/Churyumov-Gerasimenko on 12 November 2014. Philae is equipped with two gas analysers: The Cometary Sampling and Composition experiment (COSAC) and the gas chromatograph and mass spectrometer Ptolemy. Aims. COSAC is designed for in situ analysis of organic molecules on 67P while Ptolemy is optimised to measure ratios of stable isotopes. Methods. On 12 to 14 November 2014, both instruments measured the organic composition of the comet nucleus material through seven measurements in sniffing mode during Philae’s hopping and at its final landing site Abydos. We compare the temporal evolution of intensities of several ion species identified by both mass spectrometers. For COSAC, this is the first analysis of the temporal behaviour of the measured ion species. Results. All ion species showed the highest intensities in the first spectra measured by both instruments approximately 20 to 30 min after Philae’s first touchdown at Agilkia, and a decay during the six consecutive measurements at Abydos. Both instruments measured an almost identical decay of the water peak ( m / z 18), and CO ( m / z 28) behaved similarly. In the COSAC measurements, the peak at m / z 44 decays much slower than all the other ion species, including the water peak. In particular, the m / z 44 peak decays much slower in the COSAC measurements than in the Ptolemy data. This supports our earlier interpretation that COSAC analysed, for the first time, a regolith sample from a cometary nucleus in situ, while Ptolemy measured cometary gas from the ambient coma. The m / z 44 peak measured by COSAC was likely dominated by organic species, whereas the peak measured by Ptolemy was interpreted to be mostly due to CO_(2) . Ion species heavier than m / z 30 tend to decay somewhat slower in the COSAC measurements than in the Ptolemy data, which may be related to differences in the exhaust designs between both instruments.
机译:语境。 Rosetta Lander Philae于2014年11月12日成功登陆了Comet 67P / Churyumov-Gerasimenko的核心。Philae配备了两个天然气分析仪:Cometry采样和组成实验(COSAC)和气相色谱仪和质谱仪Ptolemy。目标。 COSAC设计用于67倍的有机分子的原位分析,而Ptolemy经过优化以测量稳定同位素的比率。方法。在2014年11月12日至14日,这两种仪器通过腓利跳跃期间和最终着陆位点Abydos测量了杂乱模式中的七次测量的彗星核材料的有机组合物。我们比较两种质谱仪鉴定的几种离子物种强度的时间演变。对于COSAC,这是对测量离子物种的时间行为的第一次分析。结果。所有离子物种都显示出在Agilkia在Agilkia的第一次触地区后约20至30分钟测量的第一光谱中的最高强度,以及Abydos的六次连续测量期间的衰减。这两个仪器测量了水峰(M / z 18)的几乎相同的衰减,并且CO(M / Z 28)表现得同样。在COSAC测量中,M / Z 44的峰值比所有其他离子物种衰减得多,包括水峰。特别地,M / Z 44峰值在COSAC测量中衰减比在Ptolemy数据中的速度得多。这支持我们之前的解释,首次分析了来自核心核的钙舒CoSac,而Ptolemy测量了来自环境昏迷的彗星气体。 Cosac测量的M / Z 44峰可能由有机物种主导,而通过帕洛米测量的峰被解释为主要是由于CO_(2)。离子物种比m / z 30重,倾向于在Cosac测量中衰减比在Ptolemy数据中略微慢,这可能与两个仪器之间的排气设计的差异有关。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号