从非引力和扭矩看67P/丘留莫夫-格拉西缅科彗星上不同的水活性和动量传递

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2024-09-27 DOI:10.1051/0004-6361/202450728
N. Attree, P. Gutiérrez, O. Groussin, J. Bürger, H. U. Keller, T. Kramer, R. Lasagni Manghi, M. Läuter, P. Lemos, J. Markkanen, R. Marschall, C. Schuckart
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引用次数: 0

摘要

目的我们研究了同时拟合彗星67P/楚留莫夫-格拉西缅科的非重力、扭矩和水的总排气率(如 "罗塞塔 "所观测到的)的能力,以制约彗星物质的复杂热物理模型。我们通过测试更详细的地貌映射、所使用的形状模型的分辨率、形状模型上相邻面的自热、排气解决方案中的热惯性以及气体与原子核之间动量耦合的变化等因素的影响,扩展了之前根据 "罗塞塔 "观测结果拟合地理定义的表面排气模型的工作。我们还直接比较了文献中的非重力加速度曲线。我们纠正了前一篇论文中计算极点方向的错误。我们发现,在模型的假设条件下,非重力和扭矩是由核内的水升华驱动的,热惯性和自热只有很小的影响,空间均匀的活动无法解释67P的非重力动力学,空间均匀的动量传递无法解释67P的非重力动力学,不同的地形类型对日照有不同的瞬时反应。67P/Churyumov-Gerasimenko上朝南的合并地形具有较高的排气通量、对日照的陡峭响应以及较大的气体动量传递系数。相反,朝北的地形表现不同,几乎不产生水排气,动量传递效率也较低。多尘地形的出气率和动量传递效率也较低,在彗星接近太阳时,其挥发性成分要么消耗殆尽,要么被回落物掩埋。动量传递似乎与日照有关,这可能是由于流经的尘埃被加热后气体温度升高所致。
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Varying water activity and momentum transfer on comet 67P/Churyumov-Gerasimenko from its non-gravitational forces and torques
Aims. We investigate the ability of a simultaneous fitting of comet 67P/Churyumov-Gerasimenko’s non-gravitational forces, torques, and total water-outgassing rate, as observed by Rosetta, to constrain complex thermophysical models of cometary material.Methods. We extend the previous work of fitting geographically defined surface outgassing models to the Rosetta observations by testing the effects of a more detailed geomorphological mapping, the resolution of the shape-model used, self-heating by neighbouring facets on the shape-model, thermal inertia in the outgassing solution, and the variation in the momentum coupling between the gas and the nucleus. We also directly compare the non-gravitational acceleration curves available in the literature.Results. We correct an error in the calculation of pole-orientation in the previous paper. We find that, under the assumptions of the model, non-gravitational forces and torques are driven by water sublimation from the nucleus, thermal inertia and self-heating have only minor effects, spatially uniform activity cannot explain 67P’s non-gravitational dynamics, spatially uniform momentum transfer cannot explain 67P’s non-gravitational dynamics, and different terrain types have different instantaneous responses to insolation.Conclusions. Consolidated terrain facing south on 67P/Churyumov-Gerasimenko has a high outgassing flux, a steep response to insolation, and a large gas momentum transfer coefficient. Instead, that facing north behaves differently, producing little to no water outgassing, and with a lower momentum transfer efficiency. Dusty terrain also has a lower outgassing rate and momentum transfer efficiency, and either depletes its volatile component or is buried in fall-back as the comet approaches the Sun. Momentum transfer appears correlated with insolation, likely due to an increased enhancement in the gas temperature as the dust it flows through is heated.
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