Gas and dust productions of Comet 103P/Hartley 2 from millimetre observations: Interpreting rotation-induced time variations

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• 作者：J茅r茅mie Boissier ; Dominique Bockel茅e-Morvan ; Nicolas Biver ; Pierre Colom ; Jacques Crovisier ; Raphael Moreno ; Vladimir Zakharov ; Olivier Groussin ; Laurent Jorda ; Darek C. Lis
• 关键词：Comets ; coma ; Comets ; dust ; Radio observations
• 刊名：Icarus
• 出版年：15 January, 2014
• 年：2014
• 卷：228
• 期：Complete
• 页码：197-216
• 全文大小：4496 K

文摘

Comet 103P/Hartley 2 made a close approach to the Earth in October 2010. It was the target of an extensive observing campaign including ground- and orbit-based observatories and was visited by the Deep Impact spacecraft in the framework of its mission extension EPOXI. We present observations of HCN and CH₃OH emission lines conducted with the IRAM Plateau de Bure interferometer on 22-23, 28 October and 4, 5 November 2010 at 1.1, 1.9 and 3.4 mm wavelengths. The thermal emission from the dust coma and nucleus is detected simultaneously. Interferometric images with unprecedented spatial resolution of 鈭?00 to 鈭?00 km are obtained. A sine-wave like variation of the thermal continuum is observed in the 23 October data, that we associate with the nucleus thermal light curve. The nucleus contributes up to 30-55% of the observed continuum emission. The dust thermal emission is used to measure the dust production rate. The inferred large dust-to-gas ratio (in the range 2-6) can be explained by the unusual activity of the comet for its size, which allows decimeter size particles and large boulders to be entrained by the gas due to the small nucleus gravity. The rotational temperature of CH₃OH is measured with beam radii from 鈭?50 km to 鈭?500 km. We attribute the increase from 鈭?5 K to 鈭?6 K with increasing beam size to radiative processes. The HCN production rate displays strong rotation-induced temporal variations, varying from 鈭?.3 脳 10²⁵ s^鈭? to 鈭?.0 脳 10²⁵ s^鈭? in the 4-5 November period. The HCN production curve, as well as the CO₂ and H₂O production curves measured by EPOXI, are interpreted with a geometric model which takes into account the complex rotational state of 103P/Hartley 2 and its shape. The HCN and H₂O production curves are in phase, showing that these molecules have common sources. The 鈭?.7 h delay, in average, of the HCN and H₂O production curves with respect to the CO₂ production curve suggests that HCN and H₂O are mainly produced by subliming icy grains. The scale length of production of HCN is determined to be on the order of 500-1000 km, implying a mean velocity of 100-200 m s^鈭? for the icy grains producing HCN. From the time evolution of the insolation of the nucleus, we show that the CO₂ production is modulated by the insolation of the small lobe of the nucleus. The three-cycle pattern of the production curves reported earlier is best explained by an overactivity of the small lobe in the longitude range 0-180掳. The good correlation between the insolation of the small lobe and CO₂ production is consistent with CO₂ being produced from small depths below the surface. The time evolution of the velocity offset of the HCN lines, as well as the displacement of the HCN photocenter in the interferometric maps, are overall consistent with this interpretation. Other localized sources of gas on the nucleus surface are also suggested.