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تسجيل مستخدم جديدA Herschel Study of D/H in Water in the Jupiter-Family Comet 45P/Honda-Mrkos-Pajdusakova and Prospects for D/H Measurements with CCAT
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We present Herschel observations of water isotopologues in the atmosphere of the Jupiter-family comet 45P/Honda-Mrkos-Pajdusakova. No HDO emission is detected, with a 3 sigma upper limit of 2.0 10-4 for the D/H ratio. This value is consistent with the earlier Herschel measurement in the Jupiter-family comet 103P/Hartley 2. The canonical value of 3 10-4 measured pre-Herschel in a sample of Oort-cloud comets can be excluded at a 4.5 sigma level. The observations presented here further confirm that a diversity of D/H ratios exists in the comet population and emphasize the need for additional measurements with future ground-based facilities, such as CCAT, in the post-Herschel era.
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We report on photometry and imaging of the Jupiter Family Comets 41P/Tuttle-Giacobini-Kresak and 45P/Honda-Mrkos-Pajdusakova with the TRAPPIST-North telescope. We observed 41P on 34 nights from February 16, 2017 to July 27, 2017 pre- and post-perihel
ion (r$_h$=1.04 au), while we collected data for comet 45P from February 10 to March 30 after perihelion (r$_h$=0.53 au). We computed the production rates of the daughter species OH, NH, CN, C$_3$ and C$_2$ and we measured the dust proxy, Af$rho$, for both comets. The peak of water production rate of 41P was (3.46$pm$0.20)$times$10$^{27}$ molecules/s on April 3, 2017 when the comet was at 1.05 au from the Sun. We have shown that the activity of 41P is decreasing by about 30% to 40% from one apparition to the next. We measured a mean water production rate for 45P of (1.43$pm$0.62)$times$10$^{27}$ molecules/s during a month after perihelion. Our results show that these Jupiter Family Comets had low gas and dust activity and no outburst was detected. Relative abundances, expressed as ratios of production rates and Af$rho$ parameter with respect to OH and to CN, were compared to those measured in other comets. We found that 41P and 45P have a typical composition in term of carbon bearing species. The study of coma features exhibited by the CN gas species allowed the measurement of the rotation period of 41P, showing a surprisingly large increase of the rotation period from (30$pm$5) hrs at the end of March to (50$pm$10) hrs at the end of April, 2017 in agreement with recent observations by other teams.
Studying materials released from Jupiter-family comets (JFCs) as seen in their inner comae, the envelope of gas and dust forming as the comet approaches the Sun, provides an improved understanding of their origin and evolutionary history. As part of
a coordinated, multi-wavelength observing campaign, we observed comet 45P/Honda-Mrkos-Pajduv{s}{a}kov{a} during its close approach to Earth in February 2017. Narrowband observations were taken using the Bok 90 telescope at KPNO on February 16 and 17 UT, revealing gas and dust structures. We observed different jet directions for different volatile species, implying source region heterogeneity, consistent with other ground-based as well as in situ observations of comet nuclei. A repeating feature visible in CN and C$_2$ images on February 16, was recovered on February 17 with an interval of $7.6pm0.1$ hours, consistent with the rotation period of the comet derived from Arecibo Observatory radar observations. The repeating features projected gas velocity away from the nucleus is 0.8 km/s, with an expansion velocity as 0.5 km/s. The amount of CN material released in one cycle has a lower limit of 11 kg, depending on composition, a quantity small enough to be produced by repeated exposure of nucleus ices to sunlight. This repeating CN jet forming within 400 km of the nucleus may be typical of inner coma behavior in JFCs. Similar repeating CN features could exist and be common in other observed comets, but obscured by other processes and daughter product species as viewed from distances further than the scale length of CN molecules.
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