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An Early Look of Comet C/2013 A1 (Siding Spring): Breathtaker or Nightmare?
DOI: 10.1088/0004-637X/787/2/115 Bibcode: 2014ApJ...787..115Y

Ye, Quan-Zhi; Hui, Man-To

The dynamically new comet, C/2013 A1 (Siding Spring), is to make a close approach to Mars on 2014 October 19 at 18:30 UT at a distance of 40 ± 1 Martian radii. Such an extremely rare event offers a precious opportunity for the spacecrafts on Mars to closely study a dynamically new comet itself as well as the planet-comet interaction. Meanwhile, th…

2014 The Astrophysical Journal
Rosetta 32
Formaldehyde Chemistry in Cometary Ices: On the Prospective Detection of NH2CH2OH, HOCH2OH, and POM by the On-board ROSINA Instrument of the Rosetta Mission
DOI: 10.1088/0004-637X/791/2/75 Bibcode: 2014ApJ...791...75D

Duvernay, F.; Danger, G.; Theulé, P. +2 more

The thermal reactivity of a water-dominated cometary ice analog containing H2CO and NH3 is investigated by means of Fourier transform infrared spectroscopy, mass spectrometry, and B3LYP calculations. Three products are characterized by these techniques: aminomethanol (NH2CH2OH), methyleneglycol (HOCH

2014 The Astrophysical Journal
Rosetta 24
Mass Transport around Comets and its Impact on the Seasonal Differences in Water Production Rates
DOI: 10.1088/0004-637X/788/2/168 Bibcode: 2014ApJ...788..168R

Altwegg, K.; Thomas, N.; Combi, M. R. +4 more

Comets are surrounded by a thin expanding atmosphere, and although the nucleus' gravity is small, some molecules and grains, possibly with the inclusion of ices, can get transported around the nucleus through scattering (atoms/molecules) and gravitational pull (grains). Based on the obliquity of the comet, it is also possible that volatile materia…

2014 The Astrophysical Journal
Rosetta 21
The Global Morphology of the Solar Wind Interaction with Comet Churyumov-Gerasimenko
DOI: 10.1088/0004-637X/794/1/14 Bibcode: 2014ApJ...794...14M

Mendis, D. A.; Horányi, M.

The forthcoming Rosetta-Philae mission to comet 67P/Churyumov-Gerasimenko provides a novel opportunity to observe the variable nature of the solar wind interaction with a comet over an extended range of heliocentric distance. We use a simple analytical one-dimensional MHD model to estimate the sizes of the two most prominent features in the global…

2014 The Astrophysical Journal
Rosetta 8