Title: CN Morphology Studies of Comet 103P/Hartley 2 Authors: Matthew M. Knight, David G. Schleicher
We report on narrowband CN imaging of Comet 103P/Hartley 2 obtained at Lowell Observatory on 39 nights from 2010 July until 2011 January. We observed two features, one generally to the north and the other generally to the south. The CN morphology varied during the apparition: no morphology was seen in July; in August and September the northern feature dominated and appeared as a mostly face-on spiral; in October, November, and December the northern and southern features were roughly equal in brightness and looked like more side-on corkscrews; in January the southern feature was dominant but the morphology was indistinct due to very low signal. The morphology changed smoothly during each night and similar morphology was seen from night to night. However, the morphology did not exactly repeat each rotation cycle, suggesting that there is a small non-principal axis rotation. Based on the repetition of the morphology, we find evidence that the fundamental rotation period was increasing: 16.7 hr from August 13-17, 17.2 hr from September 10-13, 18.2 hr from October 12-19, and 18.7 hr from October 31-November 7. We conducted Monte Carlo jet modelling to constrain the pole orientation and locations of the active regions based on the observed morphology. Our preliminary, self-consistent pole solution has an obliquity of 10 deg relative to the comet's orbital plane (i.e., it is centred near RA = 257 deg and Dec=+67 deg with an uncertainty around this position of about 15 deg) and has two mid-latitude sources, one in each hemisphere.
The magnitude 7.2 comet 103P/Hartley 2 will pass 1.89° from the magnitude 10.0 open cluster NGC 2432 in the constellation Puppis, at 14:00 UT, 10th December, 2010.
The magnitude 7.1 comet 103P/Hartley 2 will pass 1.52° from the magnitude 11.0 planetary nebula NGC 2440 in the constellation Puppis, at 9:00 UT, 8th December, 2010.
Analysis of the data gathered by Deep Impact probe at Comet Hartley reveals the object is surrounded by a cloud of ice chunks and fluffy snow particles. The space mission's chief scientist Dr Mike A'Hearn has told reporters that some of the chunks are very large. Read more