Rosetta - Early Orbital Operations at Comet 67P C-G, August 6, 2014 - November 13, 2014 |
Rosetta - Early Orbital Operations at Comet 67P C-G, August 6, 2014 - November 13, 2014 |
Aug 6 2014, 09:29 AM
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Senior Member Group: Admin Posts: 3108 Joined: 21-December 05 From: Canberra, Australia Member No.: 615 |
Cheers at the European Space Operations Centre.
Well done! Rosetta has arrived Time for science!!!!!!! |
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Aug 7 2014, 01:24 AM
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Junior Member Group: Members Posts: 20 Joined: 4-August 14 From: St. Louis, Missouri Member No.: 7230 |
It would appear that the neck is an "erosional" feature (not sure if erosion is the right word), and maybe not the contact boundary between 2 separate bodies. At some point in the future, the neck will sublime away and the comet will split in two. Long time lurker here jumping into the discussion of this strange object. I agree and have thought for several days now that 67P/C-G just didn't look right to be a contact binary. Looking at several of the recent highest resolution images, there are large-scale features in the 'neck' area which appear to be somewhat contiguous from the 'head' to the 'body'. These appear to exhibit similar types of features and textures as is seen in both lobes i.e. https://pbs.twimg.com/media/BuWJaVSIcAAVgZ9.jpg:large I think a contact binary resulting from a low-speed impact of 2 bodies and subsequent gap infilling with loose material may not likely exhibit features like those seen... somewhat linear and contiguous higher density erosion resistant features and surfaces. Jets of dust in the long exposure image seem to be emanating primarily from the neck area; likely from the higher albedo areas. If the neck resulted from increased ablation rates in this area of an assumed initial single somewhat spherical cometary body, quite a bit of material has been lost compared to the 2 lobes. On the other hand, 103P/Hartley and 19/P Borrelly, both of which had a bowling pin shape had jets emanating primarily from the lobes. |
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