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A few comments from my perspective as a Kuiper belter. I must say, however, that I'm not familiar at all with how these assessment groups work (which is one reason, I've subscribed and am trying to follow what's going on), so if any of my comments aren't appropriate, feel free to ignore them. 1) I think it is reasonable to subdivide the Kuiper belt subpopulations (resonant, hot, cold) into different subsections in section 3 as you did with comets. I could write some text on these that briefly summarizes what their "current status". If so, could you give me a ~specific prompt on what I need to describe? 2) Though I'm biased as a dynamicist, I think more discussion on theoretical (e.g. dynamical) studies of these populations can be discussed as important for "characterization". 3) Regarding optimal filters for chemical characterization, Trujillo and Sheppard have also been working on this and have already executed a large program at Gemini to characterize KBOs. There's also Henry Roe's Spectroscopic Survey planned for the Discovery Channel Telescope at Lowell. JWST will do an amazing job in the Kuiper belt, based on slides I've seen from John Stansberry. Hope this helps. Best, Darin On Sun, Jan 16, 2011 at 7:24 PM, Yan Fernandez <yrf@me.com> wrote:
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