Mike, Great reply.<br />A few points for further discussion.<br />There does indeed appear to be a fairly sharp cutoff in the aphelia of classic KBO's. Whether the presence of a massive companion is the <b> best </b> explanation is debatable. There are ather explanations. IIRC, the paper that proposed the migration of the gas giants for the formation of the KB, also provides an explanation for the cutoff. That's only from my memory, so I'll dig out the paper and reread it. That zone is in a 1:2 resonance with Neptune, home of the twotinos. (~ 47.6 AU semimajor axis), I think that was the reason for the cutoff.<br /><br />Now to the chart you provided, which is a great one, BTW. I used it in my Pluto descission.<br />I don't really see a bimodal distribution of inclinations. I see a large group of low inclination objects, which may or may not be a selection effect, since that's where we spend the most time looking, and objects are more concentrated. Then, there are scattered objects in the KB up to inlinations of about 35 degrees. Several of these are the larger outer solar system objects, and in the KB, only 2 of the larger KBO's are near 30 degrees, there are 3 near 20 degrees, and 3 near 25 degrees. However, I don't think the quantity shows a peak in this area.<br />When time permits, I will separate out the Classic KBOS and do a distribution of the inclinations. We'll see what it shows.<br /><br />At this point, we are still filling in the non-ecliptic population of the solar system, so it's too early to draw conclusions. It's not too early to speculate a bit, though <img src="/images/icons/smile.gif" /> <div class="Discussion_UserSignature"> <p><font color="#000080"><em><font color="#000000">But the Krell forgot one thing John. Monsters. Monsters from the Id.</font></em> </font></p><p><font color="#000080">I really, really, really, really miss the "first unread post" function</font><font color="#000080"> </font></p> </div>