Speaking as an <i>entirely</i> ignorant layman.... I do agree.<br /><br />Why this piece survived is a very interesting question, I’m sure. About the answer though, I haven't the faintest clue. Your reply does throw up a number of intriguing possibilities although I'm not remotely capable of coming to any conclusion without help. I can for instance imagine scenario's whereby a large impactor does less damage to itself and the surrounding impact site due to relative velocity, etc. For instance if a large asteroid impacts by coming up on the earth, not too fast, from behind, or at a shallow angle as you suggest, it might not destroy itself entirely in the process. Could it in this way, simultaneously leave a sufficiently wide crater <i>and</i> leave pieces of it's core behind? I don’t know.<br /><br />As for composition there is an interesting question as to it’s apparent different ingredients. But I’m sure there are many exotic bits and pieces riding the gravity well right now that we have never seen, and have no idea about. I’m sure we’re still scratching the surface when it comes to our knowledge of how the solar system developed, what remains to be discovered out there, where all the material in our solar system came from, etc. I’m absolutely sure that there are many big surprises to come.<br /><br />As for your final point, I can’t see any reason why some agglomerations of matter can’t be far, far older than others...<br /><br />But there must be some more knowledgeable chaps out there willing to speculate!<br /> <div class="Discussion_UserSignature"> <p><font size="2" color="#339966"> I wish I could remember<br /> But my selective memory<br /> Won't let me</font><font size="2" color="#99cc00"> </font><font size="3" color="#339966"><font size="2">- </font></font><font size="1" color="#339966">Mark Oliver Everett</font></p><p> </p> </div>