[meteorite-list] Fw: Last on Adamana for a while (I hope)
From: Sterling K. Webb <sterling_k_webb_at_meteoritecentral.com>
Date: Fri, 2 Mar 2007 13:07:34 -0600 Message-ID: <093801c75cfe$09e17e90$32ea8c46_at_ATARIENGINE> T'm re-posting this, as the first try didn't go through, think it was too long with all the previous messages in the thread still attached. Sorry if it's a second copy. ---------------------------------------------------------- Hi, At the risk of stepping into a private argument and collecting a wild punch, I just wanted to point out something about meteoric entry. The "stone" is most likely to fragment at the point of maximum dynamic pressure from the atmosphere (or Max Q). The dynamic pressure equals (density) x (velocity)^2 / 2. Now, the square of the object's velocity decreases exponentially, that is to say very rapidly, from the drag created by that rising pressure. A good chunk of rock is going to be slowing down at anywhere from 50 gees to perhaps 200 gees. We can measure the actual deceleration of meteors and we can test existing meteorites to determine their crushing strength, and that is the range we find. The average is about 80 gees. The density of the atmosphere increases linearly in proportion to altitude, so the pressure builds up mostly in the later stages of the entry. These three factors (rapid slowdown, weak stones, and atmospheric density) combine to USUALLY result in a low altitude fragmentation. If the stone is extremely weak ("friable") it will fragment at a higher altitude than a "normal" stone. Stones that fragment into a very large number of pieces (like Holbrook) seem to do so because they are very weak. Thus, Holbrook could be considered atypically weak and that could produce some odd behavior. While Jason is correct that the maximum pressure is exerted on the "nose" of a "nose cone," that point is also the most stable and the least subject to vibration. The external shock waves in hypersonic flight could have folded smoothly over the ablating cone-shaped portion of the mass and then become turbulent further back along the more irregular and less ablated main body of the object, producing buffeting and vibration that caused the main portion of the mass to shatter and break, while the "nose" managed to transition the hypersonic-subsonic boundary more or less intact, leaving the "second" stone to re-fragment and re-fragment, ablating until they too could also drop to subsonic velocities. It's an unusual scenario, not the "normal" breakup (if there is such a thing as a normal meteoric breakup). If you ever seen an ablating entry (or re-entry), there can be an amazing amount of tumbling and gyrations of fragments after they break loose from a larger mass. This could all be a wild fantasy but, interestingly, there is this paper that claims that a mathematical analysis of the distribution of sizes of fragments found in a meteorite fall can reveal such details as the number of breakups the object went through or if the shape of the original body deviated from the spherical: http://www.iop.org/EJ/article/0295-5075/43/5/598/node4.html by L. Oddershede (Technical University of Denmark ), A. Meibom (University of Odense, Denmark ) and J. Bohr (Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa) The authors say: "A known example is the Holbrook shower, where the presence of different thicknesses of the fusion crust shows that the meteoroid was subject to at least two fragmentation processes. The mass distribution of fragments from the Holbrook shower... seems S-shaped which might be consistent with a superposition of two power laws with different cut-off masses... The mass distributions could equally well or better be a result of three (or more) fragmentations." They are talking about the fragments called "Holbrook" only, but it is clear that the statistics suggest a "stepped" process in which a big rock breaks into two rocks, one of which breaks into multiple fragments, the largest of which could in turn break into smaller multiple fragments... They studied a number of "showers" and found some to be the result of a single fragmentation event and some to be the result of multiple fragmentations. Quite incidentally, the equations also imply the volumetric coefficient of the original shape. The Mbale Object was almost spherical (with Vc=3) while the original Sikhote-Aline meteoroid was a long cylinder (Vc=1.8). Hey, no wonder it had such a bumpy ride! A big iron splinter. Jason would be "right" in that it is counter-intuitive and does not follow the "usual" course of events for the many Holbrooks and the Venus Stone to be part of the same mass, but there are many indications that this may be an unusual fragmentation event, in which case all the usual bets could be off. Theory is one thing, but the proof is always on the ground (or in it, sometimes). Keep hunting! Sterling K. Webb ------------------------------------------------------------------ ----- Original Message ----- From: "DNAndrews" <dna1 at cableone.net> To: "Meteorite-list" <meteorite-list at meteoritecentral.com> Sent: Thursday, March 01, 2007 11:09 PM Subject: [meteorite-list] Last on Adamana for a while (I hope) Hi again, Jason... Received on Fri 02 Mar 2007 02:07:34 PM PST |
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