[meteorite-list] Prospecting for meteorites
From: Sterling K. Webb <kelly_at_meteoritecentral.com>
Date: Sat Nov 19 05:24:43 2005 Message-ID: <437EFD48.8143AE6_at_bhil.com> Hi, Some decades ago, John S. Lewis calculated that the largest IRON mass that could survive to reach the surface of the Earth was under 100 tons. This was making all the ideal assumptions: low entry velocity, low entry angle, flattened shape. He suggested that HOBA, which is about 60 tons, was originally that mass. The soil surrounding it is rich red oxydized shaley dirt and probably formed from the erosion product of a larger HOBA than today's 60 tons. The largest STONE mass, by the same calculation, would be only roughly 40 tons, but since stones are poorly consolidated, they are unlikely to be able to resist fragmenting, which seems to be the case. If there was a 40 ton stone meteorite, it would be a mass equivalent to a sphere about 10 feet in diameter (3+ meters). Objects shatter if a shock wave (like a re-entry shock wave) exceeds the speed of sound in the material of the object. Stoney meteorites that have been tested demonstrated a slow internal speed of sound. Hence, it is likely that most large stoney meteorites are shattered by their own re-entry shock waves! Sterling K. Webb --------------------------------------------------------- michel FRANCO wrote: > Hi, > > Thanks Sterling for the additionnal info about the Chinguetti meteorite > story. > > I suggest to say that there is no more controversy about the existence > of the huge mass and to stop spending time searching it. The dynamic of > fall teaches that any mass larger than 200 tons will vaporize upon > landing. The possible mass of the Chinguetti hill is over thousand of > tons. For me it is physically impossible the find this huge mass. > > Then it is true that a meteorite was found nearby that hill and that the > sun burnt rocks in the hot Sahara are covered with desert varnish, often > very black and sometimes similar to slightly alterated fusion crust. The > confusion was possible before we had knowledge of Eugene Shoemaker works > about impact craters. > > My 2 cents. > > Best regards > > Michel FRANCO > Received on Sat 19 Nov 2005 05:24:08 AM PST |
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