[meteorite-list] Fall/find statistics revisited
From: Matson, Robert <ROBERT.D.MATSON_at_meteoritecentral.com>
Date: Thu Apr 22 10:22:38 2004 Message-ID: <AF564D2B9D91D411B9FE00508BF1C86901B4EA93_at_US-Torrance.mail.saic.com> Hi All, Lars asked about statistical numbers of meteorite falls over land (i.e. # of expected meteorites per square kilometer), and as Bernd Pauli indicated, this is a thread that comes up from time to time on this list. Bernd no doubt forwarded a good number of these posts to Lars directly, but in case some new list members were interested in this subject I thought I'd re-post my last List response on the subject from April 2002. (This message was part of a thread of messages, and mine was addressing a post by Sterling Webb): "Hi Sterling and list, > I'm quoting myself here (if I don't, who will?), from my prior > post of Dec. 9, 2000, "How Many Meteorites Fall?" > "Taking the area of the Earth to be 5.1 x 10^8 km^2 and the > meteorite flux to be 23,930 yr^-1, this yields the assumed > collisional cross section of the earth to be 21,360 km^2 yr^-1. > This rate means that one meteorite per year falls on an area > of 21,320 square kilometers. The inverse function of this value > is how long we have to wait for a meteorite to fall on a > standard area, or the mean time to impact: 21,360 yr km^-2. > To put this flux into perspective, if you owned a house with a > half-acre yard, you would have to wait 10,552,000 years for a > meteorite to fall in your front or back yard or on your roof! > (On average, that is; it could happen tomorrow.)" There is one important factor that isn't included in this analysis and that is the "footprint" of each meteorite fall (assuming that the 23,930 meteorite/year flux rate is the number of exoatmospheric meteoroids per year that will produce at least one meteorite that will survive reentry). While many falls may only produce a single stone, others produce thousands or even tens of thousands. Another way of looking at it is that sometimes the meteorite gods are shooting bullets, other times shotgun blasts. Over time, when you look at the accumulated "target hits", the amount of "blank space" is quite a bit lower than if the shooter was always using .22 slugs. The probability of a meteorite *find* in a particular location then is not so much an issue of: T * Flux * A N = ------------ Ae N = expected # of meteorites in area A T = accumulation time (years) Flux = exoatmospheric earth annual flux rate (meteorites/year) A = a given area searched (km^2) Ae = earth-surface-area (km^2) Rather, it is an issue of the mean expected distance to the nearest element of any fall. One could best estimate this with Monte Carlo simulations covering a wide range of initial meteoroid sizes, amount of fragmentation, angles of reentry, etc. But the bottom line is that due to fragmentation, the probability of finding a meteorite on an old surface of, say, 1 square kilometer, is better than what the above equation would tell you. Example: T = 5000 years, Flux = 23930 met/year, A = 1 km^2, Ae = 5.1 x 10^8 km^2. N works out to 0.235 meteorites. My field experience covering a great deal of "old" surface area is that N is at least twice this value." - - - - To update the figures to the present [2003], my own grid searches over the last 4 years covering over 100 square kilometers of "old surfaces" produces a value of at least 0.5 *unpaired* meteorites per square kilometer, or about 1.3 meteorites per square mile. The average terrestrial age of these finds is unknown, but likely to be somewhere between 1000 and 10000 years. --Rob Received on Fri 13 Jun 2003 04:18:56 PM PDT |
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