[meteorite-list] Tektite QUESTION
From: Keith <littlejo_at_meteoritecentral.com>
Date: Thu Apr 22 10:08:28 2004 Message-ID: <Pine.SOL.4.33.0209201218220.22358-100000_at_katie.vnet.net> First, a good on-line article is: Wang, J., Q. Zhao, X. Chen, R. Wang, and P. Wang (2000) Age estimation of the mid-Pleistocene microtektite event in the South China Sea: A case showing the complexity of the sea-land Correlation. Chinese Science Bulletin. Vol. 45 No. 24, pp. 2277-2280. (December 2000) http://www.scichina.com/ky/0024/ky2277.pdf It can be obtained using the above URL. On Fri, 20 Sep 2002 09:15:27 +0200 in [meteorite-list] Tektite QUESTION, Bernd Pauli HD wrote: >Michael Blood wrote: >>I am sure I have it in more than one text SOMEWHERE, >>but can anyone tell me quick short the estimated age >>of the Austro-asian strewn field Tektites? >> >>"Sterling K. Webb" wrote: >> >>The figure given for the age of the Australasian field >>has been estimated at 770,000 to 780,000 years for the >>past 30 or 40 years; however, somewhere on a posting >>on CCNET which I can no longer find (&%$!), attempts >>to refine the precision of those isotopic ages came >>up with a figure about 10% to 12% older, more like >>850,000 to 900,000 years, which made sense as there >>have always been a few australites with anomalous ages >>(about 10% older). Maybe we should just call it >>somewhere short of a million. > >Hello Michael and List, >BARNES V.E. (1990) Tektite research 1936-1990 >(Meteoritics 25-3, 1990, 149-159). > >p. 155: Ages of tektites > >Lovering et al. (1972) determined that the stratigraphic >age of australites is between 24 000 and 16 000 years, >which is at considerable variance with the 700 000-year >age found for australites and the rest of the tektites in >the Australasian strewnfield by fission-track >(Fleischer and Price, 1964) and potassium-argon (K/Ar) >dating ...text deleted... The stratigraphic age assigned by Lovering et al. (1972) was found to be found badly flawed by Shoemaker and Uhlherr (1999). Lovering et al. (1972) studied the occurrence australites within the the Lake Torrens Plain in South Australia. They argued on the basis of what they considered to be the excellent state of preservation of the tektites found in the Lake Torrens Formation; the nearest Pleistocene outcrops being 15-25 km away; and their occurrence in wind blown sand that the tektites are in situ and, thus, contemporaneous with the Lake Torrens Formation. Since the Lake Torrens Formation has been dated at 16,000 to 24,000 BP, Lovering et al. (1972) argued that these tektites fell at some time around 16,000 to 24,000 BP. Shoemaker and Uhlherr (1999) reinvestigated the tektites from the Lake Torrens Formation. He found that the tektites in the Lake Torrens Formation did not come from wind-blown sands but rather alluvial sands. Also, he found the tektites came from older Pleistocene deposits, Hanson Plain Sand, that locally underlies the Lake Torrens Formation. Contrary, to what Lovering et al. (1972) concluded, they found a plausible local source for the tektites and evidence that the tektites found in the Lake Torrens Formation were reworked from the Hanson Plain Sand. As a result, Shoemaker and Uhlherr (1999) disputed the age assigned by Lovering et al. (1972) to the tektites found in the Lake Torrens Formation since they found clear evidence that these tektites were not in situ but rather reworked from older Pleistocene sediments. Gill (1965) argued for a Holocene age for australites as being only as old as 7,300 BP. In the Port Campbell area of Victoria, Australia, Gill (1965) recovered 14 australite samples within a soil profile lying above a hardpan soil zone. Wood and charcoal from the hardpan dated to about 7,300 BP. Another australite was found in a hardpan dated to about 5,700 BP. Unfortunately, Gill (1965) completely disregards the fact that soils are very dynamic systems and are churned by a number of processes as discussed by Johnson (1990) and Johnson et al. (1987). Within soils, materials of vastly differing ages, e.g. wood, charcoal, Aboriginal artifacts, and tektites, can be and are typically and randomly mixed together. The tektites simply were present in the soils before the formation of the hardpans and the age of the hardpans provide absolutely no evidence about the age of the tektites. the charcoal and other material dated were simply mixed into the soil by pedoturbation and lack any association with the australites and only date the hardpans, if anything at all. Gill (1965) also argued that the tektites were in situ because they are the " include the best preserved tektites in the world." However, Fudali (1993) showed that Gill (1965) was greatly mistaken about the degree of preservation about these tektites. In fact, contrary to what Gill (1965) argued, Fudali (1993) demonstrated tektites exhibit significant signs of weathering and transport. Fudali (1993) also found that the specimens that Gill (1965) described constitute only a very small fraction of the tektites to be found. Thus, Gill (1965) came to a badly flawed conclusion about them being in situ because he failed to realize he had studied a sample badly biased towards the more showy "perfect specimens" and unrepresentative of the state of preservation of local tektites in general. Finally, Fudali (1993) found that these australites in reality were not in situ the australites and appeared to be coming from sandy sediments older than and lying below the hardpans. If a person looks into the published literature, the age estimates offered by Gill (1965) and Lovering et al. (1972) have been very effectively discredited by Fudali (1993) and by Shoemaker and Uhlherr (1999). References Cited: Fudali, R. F., (1993) stratigraphic age of australites revisited. Meteoritics. vol. 28, no. 1, pp. 114-119. Gill, E. D. (1965) Quaternary geology, radiocarbon datings, and the age of australites. In: International studies on the quaternary-inqua cong., 7th, boulder, colorado, pp. 415-432. Special Paper no. 84, Geological Society of America, Boulder, CO. Lovering, J. F., B. Mason, G. E. Williams, and D. H. McColl (1972) Stratigraphical evidence for the terrestrial age of australites. Journal of the Geological Society of Australia. vol. 18, Part 4, no. 4, pp. 409-418. Johnson, D. L. (1990) Biomantle evolution and the redistribution of earth materials and artifacts. Soil Science. vol. 149, no. 2, pp. 84-102. Johnson, D. L., S. D. Watson, D. N., Johnson, and R. J. Schaetze (1987) Proisotropic and proanisotropic processes of pedoturbation. Soil Science. vol. 143, no. 4, pp. 278-292. Shoemaker, E. N., and H. R. Uhlherr (1999) Stratigraphic relations of australites in the Port Campbell Embayment, Victoria. Meteoritics and Planetary Science. vol. 34, no. 3, pp. 369-384. Another Reference Fudali, R. F., A. J. Miller, And A. W. R. Bevan (1991) Australites from northern Australia. Meteoritics. vol. 26, no. 2, pp. 153-155. Have Fun Keith Littleton New Orleans, LA Received on Fri 20 Sep 2002 12:36:36 PM PDT |
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