[meteorite-list] British Lower Eocene London Clay Tektites
From: Sterling K. Webb <sterling_k_webb_at_meteoritecentral.com>
Date: Thu, 24 May 2007 01:08:25 -0500 Message-ID: <006c01c79dc9$f189dd80$f54de146_at_ATARIENGINE> Hi, Aubrey, List Here is a photo of Australasian micro- and mini- microtektites found in the Indian Ocean: http://www.nio.org/projects/shamprasad/figure2%20.htm Note the similaritity of shapes. These are slightly (but not too much) larger than the London Clay micros. Here is a small photo of Eocene micromicrotektites from the Chesapeake Bay Crater: http://meteor.pwnet.org/img/impact_13.jpg There is a clear resemblance to the London Clay micros. Note the high frequency of the amber-colored micros. Photo of Chicxulub microtektites: http://geophysics.ou.edu/impacts/chicxulubtektites.jpg Note the surface degradation. These are "clean" samples. Eventually, microtektites of this age are altered into clay nodules and escape notice. Paper (with photos) of possible (very) small Devonian microtektites: http://www.wanfangdata.com.cn/qikan/periodical.Articles/zgkx-ed/zgkx2000/0003/000309.htm (The ones that were 100 to 200 micrometers were sectioned and the surface SEM'ed; results are shown in a table below the photo; scroll down.) First, microtektites degrade much faster than larger tektites. By faster, however, I mean tens of millions of years, though. These objects are remarkably "fresh" looking. One asks why have they not degraded in 35 million years? Answering my own question, the high transparency suggests a very high silica content. This would account for their degree of preservation. The black appearance that most of us think of as "typical" of tektites is the result of high iron content. I gather that they have been securely tucked away in the London Clay for all that time and not exposed nor over-wetted. I'm tempted to say that the shapes alone are almost sufficient to identify them as tektites; it looks like an illustration of Baker's famous paper on tektites form. However, what's needed is a) a bulk composition by SEM, and b) a determination of water content by infrared spectroscopy (which is non-destructive and much more accurate than destructive extraction; polish off two surface windows and scope through the clean interior). Even after 35 million years, a tektite glass is going to be distinctly drier than ANY volcanic glass and most impact glasses. I was frankly amazed that the finder would dismiss these as volcanic in origin. They look nothing like volcanic microspherules. If someone is in a more expensive mood, another good test would be the flourine-boron ratios, which serves as a kind of "thermometer" for the temperature of formation. This would easily demonstrate that they were non-volcanic. (Personally, I find the "volcanic" suggestion outlandish.) If I had to vote without tests, I'd vote "yes" to their being a tektite glass, but just as with mysterious iron objects that come crashing through one's roof, a test is really required. Since there is an ongoing controversy about a proposed multi-ringed impact feature in the North Sea (or is it only a salt basin?), with paper in Nature, etc., http://bromans.blogspot.com/2007/03/great-north-sea-impact-crater-vs-salt.html maybe the pro-Impactisitas would pay for some testing? Nothing like a handful of tektites to bolster your impact! Sterling K. Webb ------------------------------------------------------------------- ----- Original Message ----- From: Aubrey Whymark To: meteorite list ; britishandirishmeteoritesociety at yahoogroups.com Sent: Wednesday, May 23, 2007 7:46 PM Subject: [meteorite-list] British Lower Eocene London Clay Tektites Hi I just wanted to draw attention to these possible microtektites from the Lower Eocene London Clay in England. The finder, Michael Daniels, has very kindly provided a number of images and some notes. http://www.tektites.co.uk/13.html What do people think of these possible microtektites? Are they comparable with other microtektites found? Interestingly some of the microtektites seem to have extra 'spikey' features (see photos) - is this normal? Thanks, Aubrey www.tektites.co.uk P.S. out of contact from 26th May for a bit. Received on Thu 24 May 2007 02:08:25 AM PDT |
StumbleUpon del.icio.us Yahoo MyWeb |