[meteorite-list] The Eagle Has Landed, "Oued Bourdim" New Eagle Station Pallasite!
From: Ruben Garcia <rubengarcia85382_at_meteoritecentral.com>
Date: Sun, 11 Jan 2015 13:56:37 -0700 Message-ID: <CAJet4mMaQcPzRMdDhfM5phY+oF+AJ9VYg1ynW7JMzVUCY66B=w_at_mail.gmail.com> Hi all, Thank you to everyone that purchased specimens of my NEW Eagle Station Pallasite! Virtually all the larger specimens are sold - but, I just posted photos of some very nice smaller specimens. Many are priced at around the $100 range and some even less. Worth a look even if you're not in the mood to buy! http://www.mrmeteorite.com/ouedbourdimnewpes.htm BTW- I'll be selling out of Geoff Notkin's room this year so please stop by and take a look at these rare pallasites in person. On Thu, Jan 8, 2015 at 1:04 AM, Ruben Garcia <rubengarcia85382 at gmail.com> wrote: > Hello meteorite/pallasite enthusiasts, > > I am proud to introduce Oued Bourdim (provisional name) It's a New Eagle > Station Pallasite and it's just been submitted for Nom-Com approval. > http://www.mrmeteorite.com/ouedbourdimnewpes.htm > > Wikipedia says this about Eagle Station pallasites, "The Eagle Station > grouplet (abbreviated PES - Pallasite Eagle Station) is a set of pallasite > meteorite specimens that don't fit into any of the defined pallasite groups. > In meteorite classification five meteorites have to be found, so they can be > defined as their own group. Currently only four Eagle Station type > meteorites have been found." > > Thanks to Dr Laurence Garvie (ASU) Dr John Wasson (UCLA) Dr H. Chennaoui > Aoudjehane and Dr Karen Ziegler (UNM) this was true until today! > > Oued Bourdim (provisional name) Is the fifth Eagle Station pallasite to be > discovered and was just submitted for classification approval. Once this > meteorite is classified Eagle Station will become a proper pallasite group! > > I purchased all there was - a total of nearly 400 grams - from Moroccan > dealers over a three year period, in the form of small individuals. Already > much of it has disappeared into Museum/University and private collections. I > have only 140 grams of nice specimens for sale here. These individuals are > small and range from about .250 grams to 9 grams, but just because these > meteorites are small doesn't mean they're not awesome! > > This meteorite has everything going for it, beauty, rarity, and low TKW not > to mention it has the distinction of being Eagle Station # 5 - finally > making PES a proper pallasite group. > > Have you ever tried to purchase ANY Eagle Station Pallasite type? If so, you > already know it's not easy to do - there is none on the private market for > sale. It won't be long before this is all gone too! > > Institution trades are always welcome, but hurry while there is still a > selection to choose from. > > Please check below for available specimens and prices. > http://www.mrmeteorite.com/ouedbourdimnewpes.htm > > Weathering: medium > Fa: 21.2 ?0.2 > Classifier: L. Garvie, J. Wasson, K. Ziegler, H. Chennaoui Aoudjehane > Type spec mass: 116.7 > Type spec loc: ASU > Main mass: ASU > Finder: Brahim Oubadi > > Writeup history: > > (H. Chennaoui Aoudjehane, FSAC): During November 2007, Brahim Oubadi from > Bouanane (south east Morocco, near Boudnib) was searching for meteorites > near Oued Bourdim. He found many small pieces of a heavy rock (for its size) > that looked different from the surrounding materials around 32? 00' 21.1"N > and 3? 14' 15.6" W. Over the next few years Mr. Oubadi found approximately > 400 g. He sold the stones to a meteorite dealer in Boudnib, and they were > subsequently sold at the Tucson Gem and Mineral show where they were > nicknamed "Boudnib". The meteorites were found on an old > desert-varnish-covered wadi called Oued Bourdim. > > Writeup physical: > > Many small stones totaling 393 g: the largest are 48.9 g and 68.9 g, whereas > the majority is <10 g in mass. Exterior of the stones is dark colored and > the olivines are sand blasted with a waxy luster. Fusion crust largely > absent, though there are a few remaining patches on the metal. Medium to low > weathering. > > Writeup petrog: > > (L. Garvie, ASU). A 3 x 2 cm sawn surface of the 48.9 g stone shows 30 > areal% metal. Olivine grains highly fractured, rounded and <1 cm across. > Swathing kamacite to 1-mm thick and discontinuous. There are a few areas of > swathing schreibersite to 0.5 mm thick. Ropey schreibersite also present > within the swathing kamacite. Troilite rare, occurring as spheres to 1 mm in > the olivine. The bulk of the metal has a martensite decomposition structure > (Novotny et al., 1982), composed of Widmanst?tten alpha platelets (typically > <100 um long) in fine plessite matrix: schreibersite 10 to 50 um is common. > The platelets are surrounded by taenite rims. Two chromite grains present. > Excluding the 48.9 g stone, six additional stones were sectioned, polished, > and etched - all showed metal with the martensite decomposition structure. > Terrestrial Fe oxides locally replacing swathing kamacite and troilite. > Reference: Novotny, P.M., Goldstein, J.I., and Williams, D.B. (1982) > Analytical electron microscope study of eight ataxites. Geochimica et > Cosmochimica Acta, 46, 2461-2469. > > Writeup geochem: > > (J. Wasson, UCLA): Metal composition by INAA (mean of two analyses) Ni 170.3 > mg/g; Co 9.1 mg/g, Ga 8.1 ug/g, As 12.8 ug/g, Ir 5.98 ug/g, W 0.36 ug/g, Pt > 17 ug/g, and Au 1.34 ug/g. (L. Garvie, ASU): EMPA of eight separate olivine > grains give Fa21.2?0.2, FeO/MnO=99.9?9.0. (K. Ziegler, UNM): Analyses of 5 > acid-washed olivine subsamples by laser fluorination dual inlet mass > spectrometry gave, respectively, d17O -6.02, -5.98, -5.82, -6.04, -6.48; > d18O -2.17, -2.19, -1.85, -2.15, -2.98; D17O -4.88, -4.83, -4.85, -4.91, > -4.91 per mil (reference TFL slope = 0.528, values are linearized). > > Specimens: ASU 116.7 g, Ruben Garcia 158.8 g, and Bob Cuchiara 68.9 g. > > > > -- > Rock On! > > Ruben Garcia > http://www.MrMeteorite.com -- Rock On! Ruben Garcia http://www.MrMeteorite.comReceived on Sun 11 Jan 2015 03:56:37 PM PST |
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