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View a list of Authentic Materials from Space (lunar & martian meteorite, rocks from Comets and Asteroids) Moldavite, fine Minerals, Meteorites offering for Scientific Research, Research National Institutes, Space Agencies, Pharmaceutical Use (Weleda), Lunar & Martian Exploration, Space Mining Universities, Museums, Collections +Resale in all sizes &shapes.(Last Modified- Thursday, 25. March 2010) |
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Schwerelosigkeit: Den Freien Fall testen. My Zero - Gravity Experience |
| Prices will again increase Feb. 17th 2010 by at least 8% due to increasing demand + limited stock in our extraterrestrail material. | ||
Sikhote-Alin-individual 71g 185.2g
View just a few of samples of many unique, surprising & and recent additions (to be found in the individually linked sections:) |
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Quickly access any meteorite section by clicking any icon / text bar below: | |
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incl.achondrite, irons,stony-irons,unequilibrated chondrites |
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| Unique meteorites from Rumuruti parent body | ||
| meteorites from Brachina parent body | ||
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Fresh Falls - Chondrites on Sales
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Q+A on how to use this page - please read FAQ! |
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| Laboratory and Outdoors Equipment | ||
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Please check for brandnew items in indivdual sections or ask for new offers
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| New |
DaG 1051 Shergottite This martian rock (TkW 40.1g, found 2000) has a porphyritic basaltic texture consisting of large, up to mm-sized zoned olivines embedded in a fine-grained matrix of pyroxene and maskelynite (the plagioclase has been converted to maskelynite.). Minor mineral constituents include Fe-sulfide, chromite, Ti-rich chromite, and ilmenite. Based on the optical appearance the rock is similar to Dar al Gani 735 and very probably paired. Geochemistry: Mineral compositions and geochemistry: Mineral compositions: Maskelynite (plagioclase), An47-64 ; mean: An55.5±6; pyroxene, Fs19-33; mean: Fs26±4.5; olivine (range): Fa26-45.. Mineralogy: A.Bischoff, M. Horstmann InstPlanUniv. Muenster, Germany; E.Haiderr, Space-sciences.com, Vienna, ask for fair price erich.haiderer@chello.at
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Unusual: ASHE, Mars 12 ![]() http://www.lpi.usra.edu/meetings/lpsc2009/ Sales only after publishing is released and only to institutes. Available will be on preorder request only slices or segments of up to almost 3 in max. diameter.
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NWA 5080 CV3 - with very large CAI's
One meteorite of TkW 235gr was found by an anonymous finder in the Saharan desert. Mineralogy: A.Bischoff, InstPlanUniv. Muenster, Germany |
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$0,32/gr+ new in! view a fine selection of Cosmic Desert Glass – Lib. Desert Glass Kosmisches Wuestenglas! |
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Ivuna, CI/ C1 The name giver of its group Ivuna, a C1 carbonaceous chondrite, has been shown to contain abundant amounts of the three-ring PAHs phenanthrene/anthracene, C1 and C2 Carbonaceous Chondrites appear to be the product of a high-temperature synthesis. This observation counters a prevailing view that PAHs in meteorites are a thermal alternation product of preexisting aliphatic compounds, which in turn required the presence of low-temperature mineral phases such as magnetite and hydrated phyllosilicates for their formation. Michael R. Wing1 and Jeffrey L. Bada2 (1) Geoscience Department, Hobart and William Smith Colleges, 14456 Geneva, NY, USA (2) Scripps Institution of Oceanography, University of California at San Diego, 92093-0212 La Jolla, CA, USA Sealed Violes or membran box with many dozens of small fresh fragments from 5mg to 25mg Special appr. 80mg US$ 2 10. Huge demand - only 1 left.Very interesting mineralogy and texture in the microscope. As always all authenticity guarantees. |
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New! Lunar KREEP impact melt breccia - Dhofar 1442 Find 2005 TkW: 120 g in total. Fusion crust absent. Note: The mineralogy of this lunaite shows by far the highest Na2O value (appr. twice as high as all other lunaites) as well as K2O content (K2O: 0.76) of all known lunar meteorites. Most Lunaites have a K2O value of a seventh or less (of that of o 1442. Only Calcalong Creek and NWA 773 have a higher K2O value than the other lunars but still only a third of that of Dho 1442 Petrography: (Ivanova M.A., Lorenz C.A., and Nazarov M.A., Vernad.) Meteorite is a impact melt breccia containing lithic clasts, mineral fragments, glassy spherules, granulites and melt breccias embedded in a fine-grained melt matrix. It is a polymict breccia although the matrix/clasts ratio is varying from sample to sample of the meteorite. The lithic clasts population is presented by anorthosites, gabbroes, olivine gabbro-norites, gabbro-norites and norites. KREEPy and mare basalt clasts are present. The size of the clasts ranges from 0.02-8 mm; the main minerals are pyroxene and feldspar; minor - olivine, silica, chromite, ilmenite, Ca-phosphate, troilite and FeNi metal. Geochemistry: (Ivanova M.A. and Kononkova N.N. (Vernad.) Chemical compositions of mineral phases are: feldspar An73-96Ab3.7-24.8; clinopyroxene En2.6-69.5Wo5.6-42.8 (Fe/Mn = 64 at.), orthopyroxene En60.8-77.1Wo1.2-4.1 (Fe/Mn = 69 at.), olivine Fo39.9-72.2 (Fe/Mn = 93 at.); ilmenite (MgO 5.5 wt%); FeNi metal (Ni 8.0 wt%; Co 0.6 wt%). Average glassy matrix composition (wt%): SiO2 49.6; TiO2 1.76; Al2O3 17.4; Cr2O3 0.20; FeO 10.7; MnO 0.15; MgO 7.16; CaO 11.1; Na2O 0.88; K2O 0.76; P2O5 0.84. Classification: Achondrite (lunar KREEP impact melt breccia with minor features of weathering. Specimens: A total of 21.8 g of sample and two thin sections are on deposit at Vernad. An anonymous buyer holds the main mass of the meteorite. 18.89gr extremely beautiful complete endpiece/ main mass with large surface area 40x36x11mm roundish shape, greenish-brownish colour with large vessicles (up to 3mm). On sale for a short time ask for a fair sale price (as usual best price guarantee) erich.haiderer@chello.at
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All meteorites (inclusive sizes TN and MS) come individually in decorative display box! |
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As always, we have much more to offer than we are able to show you here now. Kindly email us your wishes to determine if the items you want can be prepared especially for your wishes. |
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Please bookmark page since it will be frequently updated; Thank you! Copyright Erich H.Haiderer,2006 Impressum