Moraskoite, Na2Mg(PO4)F, a new mineral from the Morasko IAB-MG iron meteorite (Poland)

被引:17
作者
Karwowski, Lukasz [1 ]
Kusz, Joachim [2 ]
Muszynski, Andrzej [3 ]
Kryza, Ryszard [4 ]
Sitarz, Maciej [5 ]
Galuskin, Evgeny V. [1 ]
机构
[1] Univ Silesia, Fac Earth Sci, Dept Geochem Mineral & Petrog, PL-41200 Sosnowiec, Poland
[2] Univ Silesia, Inst Phys, PL-40007 Katowice, Poland
[3] Adam Mickiewicz Univ, Inst Geol, PL-61606 Poznan, Poland
[4] Univ Wroclaw, Inst Geol Sci, PL-50205 Wroclaw, Poland
[5] AGH Univ Sci & Technol, Fac Mat Sci & Ceram, PL-30059 Krakow, Poland
关键词
moraskoite; new mineral; phosphate; fluoride; structure; Raman; iron meteorites; Morasko; PHOSPHATE MINERALS; MERRILLITE; RAMAN;
D O I
10.1180/minmag.2015.079.2.16
中图分类号
P57 [矿物学];
学科分类号
070901 ;
摘要
Moraskoite, a new natural phosphate of composition Na2Mg(PO4)F, has been found in the Morasko IAB-MG iron meteorite. The new phosphate occurs in a graphite-troilite inclusion enclosed in a kamacite-taenite matrix. Associated minerals in the inclusions are chlorapatite, buchwaldite, brianite, merrillite, a new phosphate phase of composition Na4MgCa3(PO4)(4), chromite, enstatite (bronzite), kosmochlor, kosmochlor-augite, olivine, albite, orthoclase, quartz, cohenite, schreibersite, nickelphosphide, altaite, pyrrhotite, sphalerite, daubreelite, djerfischerite, whitlockite and native Cu. The inclusions are rimmed by a schreibersite-cohenite halo. Moraskoite forms aggregates up to 1.5 mm in size, with individual grains 20-300 mu m across. It is colourless and transparent, with a white streak and vitreous lustre; fluorescence is weak blue in ultraviolet radiation (254 and 360 nm); hardness is 4-5; it has irregular, conchoidal fracture and cleavage is rarely observed. Calculated density (using the empirical formula) is 2.925 g cm(-3). The moraskoite structure (Pbcn, a = 5.2117(10), b = 13.711(3), c = 11.665(2) angstrom, V = 833.6(3) angstrom(3) and Z = 8) is similar to that of its synthetic analogue. The strongest diffraction lines of the moraskoite powder diffraction pattern are as follows (d(hkl), I): 3.909(75), 3.382(52), 2.955(90), 2.606(100), 2.571(96), 2.545(68), 1.691 (67). In the Raman spectrum, the following characteristic bands are distinguished (cm(-1), strong bands bold): 1114, 1027, 962, 589, 438, 336, 308, 279, 262, 244, 193, 184, 147 and 131. The Raman data prove the absence of H2O and CO2. Moraskoite is interpreted as being a primary phosphate, which crystallized together with graphite, troilite and other accessories inside the nodule.
引用
收藏
页码:387 / 398
页数:12
相关论文
共 38 条
  • [1] FLUORINE IN METEORITES
    ALLEN, RO
    CLARK, PJ
    [J]. GEOCHIMICA ET COSMOCHIMICA ACTA, 1977, 41 (05) : 581 - 585
  • [2] A petrologic study of the IAB iron meteorites: Constraints on the formation of the IAB-Winonaite parent body
    Benedix, GK
    McCoy, TJ
    Keil, K
    Love, SG
    [J]. METEORITICS & PLANETARY SCIENCE, 2000, 35 (06): : 1127 - 1141
  • [3] Buchwald V.F., 1984, Phosphate minerals, P199
  • [4] PHOSPHATE MINERALS IN PALLASITE METEORITES
    BUSECK, PR
    HOLDSWORTH, E
    [J]. MINERALOGICAL MAGAZINE, 1977, 41 (317) : 91 - 102
  • [5] The iron-nickel-phosphorus system: Effects on the distribution of trace elements during the evolution of iron meteorites
    Corrigan, Catherine M.
    Chabot, Nancy L.
    McCoy, Timothy J.
    McDonough, William F.
    Watson, Heather C.
    Saslow, Sarah A.
    Ash, Richard D.
    [J]. GEOCHIMICA ET COSMOCHIMICA ACTA, 2009, 73 (09) : 2674 - 2691
  • [6] Czajka W., 2005, PICTURE HYPOTHETIC T
  • [7] Dominik B., 1976, PRACE MINERALOGICZNE, V47, P7
  • [8] Apatite as a probe of halogen and water fugacities in the terrestrial planets
    Douce, Alberto E. Patino
    Roden, Michael
    [J]. GEOCHIMICA ET COSMOCHIMICA ACTA, 2006, 70 (12) : 3173 - 3196
  • [9] Dziel T., 2007, SEM MET 21 22 KWIETN, P17
  • [10] VOLATILE ELEMENT CHEMISTRY IN THE SOLAR NEBULA - NA, K, F, CL, BR, AND P
    FEGLEY, B
    LEWIS, JS
    [J]. ICARUS, 1980, 41 (03) : 439 - 455