Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
American Mineralogist Don't get GSW? Talk to your librarian.
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

American Mineralogist; May 2008; v. 93; no. 5-6; p. 740-744; DOI: 10.2138/am.2008.2543
© 2008 Mineralogical Society of America
This Article
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Google Scholar
Right arrow Articles by Xu, J.
Right arrow Articles by Shen, G.

Dingdaohengite-(Ce) from the Bayan Obo REE-Nb-Fe Mine, China: Both a true polymorph of perrierite-(Ce) and a titanic analog at the C1 site of chevkinite subgroup

Jinsha Xu1,*, Guamin G Yang2, Guowu Li3, Zhilan Wu4 and Ganfu Shen1

1 Chengdu lnstitute of Geology and Mineral Resources, 610082 Chengdu, China
2 China University of Geosciences (Wuhan), 430071 Wuhan, China
3 China University of Geosciences (Beijing), 100083 Beijing, China
4 Technologic Managerial Department, Bayan Obo Iron Mine, 014080 Baotou, China

Correspondence: * E-mail: xujinsha117{at}yahoo.com.cn

Dingdaohengite-(Ce), ideally Ce4Fe2+Ti2Ti2(Si2O7)2O8, is a new member of the chevkinite group minerals from the world-famous Bayan Obo REE-Nb-Fe Mine near Baotou city, Inner Mongolian Autonomous Region, North China. It occurs in the magnesian skarn in the excontact of granite within dolomitic marble. Most individual crystals vary from 0.2 to 1.0 cm in length. Associated minerals are diopside, tremolite, richterite, allanite-(Ce), magnetite, ilmenite, spinel, titanite, pyrochlore, F-rich phlogopite, fluorapatite, quartz, and fluorite, etc. Dingdaohengite-(Ce) is probably of bimetasomatic origin among Ca-Mg-carbonate rock and/or carbonatite, and REE-, F-rich postmagmatic hydrothermal solutions. The mineral is black and becoming brown black in thin fragments. It is translucent to opaque with a submetallic-metallic luster, and a brown streak. It is brittle with conchoidal fracture. No cleavage or parting is observed. Its hardness is VHN25g 606.0–717.4 kg/mm2 (Mohs hardness near 5.9). The measured density is 4.83(7) g/cm3 and the calculated density is 4.88(0) g/cm3. Its reflectance values (for {lambda} = 589 nm) are 11.4–12.5%. It is biaxial negative. The strongest six X-ray diffraction lines in the powder pattern [d in Å (I) (hkl)] are 2.7524(100)(Formula21), 2.7263(98)(313), 3.1978(68)(212), 2.5460(54)(Formula04), 2.8702(52)(020), and 3.1622(46)(Formula12).

An electron-microprobe analysis on the crystal used to collect X-ray intensity data for crystal-structure refinement gives SiO2 19.29, TiO2 18.26, Al2O3 0.04, FeO 8.49, Fe2O3 1.67, ThO2 0.16, MgO 1.32, CaO 2.17, Nb2O5 0.47, Ta2O5 0.00, La2O3 19.53, Ce2O3 28.08, Nd2O3 n.d., Y2O3 0.00, Na2O 0.00, sum 99.48 wt%; the Fe3+ /Fe2+ ratio was converted by Mössbauer spectroscopy. The empirical formula is (Ce2.13La1.49Ca0.48Th0.01){Sigma}4.11Fe2+(Ti0.88Fe2+0.47Mg0.41Fe3+0.26 Al0.01) {Sigma}2.03(Ti1.96Nb0.04){Sigma}2.00(Si2O7)2O8, based on 22 O atoms with prevalence of Ti in the C1 site of the structure. Dingdaohengite-(Ce) is monoclinic, a = 13.4656(15) Å, b = 5.7356(6) Å, c = 11.0977(12) Å, β = 100.636(2)°, V = 842.39(46) Å3, and Z = 2.

The crystal structure of dingdaohengite-(Ce) was refined with space groups P21/a and C2/m. Pseudo-extinction was found, i.e., reflections with h + k = 2n are systematically strong, while those with h + k = 2n + 1 are weak, which show that the true space group of dingdaohengite-(Ce) is P21/a (pseudo-C2/m).

Key Words: Dingdaohengite-(Ce) • P21/a (pseudo-C2/m) space group • chevkinite subgroup • new mineral • Bayan Obo • China







JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2008 by Mineralogical Society of America