Term: Astrophyllite group

Astrophyllite group

The general formula (as given by Sokolova and Hawthorne, 2016) for the astrophyllite group minerals is A2pBrC7D2(T4O12)2IXOD2XOA4XPDnWA2 where C represents cations at the M(1-4) sites in the O sheet and are commonly Fe2+, Mn, Na, Mg, Zn, Fe3+, Ca, Zr, Li; D represents cations in the H sheet and are either in 6 or 5 coordination and are Ti, Nb, Zr, Sn4+, 5Fe3+, Mg, Al; T = Si, Al; A2pBrWA2 (I block) with p =1, 2; r = 1, 2; A = K, Rb, Cs, Ba, H2O, Li, Pb2+, Na, ▫ where ▫ = vacancy; B = Na, Ca, Ba, H2O, ▫; Xo refers to anions in the O sheet not bonded to T sites, XOD = oxygen anions in common at the 3M and D vertices; XOA = OH, F anions at the common vertices of 3M polyhedra; XPD = F, O, OH, H2O, ▫, apical anions of D cations at the edges of the HOH block; WA = H2O, ▫; and for XPDn, n = 0. 1, 2. The astrophyllite group minerals form 2:1 phyllosilicate-type structures with portions of the structure described as HOH (analogous to TOT in 2:1 phyllosilicates) with T4O12 ribbons comprising the H (heterogeneous, hetero- meaning “extra”) sheet. Alternating with HOH blocks are intermediate (I) blocks along the c axis. Sokolova and Hawthorne (2016) described the astrophyllite group as a “supergroup” with three divisions (groups): the astrophyllite group, the kupletskite group and the devitoite group. HOH blocks may link directly (as in astrophyllite group, with Fe2+ dominant) or do not link (as in devitoite group) or direct linkage with Mn2+ dominant (as in kupletskite group). The linkages involve “bridges” of D-XpD-D. These titanosilicates have similar a axial lengths to phyllosilicates (both near 5.4 Å) and d(001) values (~10.9 Å , although somewhat variable vs 10.0 Å in 2:1 phyllosilicates). The supergroup divisions are:
Astrophyllite Group, Fe2+ dominant, direct HOH linkage
astrophyllite K2NaFe2+7Ti2(Si4O12)2O2(OH)4F
iobophyllite K2NaFe2+7(Nb,Ti)(Si4O12)2O2(OH)4(F,O)
zircophyllite K2NaFe2+7Zr2(Si4O12)2O2(OH)4F
bulgakite Li2(Ca,Na)Fe2+7Ti2(Si4O12)2O2(OH)4(F,O)(H2O)2
nalivkinite Li2NaFe2+7Ti2(Si4O12)2O2(OH)4F(H2O)2
tarbagataite (K ▫)CaFe2+7Ti2(Si4O12)2O2(OH)5
Kupletskite Group, Mn2+ dominant, direct HOH linkage
kupletskite-1A K2NaMn7Ti2(Si4O12)2O2(OH)4F
kupletskite-2M K2NaMn7Ti2(Si4O12)2O2(OH)4F
kupletskite-(Cs) Cs2NaMn7Ti2(Si4O12)2O2(OH)4F
niobokupletskite K2NaMn7(Nb,Ti)2(Si4O12)2O2(OH)4(O,F)
Devitoite group
devitoite Ba6Fe2+7Fe3+2(Si4O12)2(PO4 )2 (CO3 )O2 (OH)4
sveinbergeite (H2O)2[Ca(H2O)](Fe2+6Fe3+)Ti2(Si4O12)2O2(OH)4(OH,H2O)
lobanovite K2Na(Fe2+4Mg2Na)Ti2(Si4O12)2O2(OH)4
HOH blocks are found in other (heterophyllosilicate) titanosilicates, and these minerals have been described by Ferraris and co-workers (e.g., for a partial summary, see Ferraris, 1997,
Sokolova, 2006, Jin et al., 2018). These include:
nafertisite [Na,K, ▫)4(Fe2+,Fe3+, ▫)10(Ti2O3Si12O34)(O,OH)6],
bafertisite [(Ba2(Fe,Mn)4Ti2(Si2O7)2O2(OH)2F2,
jinshajiangite (Na,Ca)(Ba,K)Fe4Ti2(Si2O7)2O2(OH)2F,
perraultite (Na,Ca)(Ba,K)Mn4Ti2(Si2O7)2O2(OH)2F,
lamprophyllite Na2(Sr,Ti,Na,Fe)4(Ti2O2Si4O14)(O,F)2,
seidozerite Na1.6Ca0.275Mn0.425Ti0.575Zr0.925(Si2O7)OF,
and many others. The titanosilicates are found in hyperagpaitic (highly peralkaline nepheline syenites) rocks.