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Astrocyanite-(Ce)

A valid IMA mineral species
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About Astrocyanite-(Ce)Hide

Formula:
Cu2(Ce,Nd,La)2(UO2)(CO3)5(OH)2 · 1.5H2O
Colour:
Bright blue
Lustre:
Vitreous, Earthy
Hardness:
2 - 3
Specific Gravity:
3.80
Crystal System:
Hexagonal
Name:
From the Greek άστρον ("astron") for "star", κυανός ("kyanos") for "blue", in allusion to its colour and habit of the aggregates, and the dominant lanthanide element in its composition.
Unique combination of elements.


Unique IdentifiersHide

Mindat ID:
404
Long-form identifier:
mindat:1:1:404:8

IMA Classification of Astrocyanite-(Ce)Hide

Classification of Astrocyanite-(Ce)Hide

5.EF.05

5 : CARBONATES (NITRATES)
E : Uranyl Carbonates
F : UO2:CO3 = 1:5
16b.1.6.1

16b : HYDRATED CARBONATES CONTAINING HYDROXYL OR HALOGEN
1 : AmBn(XO3)pZqxH2O & with (m+n):p = 1:1
11.11.17

11 : Carbonates
11 : Carbonates of Cr and U

Mineral SymbolsHide

As of 2021 there are now IMA–CNMNC approved mineral symbols (abbreviations) for each mineral species, useful for tables and diagrams.

SymbolSourceReference for Standard
Acy-CeIMA–CNMNCWarr, L.N. (2021). IMA–CNMNC approved mineral symbols. Mineralogical Magazine, 85(3), 291-320. doi:10.1180/mgm.2021.43

Physical Properties of Astrocyanite-(Ce)Hide

Vitreous, Earthy
Transparency:
Translucent, Opaque
Colour:
Bright blue
Streak:
White, blue (bluish)
Hardness:
2 - 3 on Mohs scale
Density:
3.80 g/cm3 (Measured)    3.95 g/cm3 (Calculated)

Optical Data of Astrocyanite-(Ce)Hide

Type:
Uniaxial (-)
RI values:
nω = 1.688 nε = 1.638
Max. Birefringence:
δ = 0.050
Based on recorded range of RI values above.

Interference Colours:
The colours simulate birefringence patterns seen in thin section under crossed polars. They do not take into account mineral colouration or opacity.

Michel-Levy Bar The default colours simulate the birefringence range for a 30 µm thin-section thickness. Adjust the slider to simulate a different thickness.

Grain Simulation You can rotate the grain simulation to show how this range might look as you rotated a sample under crossed polars. Each grain retains its interference colour (retardation) while its brightness falls to black at extinction and reaches a maximum between extinction positions.

Surface Relief:
Very High (positive)
Relative to Canada balsam mounting medium (n ≈ 1.537).

This shows the grain boundary and Becke line effect under plane-polarised light, based on the contrast between this mineral's average refractive index and the mounting medium. It does not take into account mineral colouration.
In focus
Interference Figure:
This shows the idealized uniaxial interference figure - the conoscopic (convergent-light, Bertrand-lens-in) view, for a grain cut with the optic axis centred and vertical. The coloured rings are isochromatics, computed with the same physics as the Michel-Lévy bar above; the dark cross is the isogyre.

For a genuinely uniaxial mineral viewed this way, that cross stays perfectly stationary if you rotate the stage - unlike a biaxial mineral, where it splits apart on rotation. That invariance is itself the standard diagnostic test for telling uniaxial and biaxial minerals apart at the microscope.
Pleochroism:
Strong
Comments:
Strongly pleochroic from bright blue to pale blue, almost colorless.

Chemistry of Astrocyanite-(Ce)Hide

Mindat Formula:
Cu2(Ce,Nd,La)2(UO2)(CO3)5(OH)2 · 1.5H2O
Element Weights:
Element% weight
O31.585 %
Ce26.986 %
U22.922 %
Cu12.239 %
C5.783 %
H0.485 %

Calculated from ideal end-member formula.

Crystallography of Astrocyanite-(Ce)Hide

Crystal System:
Hexagonal
Cell Parameters:
a = 14.96 Å, c = 26.86 Å
Ratio:
a:c = 1 : 1.795
Unit Cell V:
5,205.95 ų (Calculated from Unit Cell)
Z:
12
Morphology:
Platy {001}
Comment:
space group P6/mmm, P6mm, P622, P62m or P6m2

X-Ray Powder DiffractionHide

Powder Diffraction Data:
d-spacingIntensity
13.3 Å(40)
6.73 Å(100)
4.30 Å(50)
4.16 Å(60)
3.72 Å(90)
2.488 Å(40)
2.154 Å(40)
2.071 Å(40)
Comments:
114.6-mm Debye-Scherrer camera, copper Ka radiation

Geological EnvironmentHide

Paragenetic Mode(s):

Type Occurrence of Astrocyanite-(Ce)Hide

General Appearance of Type Material:
Delicate rostettes of tablets.
Place of Conservation of Type Material:
Institut royal des Sciences naturalles de Belgique, Brussels, Belgium.
Geological Setting of Type Material:
Oxidation product of uraninite.
Associated Minerals at Type Locality:

Synonyms of Astrocyanite-(Ce)Hide

Other Language Names for Astrocyanite-(Ce)Hide

Common AssociatesHide

Associations Based on Photo Data:
15 photos of Astrocyanite-(Ce) associated with Kamotoite-(Y)Y2(UO2)4(CO3)3O4 · 14H2O
4 photos of Astrocyanite-(Ce) associated with Shabaite-(Nd)Nd2Ca[(UO2)(CO3)3](CO3)2(H2O)10.5
4 photos of Astrocyanite-(Ce) associated with UranophaneCa(UO2)2(SiO3OH)2 · 5H2O
3 photos of Astrocyanite-(Ce) associated with UraniniteUO2
1 photo of Astrocyanite-(Ce) associated with Pendevilleite-(Y)Mg2Y3Al(UO2)2(CO3)7(OH)6(H2O)16

RadioactivityHide

Radioactivity:
Element % Content Activity (Bq/kg) Radiation Type
Uranium (U) 22.9219% 5,730,475 α, β, γ
Thorium (Th) 0.0000% 0 α, β, γ
Potassium (K) 0.0000% 0 β, γ

For comparison:

  • Banana: ~15 Bq per fruit
  • Granite: 1,000–3,000 Bq/kg
  • EU exemption limit: 10,000 Bq/kg

Note: Risk is shown relative to daily recommended maximum exposure to non-background radiation of 1000 µSv/year. Note that natural background radiation averages around 2400 µSv/year so in reality these risks are probably extremely overstated! With infrequent handling and safe storage natural radioactive minerals do not usually pose much risk.

Interactive Simulator:

Note: The mass selector refers to the mass of radioactive mineral present, not the full specimen, also be aware that the matrix may also be radioactive, possibly more radioactive than this mineral!

Activity:

DistanceDose rateRisk
1 cm
10 cm
1 m

The external dose rate (D) from a radioactive mineral is estimated by summing the gamma radiation contributions from its Uranium, Thorium, and Potassium content, disregarding daughter-product which may have a significant effect in some cases (eg 'pitchblende'). This involves multiplying the activity (A, in Bq) of each element by its specific gamma ray constant (Γ), which accounts for its unique gamma emissions. The total unshielded dose at 1 cm is then scaled by the square of the distance (r, in cm) and multiplied by a shielding factor (μshield). This calculation provides a 'worst-case' or 'maximum risk' estimate because it assumes the sample is a point source and entirely neglects any self-shielding where radiation is absorbed within the mineral itself, meaning actual doses will typically be lower. The resulting dose rate (D) is expressed in microsieverts per hour (μSv/h).

D = ((AU × ΓU) + (ATh × ΓTh) + (AK × ΓK)) / r2 × μshield

Other InformationHide

Notes:
Soluble with effervescence in dilute HCl.
Special Storage/
Display Requirements:
Radioactive
Health Risks:
This radioactive species sit always on massive uraninite and should be manipulated and stored with precautions.

Internet Links for Astrocyanite-(Ce)Hide

References for Astrocyanite-(Ce)Hide

Localities for Astrocyanite-(Ce)Hide

Showing 1 localities.

This map shows a selection of localities that have latitude and longitude coordinates recorded. Click on the symbol to view information about a locality. The symbol next to localities in the list can be used to jump to that position on the map.
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Locality ListHide

- This locality has map coordinates listed. - This locality has estimated coordinates. ⓘ - Click for references and further information on this occurrence. ? - Indicates mineral may be doubtful at this locality. - Good crystals or important locality for species. - World class for species or very significant. (TL) - Type Locality for a valid mineral species. (FRL) - First Recorded Locality for everything else (eg varieties). Struck out - Mineral was erroneously reported from this locality. Faded * - Never found at this locality but inferred to have existed at some point in the past (e.g. from pseudomorphs).

All localities listed without proper references should be considered as questionable.
DR Congo (TL)
 
  • Lualaba
    • Mutshatsha
      • Kamoto
European Journal of Mineralogy (1990) +4 other references
 
and/or  
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