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Siderite

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Siderite
General
CategoryCarbonate mineral
Formula
(repeating unit)
FeCO3
IMA symbolSd[1]
Strunz classification5.AB.05
Dana classification14.01.01.03
Crystal systemTrigonal
Crystal classHexagonal scalenohedral (3m)
H-M symbol:(32/m)
Space groupR3c
Unit cella= 4.6916
c= 15.3796 [Å];Z= 6
Identification
ColorPale yellow to tan, grey, brown, green, red, black and sometimes nearly colorless
Crystal habitTabular crystals, often curved; botryoidal to massive
TwinningLamellar uncommon on{0112}
CleavagePerfect on {0111}
FractureUneven to conchoidal
TenacityBrittle
Mohs scalehardness3.75–4.25
LusterVitreous, may be silky to pearly
StreakWhite
DiaphaneityTranslucent to subtranslucent
Specific gravity3.96
Optical propertiesUniaxial (−)
Refractive indexnω= 1.875
nε= 1.633
Birefringenceδ= 0.242
DispersionStrong
References[2][3][4]

Sideriteis amineralcomposed ofiron(II) carbonate(FeCO3). Its name comes from theAncient Greekwordσίδηρος(sídēros), meaning "iron". A valuableiron ore,it consists of 48%ironand lackssulfurandphosphorus.Zinc,magnesium,andmanganesecommonly substitute for the iron, resulting in the siderite-smithsonite,siderite-magnesite,and siderite-rhodochrositesolid solutionseries.[3]

Siderite hasMohs hardnessof 3.75 to 4.25, aspecific gravityof 3.96, a whitestreakand avitreous lustreor pearlyluster.Siderite isantiferromagneticbelow itsNéel temperatureof 37 K (−236 °C) which can assist in its identification.[5]

It crystallizes in thetrigonal crystal system,and arerhombohedralin shape, typically with curved and striated faces. It also occurs in masses. Color ranges from yellow to dark brown or black, the latter being due to the presence of manganese.

Siderite is commonly found inhydrothermalveins,and is associated withbarite,fluorite,galena,and others. It is also a commondiageneticmineral inshalesandsandstones,where it sometimes formsconcretions,which can encase three-dimensionally preservedfossils.[6]Insedimentary rocks,siderite commonly forms at shallow burial depths and its elemental composition is often related to thedepositional environmentof the enclosing sediments.[7]In addition, a number of recent studies have used theoxygen isotopic compositionof sphaerosiderite (a type associated withsoils) as aproxyfor theisotopiccomposition ofmeteoric watershortly after deposition.[8]

Carbonate iron ore[edit]

Althoughcarbonateiron ores, such as siderite, have been economically important for steel production, they are far from ideal as an ore.

Their hydrothermal mineralisation tends to form them as smallore lenses,often following steeplydippingbedding planes.[i]This makes them not amenable toopencast working,and increases the cost of working them by mining with horizontalstopes.[10]As the individual ore bodies are small, it may also be necessary to duplicate or relocate the pit head machinery,winding engineand pumping engine, between these bodies as each is worked out. This makes mining the ore an expensive proposition compared to typicalironstoneorhaematiteopencasts.[ii]

The recovered ore also has drawbacks. The carbonate ore is more difficult tosmeltthan a haematite or other oxide ore. Driving off the carbonate as carbon dioxide requires more energy and so the ore 'kills' theblast furnaceif added directly. Instead the ore must be given a preliminary roasting step. Developments of specific techniques to deal with these ores began in the early 19th century, largely with the work ofSir Thomas LethbridgeinSomerset.[12]His 'Iron Mill' of 1838 used a three-chambered concentric roasting furnace, before passing the ore to a separate reducing furnace for smelting. Details of this mill were the invention of Charles Sanderson, a steel maker of Sheffield, who held the patent for it.[13]

These differences between spathic ore and haematite have led to the failure of a number of mining concerns, notably theBrendon Hills Iron Ore Company.[14]

Spathic iron ores are rich in manganese and have negligible phosphorus. This led to their one major benefit, connected with theBessemer steel-making process.Although the first demonstrations by Bessemer in 1856 were successful, others' initial attempts to replicate his method infamously failed to produce good steel.[15]Work by the metallurgistRobert Forester Mushetshowed that the reason for the discrepancy was the nature of the Swedish ores that Bessemer had innocently used; they were very low in phosphorus. Using a typical European high-phosphorus ore in Bessemer's converter gave a poor quality steel. To produce high quality steel from a high-phosphorus ore, Mushet realised that he could operate the Bessemer converter for longer, burning off all the steel's impurities including the unwanted phosphorus but also the carbon (which is an essential ingredient in steel), and then re-adding carbon, along with manganese, in the form of a previously obscure ferromanganese ore with no phosphorus,spiegeleisen.[15]This created a sudden demand for spiegeleisen. Although it was not available in sufficient quantity as a mineral, steelworks such as that atEbbw Valein South Wales soon learned to make it from the spathic siderite ores.[16]For a few decades, spathic ores were therefore in demand and this encouraged their mining. In time though, the original 'acidic' liner of the Bessemer converter, made from siliceous sandstone organister,was replaced by a 'basic' liner in the newerGilchrist Thomas process.This removed the phosphorus impurities asslagproduced by chemical reaction with the liner, and no longer required spiegeleisen. From the 1880s demand for the ores fell once again and many of their mines, including those of theBrendon Hills,closed soon after.

Gallery[edit]

Notes[edit]

  1. ^Some siderite, along withgoethite,also forms inbog irondeposits,[9]but these are small and economically minor.
  2. ^Both ironstones andbanded iron formationsare sedimentary formations, thus the economically viable deposits may be considerable thicker and more extensive.[11]

References[edit]

  1. ^Warr, L. N. (2021)."IMA–CNMNC approved mineral symbols".Mineralogical Magazine.85(3): 291–320.Bibcode:2021MinM...85..291W.doi:10.1180/mgm.2021.43.S2CID235729616.
  2. ^"Siderite".Handbook of Mineralogy: Borates, Carbonates, Sulfates(PDF).Tucson, Arizona: Mineral Data Publishing. 2003.ISBN9780962209741.Archived fromthe original(PDF)on 13 March 2022.Retrieved2022-11-30.
  3. ^abSiderite,Mindat.org,retrieved2022-11-30
  4. ^Siderite Mineral Data,WebMineral,retrieved2022-11-30
  5. ^Frederichs, T.; von Dobeneck, T.; Bleil, U.; Dekkers, M. J. (January 2003). "Towards the identification of siderite, rhodochrosite, and vivianite in sediments by their low-temperature magnetic properties".Physics and Chemistry of the Earth, Parts A/B/C.28(16–19): 669–679.Bibcode:2003PCE....28..669F.doi:10.1016/S1474-7065(03)00121-9.
  6. ^Garwood, Russell; Dunlop, Jason A.; Sutton, Mark D. (2009)."High-fidelity X-ray micro-tomography reconstruction of siderite-hosted Carboniferous arachnids".Biology Letters.5(6): 841–844.doi:10.1098/rsbl.2009.0464.PMC2828000.PMID19656861.
  7. ^Mozley, P. S. (1989). "Relation between depositional environment and the elemental composition of early diagenetic siderite".Geology.17:704–706.
  8. ^Ludvigson, G. A.; Gonzalez, L. A.; Metzger, R. A.; Witzke, B. J.; Brenner, R. L.; Murillo, A. P.; White, T. S. (1998). "Meteoric sphaerosiderite lines and their use for paleohydrology and paleoclimatology".Geology.26:1039–1042.
  9. ^Sedimentary Geology,p. 304.
  10. ^Jones (2011),p. 34–35,37.
  11. ^Prothero, Donald R.; Schwab, Fred (1996).Sedimentary Geology.New York: W. H. Freeman and Company. pp. 300–302.ISBN0-7167-2726-9.
  12. ^Jones, M. H. (2011).The Brendon Hills Iron Mines and the West Somerset Mineral Railway.Lightmoor Press. pp. 17–22.ISBN9781899889-5-3-2.
  13. ^GB 7828,Charles Sanderson, "Smelting Iron Ores", issued October 1838
  14. ^Jones (2011),p. 99.
  15. ^abJones (2011),p. 16.
  16. ^Jones (2011),p. 158.