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Banded iron formation

 
Sci-Tech Dictionary: banded iron formation
 
(¦band·əd ′ī·ərn för′mā·shən)

(geology) A sedimentary mineral deposit consisting of alternate silica-rich (chert or quartz) and iron-rich layers formed 2.5-3.5 billion years ago; the major source of iron ore.


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Sci-Tech Encyclopedia: Banded iron formation
 

Banded iron formation is a sedimentary rock that was commonly deposited during the Precambrian. It was probably laid down as a colloidal iron-rich chemical precipitate, but in its present compacted form it consists typically of equal proportions of iron oxides (hematite or magnetite) and silica in the finely crystalline form of quartz known as chert. Its chemical composition is 50% silicon dioxide (SiO2) and 50% iron oxides (Fe2O3 and Fe3O4), to give a total iron content of about 30%. Banding is produced by the concentration of these two chemical components into layers about 1–5 cm (1/2–2 in.) thick; typical banded iron formation consists of pale silica-rich cherty bands alternating with black to dark red iron-rich bands (see illustration). These contrasting layers are sharply defined, so that the rock has a striped appearance; banded iron formation is normally a hard, tough rock, highly resistant both to erosion and to breaking with a hammer.

Folded banded iron formation from the Ord Range, Western Australia. The distance between top and bottom of the polished face of the sample is about 15 cm (6 in.). Chert jasper bands alternate with dark magnetite-rich bands. The thin pale layers of irregular thickness are bands of asbestiform amphibole, now replaced by silica, to give the semiprecious material “tiger-eye.” (<i>Photo courtesy of John Blockley</i>)
Folded banded iron formation from the Ord Range, Western Australia. The distance between top and bottom of the polished face of the sample is about 15 cm (6 in.). Chert jasper bands alternate with dark magnetite-rich bands. The thin pale layers of irregular thickness are bands of asbestiform amphibole, now replaced by silica, to give the semiprecious material “tiger-eye.” (Photo courtesy of John Blockley)

The world's iron and steel industry is based almost exclusively on iron ores associated with banded iron formation. Banded iron formation itself may be the primary ore, from which hematite or magnetite is concentrated after crushing. But the main ore now mined globally is high-grade (greater than 60% iron) material that formed within banded iron formation by natural leaching of its silica content.


 
Wikipedia: Banded iron formation
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2.1 billion year old banded iron formation
Close-up of Banded Iron Formation specimen from Upper Michigan. Scale bar is 5.0 mm.

Banded iron formations (also known as banded ironstone formations or BIFs) are a distinctive type of rock often found in primordial (Precambrian) sedimentary rocks. The structures consist of repeated thin layers of iron oxides, either magnetite (Fe3O4) or hematite (Fe2O3), alternating with bands of iron-poor shale and chert. Some of the oldest known rock formations, formed around three thousand million years before present (3 Ga), include banded iron layers, and the banded layers are a common feature in sediments for much of the Earth's early history. Banded iron beds are less common after 1.8 Ga, although some are known that are much younger.

The total amount of oxygen locked up in the banded iron beds is estimated to be perhaps twenty times the volume of oxygen present in the modern atmosphere. Banded iron beds are an important commercial source of iron ore, such as the Pilbara region of Western Australia and the Mesabi Range in Minnesota.

Contents

Origins

The conventional concept is that the banded iron layers were formed in sea water as the result of oxygen released by photosynthetic cyanobacteria (bluegreen algae), combining with dissolved iron in Earth's oceans to form insoluble iron oxides, which precipitated out, forming a thin layer on the substrate, which may have been anoxic mud (forming shale and chert). Each band is similar to a varve, to the extent that the banding is assumed to result from cyclic variations in available oxygen. It is unclear whether these banded ironstone formations were seasonal, followed some feedback oscillation in the ocean's complex system or followed some other cycle.[1] It is assumed that initially the Earth started out with vast amounts of iron dissolved in the world's acidic seas. Eventually, as photosynthetic organisms generated oxygen, the available iron in the Earth's oceans was precipitated out as iron oxides.[citation needed] At the tipping point where the oceans became permanently oxygenated, small variations in oxygen production produced pulses of free oxygen in the surface waters, alternating with pulses of iron oxide deposition.

Water flowing over iron-rich beds

Snowball Earth scenario

Until 1992,[2] it was assumed that the rare, later (younger) banded iron deposits represent unusual conditions where oxygen was depleted locally and iron-rich waters could form then come into contact with oxygenated water. An alternate explanation of these later deposits is undergoing much discussion as part of the Snowball Earth hypothesis. This hypothesis states that an early equatorial supercontinent (Rodinia) was totally covered in an ice age (implying the whole planet was frozen at the surface to a depth of several kilometers). In this case the Earth's free oxygen may have been nearly or totally depleted during a severe ice age circa 750 to 580 million years ago (mya). Dissolved iron then accumulated in the oxygen-poor oceans (from seafloor hydrothermal vents, say). Following the thawing of the Earth, the seas became oxygenated once more causing the precipitation of the iron.

Another mechanism for BIF-formatíon, also proposed in the context of the Snowball Earth discussion, is by deposition from metal-rich brines in the vicinity of hydrothermally active rift zones.[3] Alternatively, some geochemists suggest that BIFs could form by direct oxidation of iron by (non-photosynthetic) autotrophic microbes.[4]

See also

References

  1. ^ Good discussions for the layman are in Cesare Emiliani, Plant Earth 1992:407f, and Tjeerd van Andel, New Views on an Old Planet 2nd ed. 1994:303-05.
  2. ^ Kirschvink, Joseph (1992). "Late Proterozoic low-latitude global glaciation: the Snowball Earth", in J. W. Schopf; C. Klein: The Proterozoic Biosphere: A Multidisciplinary Study. Cambridge University Press.
  3. ^ Eyles, N.; Januszczak, N. (2004). "’Zipper-rift’: A tectonic model for Neoproterozoic glaciations during the breakup of Rodinia after 750 Ma". Earth-Science Reviews 65 (1-2): 1-73. Retrieved on 2008-02-04.
  4. ^ Andreas Kappler et al.: Deposition of banded iron formations by anoxygenic phototrophic Fe(II)-oxidizing bacteria. Geology, November 2005, v. 33, no. 11, p. 865–868. (pdf, 250 Kb) (doi:10.1130/G21658.1 Abstract)

 
 

 

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