Iridescent Iron Oxides
Abstract
Iridescent iron oxides known as rainbow hematite and turgite are found in a variety of localities worldwide and display a variety of beautiful interference colors. Usually, there is a thin layer of nanocrystals containing aluminum and phosphorous coats, such as with hematite, although one example of aluminum with arsenic is presented. Infrared spectra of samples with thicker layers of these nanocrystals show absorption in the phosphate region. The thin films that range from tens to hundreds of nanometers thick are believed to cause the color. High-resolution secondary electron imaging shows that the thin film consists of nanocrystals arranged in three directions (120° apart). The rod-shaped crystals have a width from 5 to 35 nm and display the same morphology on all samples, irrespective of if they contain phosphorus or arsenic. The minute crystals have failed to produce either an X-ray powder diffraction pattern, an electron back-scatter diffraction pattern in SEM, or an electron diffraction ring pattern under TEM. Raman spectra are dominated by hematite features. Infrared ATR spectra of the bulk material show mostly hematite with occasional minor amounts of goethite and phosphate.
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Acknowledgement
Rock H. Currier (Jewel Tunnel Imports) drew the authors’ attention to this problem and provided numerous research samples. Robert Housley, Benny Fenn, PA Schroeder and Paul M Adams provided additional samples. Mineracoes Brasileiras Reunidas S.A. is thanked for permission to collect samples at their mines.
Funding
Contributions
G.R.R. conducted the spectroscopic and wet-chemistry experiments. C.M. conducted the electron-beam experiments. Both authors contributed figures and contributed to the drafting of the manuscript. All authors have read and agreed to the published version of the manuscript.
Data Availability
The authors confirm that the data supporting the findings of this study are available within the article. Additional spectra and electron microscope image are available from the authors.
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Additional details
- White Rose Foundation
- National Science Foundation
- EAR-9804871
- National Science Foundation
- EAR-0337816
- National Science Foundation
- DMR-0080065
- Accepted
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2025-01-21Accepted
- Available
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2025-01-23Published
- Caltech groups
- Division of Geological and Planetary Sciences
- Publication Status
- Published