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A rusty green early ocean?

Date:
January 31, 2017
Source:
Weizmann Institute of Science
Summary:
How were Earth's solid deposits of iron ore created? One researchers suggests that, billions of years ago, "green rust" formed in seawater and sank to the ocean bed, becoming an original source of banded iron formations. While this would have been just one means of iron deposition, green rust seems to have delivered a large proportion of iron to our early ocean.
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Though they may seem rock solid, the ancient sedimentary rocks called iron formations -- the world's chief economic source of iron ore -- were once dissolved in seawater. How did that iron go from a dissolved state to banded iron formations? Dr. Itay Halevy and his group in the Weizmann Institute of Science's Department of Earth and Planetary Sciences suggest that, billions of years ago, the "rust" that formed in the seawater and sank to the ocean bed was green -- an iron-based mineral that is rare on Earth today but might once have been relatively common. Their findings were published in Nature Geoscience.

We know there was dissolved iron in the early oceans -- a strong indication that Earth's free oxygen concentrations were exceedingly low. Otherwise, the iron would have reacted with oxygen to form iron oxides, which are the rusty red deposits familiar to anyone who's left a bike out in the rain. Today, says Dr. Halevy, iron is delivered from the land to the oceans as small insoluble oxide particles in rivers. But this mode of sedimentation only came about as free oxygen accumulated in Earth's atmosphere, about 2.5 billion years ago. With almost no oxygen, the oceans were iron-rich, but that did not mean that iron remained dissolved in seawater indefinitely: it ultimately formed insoluble compounds with other elements and settled to the seabed to give rise to banded iron formations.

The idea that one of those insoluble compounds could be a rusty green mineral occurred to him during his doctoral research, says Dr. Halevy, when he was trying to recreate the conditions on early Mars, including its rusty-red iron sediments. "I got some green stuff I didn't recognize at first, which quickly turned orange when I exposed it to air. With a little more careful experimentation, I found that this was a mineral called green rust, which is extremely rare on Earth today, owing to its affinity for oxygen." Today, green rust quickly transforms into the familiar red rust, but with not much free oxygen around, Dr. Halevy reasoned, it could have been an important way for dissolved iron to form solid compounds and settle to the sea floor.

Support for these ideas comes from Sulawesi, Indonesia, where green rust forms today in iron-rich, oxygen-poor Lake Matano, thought to be similar to the seawater that existed during extended periods of Earth's early history. To test his ideas in detail and explore their significance, Dr. Halevy set up experiments in which he and his team recreated, as closely as possible, the conditions of the ancient, oxygen-free, Precambrian ocean. They found that green rust not only forms under these conditions, but that when left to age, it transforms into the minerals found in Precambrian iron formations -- a combination of iron-bearing oxides, carbonates, and silicates.

Could green rust have been a main vehicle for settling iron out of seawater? Dr. Halevy and his team developed models to depict the iron cycle in Earth's early oceans, including the possibility of green rust formation and competition with other mineral shuttles of iron to the seafloor. Their findings suggest that green rust was probably a major player in the iron cycle. The iron in the green rust later transformed into the minerals we can now observe in the geologic record. "Of course, it would have been one of several means of iron deposition, just as a number of different processes are involved in chemical sedimentation in the oceans today," says Dr. Halevy. "But as far as we can tell, green rust should have delivered a substantial proportion of iron to the very early ocean sediments."


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Materials provided by Weizmann Institute of Science. Note: Content may be edited for style and length.


Journal Reference:

  1. I. Halevy, M. Alesker, E. M. Schuster, R. Popovitz-Biro, Y. Feldman. A key role for green rust in the Precambrian oceans and the genesis of iron formations. Nature Geoscience, 2017; DOI: 10.1038/ngeo2878

Cite This Page:

Weizmann Institute of Science. "A rusty green early ocean?." ScienceDaily. ScienceDaily, 31 January 2017. <www.sciencedaily.com/releases/2017/01/170131080007.htm>.
Weizmann Institute of Science. (2017, January 31). A rusty green early ocean?. ScienceDaily. Retrieved March 28, 2024 from www.sciencedaily.com/releases/2017/01/170131080007.htm
Weizmann Institute of Science. "A rusty green early ocean?." ScienceDaily. www.sciencedaily.com/releases/2017/01/170131080007.htm (accessed March 28, 2024).

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