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Fossilized Magnetotactic Bacterium in the Orgueil Meteorite What'sNEW

Orgueil Fossil
Electron microscope photo of an acid resistant "filamentary microstructure" containing "electron dense bodies" in the Orgueil meteorite, discovered by Sam L. VanLandingham and W. C. Tan in 1966. Length is approximately 6 micrometers. (View larger 60K gif)

In 1966, W. C. Tan and Sam L. VanLandingham examined samples of the Orgueil meteorite. Orgeuil is a carbonaceous meteorite like the Murchison meteorite (but Orgueil lacks chondrules). It was seen as it fell near Orgueil, France, on May 14, 1864. Samples of it have been extensively studied, especially by Bart Nagy, whose photos of lifelike fossils in it were published in Nature, in the early 1960s. The above photo was among several dozen by Tan and VanLandingham of fossils in Orgueil that looked biological to them. It was among a handful published in a brief article in the Journal of the Royal Astronomical Society, in 1967 (1).

In those days, Tan and VanLandingham had no idea what the "filamentary microstructures" like this one might be, because they had never heard of magnetotactic bacteria. Today however, we do know about such bacteria. They ingest iron and retain it in particles which cause the bacteria to align themselves with a magnetic field. If enough of the bacteria become fossilized together, the product will be a "natural magnet". Sam VanLandingham says that the Orgueil sample in which the fossil was found had many similar fossils, all neatly aligned.

When seen through a transmission electron microscope, the most striking feature of magnetotactic bacteria is the magnetosomes inside them. These membrane-bound particles of magnetite (iron oxide) or greigite (iron sulfide) appear as dark, regularly spaced inclusions whose geometry and spacing vary from one species to another. (In this example they resemble dark portholes on a tiny submarine.)

The picture below shows a typical magnetotactic bacterium, of the species Rhodopseudomonas rutilis. Its size and shape are very similar to those of the fossil above. Most telling, however, is the match in size, shape and spacing of the magnetosomes. In 1998, NASA's Richard Hoover first showed the above photo to Russian bacteriologist Mikhail Vainshtein, who studies magnetotactic bacteria. He recognized it immediately. The photo below came from Vainshtein's collection (2,3).

Rhodopseudomonas rutilis
Transmission electron microscope photo of a purple photosynthetic bacterium of the species Rhodopseudomonas rutilis provided by Mikhail Vainshtein of the Russian Academy of Sciences. Scale bar = .5 micrometer.

The fossil from the Orgueil meteorite, photographed in 1966, was first identified as a magnetotactic bacterium like the one in the lower photo only this year [1998]. We suggest that this evidence of a fossilized bacterium in a carbonaceous meteorite cannot be easily dismissed.

What'sNEW since 1998

Richard Hoover comments, 18 May 2016: Ed Anders's claim of contamination in Orgueil, in 1964, hindered research for forty years.
3 Mar 2011: Fossilized bacteria in meteorites are obvious.
More Evidence for Indigenous Microfossils in Carbonaceous Meteorites, a new webpage posted 15 Aug 2010.
2 Aug 2004: Microfossils in a meteorite.
magnetosomes Cells' magnets bared, by Helen Pearson, Nature Science Update, 17 Dec 2002. (See photo at right.)
In a Reply we discuss the possibility that the fossil is an earthly contaminant, 14 September 1998.


1. W. C. Tan and S. L. VanLandingham, "Electron microscopy of biological-like structures in the Orgueil carbonaceous meteorite," p 237 v 12 Geophys. J. Royal Astr. Soc., 1967.
2. M. Vainshtein, N. Suzina and V. Sorokin, "A new type of magnet-sensitive inclusions in cells of photosynthetic purple bacteria", p 182-186 v 20 System. Appl. Microbiol. (1997).
3. (photo also published in) Richard Hoover, Alexei Yu. Rozanov, S. I. Zhmur and V. M. Gorlenko, "Further Evidence of Microfossils in Carbonaceous Chondrites" [abstract], in Instruments, Methods, and Missions for Astrobiology, Richard B. Hoover, Editor, Proceedings of SPIE Vol. 3441, p 203-216 (1998).

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