Metal, iron, & nickel

Take-home message

The metal in meteorites strongly attracts a magnet. If you have a piece of metal or a rock that contains metal but it does not attract a magnet, then it is not a meteorite. Meteorites do not contain visible grains or chunks of nonferrous metals like aluminum, manganese, chromium, copper, brass, or gold.

If you have a piece of metal that does attract a magnet and want to know if it is an iron meteorite, then obtain a chemical analysis for the elements iron (Fe), cobalt (Co), nickel (Ni), chromium (Cr), and manganese (Mn). Iron meteorites will have 75-95% Fe, 5-25% Ni, 0.2-2% Co, and <0.05 % (<500 ppm) each of Cr and Mn. A metallurgical testing lab can provide this analysis. I recommend testing for Cr and Mn because most industrial (man-made) iron contains higher concentrations of these elements than does metal in meteorites. If the metal contains more than 0.05% chromium or manganese, then it is not a meteorite.

Iron-nickel metal

More than 95% of all meteorites contain iron-nickel (FeNi) metal. As a consequence, meteorites have concentrations of nickel that are much greater than that of nearly any terrestrial rock.

“Iron-nickel” means that the metal is mostly iron but it also contains 5-30% nickel. The metal occurs as two different alloys known as kamacite (lower nickel concentration) and taenite (higher nickel concentration). Both alloys strongly attract magnets. Neither alloy occurs naturally in Earth rocks, so a natural rock that contains kamacite or taenite is a meteorite.

Many people tell me that they can “see” nickel in their rock. No. You cannot see nickel in a meteorite. You can see iron-nickel metal, but it is impossible to determine if the metal contains nickel just by looking. It requires a chemical analysis to determine if the metal contains enough nickel to be consistent with a meteorite. A metal detector cannot identify nickel. A positive response from a nickel allergy test kit (below) is not sufficient to prove that the metal contains enough nickel for the metal to be of meteoritic origin.

The metal in meteorites also contains a few tenths of a percent cobalt; the nickel/cobalt ratio in meteoritic metal is usually in the 10-25 range. Iron-nickel metal in meteorites also has high concentrations (by terrestrial standards) of rare metals like gold, platinum, and iridium. It is usually easiest and cheapest to test for nickel, however, because it is more abundant and easier to measure than the rare metals.

Ordinary chondrites

**A sawn face of the Faucett (Missouri) H5 chondrite. All the light-colored specks are grains of iron-nickel metal.** **Photo credit: Randy Korotev**

Most metal-bearing meteorites are stony meteorites known as ordinary chondrites; the rest are other types of chondrites, brecciated achondrites, irons, pallasites, and stony irons (see statistics). Among ordinary chondrites, the most common type, H-group chondrites (45%), have the most metal, 15-20% by mass. L-group chondrites (40%) have some metal, 7-11%. LL-group chondrites (15%) have the least metal among ordinary chondrites, 3-5%. Because chondrites are rich in metal and the metal is rich in nickel, all chondrites have bulk (whole-rock) concentrations of nickel of 1.0-1.8% (i.e., 10,000-18,000 ppm). That is 100-1000 times greater than practically any terrestrial (earth) rock. An earth rock with as much as 1.0-1.8% Ni would be a nickel ore. In terrestrial rocks the nickel is not contained in metal, however, but in silicate and sulfide minerals.

One cannot determine if a rock contains high concentrations of nickel just “by looking.” FeNi metal looks just like Fe metal. A chemical analysis is required. Metal detectors cannot determine if a rock contains 1-2% Ni or that a chunk of metal contains 5-30% nickel.

Many people have told me, “But, I see metal!” when there really isn’t any. Sometimes it is hard to tell the difference between metal and shiny nonmetals like some sulfide and oxide minerals or micas. If the “metal” is yellowish, then it is not metal but pyrite (“fool’s gold”). If the rock contains shiny bits but it does not attract a cheap ceramic magnet, then it is not a meteorite.

One easy test for grains or slabs that are at least a few millimeters in size is simply to measure the electrical resistance with an ohmmeter. You can buy handheld multimeters in any good hardware store for $30. In resistance mode (ohms), putting the leads some distance apart on any of these iron meteorites would give a low resistance – <100 or probably <10 ohms. This test may not work on an ordinary chondrite because the iron grains are not connected. Shiny hematite or pyrite aggregates will have high electrical resistance because they do not conduct electricity.

Some rare meteorites do not contain any appreciable metal and, consequently, they have low concentrations of Ni. Unbrecciated achondrites are poor in metal. In other words, many of the rarest types of meteorites contain little or no metal and have low nickel concentrations, just like earth rocks.

Iron meteorites

Iron meteorites, of course, are nearly 100% metal, although many contain the iron sulfide mineral troilite. The concentration of nickel in iron meteorites, typically 5-30%, is much greater than that in industrial metals except for high-nickel steels. The concentration of nickel in industrial iron is usually <1%.

Most collectors would agree that the most attractive iron meteorite is Sikhote-Alin (IIAB). At least 23 tons in mass, the meteorite is the largest to fall in historical times. It fell in the Sikhote-Alin mountains of eastern Russia on February 12th, 1947. **Photo credit: Randy Korotev**

**Thousands of pieces of Sikhote-Alin have been recovered. This is a collection of Sikhote-Alin “shrapnel.” Sikhote-Alin is not a “ruster” like Campo del Cielo (below).** **Photo credit: Randy Korotev**

Widmanstätten pattern

Iron meteorites are from the metallic core of asteroids. The iron cools so slowly that large grains of interlocking metal form. If an iron meteorite is sawn, polished, and etched with an appropriate weak acid solution, the individual metal grains are revealed in a geometric pattern called a Widmanstätten pattern.

*Left*: A softball-size piece of the 50-ton Campo del Cielo (Argentina) iron meteorite. *Right*: Sawn, polished, and etched slab of the meteorite. Notice the coarse Widmanstätten pattern. Among collectors, Campo del Cielo is known as a “ruster” because of its tendency to easily rust (far right). **Photo credit: Randy Korotev**

Sawn, polished, and etched slab of the Gibeon iron meteorite (Namibia). Gibeon, one of the largest meteorites (26 tons), has a finer Widmanstätten pattern than does Campo del Cielo. Widmanstätten patterns only occur on sawn, polished, and etched faces of an iron meteorite. The linear *lamellae* are intergrowths of crystals of kamacite and taenite. The crystals are large because they cooled slowly over millions of years in the core of an asteroid. One consequence of this slow cooling is that iron meteorites do not easily bend or break unless they are badly rusted. **Photo credit: Randy Korotev**

A sawn, polished, etched slice of Glorieta Mountain (New Mexico, USA) showing the fine Widmanstätten pattern. The meteorite is classified as an anomalous pallasite. Perhaps as many as 28 pieces of this meteorite have been found with a total mass of 186 kg. Only a few of the pieces contain obvious olivine; this piece does not. Photo credit: Randy Korotev

Widmanstätten patterns do not occur in stony meteorites. They are only seen in iron meteorites and pallasites.

A sawn, polished, etched slab of the Canyon Diablo iron (Arizona, USA) meteorite showing the Widmanstätten pattern and large, round troilite (iron sulfide) inclusions. The meteorite specimen is the property of the Collection of the Arizona State University Center for Meteorite Studies.

Pallasites and mesosiderites

Pallasites and mesosiderites are the two types of stony-iron meteorites. Only about 0.2% of known meteorites are pallasites and 0.4% are mesosiderites. Stony-iron meteorites are typically about 50:50 stone:metal.

Pallasites

Pallasites come the boundary between the metallic core and rocky mantle of an asteroid.

An iron meteorite or pallasite that has been buried in the ground for a long time is often unspectacular – until someone hits it with a plow. This is the Conception Junction pallasite found by a landowner in Missouri in 2006. There are many rounded olivine grains imbedded in shiny iron-nickel metal on the sawn surface. Photo credit: Randy Korotev

A sawn slice of Conception Junction. It has experienced considerable weathering and rusting, at least near the exterior. The rounded dark material is the silicate mineral olivine. The lighter gray material is iron-nickel metal. Photo credit: Randy Korotev

A slice of the Brahin pallasite. The meteorite was found in 1968 by a school girl in the Republic of Belarus. Again, the rounded dark materials are grains of olivine. The lighter gray material is iron-nickel metal. **Photo credit: Randy Korotev**

Mesosiderites

Most mesosiderites are breccias formed by collision in asteroid belts of stony asteroids like eucrites and iron asteroids.

In photographs of mesosiderites, I have never seen one that I would call “attractive.”

*Left:* DOM (Dominion Range) 10122 (Antarctica, 171 g), *Right:* Reflected light image of a polished section of DOM 10122. The white material is FeNi metal and troilite, the dark parts are mainly pyroxene. Photo credit: NASA/JSC

**A polished face of the Mincy (Missouri, not Mississippi) mesosiderite in the National History Museum, Vienna. The large green grain is an olivine. Photo credit: MeteoriteCollector.org**

**Fragments of Cumulus Hills 04021 (61 g) and 04032 (85 g) from Antarctica. Photo credit: NASA/JSC**

*Top:* Reflected light image of Cumulus Hills 04210. The whitest grains are metal. *Bottom:* Crossed-polarized image of the same section. The matrix is broken grains of pyroxene, plagioclase, FeNi metal and sulfides. Photo credit: NASA/JSC

Other metal-rich meteorites

Gujba, a CB chondrite, fell in Nigeria in 1984. Only about 22 CB chondrites are known. Gujba and some other CB chondrites have *rounded* metal grains, which are otherwise very rare in meteorites. Like Canyon Diablo (above), it also has rounded blebs of troilite. Notice that this specimen has not been polished thoroughly so the saw marks are still very evident in the metal. Thanks to Karl for loan of the Gujba specimen. **Photo credit: Randy Korotev**

Metal grains reflecting light in a sawn slice of Tafassasset, a primitive achondrite from Niger. Note the saw marks in the metal grains. Saw marks are a good way to distinguish metal from shiny sulfide minerals like pyrite. Sulfide grains will not look so severely and concentrically scraped. This why I recommend sawing to breaking, grinding, sandpaper, or a file.

Industrial slag

Rounded metal blebs usually mean that the “rock” is a piece of slag. In slags, the metal will be dispersed less evenly than in a meteorite and will usually contain vesicles (gas bubbles) in the matrix because the matrix was molten. Thanks to Jeff for the sample.

With a few rare and exceptions, naturally occurring terrestrial rock do not contain iron metal or iron-nickel metal. There are two reasons. First, the Earth formed from the same kind of material as the asteroids but early in Earth’s history the iron-nickel metal that it contained sank to form the Earth’s core. Second, any metal that did not sink has oxidized (rusted) over Earth’s long history. The Earth’s environment is far more oxidizing (oxygen atmosphere and water) than space, where meteorites originate. Earth rocks do contain iron and nickel, but only in oxidized (non-metallic) form. Therefore, if you find a rock that contains iron-nickel metal, then it is almost certainly a meteorite.

When someone walked into my office with this chunk of metal, I thought “Whoa, this could be an iron meteorite!” The “hole” at the lower left was suspicious, however, and when we sawed into it (inset, upper right), it was full of vesicles. Iron meteorites are cores of asteroids that cooled from liquids over millions of years. They do not contain vesicles. (The elongated “hole” in Gibeon, above, is not a vesicle, it is a void where a troilite grain was “plucked” during sawing of the meteorite.) Also, when we analyzed this chunk of metal, there was much less that 1% nickel. I do not know how this thing formed, but it is man-made.

Many people find slags, other by-products of metal manufacturing, and man-made metal things. Some may have been from forges or blacksmith shops that are more than 100 years old. Others appear to have fallen from the sky for unknown reasons (see Getafe). Metal in slags and industrial by-products is mostly iron. Such materials will probably contain little nickel (much less than 1%). So, if you can determine that the sample has little or no nickel, then the sample is not a meteorite. Also, as noted above, the metal in meteorites has very low concentrations of chromium and manganese, <0.05%. These two elements are common in man-made metals, however.

Look at how metal grains are distributed in these photos of ordinary chondrites. The metal does not occur in big round globules. Globs are typical of slags. Notice that the metal is sufficiently soft that saw marks and smearing can be seen on the sawn faces. Sulfide minerals do not do that. Note that the meteorites do not contain vesicles. Vesicles (gas bubbles) are typical of slags, however.

Bottom Line

If you have a piece of metal or a rock that contains metal and the metal contains >5% nickel (Ni), then it is probably a meteorite. If the metal contains <5% nickel, however, then the metal chunk or rock is not a meteorite. Also, if the metal contains >0.1% chromium (Cr) or manganese (Mn), then it is almost certainly not a meteorite.

If you have a rock that contains between 1.0 and 1.8% nickel (whole-rock analysis), whether or not it appears to contain metal, then the rock might be a meteorite (ordinary chondrite).

If you have a rock that does not contain metal and has a low concentration of nickel (<1% = <10,000 ppm), then it could still be a rare type of meteorite, an unbrecciated achondrite. The probability is exceedingly small, however, because nearly all (guesstimate: >99.999%) Earth rocks have the same properties – absence iron-nickel metal and low concentrations of nickel (<0.3%).

The DMG test for nickel

I have had some success using a nickel allergy test kit to determine whether metal contains nickel. Such kits are available at well-stocked pharmacies and can be ordered on the internet. All such tests rely on DMG (dimethylglyoxime), which forms a complex that has a distinct pinkish color with ionic nickel or palladium.

Some people have allergies to nickel and metal alloys that contain nickel. The kit I tested was designed to determine whether “metallic objects” contain nickel. It consisted of 2 dropper bottles. “Solution A” was DMG in alcohol. “Solution B” was a weak solution of ammonium hydroxide in water.

The directions read “Place one drop of solution A and one drop of solution B on a cotton-tipped applicator (use equal amounts of both solutions). Rub wet applicator firmly against the test object for 15 seconds. If applicator turns red, the object contains nickel.”

Following these directions, I was unable to get a positive result on an iron meteorite that contains 6% nickel. The applicator did not turn red, but it did turn a rusty brown color. The problem as I see it, is that the test requires ionic (oxidized) nickel and ammonium hydroxide does not liberate much ionic nickel from metal.

As an experiment, I applied a tiny drop of 1% hydrochloric acid (0.3 molar) to the meteorite, waited 15 seconds, and repeated the DMG test by swabbing the acid drop. This time I got a positive result (left). The acid dissolved a small portion of the meteorite, putting nickel ions in solution. The manufacturer of the test kit is not likely to suggest this work-around because hydrochloric acid is very corrosive and is likely to ruin jewelry and other metals if used incorrectly. (I rinsed the meteorite in much water after the test.)

I tried the test also on a sawn face of an ordinary (H group) chondrite and also obtained a positive result.

So, what do you do? Hydrochloric acid is available to consumers is building supply stores as “muriatic acid.” It is used to clean mortar off masonry, among other things. It is extremely nasty stuff, and may not be available in quantities less than a gallon, which is enough to ruin a significant portion of your car. Dilute it 50-to-1. The DMG test will not work if the solution is too acidic. Dilute battery acid (sulfuric acid) would probably also work. Some liquid toilet bowl cleaners contain acids strong enough to dissolve metal. They are usually already colored, however.

Some people have contacted me saying that they obtained a positive result (pink color) when they applied this test to rocks that do not contain metal. I do not understand this. The test is designed for metal and the test is sensitive, but very few terrestrial rocks contain enough nickel to give a pink color. Remember, you are looking for strawberry pink, not rusty pink.

Note added later: I recently used this test on an iron meteorwrong that someone brought to us. When I used the nickel allergy test kit as is, the results are negative – no pink = no nickel. When I apply a bit of hydrochloric acid first, I did get a positive result – a pink cotton swab. Later, I did a real chemical analysis for Ni and obtained 600 ppm. This is a lot of nickel but is still 100 times too low for an iron meteorite. (Concentrations of cobalt, gold, and iridium were also much too low for a meteorite.)

The DMG test is very sensitive to nickel and can lead to a “false positive” with some metal samples. A negative (no pink) result probably means that the metal is not from a meteorite. A positive result means that it might be a meteorite or it might not! A correspondent who has done more research on this than I have claims that if the pink color fades away after 5 minutes, then the metal contains Ni, but not enough to be of meteoritic origin.

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