Canyon Diablo Metallic Spheroids are found in the soil
surrounding the famous Meteor Crater in Arizona. When the large body that created the famous Meteor
Crater impacted, the majority of it vaporized. This created a
huge cloud of hot Iron/Nickel vapour and as the cloud cooled,
the iron started to condense and fall from the sky as an
Iron/Nickel rain. The ground within about 8 kilometres of the
crater contains a huge quantity of these droplets but they are
very difficult to separate out. The spheroids below were originally collected by Harvey Nininger
and are part of the Meteorites Australia Collection (0.4mm diameter - MA.02.0131 and 1.4mm diameter
MA.02.0132).
Dr. Harvey H. Nininger realised that these spheroids probably represented
the missing main mass of the Canyon Diablo meteorite that others
had believed would still be found buried deep within the crater.
Nininger talks about the spheroids in his 1972 book; “Find A
Falling Star” of which some is excerpted below.
Find A Falling Star (1972), Harvey H. Nininger, Chapter 11 -
Discovery (pp175-187)
"During the frequent meteorite-hunting excursions that Addie,
Margaret and I made in the summer of 1946, my interest turned
more to the dust and small particles of sand grain-size that
continually collected on our magnets. Back at the trailer below
Mt. Elden I spent many hours going over these small particles
which en masse always gave a strong chemical reaction for
nickel.
I suspected during that summer that I was finding the
condensation products which Merrill had declared were lacking
and which the Moulton explosion-theory seemed to require for its
verification, but our trailer facilities were not adequate for
the complete examination which the several types of material
that we were collecting required.
In the sorting of fragments gathered during the magnetic rake
survey of 1939 we had discarded all material that would pass an
eight-mesh screen. As we sifted out and cast away this great
bulk of fine particles, I had begun to wonder whether perhaps we
were culling the most important part of our harvest, and so I
had bagged up a goodly sample of the discard for laboratory
study and carried it back to Denver, but I had not got around to examining it.
The greatest keys to my evolving theory about the crater were
found in my boxes of soil samples. I was beginning to be certain
that neither I nor anyone else had given to the soil in the
environs of the crater the careful attention deserved, and when
I turned my attention to the small particles of various
descriptions that crowded the soil, the most exciting avenues of
exploration and speculation were opened.
The metal-center pellets made up but a small part of the
magnetics gathered. At least a hundred particles must have been
tested, individually, before finally, when one more particle was
dissolved and subjected to the dimethylglyoxime test, a
beautiful strawberry red appeared in the test tube.
Surprisingly, the nickel-bearing particle was neither round nor
black, as I had expected; it was brown and had a somewhat lumpy
surface, though it tended toward the spherical in shape.
Once we had learned how to recognize these and separate them from
the several other kinds of magnetic particles, we took hundreds
of samples on all sides of the crater and found that these
metallic droplets were whole present in the top soil to an
extent that projected to thousands of tons! Here, then, was the
proof of Dr. Moulton’s explosion theory.
I could think of no other way to account for these little
droplets, two and a half times as rich in nickel as similar
sized irregular fragments, than that they were condensation
droplets from a meteoritic cloud produced by the explosion which
Moulton had hypothesized. I named these droplets metallic
spheroids.
The survival of these tiny bits of pure metal was exciting. The
spheroids, so tiny that 280,000 of them would weigh an ounce,
were found as far from the crater as five miles. At that
distance they were distributed at a rate of a few hundred pounds
to the square mile; close to the crater rim the concentration
was on the order of a thousand tons per square mile. We measured
the quantity of spheroids in sixty different locations on state
lands and estimated that from 4,000 to 8,000 tons must be
present in the upper four inches of soil within an average
radius of two and one-half miles from the crater rim. By
projection, taking into account the processes of weathering, it
is not unreasonable to estimate that the original deposit
totaled as much as 100,000 to 200,000 tons."
Two (1 gram) vials of Canyon Diablo Metallic Spheroids. (0.4mm left, 1.4mm right)
Canyon Diablo (IAB) - 660.5g Sculptured &
Regmaglypted Individual (MA.06.0058)