HONOLULU 1825 (HAWAII)
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Honolulu L5 vnd.; Oahu, Hawaii USA, fell 1825 Sept. 27, 0.366 g, ex coll. R. Elliott |
On September 27, 1825 several stones weighing 3 kg in total fell near Honolulu, Oahu Island, Hawaii, USA.
On September 26, 1825, a Russian expedition of circumnavigation on the ship Predpriyatie (Enterprise) reached the Hawaiian
islands.
Its captain, Otto Kotsebu: Next morning after we arrived we became witnesses of a fantastic natural phenomena which we
could see from the beginning to the end. In a crystal-clear sky a solid black cloud formed above the island. The darkest part
of this mysterious cloud loomed above the town of Ganaruro. A total calm suddenly changed to a storm wind blowing from the
northeast. Simultaneously a terrific noise came from the cloud, as if a multitude of ships had begun firing their cannons.
Thunderclaps followed each by other, as if opponents were exchanging broadsides. This noise stopped after several minutes,
when two stones fell into the streets of Ganaruro, breaking into several pieces when they struck the Earth. People picked
up these pieces, which were still warm.
TUCSON 1850 (ARIZONA)
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Tucson IRUNGR ATAX; Arizona, USA, found 1850, 2 masses @ 975 kg, part slice 2.75 g |
The above slice was cut from piece #122a.
H. H. Nininger had a 940 g crescent-shaped slice (labelled #122a) in his collection (H. H. Nininger, The Nininger Collection
of Meteorites, American Meteorite Museum, 1950). In 1960 the Arizona State University (ASU) purchased the Nininger Collection.
On July 1, 1960 the American Meteorite Laboratory was established by Glenn and Margaret Huss (the daughter of H. H. and
Addie Nininger) as successor to the American Meteorite Museum, formerly operated by Margarets parents. Because Niningers
collection was sold to ASU, G. and M. Huss had no collection now, but a limited number of meteorites on consignment for distribution
from Nininger, e.g. a 47.3 gram part slice of the Tucson meteorite with the number H299.1 (Glenn I. Huss, The Huss Collection
of Meteorites, Denver CO, 1976).
In 1985 the American Meteorite Museum states a specimen #122a of 574.2 g and a piece of #122a.1 of 148. 0 g which was
obviously cut from the #122a specimen (Ch. F. Lewis, J. A. Wrona, C. B. Moore: Catalog of Meteorites, Center for Meteorite
Studies, Arizona State Univ. 1985).
So the above small slice was traded with ASU but comes originally from the famous H.H. Nininger collection.
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Left: old scetch of the Tucson Ring, right: both masses at the Smithsonian |
Two masses of the Tucson meteorite were found in 1850, but native people must have known about these masses of iron for centuries
before that. One was the ring-shaped Irwin-Ainsa mass, the second the paired, bean-shaped, Carleton mass. The meteorites consist
of 92% iron with 8% silicate inclusions, which is very high for an iron meteorite. Tucson may be the result of an impact between
an iron asteroid and a stony asteroid. The parent body of the Tucson meteorite cooled rapidly, so there is no Widmanstätten
pattern present. The Tucson meteorite is classified as an ungrouped ataxite iron with silicate inclusions.
Each of the Tucson masses has its unique history. The first recovered and the larger of the two is the 688 kg ring-shaped
mass, also called the Ring or Signet, Ainsa and Irwin-Ainsa Meteorite at various times in history: The earliest account of
the meteorites is by a Sonoran official, Jose Francisco Velasco, who says several iron masses were found between Tucson and
Tubac, in Puerto de los Muchachos and at the foot of Sierra de la Madera. One mass, he said, was taken to Tucson. Later,
the second known mass, Carleton, was also transported from the mountains to Tucson. Both masses had been used as anvils in
blacksmith shops.The Mexican troops left Tucson in 1856, leaving behind the famous meteorites. In 1860, the Smithsonian Institution
asked Lieutenant Irwin, an army physician and amateur naturalist in the area, to go to Tucson to recover the Tucson Ring meteorite.
He found it, pulled it out of the ground, and entrusted it to a man who was to go to the coast and deliver it by ship to the
museum. The man carried out his mission, but told the Smithsonian that his great-grandfather had discovered the meteorite.
The family name, Ainsa, was given to the meteorite. Irwin attempted for many years to re-establish the truth before the deception
was finally recognized.
The ring shape with the huge hole of the Tucson meteorite is unique among the large meteorites. What caused the huge hole
is difficult to say. One explication might be that a huge nodule of troilite had occupied this cavity. When the parent body
passed through the atmosphere, this less-resistant metal melted.
The other mass, originally weighing 287 kg, is named the Carleton Meteorite because it was confiscated by Colonel Carleton
during the Civil War and sent to San Francisco.
Today, both fragments of the Tucson meteorite can be admired at the Smithsonian National Museum of Natural History, Washington,
D.C. in the Hall of Geology, Gems, and Minerals.
WILLAMETTE 1902 (OREGON)
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Willamette IIIAB Om; OR USA; found 1902, 14.7 g etched slice (ex. coll. ETH / JNMC Zurich) |
In 1902, in the Willamette Valley of Oregon, a Welsh immigrant named Ellis Hughes discovered the Willamette meteorite but
unfortunately it was on land owned by the Oregon Iron and Steel Company. With the help of his young son and a horse, Mr. Hughes
moved the meteorite in secret to his own land, which was many weeks of hard work to cover a 1200 m distance. Mr. Hughes then
claimed ownership and showed it to the public for a few cents entrance fee. Unfortunately one of the first visitors was a
man from the Oregon Iron and Steel Company and so the moving was discovered, and after a lawsuit, the company became owner.
The meteorite was purchased by Mrs. William E. Dodge in 1905, for $26,000 (an equivalent value of more than half a million
$ today) and donated to the American Museum of Natural History in New York City where it is now on display.
In old times the meteorite was reputedly a venerated object by Native American tribes in that area, so the Confederated
Tribes of the Grand Ronde Community of Oregon, a group of Native American tribes, claimed to have used the meteorite to perform
an annual ceremony. These tribes requested that the meteorite has to be returned. Finally they reached an agreement with the
museum in 2000, allowing tribal members to conduct their private ceremony once a year.
In 2007, Representative John Lim introduced a resolution that would demand that the museum has to return the Meteorite
to Oregon, but fortunately the Confederated Tribes said they were not consulted, did not support the resolution and were content
with the arrangement with the museum.
Here you will find more infos about the Willamette meteorite:
Willamette meteorite, Rose Center, NYC
Willamette meteorite, Agreement
Henry A. Ward, the Willamette meteorite
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Old glass(!) slide (8 x 10 cm) showing the Willamette meteorite and two kids. |
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Old Postcard: The Willamette Meteorite , American Museum - Hayden Planetarium, NYC |
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Old photo (28 x 35cm): Willamette meteorite and unknown lady. |
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Old coloured b/w postcard: Meteorite that Fell at Oregon City, Oregon |
HOLBROOK 1912 (ARIZONA)
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Holbrook L/LL6; fell in the USA 1912 July 19, 2.7 g/3.0 g/3.4 g and 3.5 g (ex. AMNH, N.Y.) |
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Holbrook L/LL6, AZ USA, 38.3 g with original label |
CUMBERLAND FALLS (KENTUCKY)
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Cumberland Falls, USA 1919, Aubrite, 2.96 g |
JOHNSTOWN (COLORADO)
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Johnstown Diogenite; CO USA, fell 1924, 1.934 g |
PIÑON (NEW MEXICO)
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Pinon IRUNGR ATAX anom; found in NM USA in 1928, 1.6 g, w. orig. envelope, ex coll. JNMC/ETH Zurich. |
PASAMONTE (NEW MEXICO)
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Pasamonte Eucrite; NM USA, fell 1933, 1.626 g |
KENDLETON (TEXAS)
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Kendleton L4 br.; TX USA; fell 1939 May 2, cut fragment 21.6 g, ex JNMC, Zurich. |
PEÑA BLANCA SPRING (TEXAS)
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Peña Blanca Spring AUB, TX USA, Fell 1946, 10.8 g |
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Peekskill H6 mbr.; fell in NY USA 1992 October 9. 1.70 g (ex coll. A. Lang, N.Y.)) |
PARK FOREST (ILLINOIS)
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Park Forest, USA, L5, March 26, 2003, 9.9 g |
NEW ORLEANS (LOUISIANA)
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New Orleans H5; USA, fell through a roof (arrow!) on Sept. 23, 2003, 12.2 g (ex Hupé Coll.) |
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