
![]() Henbury Craters, Australia |
Iron. Octahedrite, medium. (IIA) “CM” REF: P. 165,
“HBIM” REF: P. 638, and “ARN’S” REF: P. 130. Also see “Meteorite Craters and
Impact Structures of the Earth”, P. Hodge, P. 67-70 for additional
information on the Henbury Craters. O. Richard Norton, in “Rocks From
Space”, has provided a condensed description of the theory on the formation
of the craters, with descriptions of the iron meteorites found there. See
pages 138-142, where Norton has included several black and white photos of
specimens, as well as an aerial view showing three of the craters.
The Henbury Crater field includes approximately 13 craters, and was first identified about 1931. The Aborigines, however, were aware of the Henbury Craters at a much earlier date and, based upon their legends, it is speculated by researchers that when the Henbury event occurred, it may have been witnessed by the Aborigines living in the area at that time. The largest crater is elliptical, measuring approximately 720 X 360 feet (another report gives the size as 180 X 140 meters), and the smallest crater measures only about 6 meters in diameter. |
The distribution and appearance of Henbury irons suggests that the Henbury Craters were formed by a small swarm of many individual meteorites. Many the meteorites fell intact and buried themselves, and recovered examples of this type sometimes show the typical regmaglypts and flight orientation seen on iron meteorites from other worldwide localities. Most of the larger members of the fall, however, are presumed to have exploded before, and/or upon impact, producing quantities of bent and/or twisted masses with shrapnel-like form. Many specimens have sharp, ragged edges, attesting to the great forces and heat to which they were subjected. Polished and etched specimens from Henbury will show different characteristics, depending upon their method of formation, i.e.: 1. original, unshocked specimens which fell and were not effected by the explosions, or 2. shocked specimens which were subjected to stress by high heat, or mechanical deformation caused by the above-ground, as well as inter-crater explosions. Some polished/etched specimens will exhibit stressed areas, as well as areas where the Widmanstatten pattern is pronounced, and sharply defined.
All of the specimens in the following photographs were legally field collected circa 1971. The natural specimens all have a thin, reddish-brown outer oxide layer, typically found on Henbury specimens.
Items 1771, 1772, and 1780 have been professionally prepared, and the slightly higher price / gram reflects the cost of specimen preparation.
NOTE: Any of the natural specimens weighing > 100 grams can be custom cleaned
if you would prefer the matte-luster, metallic steel gray surface for exhibit
purposes. Since the natural reddish-brown oxide layer is quite thin on Henbury
irons, a very minimal amount of weight loss is experienced in the cleaning
process – usually less than .50 gram on the smaller specimens, up to only 1.0
to 2.0 grams on the larger pieces.
Click on specimens to see larger pictures |
C = cut ( ) = quantity of cuts
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![]() 1766 |
![]() 1767 |
![]() 1768 |
![]() 1769 |
![]() 1770 |
![]() 1771 |
![]() 607G |
![]() 1772 |
![]() 1773 |
![]() 1774 |
![]() 1775 |
![]() 1776 |
![]() 1777 |
![]() 607N |
![]() 1778 |
![]() 1779 |
![]() 1780 |
![]() 607R |
![]() 607S |
![]() 607T |
![]() 1781 |
![]() 1782 |
![]() 607W |
![]() 1783 FRONT |
![]() 1783 LEFT SIDE |
![]() 1783 BACK |
![]() 1783 RIGHT SIDE |
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Copyright 1998-2012 by Mineralogical Research Co.
All rights reserved.