NWA 2921 was discovered
during 2005 in the Sahara Desert, Africa. This meteorite has
been classified as a Rumurutiite Chondrite, R3.8 with a Shock
Rating of S1 and a Weathering Level of W3.
The specimen below is a 44.4g Halved Individual displaying an
obvious dark, unequilibrated, primitive clast. The clast
deceivingly resembles a carbonaceous chondrite and appears to
consist of chondrules and chondrule fragments set in a dark,
fine-grained matrix. The darkening of the clasts in R-Chondrites
is caused by the dispersion of sulphide grains and have been found to be
considerably
unaltered since their formation. In fact some clasts have been found to
be as low as a 3.2 subgroup and probably represent the most
primitive lithology yet found in the Rumurutiites.
The Rumuruti
parent-body underwent thermal metamorphism after formation and subsequently the
other petrologic types 4, 5 and 6 have also been found in
R-Chondrite meteorites. The parent-body later underwent impact
processes which excavated and liberated this material including
the primitive type-3 clasts. This is evident in the samples
found here on Earth such as the individual below which are
usually
regolith/genomict breccias. (Click
here
for the Meteorites Australia Glossary).
This specimen is pictured on Page 88 and 89
of O. Richard Norton's wonderful "Field Guide to Meteors and
Meteorites" and is part of the Meteorites Australia Collection (MA.06.0020).
NWA 2921 (R3.8) - 19.5g Half Individual
(Click image to enlarge in new window.)
NWA 2921 (R3.8) - 23.7g Half Individual
(Click image to enlarge in new window.)
NWA 2921 (R3.8) -
44.4g Individual before slicing.
(Click image to enlarge in new window.)