Hammadah al Hamra 237 (HaH 237)
Hammadah al Hamra 237 (HaH 237) was
discovered on October 18th, 1997 in the form of a single stone
weighing 3.17kg in the Ash Shati' area of Libya. It was
initially listed as a CH-Chondrite but after extensive studies
of meteorites in this clan it was later reclassified into the CB3b
group. This meteorite has a Shock Rating of S3 and a Weathering
Level of W2.
The CB b chondrite
metal appears to have formed
by a process very similar to that of the CH-Chondrites, but the
CBb
meteorite components
experienced even less thermal alteration following their
formation and are among the most primitive materials known to
have formed in the solar nebula. (Campbell, Humayun & Weisburg,
2005)
Iron/Nickel (Fe,Ni) metal and chondrule
silicates are the main components in HaH 237. These high
temperature components are held together by shock melts
consisting of droplets of dendritically intergrown Fe,Ni-metal/sulfide
embedded in silicate glass, which is substantially more FeO-rich
(30–40 wt%) than the chondrule silicates (FeO <5 wt%). Fine-grained matrix material, which is a major component
in most other chondrite classes, is extremely scarce in HaH 237.
(Meibom et al, 2004)
The Iron/Nickel (Fe/Ni) component in HaH 237 is
considerably high at about 57% but the overall bulk composition
of Iron (Fe) is 69.6 wt%. It also contains a very small
amount (<1%) of CAI's (Calcium-Aluminium-Rich Inclusions) which
measure a tiny 50-400µm. The characteristics of the CAI's in HaH
237 are inconsistent with an impact origin with these metal-rich
meteorites. Instead it is suggested that the components in CB
chondrites are pristine products of large-scale,
high-temperature processes in the solar nebula and should be
considered true chondrites. (Krot et al, 2001)
This specimen
is part of the Meteorites Australia Collection (MA.07.0037).
Shock melts in QUE 94411, Hammadah al Hamra 237, and Bencubbin:
Remains of the missing matrix?
Anders Meibom, Kevin Righter, Nancy Chabot, Greg Dehn, Angelo
Antignano, Timothy J. McCoy, Alexander N. Krot, Michael E.
Zolensky, Michael I. Petaev, and Klaus Keil.
(14.1MB)
Compositions of unzoned and zoned metal in the CBb chondrites
Hammadah al Hamra 237 and Queen Alexandra Range 94627.
Andrew J. Campbell, Munir Humayunz, and Michael K. Weisberg.
(1.47MB)
Refractory calcium-aluminium-rich inclusions and
aluminium-diopside-rich chondrules in the metal-rich chondrites
Hammadah al Hamra 237 and Queen Alexandra Range 94411.
Alexander N. Krot, Kevin D.
McKeegan, Sara S. Russell, Anders Meibom, Michael K. Weisberg,
Jutta Zipfel, Tatiana V. Krot, Timothy J. Fagan and Klaus Keil. (3.39MB)
Volatile-poor Chondrules in CH Carbonaceous Chondrites:
Formation at high ambient nebular temperature.
Alexander N. Krot, Anders Meibom and Klaus Keil.
(31.6kb)
Chondrules of the very first generation in Bencubbin/CH-like
meteorites QUE 94411 and Hammadah al Hamra 237: Condensation
origin at high ambient nebular temperatures.
Alexander N. Krot, Anders Meibom, Sara S. Russell, Edward Young,
Conel M. Alexander, Kevin D. McKeegan, Gary Lofgren, Jeff Cuzzi,
Jutta Zipfel, and Klaus Keil.
(298kb)
HaH 237 (CB3b) - 2.83g Partslice.
HaH 237 (CB3b) - 2.83g Partslice.
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