Yes, Kakangari is a unique chondrite

@article{Davis1977YesKI,
  title={Yes, Kakangari is a unique chondrite},
  author={Andrew M. Davis and Lawrence Grossman and R. Ganapathy},
  journal={Nature},
  year={1977},
  volume={265},
  pages={230-232}
}
THE Kakangari chondrite seems to be the only representative so far recognised of a new class of chondrites. Mason and Wiik1 noted a similarity between Kakangari and Mokoia (C3(V)) in bulk chemical composition when expressed on a volatile-free basis, but pointed out that the higher metal content of Kakangari suggests a relationship between it and Renazzo (C2). Recognising that Renazzo contains much less troilite and much more FeO than Kakangari, however, they concluded that Kakangari was a new… Expand
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Noble gases in the unique chondrite, Kakangari
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References

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Is Kakangari a unique chondrite?
THE Kakangari meteorite, possibly a unique member of a distinct chemical class of chondrite, fell in India in 1890. Two stones were seen to fall, and though one was soon destroyed the bulk of theExpand
Determination of REE, Ba, Fe, Mg, Na and K in carbonaceous and ordinary chondrites
Abstract Precise determination of REE and Ba abundances in three carbonaceous (Orgueil Cl, Murchison C2 and Allende C3) and seven olivine-bronzite chondrites were carried out by mass spectrometricExpand
Chemical sub-groups amongst HL chondrites
Abstract Eight HL or Type III carbonaceous chondrites have been analysed for Si, Mg, Al, Ca, Ti, Mn, Na, K and P by X-ray fluorescence spectrometry. Slight differences in composition were observedExpand
Abundance patterns of thirteen trace elements in primitive carbonaceous and unequilibrated ordinary chondrites
Abstract A neutron activation analysis technique was used to determine Au, Re, Co, Mo, As, Sb, Ga, Se, Te, Hg, Zn, Bi and Tl in 11 carbonaceous chondrites, 12 unequilibrated ordinary chondritesExpand
The composition of the stony meteorites (IV) some analytical data on Orgueil, Nogoya, Ornans and Ngawi
Abstract New analytical data on Fe, Si, Mg, Ca, Al, Mn, K, Ti and P in three carbonaceous chondrites (Orgueil, Nogoya and Ornans) and one LL-group chondrite (Ngawi) are presented and compared withExpand
Abundance of 17 trace elements in carbonaceous chondrites.
Abstract Seventeen trace elements (Ag, Au, Bi, Br, Cd, Cs, Ge, In, Ir, Rb, Re, Sb, Se, Te, Tl, U and Zn) were measured by neutron activation analysis in 8 C1 samples (1 Alais, 3 Ivuna, 4 Orgueil) andExpand
Fine structures of mutually normalized rare-earth patterns of chondrites
Abstract REE abundances in ten chondrites (nine falls and one find) were determined very accurately by mass-spectrometric stable isotope dilution techniques. All of the chondrites have differentExpand
Chemical fractionations in meteorites—VI. Accretion temperatures of H-, LL- and E-chondrites, from abundance of volatile trace elements
Abstract Extending our earlier work on 11 L-chondrites, we have measured 9 volatile elements (Ag, Bi, Cs, In, Rb, Tl, Se, Cd, Zn) by neutron activation analysis in 11 LL- and 10 E-chondrites; theExpand
Trace elements in the Allende meteorite. II - Fine-grained, Ca-rich inclusions
Abstract Nine fine-grained feldspathoid-, grossular-, spinel-, pyroxene-bearing inclusions from the Allende meteorite were analysed by instrumental neutron activation analysis. On the average, theseExpand
Chemical fractionations in meteorites—IV abundances of fourteen trace elements in L-chondrites; implications for cosmothermometry
Abstract A neutron activation procedure for Ag, Au, Bi, Br, Cd, Cs, Cu, Ga, In, Pd, Rb, Te, Tl and Zn has been developed and applied to 12 chondrites (11 L3 to L6 and 1 LL3-4). Correlations betweenExpand
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