Ringwoodite in shocked chondrites

Computer Science

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Chondrites, Meteoritic Composition, Meteoritic Microstructures, Mineralogy, Phase Transformations, Pressure Effects, Scanning Electron Microscopy, Temperature Effects, Transmission Electron Microscopy

Scientific paper

Since the discovery of ringwoodite in the meteorite Tenham, further studies confirmed that this mineral occurs preferentially in melt veins and melt pockets of highly shocked L chondrules. Except for some special Transmission Electron Microscopy (TEM) studies a comprehensive study of this high-pressure phase of olivine in the general scope of shock metamorphism of chondrites is missing. Eighteen ringwoodite-bearing L6(S6) chondrites were studied, some of them in more detail: L6(S6)-Catherwood, L6(S6)-Coorara, L6(S6)-Johnson City, L6(S6)-Pampa del Infierno, L6(S6)-Tenham, and L5-6(S6)-Acfer 040. They were analyzed by the optical microscope, Scanning Electron Microscopy (SEM), microprobe, and TEM. Ringwoodite is formed in chondrites at locations where localized melting occurs by shock waves exceeding 50 GPa. The localized shock-pressure and temperature concentrations are obviously favorable for the kinetics of the olivine-spinel transition. Ringwoodite crystallizes most probably not during the short peak pressure pulse but rather during the more extended phase of pressure release, where the temperature is still extremely high, presumably near the solidus of chondrites. The observed chemical variation of individual ringwoodite grains and the indication that wadsleyite coexists with ringwoodite, could be explained as follows. On release from a high-pressure-shock state, olivine transforms to an assemblage of the Beta phase (wadsleyite) and the gamma phase (ringwoodite) in the pressure range between about 20 and 13 GPa. In the two-phase region, where the Beta and gamma phases coexist under equilibrium conditions, the two phases would have compositions in the range Fa(13-25) and Fa(25-31) respectively if the primary olivine composition is 24-25 mol% Fa. This range is very near to the observed chemical variation within polycrystalline ringwoodite grains Fa(19-31).

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Ringwoodite in shocked chondrites does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Ringwoodite in shocked chondrites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ringwoodite in shocked chondrites will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-822343

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.