Computer Science
Scientific paper
Jul 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979natur.280..116h&link_type=abstract
Nature, vol. 280, July 12, 1979, p. 116-119. Research supported by the Natural Environment Research Council.
Computer Science
22
Chemical Composition, Chondrites, Meteorites, Mineral Deposits, Planetary Evolution, Temperature Effects, Abundance, Crystallization, Czechoslovakia, Energy Spectra, Glass, Minerals, Phase Diagrams, Tieschitz Meteorite, Chondrules, Chondrites, Origin, Olivines, Pyroxenes, Composition, Petrology, Meteorites, Metamorphism, Volatiles, Silicates, Geochemistry, Electron Microscopy, Nepheline, Accretion, Fractional Crystallization, Pressure Gradients, Viscosity
Scientific paper
The Tieschitz, H3, chondritic meteorite apparently formed as part of a
parent-body by the accretion of both molten and solid materials with a
mean temperature of 800 + or - 100 C, followed by slow cooling to lower
temperatures. The data argue against the currently accepted model of
equilibration with a cooling gas of solar composition.
Agrell Stuart O.
Ashworth John R.
Bevan Alex W. R.
Hutchison Robert
No associations
LandOfFree
Accretion temperature of the Tieschitz, H3, chondritic meteorite 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 Accretion temperature of the Tieschitz, H3, chondritic meteorite, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accretion temperature of the Tieschitz, H3, chondritic meteorite will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1557487