2015
DOI: 10.1016/j.pss.2014.11.009
|View full text |Cite
|
Sign up to set email alerts
|

Csátalja, the largest H4–5 chondrite from Hungary

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2

Citation Types

0
10
0

Year Published

2017
2017
2022
2022

Publication Types

Select...
5

Relationship

0
5

Authors

Journals

citations
Cited by 5 publications
(10 citation statements)
references
References 39 publications
0
10
0
Order By: Relevance
“…The higher shock-in duced IR shift of the Csátalja-2 sam ple than in Csátalja-1 is caused by a higher amount of shock melting. Com par ing our Raman FWHM val ues to those of Kovács et al (2015b) on this me te or ite, the peak shock pres sure somewhat ex ceeded 15 GPa in the case of olivines, so higher than Kovacs et al es ti mated.…”
Section: Evaluation Of Estimated Shock Stagesmentioning
confidence: 47%
See 1 more Smart Citation
“…The higher shock-in duced IR shift of the Csátalja-2 sam ple than in Csátalja-1 is caused by a higher amount of shock melting. Com par ing our Raman FWHM val ues to those of Kovács et al (2015b) on this me te or ite, the peak shock pres sure somewhat ex ceeded 15 GPa in the case of olivines, so higher than Kovacs et al es ti mated.…”
Section: Evaluation Of Estimated Shock Stagesmentioning
confidence: 47%
“…As a sum mary, FWHM val ues of py rox enes oc ca sion ally in di cate dif fer ent shock stages (S3-S4) than do the op ti cal ob ser va tions. Csátalja-2 py rox enes and olivines are more strongly shocked than in the ref er ence value of Kovács et al (2015b) as the first mea sure ment from the same me te or ite. The min er als in mixed clasts show sim i lar shock stages to each other in the Csátalja-2 sam ple (S4-S5).…”
Section: Evaluation Of Estimated Shock Stagesmentioning
confidence: 92%
“…In this work, a “recently” found (in August 2012) H chondrite called Csatalja (H4, S2, W1) is analyzed, focusing mainly on the shock‐driven alteration. The meteorite shows several shock‐produced features and recrystallized units (Kovács et al., 2015). It is known that shock impact pulverization in the parent body of these meteorites has produced brecciated structures; however, using detailed textural and compositional analysis, we aim to understand which steps of the evolution of such a body could be decoded.…”
Section: Introductionmentioning
confidence: 99%
“…on its surface(Kov acs et al, 2015).• Central shearing zone: The most heavily fractured zone with brecciated texture and rectangular clasts characterized by cataclastic texture in numerous shock veins; the of microfracture infiltrations. It is bordered by a clastic shock vein from the average inner volume of the sample.…”
mentioning
confidence: 99%
“…The elements included in the sample are vaporized, atomized and excited in hot plasma generating an atomic and ionic spectrum that is characteristic of the elemental composition of the sample [1]. LIBS has been widely employed in the chemical analysis of meteorites of diverse nature using different laboratory based set-ups [2][3][4][5]. Stand-off LIBS at distances up to 8.…”
Section: Introductionmentioning
confidence: 99%