2009
DOI: 10.1111/j.1945-5100.2009.tb00735.x
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Shergottites Dhofar 019, SaU 005, Shergotty, and Zagami: 40Ar‐39Ar chronology and trapped Martian atmospheric and interior argon

Abstract: Ar and other chronometers argue for primary rather than secondary events. The cosmic ray exposure ages calculated from cosmogenic argon are 15.7 ± 0.7 Ma (Dhofar 019), 1.0-1.6 Ma (SaU 005), 2.1-2.5 Ma (Shergotty) and 2.2-3.0 Ma (Zagami).

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Cited by 17 publications
(22 citation statements)
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“…, these extractions form a trend almost parallel to the 39 Ar/ 40 Ar axis, as well as indicating an age close to 0 Ga. As impact ejection is too weak to reset the Ar‐Ar clock (see studies on numerous Martian meteorites where Ar‐Ar ages are always higher than CRE ages, for example, Korochantseva et al. , ; Meyer ), partial resetting of the clock requires a stronger thermal event preceding the mild ejection impact. Correcting the intermediate‐temperature fractions of 1180–1270 °C for trapped Ar with 40 Ar/ 36 Ar ratios of 17.5 ± 0.2 (Fig. ), a weighted mean age of 890 ± 230 Ma is obtained (Fig.…”
Section: Resultsmentioning
confidence: 87%
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“…, these extractions form a trend almost parallel to the 39 Ar/ 40 Ar axis, as well as indicating an age close to 0 Ga. As impact ejection is too weak to reset the Ar‐Ar clock (see studies on numerous Martian meteorites where Ar‐Ar ages are always higher than CRE ages, for example, Korochantseva et al. , ; Meyer ), partial resetting of the clock requires a stronger thermal event preceding the mild ejection impact. Correcting the intermediate‐temperature fractions of 1180–1270 °C for trapped Ar with 40 Ar/ 36 Ar ratios of 17.5 ± 0.2 (Fig. ), a weighted mean age of 890 ± 230 Ma is obtained (Fig.…”
Section: Resultsmentioning
confidence: 87%
“…; and shocked plagioclase by Korochantseva et al. ). This high‐temperature degassing is characterized by rather constant K/Ca ratios (the last ~30% of the fractional 39 Ar release, corresponding to the temperatures ˃1240 °C; Fig.…”
Section: Resultsmentioning
confidence: 97%
“…Reported crystallization ages are relatively young (<1 Ga) compared with the nakhlites (about 1.3 Ga), with a number between 165 and 180 Ma (e.g., Shergotty; Nyquist et al. 2001a) whereas others have ages of 700–900 Ma (e.g., SaU 005; Korochantseva et al. 2009).…”
Section: Introductionmentioning
confidence: 99%
“…Ages for Martian meteorites are from Korochantseva et al. () and from the compilation in Brandon et al. ().…”
Section: Discussionmentioning
confidence: 99%
“…Yang et al (2015). Ages for Martian meteorites are from Korochantseva et al (2009) and from the compilation in Brandon et al (2012). b) Zr/Nb versus Nb/Th diagram adopted after Condie (2018).…”
Section: Irradiation Recordsmentioning
confidence: 99%