Dhofar 287 is a lunar meteorite found in Oman in 2001, which consists of a major portion (95%) of low-Ti mare basalt (Dho 287A) and a minor attached part ( 5%) of regolith breccia (Dho 287B). Here, we report the U–Pb systematics of Dho 287A using data collected with a Sensitive High Resolution Ion Microprobe (SHRIMP). In-situ analyses of five merrillite and three apatite grains, which are resistant to secondary petrologic events, resulted in a total Pb/U isochron age of 3.34 ± 0.20 Ga, in 238U/206Pb–207Pb/206Pb–204Pb/206Pb 3-D space (95% confidence level). The observed Pb–Pb isochron of these eight phosphates coupled with four plagioclase grains also yielded a 207Pb/206Pb age of 3.35 ± 0.13 Ga. This formation age, when considered as the cry...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...
To investigate the formation and early evolution of the lunar mantle and crust we have analysed the ...
The 14 lunar meteorites identified thus far were found in Antarctica, the Sahara desert, and Austral...
Dhofar 287 (Dho 287) is a new lunar meteorite, found in Oman on January 14, 2001. The main portion ...
Chronological studies of brecciated lunar meteorites have proved difficult, because they are mixture...
Dhofar 287 (Dho 287), a recently found lunar meteorite, consists in large part (95%) of low-Ti mare...
Lunar meteorites provide a potential opportunity to expand the study of ancient (>4000 Ma) basalt...
The origin and evolution of the Moon remain controversial 1,2, with one of the most important questi...
U-Th-Pb isotopic data were determined on mineral separates of the diabasic lunar meteorite, Yamato-7...
4Constraining the duration of magmatic activity on the Moon is essential to understand how the lunar...
We conducted a thorough analysis of the feldspathic breccia meteorite Dhofar 1428 with the aim of be...
Miller Range (MIL) 13317 is a heterogeneous basalt‐bearing lunar regolith breccia that provides insi...
The petrogenesis of four lunar highlands meteorites, Dhofar 025 (Dho 025), Dhofar 081 (Dho 081), Dar...
The petrogenesis of four lunar highlands meteorites, Dhofar 025 (Dho 025), Dhofar 081 (Dho 081), Dar...
Glass beads formed by ejection of impact-melted lunar rocks and soils are an important component of ...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...
To investigate the formation and early evolution of the lunar mantle and crust we have analysed the ...
The 14 lunar meteorites identified thus far were found in Antarctica, the Sahara desert, and Austral...
Dhofar 287 (Dho 287) is a new lunar meteorite, found in Oman on January 14, 2001. The main portion ...
Chronological studies of brecciated lunar meteorites have proved difficult, because they are mixture...
Dhofar 287 (Dho 287), a recently found lunar meteorite, consists in large part (95%) of low-Ti mare...
Lunar meteorites provide a potential opportunity to expand the study of ancient (>4000 Ma) basalt...
The origin and evolution of the Moon remain controversial 1,2, with one of the most important questi...
U-Th-Pb isotopic data were determined on mineral separates of the diabasic lunar meteorite, Yamato-7...
4Constraining the duration of magmatic activity on the Moon is essential to understand how the lunar...
We conducted a thorough analysis of the feldspathic breccia meteorite Dhofar 1428 with the aim of be...
Miller Range (MIL) 13317 is a heterogeneous basalt‐bearing lunar regolith breccia that provides insi...
The petrogenesis of four lunar highlands meteorites, Dhofar 025 (Dho 025), Dhofar 081 (Dho 081), Dar...
The petrogenesis of four lunar highlands meteorites, Dhofar 025 (Dho 025), Dhofar 081 (Dho 081), Dar...
Glass beads formed by ejection of impact-melted lunar rocks and soils are an important component of ...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...
To investigate the formation and early evolution of the lunar mantle and crust we have analysed the ...
The 14 lunar meteorites identified thus far were found in Antarctica, the Sahara desert, and Austral...