Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/93577/1/j.1945-5100.1996.tb02069.x.pd
The Moon is the only planetary body, besides Earth, from which there are samples from known location...
Sample 12032,366-18 is a 41.2 mg basaltic rock fragment collected during the Apollo 12 mission to th...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Isotopic studies of mare basalts have led workers to conclude that their sources are heterogeneous o...
Lunar meteorites provide a potential opportunity to expand the study of ancient (>4000 Ma) basaltic ...
Precise crystallisation ages have been determined for a range of Apollo basalts from Pb-Pb isochrons...
Anorthosite 60015 contains the lowest initial Sr-87/Sr-86 ratio (0.69884 + or - 0.00004) yet reporte...
Miller Range (MIL) 13317 is a heterogeneous basalt‐bearing lunar regolith breccia that provides insi...
The basaltic suites collected at the Apollo 12 landing site have been interpreted as representing a ...
Establishing the age of the Moon is critical to understanding solar system evolution and the formati...
The nature of the early lunar magmatic and impact histories remains a fundamental, yet poorly unders...
The origin and evolution of the Moon remain controversial 1,2, with one of the most important questi...
Lunar sample 15474,4 is a tiny fragment of olivine-augite vitrophyre that is a mare basalt. Although...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...
We conducted a thorough analysis of the feldspathic breccia meteorite Dhofar 1428 with the aim of be...
The Moon is the only planetary body, besides Earth, from which there are samples from known location...
Sample 12032,366-18 is a 41.2 mg basaltic rock fragment collected during the Apollo 12 mission to th...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Isotopic studies of mare basalts have led workers to conclude that their sources are heterogeneous o...
Lunar meteorites provide a potential opportunity to expand the study of ancient (>4000 Ma) basaltic ...
Precise crystallisation ages have been determined for a range of Apollo basalts from Pb-Pb isochrons...
Anorthosite 60015 contains the lowest initial Sr-87/Sr-86 ratio (0.69884 + or - 0.00004) yet reporte...
Miller Range (MIL) 13317 is a heterogeneous basalt‐bearing lunar regolith breccia that provides insi...
The basaltic suites collected at the Apollo 12 landing site have been interpreted as representing a ...
Establishing the age of the Moon is critical to understanding solar system evolution and the formati...
The nature of the early lunar magmatic and impact histories remains a fundamental, yet poorly unders...
The origin and evolution of the Moon remain controversial 1,2, with one of the most important questi...
Lunar sample 15474,4 is a tiny fragment of olivine-augite vitrophyre that is a mare basalt. Although...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...
We conducted a thorough analysis of the feldspathic breccia meteorite Dhofar 1428 with the aim of be...
The Moon is the only planetary body, besides Earth, from which there are samples from known location...
Sample 12032,366-18 is a 41.2 mg basaltic rock fragment collected during the Apollo 12 mission to th...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
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