A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has become a central tenet of recent models describing planetary dynamics and the potential habitability of early terrestrial environments. The prevalence of ∼3.9 Ga∼3.9 Ga crystallization ages for lunar impact-melt breccias and U–Pb isotopic compositions of lunar crustal rocks provide the primary evidence for a short-lived, cataclysmic episode of late heavy bombardment at that time. Here we report U–Pb isotopic compositions of zirconolite and apatite in coarse-grained lunar melt rock 67955, measured by ion microprobe, that date a basin-scale impact melting event on the Moon at 4.22±0.01 Ga4.22±0.01 Ga followed by entrainment within lower grade ejec...
The U-Pb systems of apatite and merrillite grains within four separate Apollo 14 impact melt breccia...
Lunar breccia 73217 is composed of plagioclase and pyroxene clasts originating from a single gabbron...
Two general classes of lunar impact breccias have been recognised: fragmental breccias and melt brec...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Radiometric dating and compositional clustering of lunar impact-melt rocks form the backbone of the ...
The nature of the early lunar magmatic and impact histories remains a fundamental, yet poorly unders...
Lunar impact melt breccias provide a unique record of the timing and frequency of collisional events...
Lunar meteorites represent a more random sampling of lunar material than the Apollo or Luna collecti...
New zircon UPb and trace element investigations from Apollo 14 lunar impact breccia sample #14311 re...
New zircon UPb and trace element investigations from Apollo 14 lunar impact breccia sample #14311 re...
We studied 42 impact-melt clasts from lunar feldspathic regolith breccias MacAlpine Hills (MAC) 8810...
Planetary bodies in our Solar System, including the Moon, were exposed to an intense asteroid bombar...
In a histogram of lunar impact ages from the Apollo 16 site, there is a spike circa 3.9 Ga that has ...
Deformed lunar zircons yielding U-Pb ages from 4333 Ma to 1407 Ma have been interpreted as dating di...
Samples of lunar rock returned by the Apollo and Luna missions show a cluster of impact melt ages be...
The U-Pb systems of apatite and merrillite grains within four separate Apollo 14 impact melt breccia...
Lunar breccia 73217 is composed of plagioclase and pyroxene clasts originating from a single gabbron...
Two general classes of lunar impact breccias have been recognised: fragmental breccias and melt brec...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Radiometric dating and compositional clustering of lunar impact-melt rocks form the backbone of the ...
The nature of the early lunar magmatic and impact histories remains a fundamental, yet poorly unders...
Lunar impact melt breccias provide a unique record of the timing and frequency of collisional events...
Lunar meteorites represent a more random sampling of lunar material than the Apollo or Luna collecti...
New zircon UPb and trace element investigations from Apollo 14 lunar impact breccia sample #14311 re...
New zircon UPb and trace element investigations from Apollo 14 lunar impact breccia sample #14311 re...
We studied 42 impact-melt clasts from lunar feldspathic regolith breccias MacAlpine Hills (MAC) 8810...
Planetary bodies in our Solar System, including the Moon, were exposed to an intense asteroid bombar...
In a histogram of lunar impact ages from the Apollo 16 site, there is a spike circa 3.9 Ga that has ...
Deformed lunar zircons yielding U-Pb ages from 4333 Ma to 1407 Ma have been interpreted as dating di...
Samples of lunar rock returned by the Apollo and Luna missions show a cluster of impact melt ages be...
The U-Pb systems of apatite and merrillite grains within four separate Apollo 14 impact melt breccia...
Lunar breccia 73217 is composed of plagioclase and pyroxene clasts originating from a single gabbron...
Two general classes of lunar impact breccias have been recognised: fragmental breccias and melt brec...