Lunar cryptomaria: Physical characteristics, distribution, and implications for ancient volcanism

@article{Whitten2015LunarCP,
  title={Lunar cryptomaria: Physical characteristics, distribution, and implications for ancient volcanism},
  author={Jennifer L. Whitten and James W. Head},
  journal={Icarus},
  year={2015},
  volume={247},
  pages={150-171}
}
Lunar cryptomaria: Mineralogy and composition of ancient volcanic deposits
Lunar Cryptomare: New Insights Into the Balmer‐Kapteyn Region
Cryptomaria record the early mare volcanisms and put important constraints on the lunar thermal and volcanic history and on the early partial melting of the mantle. This work focuses on the
Volcanic Processes in the Gassendi Region of the Moon
The lunar floor‐fractured crater Gassendi and surrounding area were examined with high‐resolution Lunar Reconnaissance Orbiter imagery and other remote sensing data to characterize and understand the
New Insights Into Lithology Distribution Across the Moon
Lithology distribution across the Moon is pivotal for understanding lunar evolution. However, so far, the distribution of lunar rock suites is still uncertain; as a result, many related core issues
Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes
Flooding of the lunar surface by ancient mare basalts has rendered uncertain the ages of lunar geochemical terranes and several impact basins. Here we combine craters having recognizable surface
The nature and origin of Mafic Mound in the South Pole‐Aitken Basin
“Mafic Mound” is a distinctive and enigmatic feature 75 km across and 1 km high near the center of the vast South Pole‐Aitken Basin (SPA). Using several modern data sets, we characterize the
...
...

References

SHOWING 1-10 OF 146 REFERENCES
Cryptomare magmatism 4.35 Gyr ago recorded in lunar meteorite Kalahari 009
TLDR
It is suggested that mare basalt volcanism on the Moon started as early as 4.35 ± 0.15 billion years ago, relatively soon after its formation and differentiation, and preceding the bulk of lunar volcanism which ensued after the late heavy bombardment around 3.8-3.9 Gyr.
Lunar Impact Basins and Crustal Heterogeneity: New Western Limb and Far Side Data from Galileo
Multispectral images of the lunar western limb and far side obtained from Galileo reveal the compositional nature of several prominent lunar features and provide new information on lunar evolution.
Buried stratigraphic relationships along the southwestern shores of Oceanus Procellarum: Implications for early lunar volcanism
The composition of mare-highland boundaries is investigated in the region of southwestern Oceanus Procellarum using multispectral images from the Galileo solid-state imaging system. The data are
Lunar volcanism in space and time.
Lunar volcanic deposits are dominated by areally extensive mare units occurring in regionally low areas predominantly on the lunar near side. Data obtained from lunar orbit and earth-based
Geochemical anomalies on the eastern limb and farside of the moon
A variety of orbital geochemistry and photogeologic data was used to investigate major geochemical anomalies on the east limb and farside of the moon and to determine the processes responsible for
Major lunar crustal terranes: Surface expressions and crust‐mantle origins
In light of global remotely sensed data, the igneous crust of the Moon can no longer be viewed as a simple, globally stratified cumulus structure, composed of a flotation upper crust of anorthosite
...
...