The Lunar Basin Sequence Based on Absolute Model Ages Derived via Buffered Non-Sparseness Correction: Implications for Impactor Population(s)

Csilla Orgel(European Space Research and Technology Centre), H. Hiesinger(University of Münster), Christian Riedel(Freie Universität Berlin), T. Kneissl(Planetary Science Institute), C. I. Fassett(Johns Hopkins University Applied Physics Laboratory), C. H. van der Bogert(University of Münster), G. Michael
LPI
March 1, 2018
Cited by 1

Related Papers

Lunar Reconnaissance Orbiter Camera (LROC) Instrument Overview
|Space Science Reviews|2010|994
Valley network-fed, open-basin lakes on Mars: Distribution and implications for Noachian surface and subsurface hydrology
|Icarus|2008|471
Ages and stratigraphy of mare basalts in Oceanus Procellarum, Mare Nubium, Mare Cognitum, and Mare Insularum
|Journal of Geophysical Research Atmospheres|2003|468
The timing of martian valley network activity: Constraints from buffered crater counting
|Icarus|2008|465
Possible Ancient Oceans on Mars: Evidence from Mars Orbiter Laser Altimeter Data
|Science|1999|415