Technische Universität Berlin, Institute of Geodesy and Geoinformation Science
Strasse des 17. Juni 135, 10623 Berlin, Germany
Lunar impact basins are the oldest and most prominent landmarks on the Moon. They are the only remnants of the late heavy bombardment and represent a basis for understanding the early evolution of the terrestrial planets. In order to better constrain the mass, distribution, and timing of the late accretion flux, the morphological features, as well as the gravitational signature of the impact basins will be investigated in detail.
Former studies of the impact basin characteristics, such as ring diameter, center point position, or depth were based on data, which were limited in resolution and accuracy. With the most recent data from current missions, features of each basin can be revised. Using Lunar Orbiter Laser Altimeter (LOLA) data from Lunar Reconnaissance Orbiter (LRO), we will map the topography for each basin candidate. Since older basins are often highly degenerated due to later impacts or erosion, the gravitational signature depicts an important feature for recognizing single basins and their individual characteristics. We will use high-resolution Gravity Recovery and Interior Laboratory (GRAIL) measurements for calculating Bouguer gravity anomalies.
Main objective of our work is the itemization of a full lunar basin inventory with revised characteristics of each candidate. For estimating the certainty of a lunar impact basin, a correlation algorithm will be developed, giving a numerical value for the confidence level, at which a basin is identified. For confirmed basins, we will make new measurements and produce a catalogue involving geographic coordinates, number of rings and their diameters, and depths of the basin floors.
The high-resolution gravity data provided by Gravity Recovery and Interior Laboratory (GRAIL) mission enables detailed modeling of subsurface structures of the Moon. We investigated the coherence between gravity signature (Bouguer anomalies) of lunar impact basins and their relative ages. Since various factors seem to have major influence on the gravity signature no direct correlation to age could be found.
Figure 1: Bouguer anomaly map of the Apollo basin using a crustal density of 2900 kg/m³
Figure 2: Topography map of the Apollo basin; the given altitudes refer to the mean elevation of 1737.1 km
Wahl, D. and J. Oberst, 2019: Lateral variation in bulk density and porosity of the upper Lunar crust from high-resolution gravity and topography data: comparison of different analysis techniques. ISPRS Ann. Photogramm. Remote Sens. Spatial Inf. Sci., IV-2/W5, 527-532. 10.5194/isprs-annals-IV-2-W5-527-2019
Wahl, D. (2019): Lateral variations in bulk density and porosity of the upper lunar crust from high-resolution gravity and topography data: comparison of different analysis techniques. Oral presentation at ISPRS Geospatial Week, Enschede, Netherlands.
Wahl, D. (2019): Bulk Density and Porosity of the upper lunar crust from high-resolution GRAIL and LOLA data. Poster presentation at European Lunar Symposium, Manchester, UK.
Wahl, D. (2017): European Lunar Symposium (ELS), Muenster.
Wahl, D. (2017): European Planetary Science Congress (EPSC), Riga.
Wahl, D. (2017): Paneth Colloquium, Noerdlingen.