P054-0019
Missions to Difficult Lunar Terrains with “Mote” Ballistic Penetrators
Abstract:
Ballistic penetrators allow for the rapid initial scientific investigation of difficult to reach terrain such as the polar Permanently Shadowed Regions (PSRs), lava tube pits and skylights, or volcanic vents, or geographically spread areas of interest such as the lunar swirl regions. The planned CLPS landing in the Schrödinger Basin impact melt expected in Q2 2024 shows the potential for enhancing lunar research with ballistic penetrators. The impact melt is in the Southern edge of Schrödinger crater, roughly 60 km from the PSR in Nefed'ev Crater and ~100 km from the apparent volcanic vent forming the Schrödinger-G pit. A Mote deployment in Nefed’ev crater would provide geological and compositional data on the icy subsurface material deep in the PSR, while a deployment within or on the rim of the Schrödinger-G pit would provide similar data on the pyroclastic material in the vent. In either case the Motes would confirm the ability of the terrain to bear a lander or rover and would provide a initial scientific analysis of the type of icy or volcanic material present in the explored region as a precursor to any subsequent scientific exploration by rovers or astronauts.