VOILA on LUVMI-X: Volatiles Detection in the Lunar Polar Region with Laser-Induced Breakdown Spectroscopy

Kurzfassung

With the confirmation of water ice in the lunar polar regions, the Moon has recently come into the focus of attention of international space agencies again. Volatiles, specifically water and hydrogen, are important resources both for life support and for potential applications as fuels and propellants for spacecraft. In-situ resource utilization (ISRU) of volatiles could significantly reduce the costs of a sustained presence on the Moon and could be beneficial for the future human deep space exploration of the solar system. The detection of volatiles is therefore an important scientific goal for future robotic missions to the Moon. The LUVMI-X project (Lunar Volatiles Mobile Instrumentation Extended) is developing an initial system design as well as payload and mobility breadboards for the detection of volatiles in the lunar polar region on a small, lightweight rover. The LUVMI-X rover is shown in Figure 1. One proposed scientific payload is VOILA (Volatiles Identification by Laser Ablation), which is jointly developed by OHB System AG (OHB), Laser Zentrum Hannover (LZH), and the German Aerospace Centers Institute of Optical Sensor Systems (DLR-OS). VOILA will use laser-induced breakdown spectroscopy (LIBS) to analyze the elemental composition of the lunar surface, with a special focus on detecting and quantifying hydrogen and oxygen as indicators for water. LIBS is a versatile technique that requires only optical access to its target [4]. A LIBS spectrum is obtained within seconds, making it well-suited for quick analyses of multiple targets in proximity to the rover. LIBS was first used in space by the ChemCam instrument on board NASAs Curiosity rover on Mars. The first LIBS instrument on the Moon was supposed to operate on board the Pragyan rover of Indias Chandrayaan-2 mission. However, the Chandrayaan-2 lander failed a soft landing in September 2019. Here, we present a summary of the VOILA instrument design and its intended capabilities for volatiles detection at the lunar south pole.