LUVMI: an innovative payload for the sampling of volatiles at the Lunar poles

The ISECG identifies one of the first exploration steps as in situ investigations of the moon or asteroids. Europe is developing payload concepts for drilling and sample analysis, a contribution to a 250kg rover as well as for sample return. To achieve these missions, ESA depends on international partnerships. Such missions will be seldom, expensive and the drill/sample site selected will be based on observations from orbit not calibrated with ground truth data. Many of the international science community’s objectives can be met at lower cost, or the chances of mission success improved and the quality of the science increased by making use of an innovative, low mass, mobile robotic payload following the LEAG recommendations. LUVMI provides a smart, low mass, innovative, modular mobile payload comprising surface and subsurface sensing with an in-situ sampling technology capable of depth-resolved extraction of volatiles, combined with a volatile analyser (mass spectrometer) capable of identifying the chemical composition of the most important volatiles. This will allow LUVMI to: traverse the lunar surface prospecting for volatiles; sample subsurface up to a depth of 10 cm (with a goal of 20 cm); extract water and other loosely bound volatiles; identify the chemical species extracted; access and sample permanently shadowed regions (PSR). The main innovation of LUVMI is to develop an in situ sampling technology capable of depth-resolved extraction of volatiles, and then to package within this tool, the analyser itself, so as to maximise transfer efficiency and minimise sample handling and its attendant mass requirements and risk of sample alteration. By building on national, EC and ESA funded research and developments, this project will develop to TRL6 instruments that together form a smart modular mobile payload that could be flight ready in 2020. The LUVMI sampling instrument will be tested in a highly representative environment including thermal, vacuum and regolith simulant and the integrated payload demonstrated in a representative environment

Assessing the Distribution of Water Ice and Other Volatiles at the Lunar South Pole with LUVMI-X: A Mission Concept

The search for exploitable deposits of water and other volatiles at the Moon’s poles has intensified considerably in recent years, due to the renewed strong interest in lunar exploration. With the return of humans to the lunar surface on the horizon, the use of locally available resources to support long-term and sustainable exploration programs, encompassing both robotic and crewed elements, has moved into focus of public and private actors alike. Our current knowledge about the distribution and concentration of water and other volatiles in the lunar rocks and regolith is, however, too limited to assess the feasibility and economic viability of resource-extraction efforts. On a more fundamental level, we currently lack sufficiently detailed data to fully understand the origins of lunar water and its migration to the polar regions. In this paper, we present LUVMI-X, a mission concept intended to address the shortage of in situ data on volatiles on the Moon that results from a recently concluded design study. Its central element is a compact rover equipped with complementary instrumentation capable of investigating both the surface and shallow subsurface of illuminated and shadowed areas at the lunar south pole. We describe the rover and instrument design, the mission’s operational concept, and a preliminary landing-site analysis. We also discuss how LUVMI-X fits into the diverse landscape of lunar missions under development

Candidate landing sites and possible traverses at the South Pole of the Moon for the LUVMI-X rover

Lunar volatiles, such as water, are considered to be a crucial resource for In Situ Resource Utilization (ISRU) in using the Moon as an enabling platform for future space exploration. As water is most likely to be found in the form of ice at the lunar poles (temperature of stability in vacuum: 110K), multiple missions target the South Pole cold traps. With challenging conditions (rough topography, low illumination, low temperatures, and limited Earth visibility; and references within), the South Pole comprises numerous PSR (Permanently Shadowed Regions) which are cold enough to capture and retain volatiles such as water ice (annual average temperatures of 40K). Funded by the EU program Horizon 2020, Space Applications Services coordinates the LUVMI-X (LUnar Volatiles Mobile Instrument) project, where the company develops a robotic platform and international partners develop a dedicated payload suite, aimed at sampling and analyzing lunar volatiles in these polar regions. LUVMI-X is a commercial rover with modular interfaces to facilitate the integration of payloads from the community. The goal of this paper is to find suitable landing sites and study areas for this rover, that are both scientifically interesting and technically reachable

LUVMI – Volatile Extraction and Measurements in Lunar Polar Regions

The low inclination of the lunar orbit allows areas in high latitudes to remain in eternal darkness.   These Permanently Shadowed Regions (PSR) are never illuminated by heating sunlight and are some of the coldest places in the Solar System which are thought to contain vast deposits of water and other volatiles.  In‐situ measurements are required as a definite proof of the existence of water and other volatiles in and around a PSR. The LUnar Volatiles Mobile Instrumentation (LUVMI) is an autonomous, low mass, modular rover consisting of surface and subsurface sensing instruments with an in‐situ sampling and analysis technology capable of depth resolved volatile extraction and characterisation.  With a total mass of less than 20 kg LUVMI is intended as an additional mobile payload for a lunar polar lander mission that will add the capability of allowing access to a PSR.  Volatile extraction from the lunar regolith will be carried out by the Volatiles Sampler (VS), which will sample the subsurface up to a depth of 10 cm, extract water and other loosely bound volatiles through heating.  The design of the VS provides efficient volatile sample transfer and minimizes sample handling requirements.  Evolved volatile characterisation will be performed by the Volatiles Analyser (VA) which is a miniature mass spectrometer based on the Ptolemy mass spectrometer instrument on‐board Philae, the ESA Rosetta Lander. We will discuss the LUVMI rover concept, the current concept of operations and the design of the mass spectrometer extraction systems

LUVMI Rover to Characterise Volatile Content in Lunar Polar Regions

The low inclination of the lunar orbit allows areas in high and low latitudes to remain in eternal darkness. These Permanently Shadowed Regions (PSR) are never illuminated by sunlight and are some of the coldest places in the Solar System and could contain vast deposits of water and other volatiles. In-situ measurements are required as a ‘ground-truth’ measurement to determine the existence volatiles in these regions. The LUnar Volatiles Mobile Instrumentation (LUVMI) is an autonomous, low mass, modular rover concept consisting of surface and subsurface sensing instruments with an in-situ sampling and analysis technology capable of depth resolved volatile extraction and characterisation. Volatile extraction from the lunar regolith will be carried out by the Volatiles Sampler (VS), which will sample the subsurface up to a depth of 20 cm, extract water and other loosely bound volatiles through heating. The design of the VS provides efficient volatile sample transfer and minimizes sample handling requirements. Evolved volatile characterisation will be performed by the Volatiles Analyser (VA) which is a miniature ion trap mass spectrometer based on the Ptolemy mass spectrometer instrument on-board Philae, the ESA Rosetta Lander. LUVMI-X (eXtended) will add the capability of allowing direct access to a PSR(s) via a miniature instrumented low velocity projectile that will be launched from the rover platform into areas of interest that are inaccessible to the rover. We will discuss the LUVMI test campaign conducted in December 2018, the current LUVMI-X configuration, the design of the mass spectrometer extraction systems and recent laboratory results obtained with volatile doped regolith simulant

LUVMI: A concept of low footprint lunar volatiles mobile instrumentation

The International Space Exploration Coordination Group (ISECG) identifies one of the first exploration steps as in situ investigations of the Moon or asteroids. Europe is developing payload concepts for drilling and sample analysis, a contribution to a 250kg rover as well as for sample return. To achieve these missions, ESA depends on international partnerships. Such missions will be seldom, expensive and the drill/sample site selected will be based on observations from orbit not calibrated with ground truth data. Many of the international science community’s objectives can be met at lower cost, or the chances of mission success improved and the quality of the science increased by making use of an innovative, low mass, mobile robotic payload following the LEAG recommendations. As a main objective LUVMI is designed specifically for operations at the South Pole of the Moon with a payload accommodated by a novel lightweight mobile platform (rover) with a range of several kilometers. Over the 2 years duration of the project, the scientific instruments payload will be developed and validated up to TRL 6. LUVMI targets being ready for flight in 2020 on an ESA mission partially supported by private funding