UK-NLSI Node Capabilities and Research Interests

As SSERVI’s first European partner, the UK-Node is comprised of 15 institutions and is based out of the Open University. Their research focuses on the following main topics:

• Lunar volcanism, magma ocean evolution and structure of the lunar crust
• Lunar crustal composition using X-ray fluorescence spectroscopy from orbit
• Petrology and geochemistry of lunar samples returned by Apollo and Luna missions and lunar meteorites.
• Radiometric age dating of lunar samples using a variety of analytical techniques.
• Application of traditional and non-traditional stable isotopic techniques to study lunar samples for understanding the origin and evolution of the Moon.
• Digital elevation modelling, lunar topography and cartography.
• Lunar astrobiology, including studies of the survivability of terrestrial materials on the Moon.
• Development of instrumentation for lunar orbiters and landers (e.g. X-ray spectrometers UV/Vis/NIR spectrometers, seismometers, penetrometers, Gas Analysis Package (GAP) etc)
• Development of lunar regolith drilling, sample acquisition and processing systems
• Space and Planetary Robotics
• Whole Earth imaging from the Moon for comparison with exoplanets.
• Exoplanetary Auroral Kilometric Radiation
• Development of in situ detection and analysis of polar volatiles
• Lunar in-situ resource utilization (ISRU) studies and applications
• Surface heat flow and thermal properties, lunar magnetism
• Lunar dust and impact physics
• Exploration architecture studies
• Space weathering studies of the Moon and other airless bodies
• Optical interferometry
• Development of curation faculties for returned samples.

For more information, contact:
Mahesh Anand
Open University

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SSERVI Science Teams

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    The farside of the Moon has always been a mystery and is only accessible by spacecraft. New compositional information from the Moon Mineralogy Mapper (M3) onboard Chandrayaan‐1 has identified a suite of highly unusual rock types exposed at small areas within the farside Moscoviense Basin. M3 is a state‐of‐the art visible and near‐infrared imaging spectrometer that was a guest instrument on Chandrayaan‐1, the Indian Space Research Organization’s (ISRO) first mission to the Moon. The instrument is designed to measure accurately the diagnostic mineral absorption bands of solar radiation reflected from the lunar surface.

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