Lunar sub-surface temperatures

The influence of the insulating properties of lunar regolith was shown in the sub-surface temperature tests performed by the Apollo missions, with no significant temperature fluctuations occurring below 80 cm from the lunar surface even if surface temperatures fluctuated >200 K between lunar days and nights (Heiken et al, 1991). Key to the thermal insulation of the regolith is its low density near the surface having the greatest insulative effect with the lunar regolith becomes denser with depth. As the regolith becomes denser, the thermal conductivity of the regolith increases (Hayne et al, 2017). Thermal modelling software, Oxford 3D Thermal Model, which mapped the lunar surface temperatures effect on the thermal influence at the lunar south pole sub-surface over a lunar year found areas with brief illumination with surface temperatures >120 K could have sub-surface temperatures <112 K that can sustain long-term stable water ice at depths of <30 cm (Paige et al, 1992; King et al, 2020). Further to this, the observation of water molecules or other hydroxyls by the NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA) in non-permanently shadowed regions (PSRs) on the Moon, indicated that water could be present beyond PSRs (Honniball et al, 2021). Using the Oxford 3D Thermal Model in selected regions in the lunar south pole, can provide insights into the location and depth of cold traps that could sustain water ice.