2021
DOI: 10.1130/abs/2021am-369817
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Improved Rock Abundance and Lunar Nighttime Temperature Maps From Diviner

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“…Mass wasting could cause rocks from the wall to roll onto the units in the depression (see e.g., Elder et al., 2017, Figure 3), and, as mentioned previously, a greater abundance of small rocks can result in a lower H‐parameter. It is also likely that radiative heating from the warmer surrounding rocky pit walls results in the pit floor units staying warmer throughout the night, as is shown to occur at the floors of impact craters and at rilles (Bandfield et al., 2011; Powell et al., 2022). While this would not affect the ability to constrain RA using anisothermality (Bandfield et al., 2011), it could yield elevated regolith temperatures.…”
Section: Discussionmentioning
confidence: 99%
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“…Mass wasting could cause rocks from the wall to roll onto the units in the depression (see e.g., Elder et al., 2017, Figure 3), and, as mentioned previously, a greater abundance of small rocks can result in a lower H‐parameter. It is also likely that radiative heating from the warmer surrounding rocky pit walls results in the pit floor units staying warmer throughout the night, as is shown to occur at the floors of impact craters and at rilles (Bandfield et al., 2011; Powell et al., 2022). While this would not affect the ability to constrain RA using anisothermality (Bandfield et al., 2011), it could yield elevated regolith temperatures.…”
Section: Discussionmentioning
confidence: 99%
“…This means that the depression walls take up a larger portion of the local FOV and therefore contribute a larger amount of additional radiation to the IMP units on the floor of Sosigenes. Future thermal modeling efforts (e.g., Powell et al., 2022) could better constrain the thermophysical properties of IMPs on the floors of depressions by calculating the radiative heating from surrounding walls using a high‐resolution digital terrain model.…”
Section: Discussionmentioning
confidence: 99%
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