“…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.…”