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Volatility of Sodium in Carbonaceous Chondrites at Temperatures Consistent with Low-perihelion Asteroids

  • Authors: Joseph R. Masiero, Björn J.R. Davidsson, Yang Liu, Kelsey Moore, and Michael Tuite

2021 The Planetary Science Journal 2 165.

  • Provider: AAS Journals

Caption: Figure 1.

Left: surface temperature at three specific latitudes as a function of time from aphelion to perihelion. The vertical extension of data point clusters illustrates the range of day–night temperature variations. One rotation period every second week is plotted for clarity. Right: temperature as a function of depth for a handful of rotational phases, valid at perihelion for latitude 9° S. Note that this particular revolution is not plotted in the left figure.

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