Figure 2
From: The best temperature range to acquire reliable thermal infrared spectra from orbit
Surface temperature ranges of several Solar System bodies. The light cyan window encloses the values of volume expansion discussed in this work; orange bars show surface temperature range of several Solar System bodies that match the range discussed in this work; black circles indicate the evolution of volume as a function of temperature for olivine Mg1.84Fe0.16SiO4 here investigated.
