Skip to main content
Planetary Science
Figure 3 | Planetary Science

Figure 3

From: Experimental and theoretical simulation of sublimating dusty water ice with implications for D/H ratios of water ice on Comets and Mars

Figure 3

Evolution of the pressure at the 20mtorr manometer and the temperature sensor near the sample surface for the run described in Figure 4, panel E. The time of first illumination by the lamp is given by a vertical grey bar. Note the large decrease in pressure observed over the course of the run compared to a lack of an appreciable temperature change.

Back to article page