Planetary Science

Table 3 Pressure/temperature decay parameters for palagonite runs

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

*Run*	P _START *(mtorr)*	T _SURF* *(K)*	P _END *(mtorr)*	T _SURF* *(K)*
0**	11	216	0.53	195
7	2.5	205	0.21	189
8A	2.7	206	0.060	182
8B	3.0	207	0.18	189
9	3.5	207	0.049	181
10	2.9	206	0.040	180
11	4.8	210	0.034	179
12	6.6	212	0.043	181

*Based on Starting/Ending Pressure (Saturation Assumed) may not be representative of the actual temperature
**Slowly frozen ice from [20]

Back to article page