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Science 9 November 2001:
Vol. 294. no. 5545, pp. 1326 - 1328
DOI: 10.1126/science.1062492


Abstract
Full Text
Thickness of a Europan Ice Shell from Impact Crater Simulations
E. P. Turtle and E. Pierazzo

Supplementary Material

Water-ice is characterized by an unusual and complicated phase diagram because the solid is less dense than the liquid. The slope of the solid-liquid phase boundary changes from negative for P name 2 kbar to positive for P name 2 kbar. Such an abrupt change in slope cannot be handled by ANEOS and must be avoided. This was accomplished by artificially interpolating the phase boundary above 2 kbar down to zero-pressure, effectively extending the liquid field to lower temperatures than in reality, with a freezing point of 235.6 K. However, this change involves a very small region of the pressure range involved in an impact event, and does not significantly affect the final determination of the equation of state of water.

Experimental shock data show that the solid-solid phase transitions do not seem to influence the Hugoniot of solid ice. However, these experiments also show that the Hugoniot curve of ice lies slightly below that of liquid water, which suggests that ice undergoes a solid-solid phase transition to a denser phase, most probably ice VI (1, 2). The consequence is an increase of the amount of irreversible work done by the shock wave, which increases the post-shock temperature of the ice. This behavior is similar to the case of a porous material (3) and results in lower shock melting and vaporization pressures. Unfortunately, the current version of ANEOS does not simultaneously handle solid-solid and solid-liquid phase transitions. Because in impact events the solid-liquid and solid-vapor transitions are most important for water, we chose ANEOS to represent the melt curve, ignoring the details of solid-solid transitions. Our reference model ice, therefore, has only one solid phase with density of 1.1 g/cm3, within the density range for the various phases of ice.

Experimental data exist for both liquid water and ice shocked to high pressures and temperatures (4-7). Most experimental studies use ice I between 258 K and 263 K, or liquid water at 298 K. Recently, some work has been carried out for porous ice at much lower temperatures (2), but it is limited to very low shock states (<1 GPa). We adjusted the ANEOS input parameters (Web table 1) to best fit the phase boundary curves for both the solid-liquid and liquid-vapor transitions, and to obtain a Hugoniot curve that fits the experimental data. The only differences between the ANEOS equations of state for ice and liquid water are in the coefficients for the linear relation between shock and particle velocity. Different Hugoniot curves can be obtained for the same material by varying its starting density and temperature. To compare with the experimental data, we determined separate Hugoniot curves for ice (starting density of 0.915 g/cm3, T = 258 K) and water (starting density of 0.998 g/cm3, T = 298 K).

The main disadvantage of the current version of ANEOS is its inability to correctly represent gas phases because it cannot treat the vapor phase as a molecular gas. This results in a much higher critical point and a misrepresentation of the vapor side of the liquid-vapor phase boundary. While this effect could influence the final phases of a hydrocode simulation by changing the behavior of water/ice during the expansion of the vapor plume, it does not affect the material's shock state, which is the focus of our study.

The melt regions are constructed by determining the distance from the impact point at which the shock pressures corresponding to the incipient and complete melting entropies for water were achieved. Given the overextension of the liquid region in the EoS, the ice ANEOS underestimates the melting pressures in the region where the ice is warmer. To account for this, we assume that the threshold shock pressure for complete melting of the warm ice (T>240 K) is 1 GPa.


Supplemental Table 1. ANEOS EoS parameters for ice, values for liquid water in parentheses when different from ice.
ParameterIce
(Water)
Description
Nel2Number of elements in the compound
EoS4Type of EoS (solid/gas with electronic terms and detailed treatment of liquid/vapor region)
name01.1Reference density (g/cm3)
T0233.15Reference temperature (K)
P00Reference pressure (GPa)
C1.6 (1.8)Coefficient of shock-material velocity linear relation (km/s)
name00.3Reference Grüneisen coefficient
name0522.24Reference Debye temperature (K)
S0.5 (1.3)Slope of shock-material velocity linear relation
3name023x limit of name for large compressions
Esep6250Zero-temperature separation energy (J/g)
Tm235.6Melting temperature (K)
c530Parameter for low-density modification of critical point (not used)
c540Same as above
H00Thermal conduction parameter (not included)
c410Same as above
namemin0Lowest allowed solid density (g/cm3)
D10name1: start of solid-solid phase transition (g/cm3)
D20name2: end of solid-solid phase transition (g/cm3)
D30Pressure at center of phase transition at zero-T (GPa)
D40dp/dname at high-P phase transition
D50d2p/dname2 at high-P phase transition
Hfus230Heat of fusion for melting (J/g)
nameliq/names1Liquid/solid density at melting point
Up0Upper limit for cold compression (expanded states)
L00Lower limit for cold compression (expanded states)
name0.5Parameter for liquid EoS correction to match Pvap data and boiling point
name0.95Same as above
name0.99Same as above
c600.4Interpolation parameter in name model
c610Same as above
c620.3Interpolation parameter in free energy expression
Flag1Ionization model flag (1 = Thomas Fermi)
Esh0Energy shift for reactive chemistry model (0 = not included)
Ssh0Entropy shift for reactive chemistry model (0 = not included)


Supplemental Figure 1. Galileo images of Europa's multiple ring impact structures Callanish (A) and Tyre (B). Both images have a resolution of 250 m/pixel and are shown such that the illumination is from the right. The images are (A) ~140 km and (B) ~180 km across.


Medium version | Full size version


Supplemental Figure 2. Galileo image of the crater Manannán. Despite its diameter of 21.8 km, Manannán does not have a well-defined central peak. The image resolution is 250 m/pixel and the illumination is from the right.


Medium version | Full size version


References

1. E. S. Gaffney, T. J. Ahrens, Geophys. Res. Lett. 7, 407 (1980).

2. S. T. Stewart, thesis, California Institute of Technology (2001).

3. H. J. Melosh, Impact Cratering: A Geologic Process (Oxford, New York, 1989).

4. A. C. Mitchell, W. J. Nellis, J. Chem. Phys. 76, 6282 (1982).

5. J. M. Walsh, M. H. Rice, J. Chem. Phys. 26, 815 (1957).

6. A. A. Bakanova, V. N. Zubarev, Yu. N. Sutulov, R. F. Trunin, Sov. Phys.-JETP 41, 544 (1975).

7. G. D. Anderson, US Army Cold Reg. Res. & Eng. Lab Res. Rept. RR-257 (Hanover, NH, 1968).





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