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Table of Contents
A comparison of ice VII formed in the H2O, NaCl–H2O, and CH3OH–H2O systems: Implications for H2O-rich planets
1 Introduction
1.1 Impurities in high-pressure ice
1.2 The ice VII-ice X phase transition
2 Experimental and analytical methods
2.1 Solutions
2.2 Symmetric diamond anvil cell
2.3 Powder X-ray diffraction
3 Results
3.1 Powder X-ray diffraction
3.2 Isothermal compression at 298K
4 Discussion
4.1 Isothermal compression of H2O ice VII
4.2 Isothermal compression of ice VII formed with NaCl
4.3 Isothermal compression of ice VII formed with CH3OH
4.4 The ice VII to ice X transition
4.5 Structural controls on impurities in ice VII
4.6 Planetary implications: H2O-rich planets
5 Conclusion
Acknowledgements
References