Lecture Notes (PDF) - Aqueous and Environmental Geochemistry

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Solar System Differentiation by Volatility10000The “Frost Line”V E M A J S U N PTemperature (K)100010010Watercondenses at170 K10.5 1 10 50Radial Distance (AU)9

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Volatile vs. Refractory Elements..Highly Refractory: Al, Ca, Ti (e.g., Al 2 O 3 )Moderately Refractory: Mg, Fe, Si (e.g., Mg 2 SiO 4 )Moderately Volatile: Na, K, S (e.g., (Na,K)AlSi 3 O 8 )Highly Volatile: H, C, N (H 2 O, CH 4 etc.)The Solar SystemGas GiantsGas GiantsTerrestrial Planets8

Solar System Differentiation by Volatility10000The “Frost Line”V E M A J S U N PTemperature (K)100010010Watercondenses at170 K10.5 1 10 50Radial Distance (AU)9

Page 1 and 2: Formation of the SolarSystemGeochem
Page 3 and 4: Nebular HypothesisCondensation of s
Page 6 and 7: Condensation of Elements…Since th
Page 10 and 11: CometsVolatile (ice) rich leftovers
Page 13: Carbonaceous ChondritesMost primiti

Lecture Notes (PDF) - Aqueous and Environmental Geochemistry

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