Offset input planet mass by volatile mass #269
Labels
interior
Physics - interior evolution
JOSS publication: PROTEUS
TBD before PROTEUS JOSS publication
Priority 1: critical
Priority level 1: highest priority – critical & fast
software
Relating to software and implementation
With #262, the user can specify a dry mantle mass as an input parameter, from which a mantle radius is calculated. It would be useful if, instead/alternatively, the user could specify the total planet mass.
This would mean subtracting-off the volatile inventory from the total input planet mass, and using the result (the dry interior mass) to solve for R_int as per the current formulation.
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