dishoom

Desorbing Interiors via Satellite Heating to Observe Outgassing Model (DISHOOM) is a planetary evolution software designed for rocky and icy planetary bodies.

The code estimates several known atmospheric escape mechanisms (dM/dt_plasma, dM/dt_energy-limited, dM/dt_surface-jeans, dM/dt_thermal-outgassing benchmarked to DSMC simulations and observations at Jupiter's moon Io. This is for direct application on any [exo]planet system where evaporation is occurring. ☄️☄️☄️☄️☄️

Models are also available to calculate diurnal atmospheric evolution for either: (a) a tidally-locked satellite (e.g. Europa , Ganymede) or (b) an asynchronously rotating planet. ^^Outputs include N [column density] versus phi [longitude] / t [time]

Premade modules are available for the following solar system objects / exoplanetary systems and are available upon request:

Solar system objects:

• Io
• Europa
• Ganymede
• Triton
• Titan
• KBOs (Pluto, Charon, Makemake, Quaoar, Eris, Sedna, 2007 OR 10)
• Halley's comet
• Comet 67 P C/G
• Luna/Chandra/Moon

Exoplanetary systems

• 55 Cancri-e
• WASP 49-b
• HD 189733b
• WASP 69-b
• HD 209458b
• WASP 121-b
• WASP 76-b
• WASP 80-b
• KELT 20-b
• WASP 19-b
• WASP 96-b

For radiative transfer coupling and computation of transmission spectra, please see:

https://github.com/andreagebek/prometheus