Examples
A collection of example input files and scripts using VPLanet that
showcase the various applications of the code. The source files for
the examples below live in the examples folder in the top-level
directory of the VPLanet repository.
View them on GitHub.
- STEEP: Coupled Stellar-Tidal Evolution of Binary Orbits
- Proxima Centauri b as a “Habitable Evaporated Core.”
- Sinusoidal Evolution of Luminosity
- Luminosity evolution for stars with mass between 0.2 and 0.6 Msun.
- Stellar Magnetic Braking
- Thermal and Magnetic Evolution of Earth’s Interior
- Earth’s Seasonal and Milankovitch Climate Cycles
- Thermal and Magnetic Evolution of Venus
- Atmospheric Erosion of H Envelopes in the Energy-, Radiation/Recombination-, and Bondi-limited Regimes
- Kepler-36 Atmospheric Escape
- Orbital Evolution of the Circumbinary Planet Kepler-16 b
- N-body Orbital Evolution of the Solar System
- Apsidal Locking of the CoRoT-7 System
- Water Loss on a Tidally Evolving Planet
- Magma ocean evolution on GJ 1132 b
- Parameter Sweep Example
- (Pre-)Main Sequence Stellar Evolution
- Accumulation of Atmospheric Oxygen due to Water Photolysis and Hydrogen Escape.
- Atmospheric Erosion of Mini-Neptunes with the Lehmer & Catling (2017) Model
- Radiogenic Heating of Earth
- The Habitable Zone
- Multiple Cassini States in One System
- Solar System Orbital Dynamics from Secular Theory
- Evolution of a Planet Orbiting a Short-Period Binary
- Tidal Locking of the Planet Candidate Gl 581 d
- Chaotic Eccentricity-Inclination Resonances
- Ice Belt Formation on High Obliquity Planets
- Hydrogen Envelope Loss on Tidally Evolving Planets
- Magma Ocean Evolution of Earth
- Evolution of Tight Stellar Binaries
- Proxima Centauri b Atmospheric Escape
- Flare frequency distribution of Proxima Centauri
- Evolution of a Wide Stellar Binary due to Galactic Effects
- The “Cosmic Shoreline”
- Water Loss on Venus
- Tidal Evolution of Earth-like Exoplanet
- Coupling Atmospheric Escape and N-Body Evolution: Application to PSR1257+12
- Accumulation of Atmospheric Oxygen due to Water Photolysis and Hydrogen Escape on the TRAPPIST-1 planets b and e with the LS16 Water loss model
- Cassini States
- Magma ocean evolution of Trappist-1 g
- Tidal Heating of Io
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Currently broken examples in need of your help!