Computation of a water-rich planetary body structure profile using SeaFreeze thermodynamics.
- Baptiste Journaux - University of Washington, Earth and Space Sciences Department, Seattle, WA, USA
- Ula Jones - University of Washington, Earth and Space Sciences Department, Seattle, WA, USA
- Karlee Tailor - Macalester College, Saint Paul, MN, USA
- Wei Dai - University of Washington, Earth and Space Sciences Department, Seattle, WA, USA
- Rory Barnes - University of Washington, Earth and Space Sciences Department, Seattle, WA, USA
This project is licensed under the MIT License :
Copyright (c) 2020, B. Journaux
Permission is hereby granted, free of charge, to any person obtaining a copy of this software and associated documentation files, to deal in the Software without restriction, including without limitation the rights to use, copy, modify, merge, publish, distribute, sublicense, and/or sell copies of the Software, and to permit persons to whom the Software is furnished to do so, subject to the following conditions:
The above copyright notice and this permission notice shall be included in all copies or substantial portions of the Software.
THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY, FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM, OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE SOFTWARE.
This work was produced with the financial support provided by the NASA Postdoctoral Program fellowship, by the NASA Solar System Workings Grant 80NSSC17K0775 and by the Icy Worlds node of NASA's Astrobiology Institute (08-NAI5-0021).