Created
November 3, 2016 01:21
-
-
Save code-for-coffee/70d06dc8090d7645e728f5fd786d2774 to your computer and use it in GitHub Desktop.
PlanetTypes.json
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
[{ | |
"name": "Asteroidan", | |
"minMass": 0, | |
"maxMass": 0.00001, | |
"desc": "Asteroidans are small irregular bodies (below the hydrostatic equilibrium) that are not able to hold a stable atmosphere." | |
}, { | |
"name": "Mercurian", | |
"minMass": 0.00011, | |
"maxMass": 0.1, | |
"desc": "Mercurians are only able to hold a significant atmospheres in the cold zones beyond the snow line (i.e. Titan)." | |
}, { | |
"name": "Subterran", | |
"minMass": 0.10001, | |
"maxMass": 0.5, | |
"desc": "Subterrans are able to hold a significant atmospheres after the outer edges of the habitable zone (i.e. Mars)." | |
}, { | |
"name": "Terran", | |
"minMass": 0.50001, | |
"maxMass": 2, | |
"desc": "Terrans are able to hold a significant atmosphere with liquid water within the habitable zone (i.e. Earth)." | |
}, { | |
"name": "Superterran", | |
"minMass": 2.00001, | |
"maxMass": 10, | |
"desc": "Superterrans are able to hold dense atmospheres with liquid water within the habitable zone." | |
}, { | |
"name": "Neptunian", | |
"minMass": 10.00001, | |
"maxMass": 50, | |
"desc": "Neptunians can have dense atmospheres in the hot zone." | |
}, { | |
"name": "Jovian", | |
"minMass": 50.00001, | |
"maxMass": 5000, | |
"desc": "Neptunians can have dense atmospheres in the hot zone." | |
}] |
Sign up for free
to join this conversation on GitHub.
Already have an account?
Sign in to comment