Difference between revisions of "Main Page"
From Planets
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# Giant planets (Jupiter, Saturn, Uranus, Neptune) | # Giant planets (Jupiter, Saturn, Uranus, Neptune) | ||
* With the Mars Models: | * With the Mars Models: | ||
| − | + | # Present-day Mars climate (with water and dust cycles) | |
| − | + | # Recent-Mars paleoclimates (e.g., Amazonian epoch) | |
| − | + | # Regional and local weathers on Mars | |
* With the Venus models: | * With the Venus models: | ||
| − | + | # Present-day Venus climate | |
| − | + | # Regional weather on Venus | |
* With the Titan models: | * With the Titan models: | ||
| − | + | # Present-day Titan | |
| − | + | # Regional and local weather on Titan | |
* With the Pluto/Triton models: | * With the Pluto/Triton models: | ||
| − | + | # Present-day Pluto/Triton climate | |
| − | + | # Long-term volatile/ice cycling on Pluto and Triton | |
You can use the menu on the left to navigate across our webpages. | You can use the menu on the left to navigate across our webpages. | ||
Revision as of 09:19, 29 March 2023
Welcome to the wiki of the Planetary Climate Models (PCM) family! Our numerical climate models cover a wide range of planets described below.
- With the Generic Models:
- Exoplanets of all kinds (rocky planets, super-Earths, mini-Neptunes, hot Jupiters, etc.)
- Paleoclimates of Solar System planets (e.g., very ancient Mars, Earth, Venus, Titan)
- Giant planets (Jupiter, Saturn, Uranus, Neptune)
- With the Mars Models:
- Present-day Mars climate (with water and dust cycles)
- Recent-Mars paleoclimates (e.g., Amazonian epoch)
- Regional and local weathers on Mars
- With the Venus models:
- Present-day Venus climate
- Regional weather on Venus
- With the Titan models:
- Present-day Titan
- Regional and local weather on Titan
- With the Pluto/Triton models:
- Present-day Pluto/Triton climate
- Long-term volatile/ice cycling on Pluto and Triton
You can use the menu on the left to navigate across our webpages.
