Difference between revisions of "Ross Planetoid"
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{{Planet Infobox | {{Planet Infobox | ||
| name = Ross Planetoid | | name = Ross Planetoid | ||
| − | | image = Ross.jpg | + | | image = Ross Planetoid.jpg |
| owner = | | owner = | ||
| system = [[Cambridge]] | | system = [[Cambridge]] | ||
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Smaller than some asteroids, the Ross Planetoid exists at a gravitational sink where ice fragments have collected over the millennia and begun to compact under their own weight into the seed of what might eventually become a planet. Ross presents a unique opportunity for the [[Cambridge Research Institute]] to study planetary formation and extend their terraforming technology. | Smaller than some asteroids, the Ross Planetoid exists at a gravitational sink where ice fragments have collected over the millennia and begun to compact under their own weight into the seed of what might eventually become a planet. Ross presents a unique opportunity for the [[Cambridge Research Institute]] to study planetary formation and extend their terraforming technology. | ||
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| + | [[Category: Bretonia]] | ||
Revision as of 21:02, 4 December 2018
| Ross Planetoid | |
 | |
| Location | 5F, Cambridge Bretonia
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| Technical information | |
| Docking | No |
| Terrain | N/A |
| Diameter | 200 km |
| Mass | 0.66 x 10e20 kg |
| Temperature | N/A |
| Escape velocity | N/A |
Smaller than some asteroids, the Ross Planetoid exists at a gravitational sink where ice fragments have collected over the millennia and begun to compact under their own weight into the seed of what might eventually become a planet. Ross presents a unique opportunity for the Cambridge Research Institute to study planetary formation and extend their terraforming technology.
