Difference between revisions of "Stellatio (world)"
Jump to navigation
Jump to search
Garnfellow (talk | contribs) |
|||
| Line 3: | Line 3: | ||
|uc=D5A4420-8|popc=2 | |uc=D5A4420-8|popc=2 | ||
|ur=D5A4420-8|popr=7 | |ur=D5A4420-8|popr=7 | ||
| + | |zonec = green | ||
| + | |ui= | ||
| + | |u0= | ||
| + | |u1= | ||
| + | |alg = | ||
| + | |class = | ||
| + | |trade = | ||
| + | |nblty = | ||
| + | |bases = | ||
|primary=M3 V | |primary=M3 V | ||
|GGcount=0 | |GGcount=0 | ||
Revision as of 13:07, 18 August 2015
| Stellatio/Vilis (Spinward Marches 1216) | |||||||||||||||||||||||||
| Classic Era (1116) | D5A4420-8
| ||||||||||||||||||||||||
| New Era (1200) | D5A4420-8
| ||||||||||||||||||||||||
| See also | UWP | ||||||||||||||||||||||||
| System Details | |||||||||||||||||||||||||
| Primary | M3 V | ||||||||||||||||||||||||
| Planetoid Belts | 1 | ||||||||||||||||||||||||
| Gas Giants | 0 | ||||||||||||||||||||||||
style="width: 220px; height: 250px;"
Jump map from Travellermap.com [1]
Stellatio is a non-industrial Imperial world with fluid oceans, located in the Vilis Subsector of the Spinward Marches. With a total population of 50,000, most people live in Stellas, an underground city near the starport. Twenty or so smaller settlements, with dozens or hundreds of people, dot the region, along with several failed settlements, but none are more than a hundred miles from Stellas.
IISS GURPS Astrographics Survey
1216 Stellatio (Imperial)
Starport: Class II.
Diameter: 4,655 miles (7,400 km).
Atmosphere: Exotic (nitrogen-carbon dioxide mix).
Hydrographics: 37%.
Climate: Tropical.
Population: 50,000.
Government: Athenian-style democracy.
Control Level: 0.
Tech Level: 5.
World Trade Number: 2.
This list of sources was used by the Traveller Wiki Editorial Team and individual contributors to compose this article. Copyrighted material is used under license from Mongoose Publishing or by permission of the author. The page history lists all of the contributions.
- ↑ "Jump Map API" and map location from Travellermap.com
|
This article was published in JTAS Online and you need to be a subscriber to see the article. You may view the entire original article here. |
