 | ||
| 天王星 : 太阳VII | ||
|---|---|---|
| 所属星系 | 太阳系 | |
| 类型 | 行星 | |
| 分类 | 冰巨行星 | |
| 是否宜居 | 否 | |
| 归属 | 地球联合帝国 | |
| 位置 | UEE星域 └ 太阳系 └─ 围绕太阳的轨道上 | |
| 自然卫星 | 5 | |
| 赤道半径 | 25,559 千米 (现实中) 2,555.9 千米 (游戏内尺寸) | |
| 重力 | 0.886G | |
| 自传周期 | 17.23992 小时 | |
| 轴倾角 | 97.77° | |
| 密度 | 1.27 g/cm³ | |
| 潮汐锁定 | No | |
| 公转周期 | 30,688.5 天 | |
| 公转速度 | 6.80 km/s | |
| 轨道半径 | 19.2184 AU (现实中) 1.92184 AU (游戏内尺寸) | |
| 轨道偏心率 | 0.046381 | |
| 远日点 | 20.11 AU (现实中) 2.011 AU (游戏内尺寸) | |
| 近日点 | 18.33 AU (现实中) 1.833 AU (游戏内尺寸) | |
| 轨道倾角 | 1.02° | |
| 在方舟星图中查看 | ||
天王星 (太阳VII)是一颗位于太阳系的冰巨行星，它的自转轴极度倾斜，使其南北两极位于大多数其他行星的赤道位置上，因而具有不寻常的侧边倒的磁场。[1]
大气成分
天王星的大气层主要由氢气和一些氦气组成。
| 化学式 | 全名 | 含量 |
|---|---|---|
| H2 | 氢气 | 83% |
| He | 氦气 | 15% |
| CH4 | 甲烷 | 2.3% |
| HD | 氟化氢 | 0.009% |
| H2S | 硫化氢 | Trace |
| NH3 | 氨气 | Ice Crystals |
| H2O | 水 | Ice Crystals |
| NH4SH | 硫氢化铵 | Ice Crystals |
| 4CH4·23H2O | 甲烷水合物 | Ice Crystals |
天然卫星
天卫五
Miranda is one of the smallest objects in the Sol System known to be in hydrostatic equilibrium. Its extreme and varied topography includes the Verona Rupes, which features the tallest cliff in the system.
天卫一
The surface of this moon is crisscrossed by an extensive network of scarps, canyons and ridges. Scientists speculate some of these canyons were carved out by liquid ammonia, methane or carbon monoxide.
天卫二
This moon's name has its roots in the Latin word "umbra", which means shadow. An appropriate reference considering Umbriel is the darkest of all Uranian moons.
天卫三
Titania is Uranus' largest moon. Enormous canyons and scarps cut through its surface. Scientists believe they were created after an interior expansion occurred during the moon's evolution.
天卫四
Uranus' second largest moon was named after a mythical faery king from a famous 16th century play. Its surface is covered in impact craters and appears red in color due to space weathering.
另可见
引用
- ↑
| 在Sol中的太空地点 |
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