Difference between revisions of "Moho/ko"
| Line 2: | Line 2: | ||
{{:Moho/Data}} | {{:Moho/Data}} | ||
| − | + | 모호(Moho)는 Kerbol space program(케르발 스페이스 프로그램)의 가장 안쪽 행성 행성이자 케르발 스페이스 프로그램의 수성입니다. 모호는 대기가 없다는 점과 자연위성이 없다는 점에서 [[Dres/ko|드레스]]와 [[Eeloo/ko|일루]]와 비슷합니다. 0.18업데이트이후로, 더 이상 케르볼에 조석고정되지 않습니다. | |
| − | + | 모호는 약간 이상하게 기울어진 궤도를 가지고, 가기가 힙듭니다. 또한, 대기가 희미한 것([[Aerobraking|에어로브레이킹]] 용)과 달들(중력 조력용)에의해 착륙하기가 어렵습니다. 이러한 요소는 모호에 관한 임무를 도전적이게 만듭니다. | |
== Topography == | == Topography == | ||
| Line 43: | Line 43: | ||
* Mass reduced. | * Mass reduced. | ||
;{{Version|0.17|}} | ;{{Version|0.17|}} | ||
| − | * | + | * 처음 추가됨 |
== Notes == | == Notes == | ||
Revision as of 13:31, 9 June 2013
모호(Moho)는 Kerbol space program(케르발 스페이스 프로그램)의 가장 안쪽 행성 행성이자 케르발 스페이스 프로그램의 수성입니다. 모호는 대기가 없다는 점과 자연위성이 없다는 점에서 드레스와 일루와 비슷합니다. 0.18업데이트이후로, 더 이상 케르볼에 조석고정되지 않습니다.
모호는 약간 이상하게 기울어진 궤도를 가지고, 가기가 힙듭니다. 또한, 대기가 희미한 것(에어로브레이킹 용)과 달들(중력 조력용)에의해 착륙하기가 어렵습니다. 이러한 요소는 모호에 관한 임무를 도전적이게 만듭니다.
Contents
Topography
Moho's surface ranges from light brown highlands to dark brown Maria. It is heavily cratered, but less so than the moons of Kerbin and Jool, suggesting erosion. Because of the lack of an atmosphere on Moho, the primary suspect of Moho's erosion is volcanism. It is probable that Moho undergoes volcanic periods, induced by tidal friction with Kerbol. The fact that this occurs in periods, likely on a geologic timescale, is proven in that volcanism of Moho was removed in 0.18. It must have been discovered just before it stopped being volcanic. The vulcanism would lead to the filling up of craters.
Moho has two very deep wells at the geographic north and south pole of a, as yet, undetermined depth. Current analysis and probes dropped into the crater at the north pole revealed it to be more than 5 km deep before the probe crashed into the ever narrowing canyon walls. It is possible that these are volcanic tubes that are as of this moment dormant. Further analysis of the canyon walls is needed before a definitive answer can be presented.
Orbital Statistics
Mohosynchronous orbit is not possible — it would require an altitude of 0.00 미터, outside of Moho's sphere of influence.
For a semi synchronous orbit of ½ Moho day (307.75 hours or 1,107,882 seconds) an orbit of 0.00 미터 above Moho is needed with a velocity of 0.00 미터/초.
Reference Frames
| 시간 배속 | 최저 고도 |
|---|---|
| 1× | 어디서든지 |
| 5× | 10 000 미터 |
| 10× | 10 000 미터 |
| 50× | 30 000 미터 |
| 100× | 50 000 미터 |
| 1 000× | 100 000 미터 |
| 10 000× | 200 000 미터 |
| 100 000× | 300 000 미터 |
Solar System Counterpart
Moho is the Kerbol System Mercury analog.
- Moho and Mercury share a similar, cratered landscape, similar to most bodies with little to no atmosphere. They are both the closest planet to their respective Sun, and neither has a natural satellite.
- Unlike Mercury, Moho has a brown texture while Mercury itself has a grey to dark grey color. In addition, Mercury has a very tenuous atmosphere, whereas Moho has no atmosphere.
Gallery
A topographic height map of Moho as at Version 0.18.2 made with the ISA MapSat plugin.
A successful landing at Moho pre-0.18. Note the engines still overheating.
A Probe wedged in the 5km deep lava well at the north pole.
A probe performing a Moho flyby.
Changes
- Entirely changed more cratered surface.
- Color changed from red to brown.
- No more superheated atmosphere.
- No longer tidally locked.
- Mass reduced.
- 처음 추가됨
Notes
