|Laythe as seen from orbit.|
|Moon of Jool|
|Semi-major axis||27 184 000 m [Note 1]|
|Apoapsis||27 184 000 m [Note 1]|
|Periapsis||27 184 000 m [Note 1]|
|Orbital inclination||0 °|
|Argument of periapsis||0 °|
|Longitude of the ascending node||0 °|
|Mean anomaly||3.14 rad (at 0s UT)|
|Sidereal orbital period||52 981 s|
|14 h 43 m 0.9 s|
|Synodic orbital period||53007.7 s|
|Orbital Velocity||3223.8 m/s|
|Equatorial radius||500 000 m|
|Surface area||3.1415927×1012 m2|
|Standard gravitational parameter||1.9620000×1012 m3/s2|
|Density||56 145.401 kg/m3|
|Surface gravity||7.85 m/s2 (0.8 g)|
|Escape velocity||2 801.43 m/s|
|Sidereal rotation period||52 980.879 s|
|14 h 43 m 0.9 s|
|Sidereal rotational velocity||59.297 m/s|
|Synchronous orbit||4 686.32 km|
|Sphere of influence||3 723 645.8 m[Note 1]|
|Atmosphere present||✓ Yes|
|Atmospheric Pressure||81.0600 kPa|
|Scale height||4000 m|
|Atmospheric height||55 262.042 m|
|Temperaturemin||-40.19 °C 232.96 K|
|Temperaturemax||6.21 °C 279.36 K|
|Oxygen present||✓ Yes|
Laythe is the first of the five natural satellites of Jool. Although mostly covered in seas, Laythe has numerous rocky, sandy islands. Laythe is tidally locked to Jool. Synchronous orbits around Laythe are not possible, as they would lie outside of its SOI, at a radius of 5,186,399 meters. A circular archipelago that is prominent in maps suggests that Laythe suffered a massive impact in its distant past.
Achieving a stable orbit around Laythe from sea level requires a delta-V of ≈2800 m/s.
Laythe has no real-world analogue. In the real-world Jupiter system, the moons Ganymede, Europa and Io form a group with an orbital resonance just like KSP's Tylo, Vall and Laythe. But while Tylo and Vall have a certain resemblance to their real-life counterparts, Laythe is very unlike the volcanic, atmosphere-less, dry Io. Instead, the presence of a liquid ocean - plus a dense atmosphere - makes Laythe more similar to the Saturnian moon, Titan. Laythe also seems very similar to what happened to Europa in 2010: Odyssey Two.
Though Laythe has liquid water on its surface, the temperature there is below zero degrees centigrade. This means that Laythe's oceans must contain another compound, most likely ionic, such as salt. Surface samples indicate that much salt is present on Laythe's surface. Unlike that of Kerbin, the air cannot be breathed by Kerbals (according to EVA reports). It is therefore possible that there are also high concentrations of salt in the air, as well as on the surface, assuming that the salt is sodium chloride. The apparent toxicity of Laythe's atmosphere (despite being similar in composition to Kerbin's) may also be a reference to the film Avatar - the moon Pandora is very similar to Earth, but its atmosphere is too toxic for humans to inhale, and the moon also orbits a gas giant, like Laythe.
According to former developer NovaSilisko, Laythe was planned to have volcanic, probably cryovolcanic, activity and high radiation levels in later versions, making it a much more hostile moon than in 0.23.
|“|| When Laythe was first discovered, it was not entered in the records because the scientist in charge thought he was looking at Kerbin.
Luckily this error was corrected when a plucky intern informed him that telescopes don’t work that way.
The intern was shortly afterwards promoted and moved to the experimental rocket testing program.
— Kerbal Astronomical Society
Laythe's atmosphere begins at 55,262 meters and is slightly thicker than Kerbin's. It is the only moon in the game which has an atmosphere.
Like all other atmospheres in the game, Laythe's atmosphere fades exponentially with increasing altitude (with a scale height of 4000 m). In general, the atmospheric pressure on Laythe at an altitude expressed in meters is:
With proper aerobraking near Laythe and Jool, reaching Laythe may require the least delta-V of all of Jool's moons. When approaching Jool on a Hohmann transfer orbit from Kerbin, aerobraking with a Jool periapsis of 119.5 km will put your apoapsis roughly near Laythe's orbit.
Another way is to approach Laythe directly, with proper timing and orbit adjustments done on the way to Jool. Laythe's orbital period makes it easy target to time and allows less Δv on arrival (only 2000 m/s), thus aerobraking on Laythe is lighter than on Jool. Diving to ~22 km will almost circularize the (retrograde) orbit.
Landing on higher points of Laythe's surface has to be done with a help of retro burns as parachutes alone are not enough to sufficiently lower velocity for landing.
Jet engines work in Laythe's atmosphere as it contains oxygen. However, their air intake efficiency is lower.
Laythe is mostly ocean. There are many craters on its surface, and some of the largest features it has may be related to impacts. Other features on the surface such as small canyons may have been carved out by flowing water that either came up through the surface, or fell as "rain" when the planet was warmer.
Laythe is the most science-rich body in the Joolean moon system. Even though Tylo has a slightly higher science multiplier for both surface and orbit, Laythe's atmosphere and oceans allow a lot more experiments to be performed which means that the total science output is higher.
|Rotational/Inertial transition||0 m|
|5×||30 000 m|
|10×||30 000 m|
|50×||60 000 m|
|100×||120 000 m|
|1 000×||240 000 m|
|10 000×||480 000 m|
|100 000×||600 000 m|
- Initial Release
- Forumpost from NovaSilisko
- Post from NovaSilisko
- A LV-N Atomic Rocket Motor has a specific impulse of 220 in 1 atm, 800 in vacuum, and the following at various Laythe altitudes:
altitude (m) 600 1464 1800 2238 2698 3296 4104 16435 specific impulse 400.7 478.2 504.2 534.8 563.7 596.5 633.7 792.4