More actions
(Initial import of old Duna page, thanks Space Peacock) |
(big cleanup and broad formatting) Tag: 2017 source edit |
||
| Line 1: | Line 1: | ||
Duna is a small dry planet and the fourth planet in the Kerbol system Kerbolar system and functions as the mars analog. its orbital eccentricity and inclination are similar to Kerbin Kerbin's making it a relatively easy destination for interplanetary ships to reach from Kerbin. it features a thin atmosphere and a relatively massive moons moon Ike . | |||
== Synopsis == | |||
''Duna the reddest planet has long been an object of study and inspiration to kerbal scientists and artists alike its thin low-pressure atmosphere allows for both aerobraking and relatively easy access to its surface. kerbal researches and sci-fi writers often discuss the discoveries that could be waiting for them in the planet planet\'s polar ice caps or on Duna's tidally locked moon Ike.'' | |||
== Surface == | |||
Duna has a desert-like reddish colored surface composed primarily of silicate rocks and sands covered by a fine layer of dust up to a few millimeters thick. This dust layer is theorized to be the result of dust storms. Dunian soil contains nutrients such as sodium potassium chloride and magnesium. The planet exhibits no tectonic activity and is believed to be geologically dead. Evidence of past tectonic activity is present however with volcanic basalt being quite common in certain regions. Surface features and exposed rocks show heavy signs of erosion by wind as well as flowing water. This combined with a the surprising amount salt in the ground indicates that Duna's surface may once have held liquid water. Duna's surface topography is mostly flat with occasional mountains and dunes. Various wikipedia impact_crater impact craters are spread out over its surface area. The majority of these are simple bowl-shaped craters with sparse wikipedia complex_crater#central-peak_craters center peak and wikipedia peak_ring peak ring formations. These craters are often eroded by the elements and overall less pronounced than those on atmosphere-less celestial bodies. For an unknown reason the northern hemisphere has significantly more impact craters. This may be explained by the impact of a comet that shattered before reaching the surface. | |||
== Polar ice caps == | |||
The most northernmost and southernmost parts of Duna's surface are covered by polar ice caps. These ice caps start at roughly 65 and -70 latitude respectively. They are estimated to be about 5 kilometers thick at their deepest point and composed of water ice and snow with a thin top layer of frozen carbon dioxide and trace amounts of dust. The northern ice cap has a deep spiraling pattern of troughs. These troughs are caused by roughly perpendicular wikipedia katabatic_wind katabatic winds that spiral due to the wikipedia coriolis_force coriolis effect. | |||
== Atmosphere == | |||
Duna has a thin cool atmosphere with a depth of 50 000 meters. Compared to the atmosphere of Kerbin, Duna's atmosphere has 1/15th the mass 1/15th the surface pressure and 1/9th the surface density. Duna's atmosphere is predominantly composed of carbon dioxide with a small fraction of nitrogen and argon as well as traces of oxygen, carbon monoxide, water, methane, and other gases. Melting of snow in the polar regions due to seasonal temperature variations is believed to be responsible for Duna's thin wispy clouds. These clouds are then carried toward the equator by a polar wikipedia jet_stream jet stream. | |||
=== Atmospheric flight === | |||
The thickness of Duna's atmosphere makes it suitable for aerocapture from a high-speed interplanetary intercept. Although parachutes will deploy on Duna the atmosphere is so thin that they are usually unable to slow a craft to a safe landing velocity and must be assisted with engines. Parachute performance can be particularly troubling when attempting to land in the highland areas. Below 5,000 meters Duna's atmosphere is thick enough to allow wings to generate enough lift for aerodynamic flight. Jet engines will not work on Duna due to a lack of oxygen in the atmosphere but other propulsion methods work well. Performing a horizontal landing with a plane is also possible. | |||
== Magnetosphere == | |||
Duna has a weak magnetic field that's about 2 the strength of Kerbin's. There is evidence that Duna once had a much more powerful magnetic field but it weakened overtime as its core cooled. | |||
== Science regions == | |||
Duna has 6 surface regions which makes it one of the most region-rich bodies second only to Kerbin and Laythe. It is an ideal place for science collection for players who are embarking on their first interplanetary journey. | |||
=== Orbital situations === | |||
class \"fandom-table\" science region altitude ranges science multiplier - high orbit 70 000 m - 47 921 949.369738 m 16.0 - low orbit 50 000 m - 70 000 m 24.0 - atmosphere 0 - 50 000 m 8.0 | |||
=== Surface regions === | |||
class \"fandom-table\" science region science multiplier - highlands 20.0 - midlands 20.0 - lowlands 20.0 - polar deserts 20.0 - north pole 20.0 - south pole 20.0 | |||
== Discoverables == | |||
Duna face it there there's nothing here yet | |||
== Version history == | |||
v0.2.0.0 | |||
<nowiki>*</nowiki> added science regions. | |||
v0.1.5.0 | |||
<nowiki>*</nowiki> updated atmospheric scattering. | |||
v0.1.2.0 | |||
<nowiki>*</nowiki> celestial body ground scatter updates. | |||
<nowiki>*</nowiki> height fog added. | |||
v0.1.0.0 | |||
<nowiki>*</nowiki> initial release. | |||
[[Category:Planets]] | |||
Revision as of 04:48, 26 November 2024
Duna is a small dry planet and the fourth planet in the Kerbol system Kerbolar system and functions as the mars analog. its orbital eccentricity and inclination are similar to Kerbin Kerbin's making it a relatively easy destination for interplanetary ships to reach from Kerbin. it features a thin atmosphere and a relatively massive moons moon Ike .
Synopsis
Duna the reddest planet has long been an object of study and inspiration to kerbal scientists and artists alike its thin low-pressure atmosphere allows for both aerobraking and relatively easy access to its surface. kerbal researches and sci-fi writers often discuss the discoveries that could be waiting for them in the planet planet\'s polar ice caps or on Duna's tidally locked moon Ike.
Surface
Duna has a desert-like reddish colored surface composed primarily of silicate rocks and sands covered by a fine layer of dust up to a few millimeters thick. This dust layer is theorized to be the result of dust storms. Dunian soil contains nutrients such as sodium potassium chloride and magnesium. The planet exhibits no tectonic activity and is believed to be geologically dead. Evidence of past tectonic activity is present however with volcanic basalt being quite common in certain regions. Surface features and exposed rocks show heavy signs of erosion by wind as well as flowing water. This combined with a the surprising amount salt in the ground indicates that Duna's surface may once have held liquid water. Duna's surface topography is mostly flat with occasional mountains and dunes. Various wikipedia impact_crater impact craters are spread out over its surface area. The majority of these are simple bowl-shaped craters with sparse wikipedia complex_crater#central-peak_craters center peak and wikipedia peak_ring peak ring formations. These craters are often eroded by the elements and overall less pronounced than those on atmosphere-less celestial bodies. For an unknown reason the northern hemisphere has significantly more impact craters. This may be explained by the impact of a comet that shattered before reaching the surface.
Polar ice caps
The most northernmost and southernmost parts of Duna's surface are covered by polar ice caps. These ice caps start at roughly 65 and -70 latitude respectively. They are estimated to be about 5 kilometers thick at their deepest point and composed of water ice and snow with a thin top layer of frozen carbon dioxide and trace amounts of dust. The northern ice cap has a deep spiraling pattern of troughs. These troughs are caused by roughly perpendicular wikipedia katabatic_wind katabatic winds that spiral due to the wikipedia coriolis_force coriolis effect.
Atmosphere
Duna has a thin cool atmosphere with a depth of 50 000 meters. Compared to the atmosphere of Kerbin, Duna's atmosphere has 1/15th the mass 1/15th the surface pressure and 1/9th the surface density. Duna's atmosphere is predominantly composed of carbon dioxide with a small fraction of nitrogen and argon as well as traces of oxygen, carbon monoxide, water, methane, and other gases. Melting of snow in the polar regions due to seasonal temperature variations is believed to be responsible for Duna's thin wispy clouds. These clouds are then carried toward the equator by a polar wikipedia jet_stream jet stream.
Atmospheric flight
The thickness of Duna's atmosphere makes it suitable for aerocapture from a high-speed interplanetary intercept. Although parachutes will deploy on Duna the atmosphere is so thin that they are usually unable to slow a craft to a safe landing velocity and must be assisted with engines. Parachute performance can be particularly troubling when attempting to land in the highland areas. Below 5,000 meters Duna's atmosphere is thick enough to allow wings to generate enough lift for aerodynamic flight. Jet engines will not work on Duna due to a lack of oxygen in the atmosphere but other propulsion methods work well. Performing a horizontal landing with a plane is also possible.
Magnetosphere
Duna has a weak magnetic field that's about 2 the strength of Kerbin's. There is evidence that Duna once had a much more powerful magnetic field but it weakened overtime as its core cooled.
Science regions
Duna has 6 surface regions which makes it one of the most region-rich bodies second only to Kerbin and Laythe. It is an ideal place for science collection for players who are embarking on their first interplanetary journey.
Orbital situations
class \"fandom-table\" science region altitude ranges science multiplier - high orbit 70 000 m - 47 921 949.369738 m 16.0 - low orbit 50 000 m - 70 000 m 24.0 - atmosphere 0 - 50 000 m 8.0
Surface regions
class \"fandom-table\" science region science multiplier - highlands 20.0 - midlands 20.0 - lowlands 20.0 - polar deserts 20.0 - north pole 20.0 - south pole 20.0
Discoverables
Duna face it there there's nothing here yet
Version history
v0.2.0.0
* added science regions.
v0.1.5.0
* updated atmospheric scattering.
v0.1.2.0
* celestial body ground scatter updates.
* height fog added.
v0.1.0.0
* initial release.