Planet Editor: Difference between revisions
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[[Category:Editors| | [[Category:Editors|1]] | ||
[[Category:Planets]] | |||
The Planet Editor is one of Thrive's five editors, and the last to be unlocked. It allows the player to edit a whole planet, including its ecosystem, atmospheric conditions, topography, and the like. The tools needed to unlock this editor are highly advanced, meaning that the player will be well into [[Space Stage]] before the possibility of unlocking the Planet Editor is available. | The Planet Editor is one of Thrive's five editors, and the last to be unlocked. It allows the player to edit a whole planet, including its ecosystem, atmospheric conditions, topography, and the like. The tools needed to unlock this editor are highly advanced, meaning that the player will be well into [[Space Stage]] before the possibility of unlocking the Planet Editor is available. | ||
== | == Star Generation == | ||
Before the planet can be generated, a star must be generated for the solar system. | |||
For the time being, we will assume all playable solar systems initially form main sequence stars (also called dwarf stars), like our sun. Other types of stars include | |||
* Supergiants | |||
* Bright Giants | |||
* Giants | |||
* Subgiants | |||
* White Dwarfs | |||
=== Luminosity, Radius, and Temperature === | |||
A star's luminosity, radius, and surface temperature are related via the following equation: | |||
L = 4πR<sup>2</sup>σT<sup>4</sup> | |||
Where: | |||
L = luminosity (in watts) | |||
R = stellar radius (in meters) | |||
T = surface temperature (in degrees Kelvin) | |||
σ = Stefan-Boltzmann constant | |||
The player will be able to set the luminosity and radius of their star. As σ is a constant, this will determine the resulting temperature of the star. | |||
=== Mass === | |||
Using the luminosity, the game can then calculate the star's mass using the following formula: | |||
L<sub>star</sub> / L<sub>sun</sub> = ( M<sub>star</sub> / M<sub>sun</sub> )<sup>a</sup> | |||
Where: | |||
L<sub>star</sub> = Luminosity of the generated star | |||
L<sub>sun</sub> = Luminosity of the sun | |||
M<sub>star</sub> = Mass of the generated star | |||
M<sub>sun</sub> = Mass of the sun | |||
a = Is a constant, which is typically set as 3.5 for main-sequence stars. | |||
=== Lifespan === | |||
The luminosity and mass of the star can be used to calculate it's lifespan. | |||
t = 10<sup>10</sup>(M<sub>sun</sub> / M<sub>star</sub>)<sup>3</sup> | |||
Where: | |||
t = The lifespan of the generated star | |||
M<sub>sun</sub> = The mass of the sun | |||
M<sub>star</sub>) = The mass of the generated star | |||
=== Habitable Zone === | |||
The game can then use these values to determine the habitable zone of the star. The inner and outer bounds (in astronomical units) of the zone can be calculated with: | |||
Inner Bound = 0.7R(T/5777)<sup>2</sup> | |||
Outer Bound = 1.5R(T/5777)<sup>2</sup> | |||
Where: | |||
R = stellar radius (in solar radii, NOT in meters) | |||
T = surface temperature of the star (in degrees Kelvin) | |||
=== Additional Notes === | |||
Star Generation: | |||
* System Type (Number of Stars: Unary, Binary, Trinary, etc.) | |||
* Luminosity | |||
** Mass | |||
** Radius | |||
** Lifetime | |||
** Temperature | |||
** Habitable Zone | |||
*** Choose where the planet exists in this zone. | |||
**** Average Planetary Temperature | |||
**** Year Length | |||
Planet Generation: | |||
* Distance | |||
* Planetary Mass, Radius, Gravity, Density | |||
* Day Length | |||
* Axial Tilt: Determines seasonal variation | |||
* Atmosphere composition (Nitrogen, oxygen, carbon dioxide, argon, hydrogen sulfide, etc.) | |||
* Moons (Affects tidal forces) | |||
** Number | |||
** Distance | |||
** Mass | |||
*** Tides | |||
* Tectonics | |||
Planet Templates: | |||
* Terran Planet | |||
* Sulfur Planet? | |||
* Silica Planet? | |||
* Chlorine Planet? | |||
* Fluorine Planet? | |||
=== The Solar System === | === The Solar System === | ||
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<nowiki>*Temperatures are designated by distance from the sun, geologic activity, etc.</nowiki> | <nowiki>*Temperatures are designated by distance from the sun, geologic activity, etc.</nowiki> | ||
== Research == | |||
https://spec-evo.fandom.com/wiki/Alien_Planets#Geology | |||
== Sources == | |||
https://cosmicreflections.skythisweek.info/2017/06/08/habitable-zones/ |
Latest revision as of 18:35, 16 September 2022
The Planet Editor is one of Thrive's five editors, and the last to be unlocked. It allows the player to edit a whole planet, including its ecosystem, atmospheric conditions, topography, and the like. The tools needed to unlock this editor are highly advanced, meaning that the player will be well into Space Stage before the possibility of unlocking the Planet Editor is available.
Star Generation
Before the planet can be generated, a star must be generated for the solar system.
For the time being, we will assume all playable solar systems initially form main sequence stars (also called dwarf stars), like our sun. Other types of stars include
- Supergiants
- Bright Giants
- Giants
- Subgiants
- White Dwarfs
Luminosity, Radius, and Temperature
A star's luminosity, radius, and surface temperature are related via the following equation:
L = 4πR2σT4
Where:
L = luminosity (in watts)
R = stellar radius (in meters)
T = surface temperature (in degrees Kelvin)
σ = Stefan-Boltzmann constant
The player will be able to set the luminosity and radius of their star. As σ is a constant, this will determine the resulting temperature of the star.
Mass
Using the luminosity, the game can then calculate the star's mass using the following formula:
Lstar / Lsun = ( Mstar / Msun )a
Where:
Lstar = Luminosity of the generated star Lsun = Luminosity of the sun Mstar = Mass of the generated star Msun = Mass of the sun a = Is a constant, which is typically set as 3.5 for main-sequence stars.
Lifespan
The luminosity and mass of the star can be used to calculate it's lifespan.
t = 1010(Msun / Mstar)3
Where:
t = The lifespan of the generated star Msun = The mass of the sun Mstar) = The mass of the generated star
Habitable Zone
The game can then use these values to determine the habitable zone of the star. The inner and outer bounds (in astronomical units) of the zone can be calculated with:
Inner Bound = 0.7R(T/5777)2
Outer Bound = 1.5R(T/5777)2
Where:
R = stellar radius (in solar radii, NOT in meters)
T = surface temperature of the star (in degrees Kelvin)
Additional Notes
Star Generation:
- System Type (Number of Stars: Unary, Binary, Trinary, etc.)
- Luminosity
- Mass
- Radius
- Lifetime
- Temperature
- Habitable Zone
- Choose where the planet exists in this zone.
- Average Planetary Temperature
- Year Length
- Choose where the planet exists in this zone.
Planet Generation:
- Distance
- Planetary Mass, Radius, Gravity, Density
- Day Length
- Axial Tilt: Determines seasonal variation
- Atmosphere composition (Nitrogen, oxygen, carbon dioxide, argon, hydrogen sulfide, etc.)
- Moons (Affects tidal forces)
- Number
- Distance
- Mass
- Tides
- Tectonics
Planet Templates:
- Terran Planet
- Sulfur Planet?
- Silica Planet?
- Chlorine Planet?
- Fluorine Planet?
The Solar System
The solar system will start out as a planetary disk. Out of that planets will form, and smash into each other, all of that good Belgium. How it happens. That's basically how you'll have your solar system form. The PE, however will be making planets that are fully fledged.
In The Beginning
You're going to start out with a sizing table, how big you want your planet to be. This will decide size and gravity, however, gravity can be slightly adjusted with a small slider. Gas giants will be made in the same way they were in the old editor, by laying down layers of gases on top of the molten liquid core.
There will be an option to randomize rock layers and landforms on the planet.
Rocky bodies are going to start out as realistic as possible. They're going to be masses of black volcanic rock with cracks corresponding to the gaps between tectonic plates. Tectonics will be a part of your planet, and you'll have continental drift and all sorts of other things that come with the rifts like ocean trenches, volcanoes, earthquakes, etc.
You start to create your planet by building with different layers of rock. You'll have a few panels of rock types- sedimentary, metamorphic, and igneous. You'll have a panel of each type with a few different types of rock on it.
The Rock Cycle will be active as well, so your planet won't stay a granite ball if you make it that way.
Building Controls
Basically, you will have brushes and paint. The brush you select will define how rock is placed, and the "paint" will be a type of rock selected from one of the rock palettes described above. You can also carve into your planet to create canyons, valleys, etc using different brushes. More brushes will populate in small features like hills, small lakes, bluffs, ground covering (except for organisms) etc. You can pour water onto any point on your planet, and also plant springs. You can designate other liquids like liquid methane if temperatures permit*. Different layers of liquid can be poured on, as long as they are of different densities they will not mix.
You can paint biomes on to your planet using brushes. Each brush has a set of rules, and some biomes, including beaches and sea zones will populate automatically.
Static VS Dynamic
Static planets never change from original settings, geologically. In God mode, you should be able to pause organic evolution on a planet as well. Dynamic planets can be affected by geologic activity, disasters, etc, and are constantly in a state of change, like our planet earth. Basically, random things happen to tectonic movement, random asteroids get hurled at your planet, etc.
That's all for now.
*Temperatures are designated by distance from the sun, geologic activity, etc.
Research
https://spec-evo.fandom.com/wiki/Alien_Planets#Geology
Sources
https://cosmicreflections.skythisweek.info/2017/06/08/habitable-zones/