Extended classification system
~Compositional Categories
The bulk composition of planets varies significantly, but the components are divided into several major groups; Gases (specifically Hydrogen and Helium) Volatiles (ices such as water, ammonia, solid nitrogen) Siderophilic elements (chiefly iron), and a wide range of atmospheric gases other than H/He. Also significant is the ratio between carbon and oxygen- worlds and systems that are oxygen-rich are dominated by oxidised rocks, while systems that are carbon-rich have more carbide-type minerals.
~Nebular Gas Fraction
Worlds categorised by H2/He content
Jovian: Gas Giant worlds. Hydrogen and helium make up more than 50% of these worlds by mass.
Neptunian: Worlds with hydrogen and helium making up between 0.1% and 50% of the total mass.
Terrestrial: Worlds with less than 0.1% of the total mass coming from hydrogen or helium.
~Volatile Content
Worlds classified by their volatile content, sometimes referred to as ices (water, ammonia, carbon dioxide, methane, etc.)
Ymirian: Volatile ices contribute more than 67% of the non-gaseous mass of these worlds.
Gelidian: Mixed rock and ice composition. Volatiles make up 33-67% of the non-gaseous mass.
Cerean: Volatiles make up 1-33% of their non-gaseous mass.
Lapidian: Volatiles contribute less than 1% to the non-gaseous mass.
~Carbon Content
Worlds classified by C/O (carbon to oxygen) ratio
Adamean: Worlds with enough excess carbon to form a graphite or diamond rich crust. C/O above 10
Carbidic: Worlds dominated by carbide minerals, with small amounts of carbonates. C/O ratio between 1 and 10.
Carbonatic: Worlds with a blend of carbonate, oxide, and carbide minerals. C/O ratio between 0.1 and 1.
Oxidic: Worlds dominated by oxide minerals and/or oxygen rich volatiles, C/O ratios less than 0.1.
~Siderophile Metal Content
Worlds classified by siderophile metal fraction. Often conflated with core fraction in rocky terrestrial worlds.
Ferrinian: Especially dense worlds with siderophile metals making up more than 80% of its non-volatile mass. These worlds are often coreless, or entirely core, depending on interpretation.
Hermian: These worlds have siderophile metals making up 50-80% of their non-volatile mass.
Telluric: Worlds with siderophile metals making up 20-50% of the non-volatile mass.
Selenian: Siderophile metals make up 0-20% of the non-volatile mass.
~Atmospheric Composition
Worlds categorised by atmospheric composition. Composition is measured at a standardized pressure of 1 bar, or the surface if pressures are below 1 bar, since atmospheric composition can vary with altitude at low and high pressures.
Jotunnian: Hydrogen-dominated atmosphere
Helian: Helium-dominated atmospheres
Ydratian: Atmospheres dominated by simple hydrides (CH4, NH3, H2O, HF)
Rhean: Atmospheres dominated by diatomic non-metals (N2, O2, F2)
Minervan: Atmospheres of other non-metal compounds (CO, CO2, SO2, NO2, HNO3, CS2, HCN)
Hephaestian: Metal and metalloid compound atmosphere (SiO2, MgO, FeO, NaCl, Na, Fe)
Edelian: Atmospheres dominated by other noble gases
~Aerosols
The appearance of worlds with thick atmospheres is mostly determined by the amount, composition, and distribution of its atmospheric aerosols, or lack thereof.
The temperature of the troposphere, at ~0.1 bar, is also used to classify these worlds into four temperature categories: Cryothermal, <90 K; Mesothermal, 90-550 K; Pyrothermal, 550-1300 K; and Hyperpyrothermal, >1300 K. These temperature classes line up with late Y, early-mid Y, T, and L-M type brown dwarfs respectively.
-Cryothermal Aerosols :: Less than 90 K
Cold worlds in the outer reaches of planetary systems and in deep space
Cryoazurian: 0-90 Kelvin. No tropospheric clouds and only faint hazes. Dull blue in color, occasionally with hints of cyan from hydrocarbon hazes in the upper atmosphere.
Frigidian: 5-20 Kelvin. Extremely cold hydrogen clouds only capable of forming on worlds that are far from any stars. White clouds with hints of grey and blue.
Neonean: 15-35 Kelvin. Very cold neon clouds.
Borean: 35-60 Kelvin. Clouds of nitrogen, carbon monoxide, or more rarely oxygen. Various colors, typically pale pink or purple, although reds, oranges, or browns may occur from discoloration from organic hazes.
Methanean: 60-90 Kelvin. Clouds of methane, ethane, and occasionally argon. Usually accompanied by moderate amounts of organic haze. Light blue to turquoise in color, but can become more of a dull green or even bronze from extensive haze.
-Mesothermal Aerosols :: 90-550 K
Worlds of intermediate temperatures and distances.
Mesoazurian: 90-550 Kelvin. Uncommon clarified atmospheres. Usually teal or green in color as a result of heavy discoloring by organic and sulfur hazes.
Tholian: 60-550 Kelvin. Various organic hazes that obstruct the surface and any clouds below. Various colors, but usually pale yellow, orange or brown.
Sulfanian: 80-180 Kelvin. Sulfur enriched ammonian worlds. Clouds of hydrogen sulfide and ammonium hydrosulfide, with lesser amounts of ammonia, hydrogen chloride, sulfur dioxide, and organic hazes. Dull yellow, orange, or gold in color.
Ammonian: 80-190 Kelvin. Clouds of ammonia, ammonium hydrosulfide, and occasionally carbon dioxide, with significant organic haze. Various colors, typically cream, peach, or orange.
Hydronian: 170-350 Kelvin. Water clouds, usually with some amount of organic hazes. Clouds are predominantly white, but can take on a yellow or brown tinge from hazes.
Acidian: 250-500 Kelvin. Clouds predominantly of sulfuric acid, with significant amounts of sulfur aerosols. Phosphoric acid and ammonium chloride clouds can occur but more rarely. Tan, taupe, or beige in color.
-Pyrothermal Aerosols :: 550-1300 K
Hot worlds close to their star or still hot from forming.
Pyroazurian: 550-1300 Kelvin. Very few clouds or hazes, especially above 900 K. Various shades of blue depending on the amount of haze.
Sulfolian: 400-1000 Kelvin. Hazes of sulfur and organosulfur compounds. Most often gold or bronze in color, but can take on more extreme green or orange hues as well.
Silicolean: Worlds with hazes of silicone oils, fluorosilicones, and other organosilicon compounds, occurring between 550 and 1000 Kelvin. Light brown or grey in color.
Chloroalkalinean: Worlds between 620 and 900 Kelvin with clouds of alkali metal chlorides. Potassium chloride is the most common of these, and may also be accompanied by other metal compounds with similar condensation curves such as zinc sulfide. These clouds can be bronze or pale green in color.
Sulfoalkalinean: Worlds between 800 and 1100 Kelvin with alkali metal sulfide clouds. There is significant overlap between sulfoalkalinean and chloroalkalinean clouds, with sulfoalkalinean clouds being significantly hotter. The most common compounds in these clouds are sodium sulfide, lithium sulfide, and lithium fluoride. These clouds are dark brown or grey in color.
-Hyperpyrothermal Aerosols :: Above 1300 K
Very hot worlds with nightsides luminous at visible wavelengths, making their natural color difficult to observe.
Hyperpyroazurian: 1300+ Kelvin. No visible cloud deck, and only slightly hazy. Silicate cirrus clouds may be present on cooler worlds. Daysides are various shades of blue depending on the amount of haze, with nightsides being colored according to thermal luminosity.
Erythronian: Worlds between 1150 and 1500 Kelvin, possessing clouds of Manganese oxides and sulfides, as well as metallic chromium. Some erythronian worlds are hot enough to host titanium and vanadium oxide hazes instead of organosulfur compounds. Clouds of this type appear dull red to dark orange in color.
Enstatian: 1300-1900 Kelvin. Silicate clouds containing magnesium, iron, and occasionally more uncommon metals. Typically grey with a tinge of blue, green, or brown.
Rutilian: Hazes of titanium and vanadium oxides occurring between about 1450 and 2000 Kelvin. These worlds are dark grey to black in color.
Refractian: 1800-2300 Kelvin. Clouds of refractory oxides, primarily aluminium oxide, titanium dioxide, and calcium oxide. Usually red, orange, or tan in color.
Carbean: 2000-2900 Kelvin. Clouds of refractory carbides such as titanium and vanadium carbide. Moderate carbon haze from dissociation of silicon carbide. Limited to carbon rich worlds. Often dark brown in color.
EpistellarAzurian: 2200+ Kelvin. Ultrahot subset of HyperpyroAzurian worlds. #414060 in color.
Aithalian: 2600-3400 Kelvin. Moderate haze of fullerenes and other carbon alotropes, overpowering any clouds present.	#1F1820 in color.
~Surface and Subsurface Conditions
Also known as terrestrial types, as they are to only worlds to even have well defined surfaces. However Neptunian and Jovian worlds can also possess surface types.
~Surface Type
Worlds categorised by the phase transition at the boundary between their atmosphere and their topmost solid or liquid surface.
Abyssal: Worlds characterised by a high pressure compressible liquid surface under a thick, vapor rich, and often supercritical fluid atmosphere.
Gaian: Worlds resembling Earth, with atmospheric vapor condensing into liquid lakes, seas, and oceans on the surface.
Tohulian: Worlds with a liquid surface under a supercritical fluid atmosphere of a different species.
Cytherean: Venus-like worlds characterised by a surface transition from a supercritical fluid to a distinct solid substrate. Like larger Neptunians and Jovians, the upper atmospheres of these worlds often host virga precipitation, which evaporates before reaching the surface.
Muspellian: Worlds where the supercritical fluid atmosphere transitions to high pressure ice at the surface. They are similar to Cytherean worlds. Muspellian worlds have crushing atmospheres, often in excess of 100,000 bar.
Barian: Worlds with a high pressure metalized liquid under a supercritical fluid atmosphere. This type is limited to Neptunian and Jovian worlds, and metallic hydrogen is nearly universally the liquid medium.
Arean: Worlds characterised as having vapor atmospheres below the triple point where atmospheric vapor can deposit and sublime to and from the surface.
Agonian: Worlds where a gaseous or vapor atmosphere above the triple pressure meets the surface without any liquids or supercritical fluids present.
Achlysian: Worlds with a gaseous or vapor atmospheres below the triple pressure, where there are no ices present on the surface.
Apnean: Airless worlds with only an exosphere and surface pressures below 0.1 nanobar [10E-5 Pa].
~Subsurface Type
Worlds categorised by phase transitions beneath the surface.
Europan: Worlds with a subglacial hydrosphere beneath a layer of solid ice.
Thalassic: Worlds with high pressure ices at the bottom of a liquid ocean.
Ganymedean: Icy worlds with high pressure ices at the bottom of a subglacial hydrosphere. Ganymedeans share features with both Europan and Thalassic worlds.
Phlegethean: Typically younger worlds with a supercritical fluid layer under a deep compressible liquid ocean.
Atlantean: Icy worlds with a supercritical fluid layer at the bottom of a subglacial hydrosphere. Combination of the Europan and Phlegethean classes.
Cryptian: Worlds with a liquid hydrosphere in caverns and subsurface fluid tables beneath or within a distinct substrate.
~Precipitation Type
Worlds categorised by their precipitation and retention of surface ices.
Thermal: Worlds too hot for any frozen precipitation to reach the surface. Typically very humid.
Tepidal: Temperatures low enough for snow and ice, but not for permanent accumulation in ice caps.
Tundral: Worlds cold enough for snow and ice to accumulate in glaciers and ice caps, but still warm enough for rain.
Glacial: Worlds where it is too cold for rain to occur. These worlds can still support liquids on the surface from warmer surface temperatures, though are usually covered in snow and ice.
~Liquid Surface Coverage
Worlds with surface liquids categorised by its coverage on the surface. This also includes liquid reservoirs that are covered by ice.
Inundic: The surface is entirely covered by liquids.
Oceanic: 90-100% of the surface is covered by a liquid or its ice.
Marine: Worlds where 60-90% of the surface is covered by a liquid, often as a single interconnected body.
Estuarine: 40-60% of the surface is covered by a liquid.
Lacustrine: 10-40% of the surface is covered by a liquid, often as shallow isolated bodies.
Conlectic: Less than 10% of the world’s surface is covered by a liquid.
~Fluids and Ice Types
There are countless different fluids that can be naturally found on worlds, though only a few of these are relatively common.
Hydrospheres are unique among these in that they can be near homogeneous mixtures of multiple fluids, unlike the more stratified layers in ices and supercritical fluids. For Gaian, Tohulian, Europan, and Cryptian worlds, if a secondary fluid type comprises more than 5% of the total, then a hybrid fluid type is used.
Aquatic: Water. Usually found as a liquid or supercritical fluid, water is one of the most common fluids. Because of its abundance, it usually dominates binary liquid mixtures with other liquids. Liquid water is usually blue in color.
Amunian: Ammonia. A common fluid, it typically occurs as a liquid, usually in conjunction with water at low to moderate concentrations. Ammonia dominated liquids, as well as ammonia ices, are less frequent.
Titanian: Short hydrocarbons, most commonly methane, ethane, and/or propane, with other organic compounds in lesser amounts. It is a very common fluid type, predominantly occurring as a liquid, but can also occur as ices. Nitrogen and carbon monoxide, slightly colder liquids, are capable of mixing with titanian seas.
Petrolic: Moderate length hydrocarbons with a composition comparable to crude oil, containing the alkanes pentane to icosane along with a wide variety of other organic compounds. The petrolic fluid type is rather common, especially on, but not limited to, carbon rich worlds. Because of the overlapping liquid ranges and low triple points of its constituents, nearly all petrolic worlds are host to liquids. Petrolic worlds are similar to Titanian worlds, but occur at higher temperatures.
Bitumic: Bitumen and other heavy organic compounds. A common fluid type that usually occurs as either a liquid or supercritical fluid, as a result of the low critical pressure of long hydrocarbons. These worlds are similar to Petrolic worlds, but occur at even higher temperatures. They can be found with varying levels of sulfur and organosulfur compounds.
Dionysian: Alcohols, primarily methanol and ethanol. A fairly common fluid type, that usually occurs as a liquid. Alcohols are miscible with many substances, like water, octane, and carbon disulfide.
Capnian: Carbon dioxide. It usually occurs as a supercritical fluid or as an ice, and is one of the most common fluid types.
Azotian: Nitrogen. It is one of the most common fluids, typically found as an ice or supercritical fluid. The Azotian type is quite ubiquitous among cold outer system worlds beyond the N2 iceline, as well as cytherean worlds with thinner atmospheres.
Monoxian: Carbon monoxide. A somewhat common fluid that is usually found as either an ice or supercritical fluid. It occurs in similar conditions to nitrogen, but as it is prone to oxidation, it is limited to more carbon rich worlds.
Oxygenean: Oxygen. A less common fluid type, found almost exclusively as a supercritical fluid. These conditions occur on worlds that have lost extreme amounts of water.
Hydrogenean: Hydrogen. A very common fluid, typically as a metallic liquid in Neptunian and Jovians, but can also much less frequently occur on large cold terrestrials in other states, usually a supercritical fluid. Liquid hydrogen is very rare, as ambient interstellar temperatures and internal heating can make a world too warm for hydrogen to condense onto the surface.
Neonic: Neon. A somewhat uncommon fluid typically found as an ice, supercritical fluid, or occasionally a liquid. It is most frequent on interstellar objects, where internal heating alone is sufficient to keep it from becoming part of the substrate.
Ignean: Magma, primarily in the form of molten metals, metal oxides, and metal carbides. One of the most common fluid types, but is often limited to the interiors of worlds. It most frequently occurs as a liquid.
Salific: Metal salts, primarily alkali chlorides and sulfates. A rare fluid, that usually occurs as either a liquid or ice. They are usually found alongside other metal compounds like lower temperature magmas and sulfur compounds.
Fortic: Nitric acid. A very uncommon fluid type, primarily as a liquid. Nitric acid is often found in solution with water, but also occasionally ammonia or dinitrogen tetroxide. It is rarely found in concentrations above around 70%.
Amylian: Oxides of nitrogen, primarily nitrogen dioxide and dinitrogen tetroxide. A rare fluid type, usually found as an ice or liquid. Will combine with water to form nitric acid.
Cyanic: Hydrogen cyanide. An uncommon fluid, usually found as either a liquid or ice. It occurs in similar, albeit slightly warmer, environments to ammonia, which it often occurs alongside. It is more common in carbon rich systems.
Hepatic: Hydrogen sulfide. An uncommon fluid, usually found as a liquid or ice. When liquid, it often occurs in combination with ammonia or water.
Ionean: Oxides of sulfur, predominantly sulfur dioxide. An uncommon fluid that occurs most often as an ice or liquid, but is also rarely found as a supercritical fluid. The IoArean type is especially common for cold volcanic worlds.
Disulfian: Carbon disulfide. A rather uncommon fluid type, usually as a liquid. Most commonly found on carbon rich volcanic worlds, and can occur alongside a wide array of compounds.
Brimstonian: Sulfur. An uncommon fluid, typically occurring as a liquid or ice. Typically occur on hot volcanic worlds enriched in sulfur. It can be found with organosulfur compounds and metal sulfides.
Vitriolic: Sulfuric acid. An uncommon fluid that usually occurs only as a liquid. Higher concentrations are somewhat more common than lower ones, as a result of azeotropic mixing with water. In addition to water, sulfuric acid can also occur alongside sulfur oxides, and more rarely phosphoric or hydrochloric acid.
Carbonylic: Metal carbonyls, primarily iron pentacarbonyl or nickel tetracarbonyl. A very uncommon fluid that is typically found as a liquid. Most often occurs on worlds with metal rich surfaces, and is sometimes in solution with petrochemicals or alcohol.
Formamian: Formamide and other simple organic compounds containing hydrogen, carbon, nitrogen, and oxygen. Formamide is an uncommon fluid, usually in a liquid state. It is usually found along various organic and inorganic compounds, including water, ammonia, alcohols, hydrogen cyanide, and formic acid.
Phosphinic: Phosphine. A very rare fluid usually found as a liquid or ice. It often occurs in solution with alcohol or carbon disulfide.
Phosphoric: Phosphoric acid. A very rare fluid type usually found as a liquid or ice. It can be found alongside water or sulfuric acid with similar frequencies.
Hydrochloric: Hydrochloric acid or hydrogen chloride. A very rare fluid, primarily a liquid. It is readily formed from sulfuric acid breaking down chloride minerals, and usually occurs alongside H2SO4. It can also form from biological processes, though more rarely. Highly concentrated hydrogen chloride is far rarer than lower concentrations.
Hydrofluoric: Hydrofluoric acid or hydrogen fluoride. An extremely rare fluid type. These worlds form through similar mechanisms to hydrochloric worlds, but are far rarer due to fluorine’s lower abundance.
~Mass
A single unified mass scale for all objects, regardless of their composition.
-Planetesimals :: Small irregular bodies
Lowerplanetesimal: 2.4E+11 to 2.4E+13 kg. Small objects just massive enough to not be affected by gas drag.
Midplantesimal: 2.4E+13 to 2.4E+15 kg. More likely to be a singular object rather than aggregate rubble pile.
Upperplanetesimal: 2.4E+15 to 2.4E+17 kg. Largest bodies unable to undergo partial differentiation.
-Planetoids :: Small semi-rounded bodies
Lowerplanetoid: 2.4E+17 to 2.4E+18 kg. May have possibly undergone partial differentiation in its past.
Midplanetoid: 2.4E+18 to 2.4E+19 kg. May be semi-rounded in appearance from past hydrostatic equilibrium.
Upperplanetoid: 2.4E+19 to 2.4E+20 kg. Can potentially maintain a rounded shape after falling out of hydrostatic equilibrium.
-Terrenes :: Medium rounded bodies
Petiterrene: 0.00004 to 0.0004 Earth masses. Massive enough to likely remain in hydrostatic equilibrium.
Lowerterrene: 0.0004 to 0.004 mE.
Midterrene: 0.004 to 0.04 Earth masses. Likely to be fully differentiated.
Upperterrene: 0.04 to 0.4 Earth masses. May be tectonically active for hundreds of millions to billions of years before becoming quiescent.
Grandterrene: 0.4 to 4 Earth masses. Capable of supporting mobile-lid tectonics and unable to completely lose an atmosphere under extreme heating.
-Giants :: Large rounded bodies
Lowergiant: 4 to 40 Earth masses. Massive enough to develop a thick hydrogen and helium envelope, which may be lost or greatly reduced after formation from high temperatures.
Midgiant: 40 to 400 Earth masses. May have undergone runaway accretion in its past.
Uppergiant: 400 to 4000 Earth masses. Largest giants unable to undergo deuterium burning. Radius is only minimally affected by mass.
~Miscellaneous Parameters
Some worlds can have peculiar characteristics which do not fall into any of the other categories. These characteristics are denoted here.
~Rotation Based Classifications
Worlds with unusual rotational parameters.
Skolian: High Obliquity worlds with an axial tilt between 45 and 135 degrees, resulting in polar regions having a higher average temperature than the equator.
Videntian: Worlds tidally locked to their primary. This includes most moons.
Stilbonian: Worlds in a spin orbit resonance with their primary, with an integer ratio between orbital and rotational period.
Aeolian: Fast spinning oblate worlds with a flatness of 0.1 or higher.
Jacobian: Worlds which spin fast enough to relax into a triaxial Jacobi ellipsoid.
Synestian: Rapidly rotating worlds with an extended toroidal atmosphere, often briefly forming as a result of planetary collisions.
~Orbital Classifications
Worlds with unusual orbital parameters.
Stevensonian Type Worlds: Worlds in interplanetary space that orbit a galaxy or cluster of stars directly.
Ikarian Type Worlds: Worlds with highly eccentric orbits, with eccentricities of 0.35 or greater.
Circumbinary Type(s) Worlds: Worlds that orbit multiple stars in a system.
~Life Based Classifications
Worlds that currently host life, have previously hosted life, or are in the process of abiogenesis.
Protobiotic: Worlds undergoing abiogenesis, rich in prebiotic molecules like protocells and other life-like organisms. Usually only a brief phase, but may become greatly extended by various planetary factors.
Microbiotic: Most common type of biotic world. These worlds host microbial life, often of low complexity.
Mesobiotic: Worlds with simple colonial, multicellular, and/or megacellular organisms.
Macrobiotic: Worlds hosting a well developed ecosystem of macroscopic multicellular, colonial, and/or megacellular organisms.
Neobiotic: Worlds that have had life introduced from another world or heavily modified by artificial means.
Postbiotic: Worlds that had once hosted life which has since completely died out.
~Planetary History Classifications
Worlds in unique or otherwise notable stages of their formation or evolution.
Chthonian: Worlds that formed with and since lost extensive hydrogen and helium envelopes.
Ragnorokian: Worlds that have survived their host star becoming a stellar remnant.
Odyssian: Worlds which originated in a different star system.
Phoenixian: Worlds that formed around non-main sequence stars.
Chaotian: A world still immersed in a protoplanetary disk.
Genesian: Artificially created planets and planet-like objects.
~Multiworld Classifications
Worlds that have interesting orbital interactions with other worlds.
Trojan: Worlds orbiting at the L4 or L5 lagrange point of another world that is at least 25 times as massive.
Janusian: Worlds that are in co-orbital resonance with another world where momentum exchange occurs regularly.
Satellite: Worlds that orbit another world, rather than a star itself.
Dioscuran: Worlds in orbit around another world less than 10 times as massive.
Rochean: Dioscuran worlds that share a common envelope. These worlds are often of very similar masses and may form contact-binaries.