Planets: Difference between revisions

! scope="col"|Rarity

|-

|Icy Body

|Very Common

| colspan="2"|''Ice world composed mainly of water ice. Worlds like this will not have had much heating in the past, forming in the cooler regions of a star system and have retained many volatiles as solids in their crust.''

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|Rocky Body

|Very Common

| colspan="2"|''Rocky world with little or no surface metal content. Worlds like this have lost most of their volatiles due to past heating, and any metallic content will form a small central core.''

|-

|[[Rocky Ice World]]

|Uncommon

| colspan="2"|''Typically formed in the cooler regions of a star system these worlds have a small metal core and thick rocky mantle with a crust of very deep ice. Geological activity is common in these worlds because of the large quantities of volatiles in the crust, often creating a thin, sometimes seasonal atmosphere.''

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|High-Metal Content World

|Common

| colspan="2"|''High metal content world with a metallic core. Worlds like this can have metallic ores near the surface in places, especially around areas of past volcanism.''

|-

|[[Metal-Rich Body]]

|Uncommon

| colspan="2"|''Metal-rich worlds like this have a large metallic core, with plentiful metallic ores even at the surface. In places, especially around areas of past or current volcanism or liquid erosion, some higher metals can be found in their elemental form too. Mining is therefore very efficient, so these worlds are highly valued.''

|-

|[[Ammonia World]]

|Very Rare

| colspan="2"|''Terrestrial ammonia world with an active ammonia-based chemistry and carbon-ammonia based life.''

|-

|[[Water World]]

|Rare

| colspan="2"|''Terrestrial water world with an active water-based chemistry and carbon-water-based life.''

|-

|[[Earth-like World]]

|Very Rare

!Rarity

|-

|Class I

|Common

| colspan="2"|''Class I or Jovian gas giants have primarily hydrogen and helium atmospheres. Colouration comes from clouds in the upper atmosphere of ammonia, water vapour, hydrogen sulphide, phosphine and sulphur. The temperature at the top of their upper cloud layers is typically less than 150 K.''

|-

|Class II

|Rare

| colspan="2"|''Class II gas giants have primarily hydrogen and helium atmospheres. Water vapour in the upper cloud layers gives them a much higher albedo. Their surface temperature is typically up to or around 250 K.''

|-

|Class III

|Common

| colspan="2"|''Class III gas giants have primarily hydrogen and helium atmospheres without distinctive cloud layers. Their surface temperature typically ranges between 350 K and 800 K. They are primarily blue in colour because of optical scattering in the atmosphere - with the chance of wispy cloud layers from sulphides and chlorides.''

|-

|Class IV

|Uncommon

| colspan="2"|''Class IV gas giants have primarily hydrogen and helium atmospheres with carbon monoxide and upper clouds of alkali metals above lower cloud layers of silicates and iron compounds, hence he brighter colours. The temperature of their upper cloud layers is typically above 900 K.''

|-

|Class V

|Very Rare

|colspan="2"|''Class V gas giants have primarily hydrogen and helium atmospheres, with thick clouds of silicates and iron compounds, even metallic iron.They are the hottest type of gas giants with temperatures at their upper cloud decks above 1400 K, and much hotter in the lower layers, often emitting a dull glow from the internal heat within.''

|-

|Helium-rich

|Very Rare

| colspan="2"|''Helium-rich gas giants have a greatly inflated percentage of helium compared to the hydrogen in their atmosphere. Much of their hydrogen has been lost over time because they have insufficient mass to hold on to it. It may also be because temperatures in their past were much higher, driving off the hydrogen at a greater rate.''

|-

|Helium Gas Giant

|Very Rare

| colspan="2"|''Helium gas giants have primarily a helium atmosphere. They have lost most or all of their hydrogen because they have insufficient mass to hold on to it over time. It may also be because temperatures in their past were much higher, driving off the hydrogen at a greater rate.''

|-

|Gas Giant with ammonia-based life

|Very Rare

| colspan="2"|''Gas giant with ammonia-based life. This is primarily a hydrogen and helium-based atmospheric gas giant, but a little below the surface cloud layers,life exists based in the ammonia-cloud layer. The chemistry of this gaseous region is far from equilibrium, with a surprising excess of oxygen and many carbon-based compounds giving it some vivid colours. As with many such gaseous living systems, it is underpinned by vast quantities of free-floating radioplankton - tiny carbon-based algae, each retaining small quantity of liquid ammonia, extracting their energy from the intense radiation flux.''

|-

|Gas Giant with water-based life

|Rare

|-

|-

|Water Giant

|Very Rare