Planets

There are two main categories of planets: Terrestrial Planets and Gas Giants. Some types of Terrestrial Planets support life or meet the conditions necessary for terraforming. Ships equipped with a Planetary Approach Suite may land on the surface of certain Terrestrial Planets.

The term planet refers to celestial bodies orbiting a star with a gravity in a specific range. The gravity of a planet has to be strong enough to hold fluids in a stable state (hydrostatic equilibrium) which prevents them from escaping the planet, and low enough to prevent nuclear processes to start as in stars.

Some astronomical objects that meet the official criteria for planet status yet also happen to orbit a planet are instead classified as natural satellites or moons. When a moon's orbit expands to the point that the barycentre of the planet-moon system falls outside the center of the planet, then both bodies would be considered planets and part of a double-planet system.

Terrestrial Planets

Image	Type	Rarity
	Icy Body	Very Common
	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.
	Rocky Body	Very Common
	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
	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.
	High-Metal Content World	Common
	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
	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
	Terrestrial ammonia world with an active ammonia-based chemistry and carbon-ammonia based life.
	Water World	Rare
	Terrestrial water world with an active water-based chemistry and carbon-water-based life.
	Earth-Like World	Very Rare
	Outdoor world with a human-breathable atmosphere and indigenous life. The atmosphere is far from chemical equilibrium as a result.

Gas Giants

Image	Type	Rarity
	Class I	Common
	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
	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
	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
	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
	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
	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
	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
	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
	Gas giant with water-based life. This is primarily a hydrogen and helium based atmospheric gas giant, but not far below the surface exists life based in the water-cloud layer just below the atmospheric surface. 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 water, extracting their energy from the intense radiation flux.
	Water Giant	Very Rare
	Water giant. Worlds like this have a large atmosphere made mainly of water vapour. It most likely formed when a large icy body warmed up enough to evaporate a large amount of its surface ice, this would in turn trigger a runaway greenhouse effect leading to a very thick atmosphere made of the evaporated ices.

Videos

Elite dangerous 1. Planets a. Gas giants

Elite Dangerous 1. Planets b. Volcanic

Elite Dangerous 1. Planets c. Class M

Elite Dangerous 1. Planets d. Rings

Elite Dangerous 1. Planets e. Others

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