Planets: Difference between revisions

Swapped high-metal content and metal-rich body descriptions back to correct titles.
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There are three main categories of '''[[:Category:Planets|planets]]''': Solid planets, water giants and [[Gas Giant|gas giants]].
There are two main categories of '''planets''': [[Terrestrial Planet]]s and [[Gas Giant]]s. Some types of Terrestrial Planets support [[Species|lifeforms]] or meet the conditions for [[terraforming]]. [[Ships]] equipped with the [[Planetary Approach Suite]] may [[Planetary Landings|land on the surface]] of Terrestrial Planets with 0 to tenuous (0.01-0.10) [[Atmosphere|atmospheres]]. Some planets have a [[Planetary Ring System|planetary ring system]].


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.  
* The [[:Category:Planets|category]] has a list of notable planets.  


Some astronomical bodies, we call planets, are not considered as planets by this definition. [[Moons]] are natural satellites orbiting a planet and do not fall into the category of planets. However, some natural satellites are considered as planets because they fit their definition.<ref>https://www.universetoday.com/85749/is-the-moon-a-planet/</ref>
== Description ==
The term planet refers to a celestial body that orbits a [[star]] with a [[gravity]] in a specific range. The gravity of a planet must be strong enough to hold fluids and plastic solids in a stable state (hydrostatic equilibrium) which prevents them from escaping the planet and it makes the body round, and low enough to prevent stellar nuclear processes to start.


== Terrestrial planet ==
Astronomical objects that meet the official criteria for planet status yet orbit a planet are instead classified as natural satellites or [[moons]]. When the [[barycentre]] of the planet-moon system falls outside the planet, then both bodies are considered planets and part of a double-planet system.<ref>[https://www.universetoday.com/85749/is-the-moon-a-planet/ Universe Today: Is The Moon A Planet?]</ref>
{| class="article-table article-table-selected" border="1" cellpadding="1" cellspacing="1"
 
==[[Terrestrial Planet]]s==
{|class="wikitable unsortable" style="text-align:center;" border="1"
|-
!Type
!Description
!Rarity
!Image
|-
|-
! scope="col"|Image
|Icy body
! scope="col"|Class
|''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.''
! scope="col" |Colour
|Very Common
! scope="col"|Rarity
|[[File:Icy body Wredguia HY-G c24-10 C 1.png|thumb|center]][[File:Icy body Wredguia HY-G c24-11 A 2.png|thumb|center]]
! scope="col"|In game description
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Rocky body
Icy-180px.png
|''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.''
</gallery>
|Very Common
|Icy planet
|[[File:Rocky body HIP 53248 AB 4 d.png|thumb|center]][[File:Rocky bodies HIP 99152 2 b a+b.png|thumb|center]]
|White - Grey - Bluish
|Very common
|Ice world composed mainly of water ice. Worlds like this will not have much heating in the past, forming in the cooler regions of a star system and have retained many volatiles as solids within their crust.
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|[[Rocky Ice World]]
Rocky-Planets-180px.png
|''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.''
</gallery>
|
Rocky planet
|White - Grey - Light blue - Light brown - Yellow
|Common
|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.
|[[File:Rocky ice world Wredguia AG-F d11-24 A 7.png|thumb|center]]
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|High metal content world
Rocky_ice.png
|''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.''
</gallery>
|Common
|Rocky ice planet
|[[File:High metal content world Wredguia ZF-F d11-23 1.png|thumb|center]][[File:High metal content world Wredguia ZF-F d11-23 2.png|thumb|center]][[File:High metal content world Wredguia AG-F d11-24 A 1.png|thumb|center]][[File:High metal content world Col 285 Sector KS-T d3-82 7.png|thumb|center]][[File:High metal content world Wredguia HY-G c24-11 A 1.png|thumb|center]][[File:High metal content world Col 285 Sector KS-T d3-82 8.png|thumb|center]]
|White - Grey - Light blue - Light brown 
|Uncommon
|Rocky ice world. Typically formed in the cooler regions of 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.
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|[[Metal-Rich Body]]
High-Metal-Content-Planets-180px.png
|''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.''
</gallery>
|High metal content planet
|Brown - Dark brown - Black - Beige
|Uncommon
|Uncommon
|High metal content 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.
|[[File:Metal-rich body Wredguia QX-K d8-8 A 3.png|thumb|center]][[File:Metal rich.png|thumb|center]]
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|[[Ammonia World]]
Metal_rich.png
|''Terrestrial ammonia world with an active ammonia-based chemistry and carbon-ammonia based life.''
</gallery>
|[[Lava Planet]], Metal rich planet
|Brown - Black (sometime with visible lava)
|Rare
|Rare
|Metal-rich world with a metallic core. Worlds like this can have metallic ores near the surface in places, especially around areas of past volcanism.
|[[File:Ammonia-World-180px.png|thumb|center]]
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|[[Water World]]
Water-World-180px.png
|''Terrestrial water world with an active water-based chemistry and carbon-water-based life.''
water.jpg|Water world
|Uncommon
THAILOAE EM-M D7-2 A 6.png|THAILOAE EM-M D7-2 A 6
|[[File:Water.jpg|thumb|center]][[File:Water world Wredguia ZI-M b36-0 5.png|thumb|center]]
</gallery>
|[[Ocean Planet]], Water world
|Blue with green, brown and white
|very rare
|Terrestrial water world with an active water-based chemistry and carbon-water-based life.
|-
|<gallery type="slideshow" position="center" widths="250">
Earthlike.png
</gallery>
|Earth-like world
|Blue with green, brown and white
|
Extremely rare
|Outdoor world with a human-breathable atmosphere and indigenous life. The atmosphere is far from chemical equilibrium as a result.
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|[[Earth-like world]]
Ammonia-World-180px.png
|''Outdoor world with a human-breathable atmosphere and indigenous life. The atmosphere is far from chemical equilibrium as a result.''
</gallery>
|[[Ammonia Planet]], Ammonia world
|Light brown. Uncommon colours are dark brown or beige
|Very rare
|Terrestrial ammonia world with an active ammonia-based chemistry and carbon-ammonia based life.
|-
|<gallery type="slideshow" position="center" widths="250">
Nonspherical-Planet.png
Non-Spherical-Planet-2.png
Nonspherical-Moon.png
</gallery>
|Nonspherical bodies
|White - Grey - Light blue - Light brown - Yellow
|Rare
|Rare
|These are planets or moons with a nonspherical shape. It's elongated and can resemble a potato.
|[[File:Earth-like World Kyaraben.jpg|thumb|center]]
|}
|}
[[Category:Planets]]
[[Category:Celestials]]


== Water Giants ==
== [[Gas Giant]]s ==
{| class="article-table" border="1" cellpadding="1" cellspacing="1"
{| class="wikitable unsortable" style="text-align:center;" border="1"
|-
!Type
!Description
!Rarity
!Image
!Image
!Rarity
!In game description
|-
|-
|<gallery type="slideshow" position="center" widths="277">
|Class I gas giant
Water_Giant.png
|''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.''
Water Giant 2.png|Water Giant
|Common
</gallery>
|[[File:Class I gas giant Wredguia HY-G c24-12 1.png|thumb|center]][[File:Class I gas giant HIP 53248 AB 4.png|thumb|center]]
|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.
|}
 
== [[Gas Giant|Gas Giants]] ==
{| class="article-table" border="1" cellpadding="1" cellspacing="1"
!Image
!Class
!Rarity 
!In game description
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Class II gas giant
Gas-Giant-Class-I.png
|''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.''
</gallery>
|Uncommon
|I
|[[File:Class II gas giant HIP 53248 AB 1.png|thumb|center]]
|Rare
|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.
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Class III gas giant
Class_II.png
|''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.''
</gallery>
|Common
|II
|[[File:Class III gas giant HIP 99152 1 a.png|thumb|center]][[File:Class III gas giant 35 Ursae Majoris 1.png|thumb|center]]
|Very 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.
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Class IV gas giant
Gas-Giant-Class-III-180px.png
|''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 the brighter colours. The temperature of their upper cloud layers is typically above 900 K.''
20170221073152_1.jpg
</gallery>
|III
|Rare
|Rare
|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.
<small>(Common in systems with stars of class A or higher)</small>
|[[File:Gas-Giant-Class-IV-180px.png|thumb|center]]
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Class V gas giant
Gas-Giant-Class-IV-180px.png
|''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.''
</gallery>
|IV
|Rare
|Rare
|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.
<small>(Common in systems with stars of class A or higher)</small>
|[[File:Gas Giant Class V.png|thumb|center]]
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Helium-rich
Gas Giant Class V.png
|''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.''
</gallery>
|V
|Very Rare
|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.
|[[File:Helium-rich Gas Giant 2.jpg|thumb|center]]
|-
|Helium gas giant
|''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.''
|Extremely Rare
(Report discoveries to explorer groups)
|[[File:Helium-rich Gas Giant.png|thumb|center]]
|-
|Gas giant with ammonia-based life
|''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 a small quantity of liquid ammonia, extracting their energy from the intense radiation flux.''
|Uncommon
|[[File:Gas giant with ammonia-based life Wredguia EP-K b37-0 3.png|thumb|center]]
|-
|Gas giant with water-based life
|''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 a small quantity of liquid water, extracting their energy from the intense radiation flux.''
|Uncommon
|[[File:Gas giant with water-based life Wredguia EP-K b37-0 4.png|thumb|center]]
|-
|Water Giant
|''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.''
|Rare
|[[File:Water Giant.png|thumb|center]]
|}
 
== Features ==
{| class="wikitable unsortable" style="text-align:center;" border="1"
|-
!Type
!Description
!Rarity
!Image
|-
|Dwarf planet
|''A dwarf planet orbits a [[Stars|star]] and has sufficient mass and [[gravity]] for a round shape, but it does not clear its orbital neighborhood of debris. Their orbital path is shared with other space objects and rocks. Dwarf planets are very common in the galaxy. Examples of dwarf planets in [[Sol]]: [[Haumea]], [[Makemake]], [[Persephone]], [[Pluto]], [[Salacia]], [[Sedna]].''
|Common
|[[File:Makemake.jpg|thumb|center]]
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|[[Atmosphere|Tenuous atmosphere]]
Helium-rich_Gas_Giant_2.jpg
|''Planets with tenuous atmospheres have surface pressures well below Earth, ranging from thin exospheres (where gases rarely collide) to denser, transient envelopes. Tenuous atmospheres are common for rocky and icy bodies, because they are a natural equilibrium between atmospheric generation and atmospheric loss.''
Helium-rich_Gas_Giant.png
|Common
</gallery>
|[[File:Water Atmosphere ED 1.jpg|thumb|center]]
|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.
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Thick fog effect
Gas_giant_with_ammonia_based_life.png
|''Rocky bodies can have a thick fog effect that covers the surface.''<ref name=":0">[https://www.reddit.com/r/EliteDangerous/comments/1wv39j2/the_fogsuper_atmosphere_mystery_of_hip_87621/ The FOG/super atmosphere mystery of HIP 87621 solved!] -SeawolvesTV - 4 Dec 2020 - Reddit</ref> ''For example "[[HIP 87621]] 2 B B" has around 400 meter high, thick fog.''<ref name=":0" /><ref>[https://inara.cz/elite/starsystem-bodies/4414405/ HIP 87621] - Star System - INARA</ref> This effect is caused by flying inside the eclipse zone of a rocky body with a water atmosphere.<ref name=":1">[https://www.youtube.com/watch?v=Mtm03vCjH1s The FOG/super atmosphere mystery of HIP 87621 solved!] - VRFlorian - 2 October 2026</ref> ''The fog is an aerosol made of tiny liquid water droplets or ice crystals in the air.'' ''These conditions are rare.''<ref name=":0" />
</gallery>
|Rare
|[[Gas Giant]] with ammonia-based life
|[[File:Thick Fog HIP 87621 2 B B.jpg|thumb|center]]
|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.
|-
|-
|<gallery type="slideshow" position="center" widths="250">
|Tidally locked
Gas_Giant_Water_Based_Life.png
|''Tidally locked planets have a matching rotation period with the host star. One hemisphere has perpetual daylight while the other has only night. The [[Moon]] is also tidally locked to [[Earth]].''
Water_based_life_gas_giant.png
|Rare
gas_giant_water_based.jpg|Gas giant, water based
|[[File:Tidally Locked Earth-like World.jpg|thumb|center]]
</gallery>
|[[Gas Giant]] with water-based life
|Very 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.
|}
|}


== Videos ==
==Videos==
<gallery>
<gallery>
File:Elite_dangerous_1._Planets_a._Gas_giants
File:Elite Dangerous Odyssey - Planetary tech 6.0
File:Elite_Dangerous_1._Planets_b._Volcanic
File:Elite Dangerous - Timelapse - Planet Rising 3
File:Elite_Dangerous_1._Planets_c._Class_M
File:Elite Dangerous- Odyssey - Exploration Montage - Episode 7
File:Elite_Dangerous_1._Planets_d._Rings
File:Elite Dangerous - Relax in Space 1 Ambient Music Deep Relaxation & Meditation & Sleep & Chill Out
File:Elite_Dangerous_1._Planets_e._Others
File:4 HOURS of Spaceflight with AMBIENT MUSIC in ELITE DANGEROUS
File:A new BLUE FOG mystery on HIP 87621?! Something very unusual happened here...
File:The Blue Phenomenon - Dense Planetary Atmosphere - Elite Dangerous Odyssey
</gallery>
</gallery>


== References ==
==References==
<references />
<references/>
 


[[ru:Планеты]]
[[zh:Planets]]
[[Category:Planets]]
[[Category:Planets]]
[[Category:Celestials]]
[[Category:Celestials]]
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[[Category:Guides]]
[[Category:Guides]]