Editing 2908: Moon Armor Index

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==Explanation==
 
==Explanation==
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{{incomplete|Created by a MARS ROVER THAT GREW 2 INCHES OVERNIGHT - Please change this comment when editing this page. Do NOT delete this tag too soon.}}
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In this “What If?”-style comic, [[Randall]] hypothesizes an imaginative situation in which each planet's moon(s) become converted into protective armor (as a form of {{w|Overburden#Analogous uses|overburden}}) to coat the respective planet. For example, the {{w|Moon}} would coat {{w|Earth}} in a 43 kilometer layer if it were molded into protective armor, almost five times the height of {{w|Mount Everest}}.  
 
In this “What If?”-style comic, [[Randall]] hypothesizes an imaginative situation in which each planet's moon(s) become converted into protective armor (as a form of {{w|Overburden#Analogous uses|overburden}}) to coat the respective planet. For example, the {{w|Moon}} would coat {{w|Earth}} in a 43 kilometer layer if it were molded into protective armor, almost five times the height of {{w|Mount Everest}}.  
  
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{| class="wikitable"
 
{| class="wikitable"
 
|-
 
|-
! Planet/<br>dwarf planet !! Surface area (km²) || Moons || Total volume (km³) || Moon shield thickness
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! Planet/<br>dwarf planet !! Surface area (km²) || Moons || Total volume (km³) || Moon shield thickness <!-- please add more info -->
 
|-
 
|-
| {{w|Earth}} || 5.1007×10^8 || {{w|Moon|1}} || 2.196×10^10 || 43&nbsp;km (27&nbsp;mi) (4.86 × height of {{w|Mount Everest}})
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| {{w|Earth}} || 5.1007*10^8 || {{w|Moon|1}} || 2.196*10^10 || 43&nbsp;km (27&nbsp;mi)
 
|-
 
|-
| {{w|Mars}} || 1.4437×10^8 || {{w|Moons of Mars|2}} || {{w|Phobos (moon)|(5695±32)}}+{{w|Deimos (moon)|(1033±19)}} || 5&nbsp;cm (2&nbsp;in)
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| {{w|Mars}} || 1.4437*10^8 || {{w|Moons of Mars|2}} || {{w|Phobos (moon)|(5695±32)}}+{{w|Deimos (moon)|(1033±19)}} || 5&nbsp;cm (2&nbsp;in)
 
|-
 
|-
| {{w|Jupiter}} || 6.1469×10^10 || {{w|Moons of Jupiter|95}} || 1.7646×10^11 || 2.87&nbsp;km (1.78&nbsp;mi)
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| {{w|Jupiter}} || 6.1469*10^10 || {{w|Moons of Jupiter|95}} || 1.7646*10^11 || 2.87&nbsp;km (1.78&nbsp;mi)
 
|-
 
|-
| {{w|Saturn}} || 4.27×10^10 || {{w|Moons of Saturn|146}} || 7.651×10^10 || 1.79&nbsp;km (1.11&nbsp;mi)
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| {{w|Saturn}} || 4.27*10^10 || {{w|Moons of Saturn|146}} || 7.651*10^10 || 1.79&nbsp;km (1.11&nbsp;mi)
 
|-
 
|-
| {{w|Uranus}} || 8.1156×10^9 || {{w|Moons of Uranus|28}} || 5.61×10^9 || 0.69 km (0.43 mi)
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| {{w|Uranus}} || 8.1156*10^9 || {{w|Moons of Uranus|28}} || ||  
 
|-
 
|-
| {{w|Neptune}} || 7.6187×10^9 || {{w|Moons of Neptune|16}} || 1.04×10^10 || 1.36 km (0.84 mi)
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| {{w|Neptune}} || 7.6187*10^9 || {{w|Moons of Neptune|16}} || ||  
 
|-
 
|-
| {{w|Pluto}} || 1.7744×10^7 || {{w|Moons of Pluto|5}} || {{w|Charon (moon)|(9.322×10^8)}}+{{w|Moons of Pluto|(approx 87100+38800+900+200)}} || 52.5&nbsp;km (32.6&nbsp;mi) (by this comic's approximation)
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| {{w|Pluto}} || 1.7744*10^7 || {{w|Moons of Pluto|5}} || {{w|Charon (moon)|(9.322×10^8)}}+{{w|Moons of Pluto|(approx 87100+38800+900+200)}} || 52.5&nbsp;km (32.6&nbsp;mi) (by this comic's approximation)
 
50.4&nbsp;km (31.3&nbsp;mi) (by full calculation)
 
50.4&nbsp;km (31.3&nbsp;mi) (by full calculation)
 
|-
 
|-
| {{w|120347 Salacia|Salacia}} || 2.27×10^6 || {{w|Actaea (moon)|1}} || 1.41×10^7 || 6.21&nbsp;km (3.85&nbsp;mi)
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| {{w|120347 Salacia|Salacia}} || 2.27*10^6 || {{w|Actaea (moon)|1}} || 1.41*10^7 || 6.21&nbsp;km (3.85&nbsp;mi)
 
|-
 
|-
| {{w|Haumea}} || 8.14×10^6 || {{w|Moons of Haumea|2}} || {{w|Hiʻiaka (moon)|(17.2×10^6)}}+{{w|Namaka (moon)|(2.57×10^6)}} || 2.43&nbsp;km (1.51&nbsp;mi)
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| {{w|Haumea}} || 8.14*10^6 || {{w|Moons of Haumea|2}} || {{w|Hiʻiaka (moon)
 +
|(17.2*10^6)}}+{{w|Namaka (moon)|(2.57*10^6)}} || 2.43&nbsp;km (1.51&nbsp;mi)
 
|-
 
|-
| {{w|50000 Quaoar|Quaoar}} || 3.78×10^6 || {{w|Weywot|1}} || 4.19×10^6 || 1.11&nbsp;km (0.69&nbsp;mi)
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| {{w|50000 Quaoar|Quaoar}} || 3.78*10^6 || {{w|Weywot|1}} || 4.19*10^6 || 1.11&nbsp;km (0.69&nbsp;mi)
 
|-
 
|-
| {{w|225088 Gonggong|Gonggong}} || 4.75×10^6 || {{w|Xiangliu (moon)|1}} || 1.44×10^6 || 0.3 km (0.19 mi)
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| {{w|225088 Gonggong|Gonggong}} || || {{w|Xiangliu (moon)|1}} || ||  
 
|-
 
|-
| {{w|Eris (dwarf planet)|Eris}} || (1.70±0.02)×10^7 || {{w|Dysnomia (moon)|1}} || 1.61×10^8 || 9.47 km (5.88 mi)
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| {{w|Eris (dwarf planet)|Eris}} || (1.70±0.02)*10^7 || {{w|Dysnomia (moon)|1}} || ||  
 
|}
 
|}
  
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This process described above assumes that all objects involved are completely spherical, which may not be the case. The act of tearing apart a solid moon, perhaps into rough gravel, might add microvoids to the new layering that bulk up the volume slightly. But neither are gravitational compression effects taken into account on an originally loose material; the planet's gravitational pull could settle some of the moon material into a slightly smaller volume than the one it occupied as lower-gravity moon.
 
This process described above assumes that all objects involved are completely spherical, which may not be the case. The act of tearing apart a solid moon, perhaps into rough gravel, might add microvoids to the new layering that bulk up the volume slightly. But neither are gravitational compression effects taken into account on an originally loose material; the planet's gravitational pull could settle some of the moon material into a slightly smaller volume than the one it occupied as lower-gravity moon.
  
The planet below could also be marginally affected by the change in its total planet-and-armor mass, for rocky planets mostly within any {{w|pedosphere}} or previously exposed outer {{w|lithosphere}}. The interaction with {{w|Titan (moon)#Lakes|surface liquids}} and atmospheres, especially in planets defined {{w|Gas giant|primarily by their gas layers}}, would depend much upon how impermeable and/or rigid the chosen layering method made the additional material. One could imagine a spherical shell of moon matter around Jupiter with such high structural strength as to resist crumbling into its gaseous maw. Alternatively, the moon material could be expected to sink towards the gaseous planet's center until it reaches a layer sufficiently dense and/or rigid to stop it sinking further. In this case the moon material would displace a volume of the planet's gas causing an increase in the planet's radius.
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The planet below could also be marginally affected by the change in its total planet-and-armor mass, for rocky planets mostly within any {{w|pedosphere}} or previously exposed outer {{w|lithosphere}}. The interaction with {{w|Titan (moon)#Lakes|surface liquids}} and atmospheres, especially in planets defined {{w|Gas giant|primarily by their gas layers}}, would depend much upon how impermeable and/or rigid the chosen layering method made the additional material. One could imagine a spherical shell of moon matter around Jupiter with such high structural strength as to resist crumbling into its gaseous maw.
  
 
==Transcript==
 
==Transcript==

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