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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)
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|(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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The usual means of comparing a moon to a planet might be to compare the volume of both. This comic compares moon volume (kilometers cubed) to planet surface area (kilometers squared); specifically, the index derives a ''linear'' indicator (the thickness of the new material) by dividing the ''area'' of the main body (proportional to the square of its uncounted radius) into the ''combined volume'' of all other bodies (proportioned cubes of their own radii), which gives an unusual dimensional analysis (dividing X kilometers-cubed by Y kilometers-squared gives a length, Z, in kilometers, not a simple dimensionless ratio).
 
The usual means of comparing a moon to a planet might be to compare the volume of both. This comic compares moon volume (kilometers cubed) to planet surface area (kilometers squared); specifically, the index derives a ''linear'' indicator (the thickness of the new material) by dividing the ''area'' of the main body (proportional to the square of its uncounted radius) into the ''combined volume'' of all other bodies (proportioned cubes of their own radii), which gives an unusual dimensional analysis (dividing X kilometers-cubed by Y kilometers-squared gives a length, Z, in kilometers, not a simple dimensionless ratio).
  
This particular methodology makes the Pluto-Charon system (Charon being roughly half the diameter and one-eighth the volume of Pluto, before even adding that of the other moons) surprisingly similar to the Earth-Moon one (our sole Moon is around one-quarter Earth's diameter, and therefore less than 2% its volume; also in comparison, the Earth and Moon are respectively slightly more than 150 times and around 3 times the volume of Pluto), but leaves them ''both'' as still standing out significantly against all other planetary comparisons, even against comparably-sized 'planet's.
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This particular methodology makes the Pluto-Charon system (Charon being roughly half the diameter and one-eighth the volume of Pluto, before even adding that of the other moons) surprisingly similar to the Earth-Moon one (our sole Moon is around one-quarter Earth's diameter, and therefore less than 2% its volume; also in comparison, the Earth and Moon are respectively slightly more than 150 times and around 3 times the volume of Pluto), but leaves them ''both'' as still standing out significantly against all other planetary comparisons.
  
 
===The complexities of armor thickness calculations===
 
===The complexities of armor thickness calculations===
The comic uses the ≈ sign to show that the formula is only an approximation: it does not take account the increase in armor surface area as it gets thicker. This approximation would be perfect for a shield of thickness zero, but for the thickest shield (Pluto) around a small celestial body the error is around 4% (52.5&nbsp;km by this approximation, but 50.4&nbsp;km by more thorough calculation). To find the correct value, we can use the formula for the volume of a sphere, V = 4/3 * pi * (where V is the volume and r is the radius). Using this formula, we can find and add together the volumes of each moon, as well as the volume of the planet, to get a total volume of the new shielded planet. Then we can find its radius using the formula r = (V / (4/3 * pi))<sup>⅓</sup>, derived from the previous formula. Subtracting the radius of the previous planet from the radius of the new planet gives us the thickness of the armor.
+
The comic uses the ≈ sign to show that the formula is only an approximation: it does not take account the increase in armor surface area as it gets thicker. This approximation would be perfect for a shield of thickness zero, but for the thickest shield (Pluto) around a small celestial body the error is around 4% (52.5&nbsp;km by this approximation, but 50.4&nbsp;km by more thorough calculation). To find the correct value, we can use the formula for the volume of a sphere, V = 4/3 * pi * r^3 (where V is the volume and r is the radius). Using this formula, we can find and add together the volumes of each moon, as well as the volume of the planet, to get a total volume of the new shielded planet. Then we can find its radius using the formula r = (V / (4/3 * pi))^1/3, derived from the previous formula. Subtracting the radius of the previous planet from the radius of the new planet gives us the thickness of the armor.
  
 
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.
+
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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