Differences

This shows you the differences between two versions of the page.

--- worldgen:pcl [2019/07/28 17:14] – sam
+++ worldgen:pcl [2020/05/27 19:43] – [References] sam
@@ Line 18: / Line 18: @@
 [[/worldgen/pcl/small_body_group|{{:worldgen:sm_small_body.jpg?nolink&100 |}}]]
 **[[./pcl/Small Body Group]]** \\
-Includes small planetoids such as asteroids or coments, generally not more than 10s of kilometres in diameter. \\
+Includes small planetoids such as asteroids or coments, generally not more than 10s of kilometres in diameter.
-\\
+~~~~
-\\
 [[/worldgen/pcl/dwarf_terrestrial_group|{{:worldgen:sm_dwarf_terrestrial.jpg?nolink&100 |}}]]
 **[[./pcl/Dwarf Terrestrial Group]]** \\
-Small rocky dwarf planets with a mass up to 0.15 of that of Earth. They are generally spherical and may have a trace atmosphere.\\
+Small rocky dwarf planets with a mass up to 0.15 of that of Earth. They are generally spherical and may have a trace atmosphere.
-\\
+~~~~
-\\
 [[/worldgen/pcl/terrestrial_group|{{:worldgen:sm_terrestrial.jpg?nolink&100 |}}]]
 **[[./pcl/Terrestrial Group]]** \\
-Rocky worlds generally from 0.02 to 5.0 Earth masses. They may have geological activity (or had it in the past) and may have a substantial atmosphere.\\
+Rocky worlds generally from 0.02 to 5.0 Earth masses. They may have geological activity (or had it in the past) and may have a substantial atmosphere.
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+~~~~
-\\
 [[/worldgen/pcl/helian_group|{{:worldgen:sm_helian.jpg?nolink&100 |}}]]
 **[[./pcl/Helian Group]]** \\
-These are rocky worlds from 3 to 17 Earth masses, also known as super-Earths. They may have dense atmospheres or thick planet-wide liquid oceans, and bridge the divide between rocky and gas worlds. \\
+These are rocky worlds from 3 to 17 Earth masses, also known as super-Earths. They may have dense atmospheres or thick planet-wide liquid oceans, and bridge the divide between rocky and gas worlds.
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+~~~~
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 [[/worldgen/pcl/jovian_group|{{:worldgen:sm_jovian.jpg?nolink&100 |}}]]
 **[[./pcl/Jovian Group]]** \\
-Range in mass from 10 to 4,000 times the mass of the Earth, up to 13 times the mass of Jupiter. They have rocky or icy cores, and a thick atmosphere generally of hydrogen or helium.\\
+Range in mass from 10 to 4,000 times the mass of the Earth, up to 13 times the mass of Jupiter. They have rocky or icy cores, and a thick atmosphere generally of hydrogen or helium.
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+~~~~
-\\
 [[/worldgen/pcl/planemo_group|{{:worldgen:sm_planemo.jpg?nolink&100 |}}]]
 **[[./pcl/Planemo Group]]** \\
-Planetary mass objects which are not bound to a star. Also known as //rogue planets//. They have have formed by themselves out in the depths of space, or have been ejected from an existing system.\\
+Planetary mass objects which are not bound to a star. Also known as //rogue planets//. They have have formed by themselves out in the depths of space, or have been ejected from an existing system.
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+~~~~
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 [[/worldgen/pcl/construct_group|{{:worldgen:sm_construct.jpg?nolink&100 |}}]]
 **[[./pcl/Construct Group]]** \\
-Artificially constructed objects of planetary scale or larger, from orbitals thousands of kilometres across to //Dyson Swarms// or //Matrioshka Brains//.\\
+Artificially constructed objects of planetary scale or larger, from orbitals thousands of kilometres across to //Dyson Swarms// or //Matrioshka Brains//.
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+~~~~
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@@ Line 65: / Line 57: @@
 This list is based on work done by //John Dollan//, and his far more complete version is at the [[http://arcbuilder.home.bresnan.net/PCLMaster.html|ArcBuilder Site]]. The original list, plus later versions, seem to have vanished from the web. There seems to be a partial copy available at [[https://archive.is/Okmio]].
-There is also a version adapted for the //Eclipse Phase// RPG available [[https://mephitjamesblog.files.wordpress.com/2016/04/astrometrics-a-gms-guide-to-exoplanets1.pdf|as PDF]] by James Mephit.
+There is also a version adapted for the //Eclipse Phase// RPG available [[https://mephitjamesblog.files.wordpress.com/2016/04/astrometrics-a-gms-guide-to-exoplanets1.pdf|as PDF]] by [https://mephitjamesblog.wordpress.com/2016/04/19/exoplanets/|James Mephit]].
 This version is based on a combination of these resources, plus some further modifications.