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blog:20180520_carbonaceous [2018/05/20 11:45] samblog:20180520_carbonaceous [2018/05/20 11:50] (current) sam
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 There's also a modifier that smooths out larger asteroids, so Ceres sized asteroids will tend to be far more spherical than smaller ones. There's also a modifier that smooths out larger asteroids, so Ceres sized asteroids will tend to be far more spherical than smaller ones.
  
-The textual descriptions of such worlds needs some work, and there's still lots of bugs in how moons get displayed on the web page, but there is progress.+The textual descriptions of such worlds needs some work (to be honest, there's not a lot that can be said about a small barren rock, so coming up with enough unique random text to make them interesting is hard), and there's still lots of bugs in how moons get displayed on the web page, but there is progress.
  
 I've also possibly decided on nomenclature for belts, giving them capital letters to denote their position. The first (innermost) belt in the system will be A, the second B etc. Named planetoids within the belt will be labelled from innermost to outermost, starting at 'a' and going onwards. This matches the naming for moons, but they have a roman numeral (for the planet) followed by a letter (e.g. our Moon would be "Sol IIIa"), which is clearer. So I might still change things. I've also possibly decided on nomenclature for belts, giving them capital letters to denote their position. The first (innermost) belt in the system will be A, the second B etc. Named planetoids within the belt will be labelled from innermost to outermost, starting at 'a' and going onwards. This matches the naming for moons, but they have a roman numeral (for the planet) followed by a letter (e.g. our Moon would be "Sol IIIa"), which is clearer. So I might still change things.
blog/20180520_carbonaceous.1526816741.txt.gz · Last modified: 2018/05/20 11:45 by sam