My model database eventually consisted of Mercury through Pluto and those moons larger than 50 km or so or otherwise noteworthy. The latter
included Deimos and Phobos for Mars, ten moons for Jupiter, sixteen for Saturn (five
embedded in the outer parts of the rings), nine for Uranus, six for Neptune, and
three for Pluto (namely Charon, Nix, and Hydra). While I judged Jupiter’s rings to be
too faint to be worth attempting to show, I exaggerated Uranus’s and
Neptune’s slightly for visibility.
Venus’s atmosphere is such a superb thermal conductor that its day and
night temperatures are identical and largely unaffected even by latitude. At
460° C (860° F) the ground is hot enough to glow a dull red so I
exaggerated that somewhat to show up on the night side (which in reality you
wouldn’t actually be able to see through the cloud cover).
Texture map data
for all of these bodies comes from widely available government sources, primarily
NASA and JPL. On Pluto and Charon the gross color areas are genuine and derive from
Hubble data; their finer details come from swatches I skimmed from asteroid photos.
Greater fidelity for Pluto and its attendants will depend on the New
Horizons flyby in 2015.
Animations and stills © 2010 Peter Blinn