Puerta del sistema exterior
This section gathers craters beyond the five primary worlds: icy moons, dwarf planets, and small bodies where impact geology becomes especially varied.
Estructura
Así la navegación principal sigue limpia, pero el investigador entra rápido a las lunas de Júpiter o Saturno.
Método Crater.world
Reconstrucción inversa, inversión cronológica, análisis bidireccional y el presente como archivo del futuro pasan a ser la regla visual.
Fichas iniciales
Vista visualPaleta: icy turquoise, deep space, and distant moonsA giant multi-ring impact structure on Callisto whose scale makes it one of the anchor objects of the outer catalog.
Vista visualPaleta: icy turquoise, deep space, and distant moonsA Europa crater with bright ejecta that helps read impact processes in the icy shell of an ocean-world candidate.
Vista visualPaleta: icy turquoise, deep space, and distant moonsA large southern-latitude crater on Ganymede, useful for comparing impact forms on the Solar System's largest moon.
Vista visualPaleta: icy turquoise, deep space, and distant moonsA giant crater on Saturn's moon Mimas, so large it nearly defines the small world's appearance.
Vista visualPaleta: icy turquoise, deep space, and distant moonsOne of Tethys's largest craters, comparable in scale to the visual identity of the moon itself.
Vista visualPaleta: icy turquoise, deep space, and distant moonsA large crater on Iapetus, interesting against the moon's strong contrast between bright and dark terrains.
