Geology of solar terrestrial planets

The inner planets. From left to right: Mercury, Venus, Earth, Mars and terrestrial dwarf planet, Ceres (sizes to scale)

Artist's conception of a protoplanetary disk

Mercury’s Caloris Basin is one of the largest impact features in the Solar System.

The so-called “Weird Terrain” was formed by the Caloris Basin impact at its antipodal point.

The geology of solar terrestrial planets mainly deals with the geological aspects of the four terrestrial planets of the Solar System, Mercury, Venus, Earth, and Mars, and one terrestrial dwarf planet, Ceres. Only one terrestrial planet, Earth, is known to have an active hydrosphere.

单词	Lobate scarp
释义	Lobate scarp 英语百科 Geology of solar terrestrial planets The geology of solar terrestrial planets mainly deals with the geological aspects of the four terrestrial planets of the Solar System, Mercury, Venus, Earth, and Mars, and one terrestrial dwarf planet, Ceres. Only one terrestrial planet, Earth, is known to have an active hydrosphere.
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Lobate scarp

Geology of solar terrestrial planets