Ius and Tithonium Chasmata in 3D

This stereoscopic image shows Ius and Tithonium Chasmata, which form part of Mars’ Valles Marineris canyon structure. It was generated from data captured by the High Resolution Stereo Camera (HRSC) on ESA’s Mars Express on 21 April 2022 during orbit 23123. The anaglyph, derived from data acquired by the nadir channel and one stereo channel of the HRSC, offers a three-dimensional view when viewed using red-green or red-blue glasses.

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