When Mars Express set sail for（开船，动身） the crater¹（火山口，弹坑） named after Portuguese² navigator Ferdinand Magellan, it found a windblown（被风吹的） plateau and mysterious rocky mounds³ nearby. Stretching across 190 x 112 km, this region of Mars covers an area of about 21 280 sq km, which is roughly the size of Slovenia. It is located to the southwest of the volcanic⁴ region Tharsis on the southern highlands of Mars, near the crater Magellan.

Named after the famous Portuguese navigator and explorer Ferdinand Magellan, the impact crater is about 100 km across. Only a small portion of the crater rim⁵（火山口边缘） is visible in this image, sitting at the lower right, because the Mars Express High-Resolution Stereo Camera (HRSC) has zeroed in on some intriguing⁶（有趣的，迷人的） features nearby.

In the west of this region (at the upper edge of the main image) there are light-coloured, irregular protrusions（突出） . These features are up to 2 km tall and are probably large rock fragments or mounds（堆，高地） of rock. However, their formation is still debated.

One possibility is that the top layer of rock was shattered（打碎，削弱） by the shockwaves from an impact. Another possible explanation would be from a process called subrosion. On Mars, subrosion is widely observed when rising magma（岩浆，糊剂） heats frozen ground water, which melts and removes subsurface material as it flows away. This leads to a honeycomb of cavities that eventually collapse⁷ due to the weight of the overlying rock layers, leaving the irregular mounds standing⁸.

The northern part of the region (to the right of the main image) displays linear（线型的，直线的） features with a preferential（优先的） northwest–southeast orientation⁹. These eventually lead to deep, well-defined valleys and are likely to be faults, formed during either an impact event or the upsurge（高潮，高涨） of the Tharsis region that created enormous stresses in the planet's crust（外壳） . Examining the geometry（几何学） of fault zones offers clues to the level and the direction of the stress exerted（外露的） on the rock.

A rather smooth, barely fractured plateau is located almost in the centre of the main image. It is possible the plateau is made up of the same material as the highly fractured（断裂的，挫伤的） mounds in the west. Fine trails run from southwest to northeast across here. These could be an indication of erosion（侵蚀，腐蚀） by fine dust particles carried on the wind, sandblasting（喷砂） the plateau smooth.

With a ground resolution（分辨率） of about 25 m per pixel, the data were acquired for the region of Magellan Crater at about 34°S/185°E, during Mars Express's orbit 6547 on 6 February 2009.