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The movie follows Angkor Vallis into the large crater Kofi (136 km diameter, centered at 56.74°N, 118.08°E), which has been flooded with lava.

The second part of the movie illustrates the remarkable range in elemental abundances displayed by the volcanic deposits that make up Mercury’s surface.

This image provides a perspective view of the central portion of Carnegie Rupes, a large tectonic landform that cuts through Duccio crater (133 km diameter, centered at 58.19°N, 307.6°E; north is to the left).

The image shows topographic heights as measured by the Mercury Laser Altimeter and surface features mapped by the Mercury Dual Imaging System.

The first frame shows an Earth-based Arecibo radar image in red overlaid on a mosaic of MESSENGER’s Mercury Dual Imaging System images, enabling for the first time the identification of the host craters for all of the radar-bright deposits.

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Tectonic landforms such as Carnegie Rupes formed by horizontal shortening in response to cooling and contraction of the planetary interior.The formation of hollows remains an active area of research, but the etched nature of the features, such as in this image, suggests that material is being lost from the surface to create the hollows.Volcanism has played a critical role in shaping Mercury’s surface.Observations by MESSENGER’s Magnetometer showed that Mercury’s magnetic field is offset along the planetary spin axis by about 20% of the planet’s radius.The internal magnetic field is 100 times weaker than that of Earth and barely stands off the solar wind at the subsolar point to form the magnetosphere.