PIA10397: "The Spider" - Radial Troughs within Caloris
Target Name: Mercury
Is a satellite of: Sol (our sun)
Spacecraft: MESSENGER
Instrument: MDIS - Narrow Angle
Product Size: 3000 x 2025 pixels (width x height)
Produced By: Johns Hopkins University/APL
Full-Res TIFF: PIA10397.tif (6.083 MB)
Full-Res JPEG: PIA10397.jpg (755.3 kB)

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The Narrow Angle Camera of the Mercury Dual Imaging System (MDIS) on the MESSENGER spacecraft obtained high-resolution images of the floor of the Caloris basin on January 14, 2008. Near the center of the basin, an area unseen by Mariner 10, this remarkable feature—nicknamed "the spider" by the science team—was revealed. A set of troughs radiates outward in a geometry unlike anything seen by Mariner 10. The radial troughs are interpreted to be the result of extension (breaking apart) of the floor materials that filled the Caloris basin after its formation. Other troughs near the center form a polygonal pattern. This type of polygonal pattern of troughs is also seen along the interior margin of the Caloris basin. An impact crater about 40 km (~25 miles) in diameter appears to be centered on "the spider." The straight-line segments of the crater walls may have been influenced by preexisting extensional troughs, but some of the troughs may have formed at the time that the crater was excavated.

These images are from MESSENGER, a NASA Discovery mission to conduct the first orbital study of the innermost planet, Mercury. For information regarding the use of images, see the MESSENGER image use policy.

Image Credit:
NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

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