As the youngest large impact basin known on Mercury, the Caloris basin has
landforms that are better preserved than in older basins, which have been
more modified by impact cratering. This figure, recently published in
Science magazine, shows a map of many linear features within Caloris basin
that formed when the near-surface rocks were subjected to large horizontal
forces. The Caloris basin contains hundreds of extensional troughs, mapped
as black lines, where the surface has been pulled apart and faulted.
Pantheon Fossae (located inside the white box of the top map and shown in
detail in the bottom image) has over 200 such troughs in a radiating
pattern, but near the outer edges of the basin interior troughs are seen
in patterns broadly concentric to Caloris basin (see PIA10606). The Caloris
basin interior also has been deformed by many wrinkle ridges, mapped as
red lines, formed when the surface was compressed or shortened
horizontally. Relationships between the extensional troughs and
contractional wrinkle ridges provide information about the evolution of
the Caloris basin and Mercury's interior.
Date Acquired: January 14, 2008
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging
System (MDIS)
Scale: Caloris basin is about 1550 kilometers (about 960 miles) in
diameter. The crater Apollodorus near the center of Pantheon Fossae is 41
kilometers (25 miles) in diameter.
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.