Dominici Crater

In this dramatic image, Dominici crater takes center-stage. Dominici is 20 km (12 mi.) in diameter, and hosts a variety of landforms including a sharp crater rim, internal slumps, and abundant hollows. Dominici is also a rayed crater, which, together with its well-preserved rim, indicate that the crater is relatively young. This scene, taken from an oblique angle, gives us a good idea of what the surface of Mercury might look like from a spacecraft window as we zoom overhead!

This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are imaged in this mode each week.

Date acquired: January 30, 2014
Image Mission Elapsed Time (MET): 33401837
Image ID: 5668405
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 1.1° N
Center Longitude: 323.5° E
Resolution: 79 meters/pixel
Scale: The crater in the image center is 20 km (about 12 mi.) across
Incidence Angle: 36.2°
Emission Angle: 41.8°
Phase Angle: 77.4°
North is to the bottom in this image

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington