PIA16363: Twin Craters: Holberg & Spitteler
 Target Name:  Mercury
 Is a satellite of:  Sol (our sun)
 Mission:  MESSENGER
 Spacecraft:  MESSENGER
 Instrument:  MDIS - Narrow Angle
 Product Size:  1269 x 1271 pixels (w x h)
 Produced By:  Johns Hopkins University/APL
 Full-Res TIFF:  PIA16363.tif (1.615 MB)
 Full-Res JPEG:  PIA16363.jpg (187.6 kB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

This NAC image features named craters Holberg and Spitteler. The craters are similar in diameters (about 61 km and 62 km respectively) and both have central peaks. The craters are nearly identical in structure but were formed by separate impacts. Holberg's more degraded appearance and higher density of superposed craters indicate that it is older than Spitteler. The slump in Holberg's wall closest to Spitteler may have been created during the Spitteler impact event.

This image was acquired as part of MDIS's high-incidence-angle base map. The high-incidence-angle base map is a major mapping activity in MESSENGER's extended mission and complements the surface morphology base map of MESSENGER's primary mission that was acquired under generally more moderate incidence angles. High incidence angles, achieved when the Sun is near the horizon, result in long shadows that accentuate the small-scale topography of geologic features. The high-incidence-angle base map is being acquired with an average resolution of 200 meters/pixel.

Date acquired: April 29, 2012
Image Mission Elapsed Time (MET): 244177131
Image ID: 1730233
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: -68.66
Center Longitude: 297.0 E
Resolution: 185 meters/pixel
Scale: Holberg, the more northern complex crater, is approximately 61 km (38 miles) in diameter.
Incidence Angle: 83.8
Emission Angle: 0.7
Phase Angle: 84.4

The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MDIS acquired 88,746 images and extensive other data sets. MESSENGER is now in a year-long extended mission, during which plans call for the acquisition of more than 80,000 additional images to support MESSENGER's science goals.

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

Image Addition Date: