PIA16777: Big Things Have Small Beginnings
 Target Name:  Mercury
 Is a satellite of:  Sol (our sun)
 Mission:  MESSENGER
 Spacecraft:  MESSENGER
 Instrument:  MDIS - Narrow Angle
 Product Size:  1024 x 1024 pixels (w x h)
 Produced By:  Johns Hopkins University/APL
 Full-Res TIFF:  PIA16777.tif (1.05 MB)
 Full-Res JPEG:  PIA16777.jpg (121.1 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:

The surface of Mercury has been extensively deformed by tectonic activity, with most of that activity due to the global-scale contraction of the planet as its interior cooled. This tectonic deformation is largely manifest as contractional lobate scarps, many of which are hundreds or even thousands of meters high. This image shows a scarp only ~150 m (500 ft.) high, considerably smaller than many of its peers across the planet. This structure's relatively small size suggests either that it accommodated but a relatively small amount of deformation over its lifetime, or that it is one of the youngest lobate scarps on Mercury.

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: April 04, 2012
Image Mission Elapsed Time (MET): 234154717
Image ID: 1222306
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 29.31
Center Longitude: 91.01 E
Resolution: 46 meters/pixel
Scale: The crater to the top right is ~18 km (11 mi.) in diameter
Incidence Angle: 51.6
Emission Angle: 14.5
Phase Angle: 38.1
North is to the bottom-right corner of this image

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.

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: