PIA19409: A Detailed Look at Raditladi Basin
 Target Name:  Mercury
 Is a satellite of:  Sol (our sun)
 Mission:  MESSENGER
 Spacecraft:  MESSENGER
 Instrument:  Mercury Dual Imaging System (MDIS) 
 Product Size:  2700 x 2200 pixels (w x h)
 Produced By:  Johns Hopkins University/APL
 Full-Res TIFF:  PIA19409.tif (5.946 MB)
 Full-Res JPEG:  PIA19409.jpg (1.054 MB)

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 MDIS mosaic provides a detailed view of the features and structures associated with the peak-ring basin Raditladi. Raditladi, first imaged during MESSENGER's first Mercury flyby and named in April 2008, continues to be an intriguing region of study, with its well-preserved features, relatively young age, exterior impact melt ponds, hollows-covered peak ring, and concentric troughs on its floor.

Instrument: Mercury Dual Imaging System (MDIS)
Center Latitude: 27.1 N
Center Longitude: 119.2 E
Scale: Raditladi has a diameter of 258 kilometers (160 miles)

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. In the mission's more than four years of orbital operations, MESSENGER has acquired over 250,000 images and extensive other data sets. MESSENGER's highly successful orbital mission is about to come to an end, as the spacecraft runs out of propellant and the force of solar gravity causes it to impact the surface of Mercury in April 2015.

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:
2015-04-16