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The Cliffs of Raditladi
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The Cliffs of Raditladi
Release Date: January 16, 2012
Topics: MLA, , , Raditladi

Date acquired: December 31, 2011
Image Mission Elapsed Time (MET): 233814606
Image ID: 1205792
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 27.7°
Center Longitude: 122.7° E
Resolution: 75 meters/pixel
Scale: The scene is approximately 77 km (48 miles) across
Incidence Angle: 36.2°
Emission Angle: 30.9°
Phase Angle: 29.4°

Of Interest: A look at the rim of the Raditladi impact basin. Raditladi is a relatively young basin and host to beautiful hollows. The depth from the floor to its rim is around 3.5 km (over 2 miles) as measured by the Mercury Laser Altimeter - twice the average depth of the Grand Canyon. Imagine the view from Raditladi's rim!

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 250-meter/pixel (820 feet/pixel) morphology base map or the 1-kilometer/pixel (0.6 miles/pixel) color base map. It is not possible to cover all of Mercury's surface at this high resolution during MESSENGER's one-year mission, but several areas of high scientific interest are generally imaged in this mode each week.

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 is scheduled to acquire more than 75,000 images in support of MESSENGER's science goals.

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

For information regarding the use of MESSENGER images, see the image use policy.


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