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The Rim of Cervantes
Click on image to enlarge.
The Rim of Cervantes
Release Date: June 3, 2011
Topics: NAC, Named Craters



Date acquired: May 26, 2011
Image Mission Elapsed Time (MET): 214857150
Image ID: 298561
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: -73.85
Center Longitude: 232.9 E
Resolution: 208 meters/pixel
Scale: This image is 300 kilometers (190 miles) from the western corner to the eastern corner
Incidence Angle: 77.8
Emission Angle: 0.6
Phase Angle: 78.2

Of Interest: The rim of the double-ring basin Cervantes cuts through the middle of this NAC image. Cervantes has a diameter of 213 kilometers and was named in honor of the Spanish novelist, playwright, and poet Miguel de Cervantes (1547-1616), best known for his novel Don Quixote.

This image was acquired as part of MDIS's high-resolution surface morphology base map. The surface morphology base map will cover more than 90% of Mercury's surface with an average resolution of 250 meters/pixel (0.16 miles/pixel or 820 feet/pixel). Images acquired for the surface morphology base map typically have off-vertical Sun angles (i.e., high incidence angles) and visible shadows so as to reveal clearly the topographic form of geologic features.

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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