Mercury Dual Imaging System (MDIS)
The double-ring basin in the lower right is Strindberg, about 189 kilometers (117 miles) in diameter.
On the Moon, areas of smooth plains are called "maria", plural of the Latin word "mare", for "sea". For example, Mare Imbrium is the Sea of Rains. After Mariner 10 obtained the first spacecraft images of Mercury in the mid-1970s, seven areas of smooth plains were given names. However, they were named "planitia", not "maria". Today's release is a mosaic of MESSENGER images centered on Suisei Planitia. Suisei is the Japanese word for the planet Mercury.
This mosaic was acquired as part of MDIS's high-resolution stereo base map. The stereo base map is used in combination with the surface morphology base map to create high-resolution stereo views of Mercury's surface, with an average resolution of 250 meters/pixel (0.16 miles/pixel or 820 feet/pixel) or better. During MESSENGER's one-year primary mission, the surface morphology base map was acquired during the first 176 days, and the second 176 days were used to acquire the complementary stereo base map.
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, MESSENGER acquired 88,746 images and extensive other data sets. MESSENGER is now in a yearlong extended mission, during which plans call for the acquisition of more than 80,000 additional images to support 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.