 Click on image to enlarge. | Zeami's Zoo of FeaturesRelease Date: April 30, 2012 Topics: Complex Craters, Hollows, Peak Ring Basins |
Date acquired: April 08, 2012
Image Mission Elapsed Time (MET): 242378498
Image ID: 1621634
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: -2.80°
Center Longitude: 212.7° E
Resolution: 186 meters/pixel
Scale: Zeami crater is 129 km (80 mi) in diameter.
Incidence Angle: 79.7°
Emission Angle: 26.7°
Phase Angle: 52.9°
Of Interest: This image, taken with the Narrow Angle Camera (NAC), gives us a good look at Zeami crater. Named for the 14th century Japanese actor and playwright Zeami Motokiyo, this crater displays a variety of features characteristic of complex craters on Mercury. We can see the remnants of an inner peak ring, terraced walls, and hollows scattered across the crater floor, especially near the top of the image.
This image was acquired as part of MDIS's high-incidence-angle base map. The high-incidence-angle base map is a major mapping activity in MESSENGER's extended mission and complements the surface morphology base map of MESSENGER's primary mission that was acquired under generally more moderate incidence angles. High incidence angles, achieved when the Sun is near the horizon, result in long shadows that accentuate the small-scale topography of geologic features. The high-incidence-angle base map is being acquired with an average resolution of 200 meters/pixel.
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.
Image Mission Elapsed Time (MET): 242378498
Image ID: 1621634
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: -2.80°
Center Longitude: 212.7° E
Resolution: 186 meters/pixel
Scale: Zeami crater is 129 km (80 mi) in diameter.
Incidence Angle: 79.7°
Emission Angle: 26.7°
Phase Angle: 52.9°
Of Interest: This image, taken with the Narrow Angle Camera (NAC), gives us a good look at Zeami crater. Named for the 14th century Japanese actor and playwright Zeami Motokiyo, this crater displays a variety of features characteristic of complex craters on Mercury. We can see the remnants of an inner peak ring, terraced walls, and hollows scattered across the crater floor, especially near the top of the image.
This image was acquired as part of MDIS's high-incidence-angle base map. The high-incidence-angle base map is a major mapping activity in MESSENGER's extended mission and complements the surface morphology base map of MESSENGER's primary mission that was acquired under generally more moderate incidence angles. High incidence angles, achieved when the Sun is near the horizon, result in long shadows that accentuate the small-scale topography of geologic features. The high-incidence-angle base map is being acquired with an average resolution of 200 meters/pixel.
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.