 Click on image to enlarge. | Small and DramaticRelease Date: August 8, 2012 Topics: Crater Chains, |
Date acquired: June 28, 2012
Image Mission Elapsed Time (MET): 249412272
Image ID: 2102840
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 45.69°
Center Longitude: 79.00° E
Resolution: 32 meters/pixel
Scale: The crater is 10 km (6.2 miles) in diameter.
Incidence Angle: 66.1°
Emission Angle: 37.9°
Phase Angle: 28.1°
Of Interest: This image shows an impact crater surrounded by smaller craters which are possibly secondaries from Rustaveli. The crater has a small central peak or floor mound, whereas the nearby craters are simple. The central crater has a sharper rim and fresher appearance than the other craters, suggesting that it is younger. The smaller craters are more degraded and less dramatic showing the passage of time on Mercury.
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 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are 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, 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): 249412272
Image ID: 2102840
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 45.69°
Center Longitude: 79.00° E
Resolution: 32 meters/pixel
Scale: The crater is 10 km (6.2 miles) in diameter.
Incidence Angle: 66.1°
Emission Angle: 37.9°
Phase Angle: 28.1°
Of Interest: This image shows an impact crater surrounded by smaller craters which are possibly secondaries from Rustaveli. The crater has a small central peak or floor mound, whereas the nearby craters are simple. The central crater has a sharper rim and fresher appearance than the other craters, suggesting that it is younger. The smaller craters are more degraded and less dramatic showing the passage of time on Mercury.
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 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are 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, 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.