 Click on image to enlarge. | On Hole-y GroundRelease Date: July 10, 2012 Topics: Albedo Contrasts, Color Images, Hollows, Scarlatti, Vents, Volcanism |
Date acquired: April 04, 2012
Image Mission Elapsed Time (MET): 242004051, 242004043, 242004047
Image ID: 1603177, 1603175, 1603176
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filters: 9, 7, 6 (996, 748, 433 nanometers) in red, green, and blue
Center Latitude: 39.84°
Center Longitude: 260.9° E
Resolution: 202 meters/pixel
Scale: The Scarlatti basin is 132 km (82 mi) in diameter.
Incidence Angle: 57.5°
Emission Angle: 0.2°
Phase Angle: 57.5°
Of Interest: This image shows the peak-ring basin Scarlatti in color. The bright, irregular depression on the interior ring of the basin is thought to be a volcanic vent. There are also hollows present in the southern section of the peak-ring that appear blue compared to the surrounding material. This basin is named for Alessandro Scarlatti and his son Domenico Scarlatti, both influential Italian Baroque composers. Both composers are known for their transitional Western music, linking the Baroque style with the later Classical style.
This image was acquired as part of MDIS's high-resolution 3-color imaging campaign. The 3-color campaign is a major mapping activity in MESSENGER's extended mission. It complements the 8-color base map (at an average resolution of 1 km/pixel) acquired during MESSENGER's primary mission by imaging Mercury's surface in a subset of the color filters at the highest resolution possible. The three narrow-band color filters are centered at wavelengths of 430 nm, 750 nm, and 1000 nm, and image resolutions generally range from 100 to 400 meters/pixel in the northern hemisphere.
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): 242004051, 242004043, 242004047
Image ID: 1603177, 1603175, 1603176
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filters: 9, 7, 6 (996, 748, 433 nanometers) in red, green, and blue
Center Latitude: 39.84°
Center Longitude: 260.9° E
Resolution: 202 meters/pixel
Scale: The Scarlatti basin is 132 km (82 mi) in diameter.
Incidence Angle: 57.5°
Emission Angle: 0.2°
Phase Angle: 57.5°
Of Interest: This image shows the peak-ring basin Scarlatti in color. The bright, irregular depression on the interior ring of the basin is thought to be a volcanic vent. There are also hollows present in the southern section of the peak-ring that appear blue compared to the surrounding material. This basin is named for Alessandro Scarlatti and his son Domenico Scarlatti, both influential Italian Baroque composers. Both composers are known for their transitional Western music, linking the Baroque style with the later Classical style.
This image was acquired as part of MDIS's high-resolution 3-color imaging campaign. The 3-color campaign is a major mapping activity in MESSENGER's extended mission. It complements the 8-color base map (at an average resolution of 1 km/pixel) acquired during MESSENGER's primary mission by imaging Mercury's surface in a subset of the color filters at the highest resolution possible. The three narrow-band color filters are centered at wavelengths of 430 nm, 750 nm, and 1000 nm, and image resolutions generally range from 100 to 400 meters/pixel in the northern hemisphere.
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.