 Click on image to enlarge. | Crater on Me, BlueRelease Date: June 18, 2014 |
Date Created: June 16, 2014
Instruments: Visible and Infrared Spectrograph (VIRS) of the Mercury Atmosphere and Surface Composition Spectrometer (MASCS) and Mercury Dual Imaging System (MDIS)
VIRS Color Composite Wavelengths: 575 nm as red, 415 nm/750 nm as green, 310 nm/390 nm as blue
Center Latitude: 42.5°
Center Longitude: 154.5° E
Resolution: 1 km/pixel
Scale: Sander crater (center) is about 50 km (31 mi.) in diameter
Of Interest: The top image is a MASCS VIRS interpolated color composite of craters Eminescu (center), with Xiao Zhao and Eastman toward the east and in Mercury's mid latitudes. The bottom image is a monochrome MDIS mosaic of the same area. Yellow areas correspond to high values in both the red and green channels, that is, high reflectance (at 575 nm) and high values of the 415-nm/575-nm reflectance ratio. In some cases these spectral characteristics are associated with fresh material (like the rays of Xiao Zhao) that has been less affected by space weathering. Hollows, such as those found on and around the central peak of Eminescu, have similar colors.
The VIRS composite shows hundreds of individual footprints tracks (minimum 100-200 m across and 3-4 km long) taken from different directions and altitudes. In locations where multiple footprints cover the same area, the footprint with the best illumination for mineralogical interpretation (usually the lowest incidence angle where shadows are minimized) is used for making the map. In areas where footprints are sparse (separated by tens of km), observations are interpolated for complete coverage of the surface. In the MDIS mosaic, some brightness variations are due to tiling of images taken at different illuminations.
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. During the first two years of orbital operations, MESSENGER acquired over 150,000 images and extensive other data sets. MESSENGER is capable of continuing orbital operations until early 2015.
Instruments: Visible and Infrared Spectrograph (VIRS) of the Mercury Atmosphere and Surface Composition Spectrometer (MASCS) and Mercury Dual Imaging System (MDIS)
VIRS Color Composite Wavelengths: 575 nm as red, 415 nm/750 nm as green, 310 nm/390 nm as blue
Center Latitude: 42.5°
Center Longitude: 154.5° E
Resolution: 1 km/pixel
Scale: Sander crater (center) is about 50 km (31 mi.) in diameter
Of Interest: The top image is a MASCS VIRS interpolated color composite of craters Eminescu (center), with Xiao Zhao and Eastman toward the east and in Mercury's mid latitudes. The bottom image is a monochrome MDIS mosaic of the same area. Yellow areas correspond to high values in both the red and green channels, that is, high reflectance (at 575 nm) and high values of the 415-nm/575-nm reflectance ratio. In some cases these spectral characteristics are associated with fresh material (like the rays of Xiao Zhao) that has been less affected by space weathering. Hollows, such as those found on and around the central peak of Eminescu, have similar colors.
The VIRS composite shows hundreds of individual footprints tracks (minimum 100-200 m across and 3-4 km long) taken from different directions and altitudes. In locations where multiple footprints cover the same area, the footprint with the best illumination for mineralogical interpretation (usually the lowest incidence angle where shadows are minimized) is used for making the map. In areas where footprints are sparse (separated by tens of km), observations are interpolated for complete coverage of the surface. In the MDIS mosaic, some brightness variations are due to tiling of images taken at different illuminations.
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. During the first two years of orbital operations, MESSENGER acquired over 150,000 images and extensive other data sets. MESSENGER is capable of continuing orbital operations until early 2015.
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.