PIA18527: Bright and Dark
 Target Name:  Mercury
 Is a satellite of:  Sol (our sun)
 Mission:  MESSENGER
 Spacecraft:  MESSENGER
 Instrument:  MASCS
Mercury Dual Imaging System (MDIS) 
 Product Size:  1826 x 2500 pixels (w x h)
 Produced By:  Johns Hopkins University/APL
 Full-Res TIFF:  PIA18527.tif (13.7 MB)
 Full-Res JPEG:  PIA18527.jpg (586 kB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

The top image is a MASCS VIRS interpolated color composite of the craters Rachmaninoff (lower left) and Copland (upper right). The bottom image is a monochrome MDIS mosaic of the same area. In the VIRS image, red areas like Copland (C) are brighter than blue areas like Rachmaninoff (R). The very bright red region in-between is a suspected volcanic vent (V). The color differences revealed in the VIRS image reveal differences in the composition of the surface rocks, as well as varying degrees of exposure to space weathering in the harsh environment of Mercury.

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.

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: 32.2
Center Longitude: 60.9 E
Resolution: 1 km/pixel
Scale: Inner Rim of Rachmaninoff (lower left crater) is 140 km (87 mi.) in diameter

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. MESSENGER acquired over 150,000 images and extensive other data sets. MESSENGER is capable of continuing orbital operations until early 2015.

For information regarding the use of images, see the MESSENGER image use policy.

Image Credit:
NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Image Addition Date: