PIA17455: The Colorfield

The Colorfield


Presented here are nine views of the same colorful section of Mercury's surface. The first two rows are eight individual images taken through narrowband color filters with center wavelengths of 433, 480, 559, 629, 748, 829, 898, and 996 nanometers (nm). The color composite on the bottom is shown with the 996, 748, and 433 nm WAC filters for red, green, and blue. Color differences on Mercury are subtle, and no prominent features stand out in examination of the eight individual grey-scale images. However, the bluish nature of the crater rays on the left and the reddish cast of the material surrounding the impact crater Erte at right become apparent when the images are co-registered.

Erte was seen recently in a three-dimensional close-up!

This image was acquired as part of MDIS's 8-color base map. The 8-color base map is composed of WAC images taken through eight different narrow-band color filters and covers more than 99% of Mercury's surface with an average resolution of 1 kilometer/pixel. The highest-quality color images are obtained for Mercury's surface when both the spacecraft and the Sun are overhead, so these images typically are taken with viewing conditions of low incidence and emission angles.

Date acquired: April 22, 2011
Image Mission Elapsed Time (MET): 211937370, 211937378, 211937372
Image ID: 161451, 161456, 161452
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: 30.04°
Center Longitude: 239.9° E
Resolution: 798 meters/pixel
Scale: The scene is about 420 km (261 mi.) across
Incidence Angle: 59.5°
Emission Angle: 0.1°
Phase Angle: 59.4°

Background Info:

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 .

Cataloging Keywords:

Name Value Additional Values
Target Mercury
Target Type Planet
Instrument Host MESSENGER
Host Type Orbiter
Instrument Mercury Dual Imaging System (MDIS)
Detector Wide Angle Camera (WAC)
Extra Keywords Color, Crater, Impact, Map, Radio
Acquisition Date
Release Date 2013-09-06
Date in Caption 2011-04-22
Image Credit NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
Source photojournal.jpl.nasa.gov/catalog/PIA17455
Identifier PIA17455