A NASA Discovery mission to conduct the first orbital study
of the innermost planet
NASA logo carnegie institution logo JHU APL logo

Why Mercury?
The Mission
Gallery
Education
News Center
Science Operations
Who We Are
FAQs
Related Links
Contacts
Home

Download iPhone/iPad app Explore orbital data with quickmap Question and Answer Mercury Orbit Insertion Where is MESSENGER? Where is Mercury now? Subscribe to MESSENGER eNews



Exposing Mercury's Colors
Click on image to enlarge.
Exposing Mercury's Colors
Release Date: October 14, 2008
Topics: Color Images, Mercury Flyby 2, Scarps, WAC



Date Acquired: October 6, 2008
Image Mission Elapsed Time (MET): 131770496 - 131770546
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
Resolution: 420 meters/pixel (0.26 miles/pixel)
Scale: Thākur crater is 118 kilometers in diameter (73 miles)
Spacecraft Altitude: about 2,500 kilometers (1,600 miles)

Of Interest: To the human eye, Mercury shows little color variation, especially in comparison to a colorful planet like Earth. But when images taken through many color filters are used in combination, differences in the properties of Mercury’s surface can create a strikingly colorful view of the innermost planet. Shown here are two color images of Thākur, named for the Bengali poet, novelist, and Nobel laureate influential in the late 19th and early 20th centuries. The image on the left was produced by combining images from three WAC filters into red, green, and blue channels, as a general representation of the color seen by the human eye (though every person sees color slightly differently, as discussed for the full-planet color images.) The right image was created by statistically comparing and contrasting images taken through all 11 of the WAC’s narrow-band color filters, which are sensitive to light not only in the visible portion of the spectrum but also to light that the human eye cannot see. This method greatly enhances subtle color differences in the rocks of Mercury’s surface, providing insight into the compositional variations present on Mercury and the geologic processes that created those color differences. Visible on the floor of Thākur crater is the intersection of two ridges, seen here in unprecedented detail for the first time with MESSENGER’s newly obtained images.

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


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


   

   Top  | Contacts
© 1999-2014 by JHU/APL