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



Lermontov's Legacy
Click on image to enlarge.
Lermontov's Legacy
Release Date: May 20, 2013
Topics: Albedo Contrasts, Craters with Bright Material, Hollows, Named Craters, Volcanism, WAC



Date acquired: February 12, 2013
Image Mission Elapsed Time (MET): 3010537
Image ID: 3507773
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filter: 9 (996 nanometers)
Center Latitude: 15.81
Center Longitude: 311.8 E
Resolution: 276 meters/pixel
Scale: Lermontov is 166 km (103 mi.) in diameter.
Incidence Angle: 49.7
Emission Angle: 28.5
Phase Angle: 78.2

Of Interest: The bright floor of the crater Lermontov, first imaged by Mariner 10, stands in contrast to the surrounding terrain of Mercury. The large depressions found in the floor have been interpreted as evidence for explosive volcanism, providing insight into Mercury's volcanic history. The surface within the crater also appears to have been altered by the formation of hollows.

This image was acquired as a high-resolution targeted color observation. Targeted color observations are images of a small area on Mercury's surface at resolutions higher than the 1-kilometer/pixel 8-color base map. During MESSENGER's one-year primary mission, hundreds of targeted color observations were obtained. During MESSENGER's extended mission, high-resolution targeted color observations are more rare, as the 3-color base map covered Mercury's northern hemisphere with the highest-resolution color images that are possible.

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.


   

   Top  | Contacts
© 1999-2014 by JHU/APL