Mozart crater on Mercury.  Approximate color representation combining three images acquired by MESSENGER Wide Angle Camera (EW0248001050I, EW0248001042G, EW0248001046F) with <b>I</b> (996.2 nm), <b>G</b> (748.7 nm), and <b>F</b> (433.2 nm) filters.  Combined in GIMP software as RGB (Red-Green-Blue), and then rotated so that north is up.<br><p>A similar image, probably from the same source images, appears in figure 9.5 (g) of <i>Mercury:  The View After <a href="//commons.wikimedia.org/wiki/MESSENGER" class="mw-redirect" title="MESSENGER">MESSENGER</a></i> edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson (Cambridge Planetary Science), which has the following caption:<br>
Enhanced color image of Mozart showing low-reflectance material (LRM) excavated in both the peak ring and as streaks with the basin ejecta.  A reddish unit, likely excavated high-reflectance red plains (HRP) material, is also visible in linear patches across the rim, especially to the south.<br>
Statistics for <b>I</b> image:<br>
Emission Angle: 19.0<br>
Incidence Angle: 9.1<br>
Latitude: 8.6<br>
Longitude: 170.1<br></p>
Phase Angle: 28.1
James Stuby based on NASA images
<a rel="nofollow" class="external text" href="https://pilot.wr.usgs.gov/">PILOT</a>, Planetary Image Locator Tool, USGS Astrogeology Science Center