Astronomy Picture of the Day
October 30, 2013

Matisse and Companions (EDM)
Matisse and Companions (EDM)

Credits: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington and Dr Paolo C. Fienga/LXTT/IPF for the additional process. and color.

This frame (which is a crop taken from an image-mosaic made out of three pictures obtained by the NASA - MESSENGER Spacecraft in October 2012) shows us the large Matisse Crater (approx. 186 Km - such as about 115,506 miles - in diameter) and its closest proximities. As you can see, two Unnamed Impact Craters formed tangentially to the Rim of Matisse Crater: one just inside, on the Edge of the Inner Rim, and the other one just outside, right on the Edge of the Outer Rim.

You may want to notice that these two Unnamed Impact Craters have really bright yellow/white/orangish Deposits on their Floors and such a color characteristics are found, as a matter of fact, at many other locations on Mercury - usually where (we believe that) massive Pyroclastic Volcanic Eruptions took place. Furthermore, and in our opinion, as IPF, the Unnamed Impact Crater located outside of Matisse seems to have - just at the center of its Floor - a very well defined (and, also, relatively recent) Collapse Pit.

Date acquired: October, 21st, 2012
Images Mission Elapsed Time (MET): 259266820, 259266840, 259266824
Images ID: 2803275, 2803280, 2803276
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 23,00° South
Center Longitude: 268,40° East
Solar Incidence Angle: 45,6° (meaning that the Sun, at the time that the picture was taken, was about 44,4° above the imaged Local Mercurian Horizon)
Emission Angle: 33,5°
Sun-Mercury-Messenger (or "Phase") Angle: 78,7°

This picture (which is a crop taken from an Original NASA - MESSENGER Spacecraft's False Colors and Map-Projected image-mosaic published on the NASA - Planetary Photojournal with the ID n. PIA 17541) has been additionally processed, contrast enhanced, magnified and then re-colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - MESSENGER Spacecraft and then looked down, towards the Surface of Mercury), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team. Different colors, as well as different shades of the same color, mean, among other things, the existence of different Elements (Minerals) present on the Surface of Mercury, each having a different Albedo (---> Reflectivity) and Chemical Composition.

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