Astronomy Picture of the Day
November 6, 2015

Features of Becquerel Crater
Features of Becquerel Crater

Credits: NASA/JPL/Arizona State University (ASU) - Credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/IPF

In this VIS image, taken by the NASA - Mars Odyssey Orbiter on February, 24th, 2005, and during its 14.192nd orbit around the Red Planet, we can see a (truly small) portion of the Floor of Becquerel Crater, including, among other interesting things, a large Layered Deposit and a series of - relatively - small Sand Dunes.

Becquerel Crater is an approx. 167 Km-diameter (such as about 103,707 miles) Impact Crater, centered at 22,1° North Latitude and 352,0° East Longitude, in the old and dusty Martian Region known as Arabia Terra, which is located in the Oxia Palus Quadrangle. Becquerel Crater was so named after Dr Antoine H. Becquerel, a French PhysicistNobel Laureate, and co-discoverer of radioactivity after he worked in this field of Science along with Marie Skodowska-Curie and Pierre Curie.

Latitude (centered): 21,2926° North
Longitude (centered): 351,7930° East
Instrument: VIS

This image (which is an Original Mars Odyssey Orbiter falsely colored and Map Projected frame published on the NASA - Planetary Photojournal with the ID n. PIA 20085) has been additionally processed, magnified to aid the visibility of the details, extra-contrast enhanced and sharpened, Gamma corrected and then re-colorized in Absolute Natural Colors (such as the colors that a normal human eye would actually perceive if someone were onboard the NASA - Mars Odyssey Orbiter and then looked down, towards the Surface of Mars), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team.

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