As the so-called "Gullies" (---> a Gully is a Ravine USUALLY formed by the Action of Running Water) form on Slopes, Sediment can become deposited to form Lobe-shaped Fans. Gullies can form with Flowing Water, but they don't have to (---> this means that the Flowing Water is NOT a so-called "condicio sine qua non" of the Gullies' formation): sometimes they can be formed by the Dry Flow of Sand and very fine Dust Grains. This HiRISE Sub-Frame (also known as Extra Detail Magnification - "EDM" for short -, according to the Technical Language that we, as IPF, like to use here), which has been obtained by the NASA - Mars Reconnaissance Orbiter on November 16, 2014, shows us that - at least one - of these abovementioned (and seemingly still) Active Gullies, is characterized by the presence, on both sides and all along its length, of quite a few fine (---> truly small, short, thin and mostly sinuous) sub-Channels. Mars Local Time: 15:41 (Middle Afternoon) This picture (which is a crop taken from a NASA - Original Mars Reconnaissance Orbiter Falsely Colored and NON-Map-Projected Sub-frame identified by the serial n. ESP_038931_1355-1) has been additionally processed, extra-magnified to allow the Readers a better view of the details, contrast enhanced, Gamma corrected, and then colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - Mars Reconnaissance 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. |