Mars from Orbit (from July 2009)
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Channels-Auqakuh_Vallis-PIA08465-02.jpgFeatures of Auqakuh Vallis (Original NASA/JPL/ASU b/w Frame)54 visiteImage information: VIS instrument;
Latitude: 31,0° North;
Longitude: 60,6° East;
Resolution: 19 meter/pixel.
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Channels-Auqakuh_Vallis-PIA08465-03.jpgFeatures of Auqakuh Vallis (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 133 visiteMareKromium
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Channels-Clanis_Vallis-MO.JPGClanis Vallis (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)54 visitenessun commentoMareKromium
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Channels-Claritas_Fossae-20071030a-PCF-LXTT.jpgChannels in Claritas Fossae (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)64 visitenessun commentoMareKromium
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Channels-Dao_Vallis-20071211a-PCF-LXTT.jpgDao Vallis (Enhanced Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)100 visitenessun commentoMareKromium
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Channels-Dao_Vallis-PIA15215-PCF-LXTT-IPF.jpgFeatures of Dao Vallis (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)71 visiteDao Vallis is a Martian Channel that, as the peculiar texture and color of its bottom and edges show us quite well, was not carved by Molten (and very fluid) Lava, but by real Water instead. Dao Vallis runs South/Westward into the Hellas Planitia Region, and it has been identified (among others, by Dr M.H. Carr) as a so-called Outflow Channel. Dao Vallis has a main Tributary Channel, known as Niger Vallis, and it extends on the Martian Southern Hemisphere's Surface for over 1200 Km. Its name, just out of curiosity, apparently comes from a Thai word meaning "star" (and God only knows why the IAU made such a bizarre and, in our opinion, pointless choice...).
However, talking again about our today's APOD Surface Feature, we can say that we know that the (possible) sources of Dao Vallis are near an extremely old Martian Volcano, called Hadriaca Patera; it is thought by many Scientists that the Water that formed it came out from the Subsurface when a huge quantity of hot Magma, erupted from Hadriaca Patera, melted, in a very short time period (in a case like this, we might be talking about minutes), huge amounts of Ice that was caught in the otherwise already frozen Ground. Anyway, much of this Water may have also been released during the occurrence of a few very large "Outburst Floods".
In addition to the above, and after a carfeul examination of Dao Vallis' now completely desiccated Riverbed, we, as IPF, strongly believe that, whatever the actual origin of the Channel might have been, Dao Vallis must have carried liquid Water for a very long time, before drying up. As a matter of fact, and as it is clearly visible in this NASA - 2001 Mars Odyssey Orbiter frame, on the bottom of the Channel can be identified several layers of dried material (Mud, likely) that, in our opinion, make the physical evidence that the desiccation process of Dao Vallis took some time before it was complete. In other words, the desiccation (or, like some Scientists say, evaporation and/or sublimation) of the Waters that ran through the Channel, was far from being semi-instantaneous or (this, of course, relatively speaking) rather fast. Furthermore, the almost complete lack of Impact Craters on the Riverbed, if seen and evaluated in direct contrast with the strong presence of Impact Craters (of various size and shape - meaning both Primary and Secondary Craters) that exist and is VERY well visible on both the edges of the Channel, proves us that, when Liquid Water ran through Dao Vallis, the strong meteoric activity which scarred most of the Surface of the Red Planet, was already ended. In other words, Dao Vallis hosted liquid and running Waters until a very (always relatively - and geologically - speaking) recent time.
Picture Data: Orbit Number: 44201; Latitude: 39,4843° South and Longitude: 86,4444° East; Instrument: VIS; Captured: December, 1st, 2011; Mars Local Time (M.L.T.): 17:39 (Late Aftrnoon)
This frame has been colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - 2001 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.MareKromium
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Channels-Dao_Vallis-PIA15215-PCF-LXTT.jpgFeatures of Dao Vallis (Saturated Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)140 visiteOrbit Number: 44201
Latitude: 39,4383° South
Longitude: 86,4444° East
Instrument: VIS
Captured: December, 1st,
Mars Local Solar Time: 17:39 (Late Afternoon)
MareKromium
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Channels-Drainage_Channel-MO.jpgDrainage Channel System (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visiteCaption NASA:"This small Channel System is located on the Outer Rim of Sytinskaya Crater".
Coord.: 43,1° North Lat. and 306,4° East Long.MareKromium
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Channels-Drainage_Channels-PCF-LXXT.JPGDraining Channels near Moreux Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)54 visitenessun commentoMareKromium
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Channels-Drainage_Channels-PIA14971-PCF-LXTT.jpgDrainage Channels on the Rim of Bakhuysen Crater (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)187 visiteOrbit Number: 43492
Latitude: 23,6637° South
Longitude: 14,8281° East
Instrument: VIS
Captured: October, 4th, 2011
Mars Local Time (M.L.T.): 09:02 (Morning Hours)
MareKromium
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Channels-Elator_Vallis-PIA14142-PCF-LXTT.jpgElator Vallis and Ganges Chasma (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)284 visitenessun commentoMareKromium
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Channels-Elator_Vallis-PIA14148-PCF-LXTT.jpgElator Vallis (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)200 visitenessun commentoMareKromium
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