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ESP_023814_1970_RED_abrowse-PCF-LXTT-00.jpg
ESP_023814_1970_RED_abrowse-PCF-LXTT-00.jpgPossible Olivine-Rich Terrain in Isidis Planitia Region (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)198 visiteMars Local Time: 14:08 (Early Afternoon)
Coord. (centered): 16,7° North Lat. and 80,1° East Long.
Spacecraft altitude: 279,9 Km (such as about 174,9 miles)
Original image scale range: 56,0 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 68 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,2°
Sun-Mars-Spacecraft (or "Phase") Angle: 38,0°
Solar Incidence Angle: 38° (meaning that the Sun is about 52° above the Local Horizon)
Solar Longitude: 350,6° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromiumOtt 08, 2011
ESP_023818_0965_RED_abrowse-PCF-LXTT.jpg
ESP_023818_0965_RED_abrowse-PCF-LXTT.jpgPotential Water-Ice Outlier persistant through Southern Summer (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)186 visiteMars Local Time: 15:46 (Middle Afternoon)
Coord. (centered): 83,5° South Lat. and 3,0° East Long.
Spacecraft altitude: 249,7 Km (such as about 156,0 miles)
Original image scale range: 50,0 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 50 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 0,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 82,4°
Solar Incidence Angle: 83° (meaning that the Sun is about 7° above the Local Horizon)
Solar Longitude: 350,8° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromiumOtt 08, 2011
ESP_023806_1645_RED_abrowse-PCF-LXTT.jpg
ESP_023806_1645_RED_abrowse-PCF-LXTT.jpgFeatures of Coprates Chasma (Saturated and Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 181 visiteMars Local Time: 14:13 (Early Afternoon)
Coord. (centered): 15,2° South Lat. and 302,3° East Long.
Spacecraft altitude: 261,6 Km (such as about 163,5 miles)
Original image scale range: 52,3 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 57 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 2,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 37,0°
Solar Incidence Angle: 35° (meaning that the Sun is about 55° above the Local Horizon)
Solar Longitude: 350,3° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromiumOtt 08, 2011
SOL589-2N178659646EFFAE93P0695L0M1-PCF-LXTT.jpg
SOL589-2N178659646EFFAE93P0695L0M1-PCF-LXTT.jpgDust Devil in the distance - Sol 589 (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)97 visitenessun commentoMareKromiumOtt 08, 2011
OPP-SOL2716-1P369295744EFFBN19P2542R7M1-PCF-LXTT.jpg
OPP-SOL2716-1P369295744EFFBN19P2542R7M1-PCF-LXTT.jpgPossible Ejecta-Boulders near Endeavour's Rim - Sol 2716 (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)117 visitenessun commentoMareKromiumOtt 08, 2011
Volcanic_Features-Pits-Ascraeus_Mons-PIA07313-02.jpg
Volcanic_Features-Pits-Ascraeus_Mons-PIA07313-02.jpgAscraeus Mons' Pit Chain (EDM/HD - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)192 visitenessun commentoMareKromiumOtt 07, 2011
Volcanic_Features-Pits-Ascraeus_Mons-PIA07313-04.jpg
Volcanic_Features-Pits-Ascraeus_Mons-PIA07313-04.jpgAscraeus Mons' Pit Chain (EDM/HD - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)194 visitenessun commentoMareKromiumOtt 07, 2011
Volcanic_Features-Lava_or_Mud_Flows-01.jpg
Volcanic_Features-Lava_or_Mud_Flows-01.jpgControversial Features of Zephyria Planum (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)116 visiteOriginal caption:"This MGS-MOC image shows a portion of a shallow Channel carved in the Plains of the Zephyria Region of Mars. This feature might be the result of the passing of either extremely fluid Lava or, perhaps, Mud".

Location near: 5,1° North Lat. and 203,7° West Long.
Image width: ~3 Km (~1,9 mi)
Season: Northern Winter
MareKromiumOtt 07, 2011
Martian_Lower_Atmosphere-Winds_and_Fog-PIA07417-01.jpg
Martian_Lower_Atmosphere-Winds_and_Fog-PIA07417-01.jpgLower Atmosphere (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)147 visitenessun commentoMareKromiumOtt 07, 2011
SOL748-02-PCF-LXTT.jpg
SOL748-02-PCF-LXTT.jpgEvidence of Volcanic Explosion? - Sol 748 (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)155 visiteCaption NASA originale:"The lower coarse-grained unit shows granular textures toward the bottom of the image and massive textures. Also shown (by the arrow) is a feature interpreted to be a "Bomb Sag" which is about 4 cm across".

Nota Lunexit: "Bomb Sag"---> (Geology) depressed and deranged Laminae mainly found in beds of fine-grained Ash or Tuff around an included Volcanic Bomb or Block which fell on and became buried in the deposit.
MareKromiumOtt 07, 2011
Dunes-Dark_Dunes-Noachis_Terra-PIA07351-01.jpg
Dunes-Dark_Dunes-Noachis_Terra-PIA07351-01.jpgDark Dunes in Noachis Terra (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)167 visiteCaption NASA originale:"This MGS-MOC image shows low albedo Sand Dunes on the Floor of an Unnameed Crater in Southern Noachis Terra".

Location near: 52.5° South Lat. and 336.9° West Long.
Image width: ~3,0 Km (~1,9 mi)
Illumination from: upper left
Season: Southern Autumn
MareKromiumOtt 06, 2011
Craters-Unnamed_Craters_with_Sedimentary_Rock_Outcrops-PIA07127-01.jpg
Craters-Unnamed_Craters_with_Sedimentary_Rock_Outcrops-PIA07127-01.jpgSedimentary Rocks (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)161 visiteCaption NASA originale:"Burial and Exhumation of Impact Craters, and their destruction by erosion, are common and repeated themes all over the Surface of Mars. Many Craters in Western Arabia Terra exhibit light-toned, Layered Outcrops of ancient Sedimentary Rock. Like the Sedimentary Rocks explored further to the South in Meridiani Planum by the Opportunity Mars Exploration Rover (MER-B), these "Intracrater Sedimentary Rocks" may have been deposited in water. This MGS-MOC image shows an example of light-toned Sedimentary Rocks outcropping in an Unnamed Crater that is much farther North than most of the similar examples in Western Arabia Terra. This one is located near 36,6° North Lat. and 1,4° West Long. and shows several old Impact Craters in various states of erosion and exhumation from beneath and within the Sedimentary Rock Materials. The image covers an area of approx. 3 Km".

MareKromiumOtt 06, 2011
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