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Piú viste - Mars from Orbit (from July 2009)
Volcanoes-Hecates_Tholus-EC-20080606a-PCF-LXTT.jpg
Volcanoes-Hecates_Tholus-EC-20080606a-PCF-LXTT.jpgThe South-Western Flank of Hecates Tholus (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visitenessun commentoMareKromium
Landslide-CC-20080421a-PCF-LXTT.jpg
Landslide-CC-20080421a-PCF-LXTT.jpgBeautiful Landslide in Coprates Chasma (Absolute Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)87 visitenessun commentoMareKromium
Craters-Unnamed_Crater-PIA14274-PCF-LXTT.jpg
Craters-Unnamed_Crater-PIA14274-PCF-LXTT.jpgUnnamed Crater with Landslide (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visitenessun commentoMareKromium
Tempe_Terra-PIA18251-PCF-LXTT-IPF-1.jpg
Tempe_Terra-PIA18251-PCF-LXTT-IPF-1.jpgFeatures of Tempe Terra (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)87 visiteIn this VIS image, taken by the NASA - Mars Odyssey Orbiter on March, 5th, 2014, and during its 54.219th orbit around the Red Planet, we can see a small portion of the Eastern Margin of the Martian Region known as Tempe Terra, where numerous Unnamed Outflow Channels can be found. In this picture, if you look at it carefully, you will be able to see an interesting and unusually-looking Craters' Cluster (approx. 13 small Impact Craters, very close to one another and showing different levels of degradation, are visible - look at the lower Right - Dx - center of the frame) and a white-colored, medium-sized Outcrop (lower center of the frame), surrounded by small, low and curvilinear Ridges whose origin is (so far) unknown.

Latitude (centered): 35,3128° North
Longitude (centered): 305,1220° East
Instrument: VIS

This image (which is a crop taken from an Original Mars Odyssey Orbiter b/w and Map-Projected frame published on the NASA - Planetary Photojournal with the ID n. PIA 18251) has been additionally processed, magnified to aid the visibility 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 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
North_Polar_Regions-Olympia_Undae-PIA06848-00.jpg
North_Polar_Regions-Olympia_Undae-PIA06848-00.jpgNorth Polar Erg: Olympia Undae (Original NASA/JPL/ASU b/w Frame)86 visiteImage information: VIS instrument;
Latitude: 81,4° North;
Longitude: 180,6° East (such as 179,4° West);
Resolution: 19 meter/pixel.
Avernus_Colles-PIA08719-PCF-LXTT.jpg
Avernus_Colles-PIA08719-PCF-LXTT.jpgChaos Terrain in Avernus Colles (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)86 visitenessun commentoMareKromium
Volcanoes-Arsia_Mons-PIA13348.jpg
Volcanoes-Arsia_Mons-PIA13348.jpgCollapse Features on the Northern Flank of Arsia Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)86 visitenessun commentoMareKromium
Zephyria_Planum-20071017a.jpg
Zephyria_Planum-20071017a.jpgZephyria Planum (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)86 visiteCaption NASA:"This image shows a small protion of Zephyria Planum, a Region South of Elysium Planitia. Winds have scoured the Region removing loose materials and scultping the rocks". MareKromium
Yardangs-Gordii_Dorsum-PIA13461.jpg
Yardangs-Gordii_Dorsum-PIA13461.jpgWindwork in Gordii Dorsum (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)86 visitenessun commentoMareKromium
South_Polar_Features-Layers-PIA13826-PCF-LXTT.jpg
South_Polar_Features-Layers-PIA13826-PCF-LXTT.jpgSouth Polar Layered Deposits (Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)86 visiteCaption NASA:"Layering in South Polar Ice is easy to see in this outlier of the Main Polar Cap".

Orbit Number: 39861
Latitude: 83,364° South
Longitude: 327,367° East
Instrument: VIS
Captured: December, 9th, 2010
Mars Local Time: 10:39 (Late Morning Hours)
MareKromium
Volcanoes-Arsia_Mons-20090225a-PCF-LXTT.jpg
Volcanoes-Arsia_Mons-20090225a-PCF-LXTT.jpgGraben and Lava Flows near Arsia Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit) 86 visiteCaption NASA:"This VIS image covers a small region of the Western Flank of Arsia Mons. The Surface of the Volcanic Flows in this Region have an odd pitted texture. The cause of this texture is unknown".

Coord.: 8° South Lat. and 237,6° East Long.
MareKromium
Candor_Chasma-03.jpg
Candor_Chasma-03.jpgCandor Chasma from MGS and 2001 Mars Odyssey85 visiteCaption originale:"The 2001 Mars Odyssey Spacecraft includes an imaging device called THEMIS which scans strips of Mars in various wavelengths. Although numerous excellent images have been returned, unfortunately quirks and light leak defects in the camera system prevent straightforward registration of images obtained in different wavelengths. The first RGB color image released from Mars Odyssey is shown in the context of a color image from Mars Global Surveyor with a faked green channel. The THEMIS image appears too dark and saturated to me but I have preserved the color balance as released. Detailed criticism must be qualified by knowledge of the heroic measures taken to 'rescue' this RGB color image. The dark gray terrain in the valley floor shows as brownish to olive greenish in the closeup, and an orange region in the lower right is seen as the edge of a larger reddish area in the central interior of Candor Chasma".
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