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OPP-SOL2476-1-GB-LXTT.jpgRocky Outcrop, Berries and Paving - Sol 2476 (Enhanced Natural Colors; credits for the additional process. and color.: Dr Gianluigi Barca - Lunexit Team)87 visitenessun commentoMareKromium
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South_Polar_Features-Layers-PIA13826-PCF-LXTT.jpgSouth Polar Layered Deposits (Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)87 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
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PSP_006653_1795_RED_abrowse-PCF-LXTT.jpgVolcanic Vent, East of Pavonis Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit) 87 visiteThis image shows an Equatorial Volcanic Vent. A Volcanic Vent is an opening in the Crust of a Planet that emits Lava (such as "molten rock") and Volcanic Gases. The rough texture of the Plains surrounding the Vent is indicative of Lava.
There is a large number of snake-like features emanating from the Vent. The parallel lines that outline the features are "Levees", which mark the edges of Channels that carried molten Lava. As Lava flows, it moves slowest at its edges and bottom because the Lava sticks to the non-flowing rocks; as a consequence of this event, the lava slows down, cools off and, in the end, it hardens.
Levees, on their side, form when the sides of the Lava Flow harden but the center of it keeps moving. As the eruption episode ends, and the Lava drains, the center is left lower than the sides producing these high-standing structures.MareKromium
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PSP_006752_1525_RED_abrowse-PCF-LXTT2.jpgFeatures of Terby Crater (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visitenessun commentoMareKromium
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Craters-Rabe_Crater-PIA13728-PCF-LXTT-3.jpgInside Rabe Crater - Wintertime (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visitenessun commentoMareKromium
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Reull_Vallis-ESA-2-PCF-LXTT.jpgPseudo-Lake in Reull Vallis (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visiteLa "risposta" Lunexit, in Absolute Natural Colors, ad uno degli orrori più grandi "Made by ESA": un (brutto e pure - leggermente - sfuocato) Mars Express Frame, colorato in arancio-giallo, verde e azzurro (!) il quale fece gridare (i soliti tre pseudo-Ricercatori prezzolati) al "Lago di Reull" (guardate il frame che precede).
Nessun "Lago", Signori: solo un Canyon colmo di sabbie ferrose ed ossidate! Meditateci sopra...MareKromium
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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) 87 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
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SOL0454-Martian_Horizon-1-PCF-LXTT.jpgGusev's "Foggy" Horizon - Sol 454 (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visitenessun commentoMareKromium
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ZZ-Mercury-Global_View_of_the_Surface-PIA14378.jpgThe Cratered Surface of Mercury (Natural Colors; credits: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington)87 visiteThis color image reveals two of Mercury's named Craters, Basho and Bartok. Basho is the Dark-Rimmed Crater to the far left of the image, and Bartok is the bright yellow crater approximately in the center. Both Craters have visible Central Peaks, but Bartok's Peaks appear blue in this image, indicating they may be made of a different material that was unearthed by the large force of the impact.
This image was acquired as part of MDIS's color base map. The color base map is composed of WAC images taken through eight different narrow-band color filters and will cover more than 90% of Mercury's Surface with an average resolution of 1 Km/pixel (0,6 miles/pixel). The highest-quality color images are obtained for Mercury's Surface when both the Spacecraft and the Sun are overhead, so these images typically are taken with viewing conditions of low Incidence and Emission Angles.
Date acquired: June, 21st, 2011
Image Mission Elapsed Time (MET): 217134583, 217134599, 217134579
Image ID: 407077, 407081, 407076
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filters: 9 (1000 nanometers), 7 (750 nanometers), 6 (430 nanometers) as red-green-blue.
Center Latitude: 3,.68° South
Center Longitude: 221,4° East
Resolution: 1806 meters/pixel
Scale: Basho, the Dark-Rimmed Crater at far left, is approx. 74 Km in diameter.
Solar Incidence Angle: 51.4° (with the Sun about 38,6° above the Local Horizon)
Emission Angle: 0,6°
Sun-Target-Spacecraft (or "Phase") Angle: 51,6°MareKromium
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Aeolian_Features-Yardangs-PIA15310-PCF-LXTT.jpgYardangs in Northern Gordii Dorsum (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visiteOrbit Number: 44508
Latitude: 12,32° North
Longitude: 212,46° East
Instrument: VIS
Captured: December, 27th, 2011MareKromium
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Volcanic_Regions-Tharsis-Lava_Flows-PIA15362-PCF-LXTT.jpgLava Fields between Echus Chasma and Tharsis (Slightly Saturated Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visiteOrbit Number: 44743
Latitude: 11,6303° North
Longitude: 276,1480° East
Instrument: VIS
Captured: January, 15th, 2012
Mars Local Solar Time: 09:59 (Middle Morning Hours)
MareKromium
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Titan-N00188978-86-MF-EB-LXTT-IPF-2.jpgPossible Aurora at Titan (Superdefinition and Absolute Natural Colors; credits for the additional process. and color.: Elisabetta Bonora and Marco Faccin/Lunexit Team)87 visitenessun commentoMareKromium
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