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Dunes_and_DD_Tracks-PIA13538-EB-LXTT-001.jpg
Dunes_and_DD_Tracks-PIA13538-EB-LXTT-001.jpgSouthern Dunes and DD Tracks (Possible True Colors; credits for the additional process. and color.: Elisabetta Bonora - Lunexit Team)85 visitenessun commentoMareKromium
Craters-Bacolor_Crater-PIA13664-PCF-LXTT.jpg
Craters-Bacolor_Crater-PIA13664-PCF-LXTT.jpgBacolor Crater (Absolute Natural Colors; additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)85 visiteCaption NASA:"Bacolor Crater is a magnificent Impact Surface Feature about 20 Km (approx. 12 miles) wide. The lines on the Ejecta Blanket surrounding the Crater rim come from a surge of superheated gas and debris flying outward in the wake of the Meteorite impact that created the Crater.

This view combines images taken during the period from September 2002 to October 2005 by the Thermal Emission Imaging System instrument on NASA's Mars Odyssey orbiter. It is part of a special set of images marking the occasion of Odyssey becoming the longest-working Mars Spacecraft in history.
The pictured location on Mars is 33° North Lat. and 118,6° East Long.".
MareKromium
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ZZ-ZZ-ZZ-ZZ-20100727_LORRIM_lg.jpgOn the Way to Pluto: Messier 785 visiteCaption NASA:"The New Horizons team calibrates the Long Range Reconnaissance Imager (LORRI) by taking pictures of the Open Star Cluster Messier 7 (M 7). This is the first LORRI image of M 7 taken during Annual Checkout (ACO); the 100-millisecond manual exposure was taken on June 25, 2010. A preliminary comparison of this image to a 2008 LORRI picture of M7 indicated no degradation or change in LORRI's performance".MareKromium
Volcanoes-Olympus_Mons-PIA13713.jpg
Volcanoes-Olympus_Mons-PIA13713.jpgPortion of the Northern Escarpment of Olympus Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)85 visitenessun commentoMareKromium
PSP_003830_1740_RED_abrowse-02.jpg
PSP_003830_1740_RED_abrowse-02.jpgLayered Bedrock in Candor Chasma (EDM n.2 - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)85 visitenessun commentoMareKromium
SOL1897-2N294770864EFFB1CNP0354R0M1.jpg
SOL1897-2N294770864EFFB1CNP0354R0M1.jpgRocky Horizon - Sol 1897 (Absolute Natural Colors; credits for the additional process. and color.: Elisabetta Bonora and Paolo C. Fienga - Lunexit Team)85 visitenessun commentoMareKromium
ZZ-Mercury-Rupes-PIA13748-0.jpg
ZZ-Mercury-Rupes-PIA13748-0.jpgBeagle Rupes and Impact Craters Sveinsdottir, Izquierdo and Kunisada (Context Frame)85 visiteWhen MESSENGER first flew by Mercury on January, 14th, 2008, MDIS acquired images of a large portion of Mercury's Surface that had never previously been seen by Spacecraft. This mosaic of NAC images shows some of the Geologic Features discovered during that first fly-by that have been subsequently named: the curving cliff face of Beagle Rupes, the elongated crater Sveinsdottir and the craters Izquierdo and Kunisada flooded with Lava.

This year, the MESSENGER spacecraft is positioned once again to visit the Solar System's Innermost Planet. However, this time, the Spacecraft won't just pass by. On March 18, 2011, a 15-minute maneuver will place MESSENGER in orbit around Mercury, making it the first Spacecraft ever to do so. The MESSENGER Mission will then begin an extensive year-long science campaign to unravel Mercury's mysteries.

Date Acquired: January, 14th, 2008
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Scale: Izquierdo Crater is approx. 170 Km (105,57 miles) in diameter
MareKromium
OPP-SOL2482-1-GB-LXTT.jpg
OPP-SOL2482-1-GB-LXTT.jpgBerries and Rocks - Sol 2482 (Absolute Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)85 visitenessun commentoMareKromium
Ganges_Chasma-20080318a.jpg
Ganges_Chasma-20080318a.jpgFeatures of Ganges Chasma (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)85 visitenessun commentoMareKromium
OPP-SOL1045-MI-MF-LXTT-3.jpg
OPP-SOL1045-MI-MF-LXTT-3.jpgOn the Surface of Meridiani Planum... - Sol 1045 (Superdefinition; credits for the additional process. and color.: Dr Marco Faccin - Lunexit Team)85 visitenessun commentoMareKromium
Channel-20090619a-PCF-LXTT.jpg
Channel-20090619a-PCF-LXTT.jpgSouthern Drainage Channel (Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)85 visitenessun commentoMareKromium
Volcanoes-Hecates_Tholus-Channels-20080702a-PCF-LXTT.jpg
Volcanoes-Hecates_Tholus-Channels-20080702a-PCF-LXTT.jpgChannels on Hecates Tholus (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)85 visitenessun commentoMareKromium
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