Inizio Registrati Login

Elenco album Ultimi arrivi Ultimi commenti Più viste Più votate Preferiti Cerca

Ultimi arrivi
Dunefields-Rabe_Crater_Dunefield-PIA14782-PCF-LXTT.jpg
Dunefields-Rabe_Crater_Dunefield-PIA14782-PCF-LXTT.jpgDunefield in Rabe Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)155 visiteOrbit Number: 42917;
Latitude: 43,768° South;
Longitude: 35,056° East;
Instrument: VIS;
Captured: August, 18th, 2011.

MareKromiumSet 24, 2011
Volcanic_Features-Lava_Flows-DP-PIA14784-PCF-LXTT.jpg
Volcanic_Features-Lava_Flows-DP-PIA14784-PCF-LXTT.jpgLava Flows in Daedalia Planum (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 131 visiteOrbit Number: 42985;
Latitude: 22,427° South;
Longitude: 237,499° East;
Instrument: VIS;
Captured: August, 23rd, 2011;
Mars Local Time (M.L.T.): 15:02 (Early Afternoon)

MareKromiumSet 24, 2011
Craters-Lau_Crater-M07_4748_4749-PCF-LXTT-01.jpg
Craters-Lau_Crater-M07_4748_4749-PCF-LXTT-01.jpgBizarre-looking "Dark Spot" near Lau Crater (EDM - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)204 visiteLa chiazza scura e senza nome che la NASA stessa definisce di "natura sconosciuta" potrebbe essere l'evidenza, secondo alcuni Ricercatori Americani ed Europei, di una minuscola area di Marte con "vegetazione". Si, avete letto bene: vegetazione, di un qualche tipo. In un'altra immagine della stessa zona, la macchia scura appare di colore verdastro e non nero. E' del tutto evidente che i sostenitori dell'idea che si tratti di vegetazione (si, ma che tipo?) ritengono che l'immagine NASA sia manipolata, mentre la NASA sostiene che i colori che vedete sono "almost real" e quindi la macchia scura, comunque, non è (nè potrebbe comunque essere) vegetazione.
Questi sono i dati e le informazioni disponibili: come vedete, c'è materiale su cui riflettere...
MareKromiumSet 23, 2011
Craters-Lau_Crater-M07_4748_4749-PCF-LXTT-00.jpg
Craters-Lau_Crater-M07_4748_4749-PCF-LXTT-00.jpgFeatures and Proximities of Lau Crater (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 183 visiteCaption NASA:"The Martian Southern Hemisphere was nearly 2 months into its Spring Season when this picture was taken by the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) on September 25, 1999. The scene covers a vast, Frost-coated Plain located South of the martian Antarctic Circle. The icy Terrain in the image has an almost pastel-like character, owing to the mixture of reddish Dust both on, in, and under the white Frost. The Frost - mostly frozen water at this time of year - is left over from Winter, which ended on August 2, 1999. One Martian Year is about 687 Earth days long, thus each of the Planet's 4 seasons are nearly twice as long as seasons on Earth.
The largest Crater visible in the upper left of the frame is Lau Crater, named for the Danish Astronomer, Hans E. Lau (1879-1918). The Dark Spot near the center of the image has no name, and its origin is unknown. The picture covers an area about 1.020 Km across by approximately 1.240 Km down.
The center is located near 76° South Lat. and 97° West Long.; North is toward the upper right. Sunlight illuminates the scene from the upper left".
MareKromiumSet 23, 2011
ESP_023173_1405_RED_abrowse-PCF-LXTT.jpg
ESP_023173_1405_RED_abrowse-PCF-LXTT.jpgGullies and Lobate Material in an Unnamed Crater located in Nereidum Montes (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)202 visiteMars Local Time: 14:21 (Early Afternoon)
Coord. (centered): 39,1° South Lat. and 309,0° East Long.
Spacecraft altitude: 260,5 Km (such as about 162,8 miles)
Original image scale range: 26,1 cm/pixel (with 1 x 1 binning) so objects ~ 78 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 15,4°
Sun-Mars-Spacecraft (or "Phase") Angle: 28,5°
Solar Incidence Angle: 40° (meaning that the Sun is about 50° above the Local Horizon)
Solar Longitude: 323,8° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromiumSet 22, 2011
OPP-SOL2718-1P369486720EFFBN19P2285L2M1-PCF-LXTT.jpg
OPP-SOL2718-1P369486720EFFBN19P2285L2M1-PCF-LXTT.jpgFeatures of Endeavour Crater - Sol 2718 (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 185 visitenessun commento4 commentiMareKromiumSet 22, 2011
OPP-SOL2721-1P369739465ESFBN19P2546L6M1-PCF-LXTT.jpg
OPP-SOL2721-1P369739465ESFBN19P2546L6M1-PCF-LXTT.jpgEndeavour's Inner Rim - Sol 2721 (Enhanced Absoolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)168 visitenessun commentoMareKromiumSet 22, 2011
OPP-SOL2704-1N368228268EFFBMP3P1725L0M1-PCF-LXTT.jpg
OPP-SOL2704-1N368228268EFFBMP3P1725L0M1-PCF-LXTT.jpgRover Tracks - Sol 2704 (Enhanced Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)145 visitenessun commentoMareKromiumSet 22, 2011
OPP-SOL2704-1N368228183EFFBMP3P1725R0M1-PCF-LXTT.jpg
OPP-SOL2704-1N368228183EFFBMP3P1725R0M1-PCF-LXTT.jpgTAU Monitoring - Sol 2704 (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)144 visitenessun commentoMareKromiumSet 22, 2011
Aeolian_features-Yardangs-2-s_015_050504_0143_4_3d_01_Yardangs_FAZ-PCF-LXTT.jpg
Aeolian_features-Yardangs-2-s_015_050504_0143_4_3d_01_Yardangs_FAZ-PCF-LXTT.jpgWind-Lanes (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)215 visiteCaption ESA originale:"Loose sand fragments were transported by wind, and impacted on the Bedrock, slowly removing parts of the Surface, like a sand-blaster. If the winds blow in the same direction for a long enough period, ‘Wind-Lanes’, as shown in the picture, can occur. On Earth, the remnants of these features which have not been eroded away are called ‘Yardangs’. Where the Surface consists of more resistant material, the force of the wind may not be strong enough to cause this sand-blasting. This might be the reason for the three flat regions (the first in the foreground on the left, and the other two on the top right), which measure about 17 by 9 Km".MareKromiumSet 22, 2011
Valles_Marineris-MRO-PCF-LXTT.jpg
Valles_Marineris-MRO-PCF-LXTT.jpgFeatures of Valles Marineris (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 179 visitenessun commentoMareKromiumSet 22, 2011
OPP-SOL287-01.jpg
OPP-SOL287-01.jpgEndurance Inner Rim - Sol 287 (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)136 visitenessun commentoMareKromiumSet 21, 2011
25353 immagini su 2113 pagina(e) 1 - 171 172 173 174 175 176 177 178 179 180 - 2113

 
 

Powered by Coppermine Photo Gallery