| Risultati della ricerca nelle immagini - "Labyrinthus" |
Adamas_Labyrinthus-PCF-LXTT.jpgAdamas Labyrinthus (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)125 visitenessun commentoMareKromium
|
|
Channel-Noctis_Labyrnthus-PIA13940-PCF-LXTT.jpgUnnamed Channel in Noctis Labyrinthus Region (Absolute Natural Colors; credits for the additional process. and coloring: Dr Paolo C. Fienga - Lunexit Team)211 visitenessun commentoMareKromium
|
|
ESP_014287_1685_RED_abrowse-00.jpgNoctis Labyrinthus (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)77 visiteThis image spans the floor and two walls of a pit in Noctis Labyrinthus, a System of deep, steep-walled Valleys on the Western Edge of Valles Marineris.
The Valleys themselves are tectonic features known as "Graben" (---> trench-like features that form in response to extension (or stretching) of the Crust). In the case of Noctis Labyrinthus, volcanic activity in the Tharsis Region may have formed a bulge, which then stretched and fractured the Crust above it.MareKromium
|
|
ESP_014287_1685_RED_abrowse-MF-LXTT.jpgNoctis Labyrinthus (EDM - possible True Colors; credits for the additional process. and color.: Dr Marco Faccin - Lunexit Team)83 visitenessun commentoMareKromium
|
|
ESP_014353_1685_RED_abrowse-01.jpgLight-Toned Deposits in Noctis Labyrinthus (EDM - Natural Colors; credits: Lunexit)78 visiteCRISM observations of this Region of the Noctis Labyrinthus formation have shown indications of Iron-bearing Sulfates and Phyllosilicate (such as "clay" ----> argilla) minerals.
HiRISE observations have revealed exposed layers which are possibly the sources of the signatures seen by CRISM.
In this image, the layering can be seen on the right side of the image.
On the lower left, instead, a large Dunefield which covers other beds can also be seen.MareKromium
|
|
ESP_018480_1725_RED_abrowse.jpgLight-toned Outcrops in Noctis Labyrinthus (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)106 visitenessun commentoMareKromium
|
|
ESP_022568_1730_RED_abrowse-PCF-LXTT.jpgFeatures of Noctis Labyrinthus (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)123 visitenessun commentoMareKromium
|
|
ESP_023359_1710_RED_abrowse-PCF-LXTT-00.jpgFeatures of Noctis Labyrinthus (CTX Frame - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)128 visiteMars Local Time: 14:01 (early afternoon)
Coord. (centered): 9,0 South Lat. and 264,1 East Long.
Spacecraft altitude: 280,8 Km (such as about 175,5 miles)
Original image scale range: 28,1 cm/pixel (with 1 x 1 binning) so objects ~ 84 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 23,8
Sun-Mars-Spacecraft (or "Phase") Angle: 53,8
Solar Incidence Angle: 30 (meaning that the Sun is about 60 above the Local Horizon)
Solar Longitude: 331,8 (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromium
|
|
ESP_023359_1710_RED_abrowse-PCF-LXTT-01.jpgFeatures of Noctis Labyrinthus (EDM - Enhanced Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)146 visiteMars Local Time: 14:01 (early afternoon)
Coord. (centered): 9,0 South Lat. and 264,1 East Long.
Spacecraft altitude: 280,8 Km (such as about 175,5 miles)
Original image scale range: 28,1 cm/pixel (with 1 x 1 binning) so objects ~ 84 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 23,8
Sun-Mars-Spacecraft (or "Phase") Angle: 53,8
Solar Incidence Angle: 30 (meaning that the Sun is about 60 above the Local Horizon)
Solar Longitude: 331,8 (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromium
|
|
ESP_024427_1740-PCF-LXTT-00.jpgFeatures of Noctis Labyrinthus (CTX Frame "A" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)200 visiteMars Local Time: 14:22 (early afternoon)
Coord. (centered): 6,0 South Lat. and 267,2 East Long.
Spacecraft altitude: 273,4 Km (such as about 170,9 miles)
Original image scale range: 27,3 cm/pixel (with 1 x 1 binning) so objects ~ 82 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 16,1
Phase Angle: 52,4
Solar Incidence Angle: 37 (meaning that the Sun is about 53 above the Local Horizon)
Solar Longitude: 14,3 (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromium
|
|
ESP_024427_1740-PCF-LXTT-01.jpgFeatures of Noctis Labyrinthus (CTX Frame "B" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visiteMars Local Time: 14:22 (early afternoon)
Coord. (centered): 6,0 South Lat. and 267,2 East Long.
Spacecraft altitude: 273,4 Km (such as about 170,9 miles)
Original image scale range: 27,3 cm/pixel (with 1 x 1 binning) so objects ~ 82 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 16,1
Phase Angle: 52,4
Solar Incidence Angle: 37 (meaning that the Sun is about 53 above the Local Horizon)
Solar Longitude: 14,3 (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromium
|
|
NoctisLabyrinthus.jpgNoctis Labyrinthus (Natural Colors + MULTISPECTRUM; credits: ESA & Lunexit)143 visiteThis image was taken by the High-Resolution Stereo Camera (HRSC), onboard ESAs Mars Express imaged the Noctis Labyrinthus Region, the Labyrinth of the Night on Mars.
The HRSC took these pictures on 25 June 2006 in orbit 3155, with a ground resolution of approx. 16 mt/pixel.MareKromium
|
|
| 25 immagini su 3 pagina(e) |
1 |
|
