| Risultati della ricerca nelle immagini - "Chaos" |
51-Smart-1_25_August_0815UTC_H.jpgGoing Down56 visiteCaption ESA originale:"This image of the Lunar Surface was taken on 25 August at 10:08 CEST (08:15 UT) by the star tracker (attitude camera) on board ESA’s SMART-1, from a distance of 59 Km above the Moon Surface. The spacecraft was travelling at a speed of 2 Km/sec.
The image is slightly smeared as the spacecraft is moving at high speed and at low altitude. This image was taken as a test, meaning that the spacecraft pointing was not optimised for star tracker imaging.
The Moon features on the photo still have to be identified".
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APOLLO 16 AS 16-4530.jpgAS 16-4530 - Seconday impact craters, faults and rifles54 visiteLinear features of external and internal origin are contrasted in this area of Southernmost Mare Tranquillitatis.
The North-trending line of overlapping, very irregular craters along the East edge of the picture is clearly a chain of secondary impact craters. Its trend is radial to Theophilus, a large crater of early Copernican age that lies about 105 Km south of this area. The flaring shapes of some of the craters and their state of preservation also suggest that Theophilus is the primary crater. The narrow, straight rifle or graben that extends westward across the picture is clearly of internal origin. It formed when tensional forces ruptured the crust, causing the floor of the rifle to subside along faults.
Straight rifles are commonly the sites of volcanic cones or of blankets of volcanic ejecta; however, there are no signs of volcanism here that can be related to this rifle.
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Aram_Chaos-PIA13744.jpgFeatures of Aram Chaos (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)124 visitenessun commentoMareKromium
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Aram_Chaos-R2200155-10-PCF-LXTT.jpgFeatures of Aram Chaos (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 185 visitenessun commentoMareKromium
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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)84 visitenessun commentoMareKromium
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Channels-Aram_Chaos-PIA13336.jpgChannels in Aram Chaos (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)95 visitenessun commentoMareKromium
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Channels_and_Chaotic_Terrain-DaoVallis-PCF-LXTT.jpgChannels and Chaotic Terrain in Dao Valles (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)66 visitenessun commentoMareKromium
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Chaos-Aurorae_Chaos-PIA08485-PCF-LXTT-1.jpgLandslide in Aurorae Chaos (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)179 visiteImage information: VIS instrument;
Latitude: 6,7° South Lat.;
Longitude: 328,8° East;
Resolution: 18 meter/pixel. MareKromium
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Chaos-Aurorae_Chaos-PIA08485-PCF-LXTT-2.jpgLandslide in Aurorae Chaos (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)177 visiteImage information: VIS instrument;
Latitude: 6,7° South;
Longitude: 328,8° East;
Resolution: 18 meter/pixel. MareKromium
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Chaos_Terrain-PCF-LXTT.jpgChaos Terrain (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)68 visitenessun commentoMareKromium
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Chaotic_Terrain-Aram_Chaos-PIA02175-00.jpgFeatures of Aram Chaos (Original NASA/JPL/ASU b/w Frame)56 visiteCaption NASA:"This image of part of Aram Chaos shows two different surface textures with distinctly different brightnesses. The lighter layer appears to be on top (therefore younger) than the darker surface".
Image information: VIS instrument;
Latitude: 2,1° North;
Longitude: 338,7° East;
Resolution: 17 meter/pixel.
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Chaotic_Terrain-Aram_Chaos-PIA02175-01.jpgFeatures of Aram Chaos (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 160 visiteCaption NASA:"This image of part of Aram Chaos shows two different surface textures with distinctly different brightnesses. The lighter layer appears to be on top (therefore younger) than the darker surface".
Image information: VIS instrument;
Latitude: 2,1° North;
Longitude: 338,7° East;
Resolution: 17 meter/pixel.
MareKromium
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