| Ultimi arrivi - THE LUNAR EXPLORER ARCHIVES |
ORIGINAL NASA APOLLO 15 - AS15-88-12007.jpgAS 15-88-12007 - Dancing in the night... (1)69 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 14 - AS14-74-10219.jpgAS 14-74-10219 - Blue reflections in the darkness77 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 14 - AS14-70-9837.jpgAS 14-70-9837 - Transient Lunar Phoenomoena? (3)100 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 14 - AS14-70-9836.jpgAS 14-70-9836 - Transient Lunar Phoenomoena? (2)87 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 14 - AS14-70-9835.jpgAS 14-70-9835 - Transient Lunar Phoenomoena? (1)73 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 14 - AS14-66-9324.jpgAS 14-66-9324 - A basket full of gold?!?117 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 12 - AS12-51-7552.jpgAS 12-51-7552 - Alien Spaceship or just a reflection? (1)79 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 12 - AS12-51-7553.jpgAS 12-51-7553 - Alien Spaceship or just a reflection? (2)66 visitenessun commentoFeb 26, 2005
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ORIGINAL NASA APOLLO 12 - AS12-47-7010.jpgAS 12-47-7010 - What is that? (2)108 visiteFeb 26, 2005
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ORIGINAL NASA APOLLO 12 - AS12-47-7009.jpgAS 12-47-7009 - What is this? (1)89 visiteFeb 26, 2005
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Volcanoes-Arsia_Mons-E05-1721_1722_arsia100.jpgArsia Mons Volcano and "spiral clouds" (Natural Colors; credits: NASA/JPL/MSSS)113 visiteCaption NASA originale:"One of the benefits of the MGS-MOC Extended Mission is the opportunity to observe how the planet's weather changes during a second full martian year. This picture of Arsia Mons was taken on June 19, 2001; Southern Spring equinox occurred the same day. Arsia Mons is a volcano nearly large enough to cover the state of New Mexico. On this particular day (the first day of Spring), the MOC wide angle cameras documented an unusual spiral-shaped cloud within the 110 Km diameter caldera - such as the summit crater - of the giant volcano. Because the cloud is bright both in the red and blue images acquired by the wide angle cameras, it probably consisted mostly of fine dust grains. The cloud's spin may have been induced by winds off the inner slopes of the volcano's caldera walls resulting from the temperature differences between the walls and the caldera floor, or by a vortex as winds blew up and over the caldera. Similar spiral clouds were seen inside the caldera for several days; we don't know if this was a single cloud that persisted throughout that time or one that regenerated each afternoon".Feb 21, 2005
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Craters-Unnamed_Crater_with_Dark_Streaks-2003_08.jpgDark Slope Streaks on the edge of an Unnamed Crater (Saturated Natural Colors; credits: NASA/MGS/MSSS)107 visiteCaption NASA originale:"This June 2003 MGS-MOC image shows a crater rim mantled with fine dust near 7.6°N, 171.8°W. Occasional avalanches of dust have created dark streaks that are tapered at their source and broaden downslope.
A suite of particularly large streaks are seen in the lower right quarter of the picture. The MOC narrow angle camera does not take color images; this full-resolution (1,5 m/pixel; 5 ft/pixel) picture has been "colorized" using data from a previous color image of Mars.
Sunlight illuminates this scene from the lower left".Feb 21, 2005
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