Sary:Moon PIA00303.jpg

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Original Caption Released with Image

About 50,000 Clementine images were processed to produce the four orthographic views of the Moon. Images PIA00302, PIA00303, PIA00304, and PIA00305 show albedo variations (normalized brightness or reflectivity) of the surface at a wavelength of 750 nm (just longward of visible red). The image projection is centered at 0 degree latitude and 90 degrees longitude. The dark albedo features Mare Smythii (image center) and Mare Marginis (above Smythii) are just visible from Earth on the extreme eastern edge of the lunar nearside. Maria Crisium (directly west of Marginis) and Mare Fecunditatis (southwest of Crisium) are familiar nearside features as seen from Earth. Maria regions are believed to be large basins formed by impacts from cosmic projectiles later filled by basaltic lava flows from volcanic eruptions. Basaltic lava flows on the basin floors give maria their dark albedo appearance.

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From Wikipedia.

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Daty sy orasaritapakaHabeMpikambanaresaka
ankehitriny4 Novambra 2014 à 13:34Vignette ho an'ny 4 Novambra 2014 à 13:341 719 × 1 719 (297 kio)Buzz-tardisWrongly rotated. Reverted to version as of 01:06, 1 January 2006
23 Febroary 2013 à 21:02Vignette ho an'ny 23 Febroary 2013 à 21:021 712 × 1 712 (295 kio)RotatebotBot: Image rotated by 180°
1 Janoary 2006 à 01:06Vignette ho an'ny 1 Janoary 2006 à 01:061 719 × 1 719 (297 kio)Pringles==Original Caption Released with Image== About 50,000 Clementine images were processed to produce the four orthographic views of the Moon. Images PIA00302, PIA00303, [[:I

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