Fichier:Moon PIA00304.jpg

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Kiɖe tɛɛ takayaɣ ‎(Kpaɣna pɩkɩsɛlɩ 1 719 nɛ pɩtalɩ 1 719 ñɩŋgʋ, takayaɣ walanzɩ : 311 kio, MIME akɩlɩ : image/jpeg)

Takayaɣ kanɛ kalɩna Wikimedia Commons. Tamasɩ lɛɛsɩ pɩzɩɣ palabɩna-kɛ nɛ tʋmɩyɛ. Pataaɖɩ kɛ-kɛdʋʋ tɔm ka-takayɩhayʋʋ ngʋ kɩkɛdʋʋ kɔ-tɔm yɔ nɛ pɩ-tɛɛ.

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Kɛdɩtʋ
English: 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 180 degrees longitude. Mare Moscoviense (dark albedo feature upper left of image center) and South Pole-Aitken Basin (dark feature at bottom) represent maria regions largely absent on the lunar farside. The Clementine altimeter showed Aitken Basin to consist of a topographic rim about 2500 km in diameter, an inner shelf ranging from 400 to 600 km in width, and an irregular depressed floor about 12 km in depth.
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Attention :
  • Near side
    Near side
  • 90 degrees East
    90 degrees East
  • Far side
    Far side
  • 90 degrees West
    90 degrees West

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Efemiye nɛ ñɩɣtʋTampɔɔWalanzɩLabɩnayʋTɔm taa nuutuu
lɛlɛɛyɔ1 Kɔlaɣ fenaɣ 2006 à 01:081 Kɔlaɣ fenaɣ 2006 à 01:08 ñɔɔzɩtʋ kɩlɛɣzɩtʋ tɛ tampɔɔ1 719 × 1 719 (311 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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