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111 - Polar Areas: Views of the South Pole
The spin axis of the Moon is nearly vertical (inclined 1,6°) to the ecliptic plane (the plane of its orbit around the Sun), in marked contrast to the Earth (axis inclination 23,5°). However, even this small inclination means that the hemispheres of the Moon experience seasons as the Pole tracks toward and away from the Sun. Clementine started its lunar mapping in the dead of Southern Winter (axis away from the Sun), but by the 2nd month of mapping, the axis had begun to point closer in that direction. These two mosaics show the difference in lighting conditions between the first month of mapping (left, maximum winter) and the second month's coverage (right, toward the solstice). 

Careful examination of the two mosaics reveals some slight shadow changes; note in particular the shadows that cover the floors of the craters Amundsen and Scott (large central peak crater at about 3 o'clock and the crater just above it). However, the large region of permanent shadow near the center of the mosaics discovered by Clementine remains virtually unchanged in the two mosaics. 
Parole chiave: The Lunar Poles

111 - Polar Areas: Views of the South Pole

The spin axis of the Moon is nearly vertical (inclined 1,6°) to the ecliptic plane (the plane of its orbit around the Sun), in marked contrast to the Earth (axis inclination 23,5°). However, even this small inclination means that the hemispheres of the Moon experience seasons as the Pole tracks toward and away from the Sun. Clementine started its lunar mapping in the dead of Southern Winter (axis away from the Sun), but by the 2nd month of mapping, the axis had begun to point closer in that direction. These two mosaics show the difference in lighting conditions between the first month of mapping (left, maximum winter) and the second month's coverage (right, toward the solstice).

Careful examination of the two mosaics reveals some slight shadow changes; note in particular the shadows that cover the floors of the craters Amundsen and Scott (large central peak crater at about 3 o'clock and the crater just above it). However, the large region of permanent shadow near the center of the mosaics discovered by Clementine remains virtually unchanged in the two mosaics.

081-The Moon from Clem-SouthPole.jpg 082-The Moon from Clem-NorthPole.jpg 035-The Moon from Clem-PolarAreas.jpg 034-The Moon from Clem-PolarAreas.jpg 040-The Moon from Clem-Apollo 16 LandingSite.jpg
Informazioni sul file
Nome del file:035-The Moon from Clem-PolarAreas.jpg
Nome album:The Clementine Files
Valutazione (3 voti):55555(Mostra dettagli)
Parole chiave:The / Lunar / Poles
Copyright:Ballistic Missile Defense Organization - Strategic Defense Initiative Organization and NASA - Clementine Mission
Dimensione del file:460 KiB
Data di inserimento:Ott 29, 2005
Dimensioni:1979 x 1436 pixels
Visualizzato:57 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=13942
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