Inizio Registrati Login

Elenco album Ultimi arrivi Ultimi commenti Più viste Più votate Preferiti Cerca

Inizio > MARS > Mars Reconnaissance Orbiter (MRO)
Ritorna alla pagina delle miniature FILE 95/2235 Torna all'inizio Guarda foto precedente Guarda foto successiva Salta alla fine
Distorted Layers in the SPLD (extra-detail mgnf - MULTISPECTRUM; credits: Lunexit)
This enhanced image (1,2 Km or 0.7 miles across) shows a section of the South Polar Layered Deposits, which are an accumulation of layers consisting mostly of water ice and dust. Perhaps their closest analog on Earth would be the Ice Caps of Greenland and Antarctica.

This image is particularly interesting because the layers are not flat-lying but rather appear "wavy" (---> ondeggianti). 
This appearance could partly be an “illusion” due to erosion after the flat-lying layers were deposited. In that case, the wavy appearance is due to the fact that the layer edges are wavy, going into and out of the plane of the outcrop exposing the layers.

Alternatively, this waviness could be due to deformation of the layers folding caused by flow of the ice. 
Here, the flow probably occurred long ago since current temperatures are too low to allow the ice to flow at a significant rate.
Parole chiave: Mars from orbit - South Polar Layered Deposits

Distorted Layers in the SPLD (extra-detail mgnf - MULTISPECTRUM; credits: Lunexit)

This enhanced image (1,2 Km or 0.7 miles across) shows a section of the South Polar Layered Deposits, which are an accumulation of layers consisting mostly of water ice and dust. Perhaps their closest analog on Earth would be the Ice Caps of Greenland and Antarctica.

This image is particularly interesting because the layers are not flat-lying but rather appear "wavy" (---> ondeggianti).
This appearance could partly be an “illusion” due to erosion after the flat-lying layers were deposited. In that case, the wavy appearance is due to the fact that the layer edges are wavy, going into and out of the plane of the outcrop exposing the layers.

Alternatively, this waviness could be due to deformation of the layers folding caused by flow of the ice.
Here, the flow probably occurred long ago since current temperatures are too low to allow the ice to flow at a significant rate.

PSP_006528_1120_RED_abrowse-01.jpg PSP_006528_1120_RED_abrowse-02.jpg PSP_005418_1075_RED_abrowse-01.jpg Phobos_Deimos-PIA10117.jpg PSP_005456_1650_RED_abrowse-01.jpg
Informazioni sul file
Nome del file:PSP_005418_1075_RED_abrowse-01.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (7 voti):55555(Mostra dettagli)
Parole chiave:Mars / from / orbit / - / South / Polar / Layered / Deposits
Copyright:NASA/JPL/University of Arizona e Lunar Explorer Italia per l'ingrandimento, l'elaborazione addizionale e la colorizzazione del frame
Dimensione del file:349 KiB
Data di inserimento:Dic 28, 2007
Dimensioni:1500 x 678 pixels
Visualizzato:54 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=19071
Preferiti:Aggiungi ai preferiti
 
 

Powered by Coppermine Photo Gallery