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 16395/25353 Torna all'inizio Guarda foto precedente Guarda foto successiva Salta alla fine
Valleys Near Ganges Chasma (natural colors; credits: Lunexit)
Several valleys as well as light-toned material are visible in this HiRISE image of a portion of Allegheny Vallis along the Plains West of Ganges Chasma.

The main valley, which starts in a pit called Ophir Cavus and extends for 155 Km into Ganges Chasma, is visible in the center of the image from left to right. Smaller and shallower valleys can be seen mostly to the north (Sx) of the image. 
The observation that there are several valleys here suggests that water flowed for some extended period of time or multiple times in order to change direction and produce different valleys. 

Light-toned material is visible on the upper surfaces of the plains but not inside the valleys, perhaps because smaller amounts of water could interact with the lava plains at these higher elevations, while in the valleys larger amounts of flowing water eroded and removed the plains unit. The light-toned nature on the upper surfaces could have resulted from chemical alteration of the lava plains or deposition of evaporites as the water disappeared and left behind minerals once carried in the water.
Parole chiave: Mars from orbit - Ganges Chasma

Valleys Near Ganges Chasma (natural colors; credits: Lunexit)

Several valleys as well as light-toned material are visible in this HiRISE image of a portion of Allegheny Vallis along the Plains West of Ganges Chasma.

The main valley, which starts in a pit called Ophir Cavus and extends for 155 Km into Ganges Chasma, is visible in the center of the image from left to right. Smaller and shallower valleys can be seen mostly to the north (Sx) of the image.
The observation that there are several valleys here suggests that water flowed for some extended period of time or multiple times in order to change direction and produce different valleys.

Light-toned material is visible on the upper surfaces of the plains but not inside the valleys, perhaps because smaller amounts of water could interact with the lava plains at these higher elevations, while in the valleys larger amounts of flowing water eroded and removed the plains unit. The light-toned nature on the upper surfaces could have resulted from chemical alteration of the lava plains or deposition of evaporites as the water disappeared and left behind minerals once carried in the water.

PHOE-SOL119-MF-LXT.jpg SaturnSpaceN00115280-N00115290.gif PHOE-SOL122-lg35921-35922-35923-2.jpg 20000608.jpg Psp_009390_2595_red.jpg
Informazioni sul file
Nome del file:Psp_009578_1715_red.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (7 voti):55555(Mostra dettagli)
Parole chiave:Mars / from / orbit / - / Ganges / Chasma
Copyright:NASA/JPL/Univ. of Arizona e Lunar Explorer Italia per il processing addizionale e la colorizzazione
Dimensione del file:975 KiB
Data di inserimento:Ott 02, 2008
Dimensioni:5770 x 2048 pixels
Visualizzato:59 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=22062
Preferiti:Aggiungi ai preferiti
 
 

Powered by Coppermine Photo Gallery