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 2217/2237 Torna all'inizio Guarda foto precedente Guarda foto successiva Salta alla fine
The "Central Uplift" of Oudemans Crater (EDM - possible Natural Colors; credits: Lunexit)
This HiRISE image covers a portion of the Central Uplift of the 120-Km diameter Oudemans Crater.
Oudemans is located at the Western end of Valles Marineris and just South of the Great Canyon System by the Noctis Labyrinthus. 
Images from the Mars Orbital Camera (MOC) were the first to reveal that this large impact crater exposed Layered Rock in its Central Uplift Feature.
Such beautifully preserved Layered Rocks, although rare, are no surprise to planetary scientists. 

First, Layered Rocks exposed in the Central Uplifts are common in terrestrial impact structures. Secondly, there is abundant layering exposed in the nearby Valles Marineris Canyon System — a gash that exposes layering down to 7 Km beneath the mean Surface. 
This suggests that Layered Materials exist to great depths in the Subsurface, which is supported by the Oudemans Central Uplift observation.

The "Central Uplift" of Oudemans Crater (EDM - possible Natural Colors; credits: Lunexit)

This HiRISE image covers a portion of the Central Uplift of the 120-Km diameter Oudemans Crater.
Oudemans is located at the Western end of Valles Marineris and just South of the Great Canyon System by the Noctis Labyrinthus.
Images from the Mars Orbital Camera (MOC) were the first to reveal that this large impact crater exposed Layered Rock in its Central Uplift Feature.
Such beautifully preserved Layered Rocks, although rare, are no surprise to planetary scientists.

First, Layered Rocks exposed in the Central Uplifts are common in terrestrial impact structures. Secondly, there is abundant layering exposed in the nearby Valles Marineris Canyon System — a gash that exposes layering down to 7 Km beneath the mean Surface.
This suggests that Layered Materials exist to great depths in the Subsurface, which is supported by the Oudemans Central Uplift observation.

PSP_001414_2165_RED_abrowse.jpg PSP_003176_1745_RED_browse-00~0.jpg PSP_001578_2000-MF-LXT.jpg PSP_001666_1530_RED.jpg ESP_016173_2005_RED_abrowse-3.jpg
Informazioni sul file
Nome del file:PSP_001602_1700_red_01~0.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (3 voti):55555(Mostra dettagli)
Dimensione del file:340 KiB
Data di inserimento:Dic 15, 2009
Dimensioni:2112 x 2000 pixels
Visualizzato:56 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=25950
Preferiti:Aggiungi ai preferiti

Commento 1 a 1 di 1
Pagina: 1

walthari   [Dic 18, 2009 at 06:33 AM]
uno spaccato stratigrafico splendido con tanto di dislocazioni (al centro dell'immagine) definibili nell'ambito di una geodinamica superficiale attiva nel passato marziano.Gli angoli netti tra le stratificazioni dislocate dalle faglie e quelle inalterate indicano un'attività geologico-strutturale posteriore alla deposizione delle rocce sedimentarie in foto.
L'alternanza cromatica tra gli strati indica invece il verificarsi di almeno due tipi di fenomeni sedimentari differenti ma alternatosi con una certa regolarità.

Commento 1 a 1 di 1
Pagina: 1

 
 

Powered by Coppermine Photo Gallery