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Geologic Contacts in Juventae Chasma (MULTISPECTRUM-2; credits Lunexit)
Many of the Troughs of Valles Marineris contain mounds composed of light-toned Layered Deposits and Scientists have been debating both the origin of these Layered Deposits and their age of deposition relative to the Troughs themselves. 
Some scientists think that the Layered Deposits formed first and then were covered by lava flows that make up the plains. Later, formation of the troughs of Valles Marineris created large openings through the plains that exposed the buried Layered Deposits. 
Others have argued that the light-toned Layered Deposits formed after the Troughs and filled up portions of the canyons. 
The chaotic terrain in Juventae is believed to have formed when subsurface water in the ground flowed away, causing collapse of the ground and leaving behind numerous hills along the floor of the Trough.

In this HiRISE image, the geologic contacts between the wallrock (darker units on the left - Sx - of the image), light-toned Layered Deposits, and darker hills of the chaotic terrain are visible. By studying the image, scientists hope to determine what are the relative ages of these different units in order to decipher the Geologic History of this Region. 

(note: a stereo image of this location could be even more helpful because it will show the three-dimensional relationships between the different units, thus revealing more information about their relative ages)

Parole chiave: Mars from orbit - Juventae Chasma Region

Geologic Contacts in Juventae Chasma (MULTISPECTRUM-2; credits Lunexit)

Many of the Troughs of Valles Marineris contain mounds composed of light-toned Layered Deposits and Scientists have been debating both the origin of these Layered Deposits and their age of deposition relative to the Troughs themselves.
Some scientists think that the Layered Deposits formed first and then were covered by lava flows that make up the plains. Later, formation of the troughs of Valles Marineris created large openings through the plains that exposed the buried Layered Deposits.
Others have argued that the light-toned Layered Deposits formed after the Troughs and filled up portions of the canyons.
The chaotic terrain in Juventae is believed to have formed when subsurface water in the ground flowed away, causing collapse of the ground and leaving behind numerous hills along the floor of the Trough.

In this HiRISE image, the geologic contacts between the wallrock (darker units on the left - Sx - of the image), light-toned Layered Deposits, and darker hills of the chaotic terrain are visible. By studying the image, scientists hope to determine what are the relative ages of these different units in order to decipher the Geologic History of this Region.

(note: a stereo image of this location could be even more helpful because it will show the three-dimensional relationships between the different units, thus revealing more information about their relative ages)

PSP_008598_2155_RED_abrowse~0.jpg PSP_008681_2550_RED.jpg PSP_008708_1780_RED_abrowse.jpg PSP_008710_1710_red-PCF-LXTT.jpg PSP_008774_1755_RED_abrowse-PCF-LXTT.jpg
Informazioni sul file
Nome del file:PSP_008708_1780_RED_abrowse.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (6 voti):55555(Mostra dettagli)
Parole chiave:Mars / from / orbit / - / Juventae / Chasma / Region
Copyright:NASA/JPL/University of Arizona e Lunar Explorer Italia per l'elaborazione addizionale e la colorizzazione MULTISPECTRUM del frame
Dimensione del file:1063 KiB
Data di inserimento:Lug 15, 2008
Dimensioni:6682 x 2048 pixels
Visualizzato:54 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=21099
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