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 1551/2237 Torna all'inizio Guarda foto precedente Guarda foto successiva Salta alla fine
Volcanic Vent, East of Pavonis Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit)  
This image shows an Equatorial Volcanic Vent. A Volcanic Vent is an opening in the Crust of a Planet that emits Lava (such as "molten rock") and Volcanic Gases. The rough texture of the Plains surrounding the Vent is indicative of Lava.

There is a large number of snake-like features emanating from the Vent. The parallel lines that outline the features are "Levees", which mark the edges of Channels that carried molten Lava. As Lava flows, it moves slowest at its edges and bottom because the Lava sticks to the non-flowing rocks; as a consequence of this event, the lava slows down,  cools off and, in the end, it hardens.

Levees, on their side, form when the sides of the Lava Flow harden but the center of it keeps moving. As the eruption episode ends, and the Lava drains, the center is left lower than the sides producing these high-standing structures.
Parole chiave: Mars from orbit - Volcanic Features - Vent

Volcanic Vent, East of Pavonis Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit)

This image shows an Equatorial Volcanic Vent. A Volcanic Vent is an opening in the Crust of a Planet that emits Lava (such as "molten rock") and Volcanic Gases. The rough texture of the Plains surrounding the Vent is indicative of Lava.

There is a large number of snake-like features emanating from the Vent. The parallel lines that outline the features are "Levees", which mark the edges of Channels that carried molten Lava. As Lava flows, it moves slowest at its edges and bottom because the Lava sticks to the non-flowing rocks; as a consequence of this event, the lava slows down, cools off and, in the end, it hardens.

Levees, on their side, form when the sides of the Lava Flow harden but the center of it keeps moving. As the eruption episode ends, and the Lava drains, the center is left lower than the sides producing these high-standing structures.

PSP_006648_1300_RED_abrowse-00-PCF-LXTT.jpg PSP_006648_2255_RED_abrowse-PCF-LXTT.jpg PSP_006653_1795_RED_abrowse-PCF-LXTT.jpg PSP_006659_1460_RED_abrowse~0.jpg PSP_006667_2150_RED_abrowse-00-PCF-LXTT.jpg
Informazioni sul file
Nome del file:PSP_006653_1795_RED_abrowse-PCF-LXTT.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (3 voti):55555(Mostra dettagli)
Parole chiave:Mars / from / orbit / - / Volcanic / Features / - / Vent
Copyright:NASA/JPL/Univ. of Arizona and Paolo C. Fienga/Lunexit Team per l'additional process. e la colorizzazione
Dimensione del file:644 KiB
Data di inserimento:Gen 31, 2011
Dimensioni:3550 x 1355 pixels
Visualizzato:84 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=28240
Preferiti:Aggiungi ai preferiti
 
 

Powered by Coppermine Photo Gallery