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 847/2237 Torna all'inizio Guarda foto precedente Guarda foto successiva Salta alla fine
Polygons in Utopia Planitia (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 
This observation, in the Utopia Planitia, is marked by Depressions in the Mantle, several of which have coalesced together and now possess Scalloped edges and Layers. 

Scalloped pits, such as these, are typical features of the Mid-Latitude Mantle and are most commonly found at approx. 55° both North and South Latitude; in the Utopia Planitia, Scalloped Terrain is found between 45-50° North latitude where the Mantle is highly discontinuous. The presence of Scalloped Pits has led to hypotheses of the removal of Sub-Surface material, possibly interstitial ice, by Sublimation. Scalloped Depressions in the Utopia Planitia have also been interpreted to be "Thermokarst Lakes" created by melting of Permafrost (frozen ground) and collapse of the dry Surface Layer. 

Scalloped Pits typically have a steep Pole-facing Scarp and a gentler Equator-facing Slope. This is most likely due to differences in solar heating.
Parole chiave: Mars from orbit - Polygons - Utopia Planitia Region

Polygons in Utopia Planitia (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)

This observation, in the Utopia Planitia, is marked by Depressions in the Mantle, several of which have coalesced together and now possess Scalloped edges and Layers.

Scalloped pits, such as these, are typical features of the Mid-Latitude Mantle and are most commonly found at approx. 55° both North and South Latitude; in the Utopia Planitia, Scalloped Terrain is found between 45-50° North latitude where the Mantle is highly discontinuous. The presence of Scalloped Pits has led to hypotheses of the removal of Sub-Surface material, possibly interstitial ice, by Sublimation. Scalloped Depressions in the Utopia Planitia have also been interpreted to be "Thermokarst Lakes" created by melting of Permafrost (frozen ground) and collapse of the dry Surface Layer.

Scalloped Pits typically have a steep Pole-facing Scarp and a gentler Equator-facing Slope. This is most likely due to differences in solar heating.

PSP_004804_1105_RED_abrowse.jpg PSP_002070_2250_RED_abrowse-03.jpg PSP_002070_2250_RED_abrowse-00.jpg PSP_005069_1670_RED_abrowse-00.jpg PSP_005069_1670_RED_abrowse-01.jpg
Informazioni sul file
Nome del file:PSP_002070_2250_RED_abrowse-00.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (4 voti):55555(Mostra dettagli)
Parole chiave:Mars / from / orbit / - / Polygons / - / Utopia / Planitia / Region
Copyright:NASA/JPL/Univ. of Arizona and Paolo C. Fienga/Lunexit Team per l'additional process. e la colorizzazione
Dimensione del file:895 KiB
Data di inserimento:Nov 27, 2010
Dimensioni:3700 x 2200 pixels
Visualizzato:88 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=27905
Preferiti:Aggiungi ai preferiti
 
 

Powered by Coppermine Photo Gallery