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Circular Feature in the South Polar Residual Cap (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)
This 4 Km-diameter Circular Surface Feature near the Edge of the South Polar Residual Cap was recognized in Mariner 9 and Viking Orbiter images taken in the '70s, but its origin could not be inferred. It was therefore targeted for HiRISE stereo imaging. 
The bright areas in this image are covered by CO2 frost, and the "Swiss Cheese" terrain typical of the South Polar Residual Cap covers much of the imaged area. 
The Dark Walls of the Circular Depression do not have as much Frost on them, and are fractured in a polygonal pattern. Apparently the Surface of the Walls has been extensively modified by thermal expansion and contraction of water ice. It also appears that the "Swiss Cheese" Terrain of the Residual Cap has buried the Floor of the Circular Depression, as well as the Terrain surrounding the Feature, making it difficult to infer its origin. 
Its circular symmetry is consistent with an impact origin, but there is no evidence of a Crater Rim or Ejecta Blanket (perhaps because they have been buried). 
The Depression may also have formed by collapse, but there is little evidence of extensional fractures that would be expected around a Collapse Pit. Analysis of HiRISE stereo data may help the interpretation of this Feature.
Parole chiave: Mars from orbit - South Polar Features - Possible Buried Impact Crater

Circular Feature in the South Polar Residual Cap (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)

This 4 Km-diameter Circular Surface Feature near the Edge of the South Polar Residual Cap was recognized in Mariner 9 and Viking Orbiter images taken in the '70s, but its origin could not be inferred. It was therefore targeted for HiRISE stereo imaging.
The bright areas in this image are covered by CO2 frost, and the "Swiss Cheese" terrain typical of the South Polar Residual Cap covers much of the imaged area.
The Dark Walls of the Circular Depression do not have as much Frost on them, and are fractured in a polygonal pattern. Apparently the Surface of the Walls has been extensively modified by thermal expansion and contraction of water ice. It also appears that the "Swiss Cheese" Terrain of the Residual Cap has buried the Floor of the Circular Depression, as well as the Terrain surrounding the Feature, making it difficult to infer its origin.
Its circular symmetry is consistent with an impact origin, but there is no evidence of a Crater Rim or Ejecta Blanket (perhaps because they have been buried).
The Depression may also have formed by collapse, but there is little evidence of extensional fractures that would be expected around a Collapse Pit. Analysis of HiRISE stereo data may help the interpretation of this Feature.

Mawrth_Vallis.jpg Santa_Maria_Crater-PIA13706-PCF-LXTT.jpg PSP_005349_0930_RED_abrowse-0.jpg PSP_005349_0930_RED_abrowse-1.jpg ESP_019747_1975_RED_abrowse.jpg
Informazioni sul file
Nome del file:PSP_005349_0930_RED_abrowse-0.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (2 voti):55555(Mostra dettagli)
Parole chiave:Mars / from / orbit / - / South / Polar / Features / - / Possible / Buried / Impact / Crater
Copyright:NASA/JPL/Univ. of Arizona and Marco Faccin-Paolo C. Fienga/Lunexit Team per l'additional process. e la colorizzazione
Dimensione del file:815 KiB
Data di inserimento:Dic 19, 2010
Dimensioni:3050 x 3500 pixels
Visualizzato:115 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=28012
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