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Inizio > THE LUNAR EXPLORER ARCHIVES > A Tribute To Mars Global Surveyor

Piú votate - A Tribute To Mars Global Surveyor
Aeolian_Features-Windstreaks-Becquerel_Crater-M0702802-01.jpg
Aeolian_Features-Windstreaks-Becquerel_Crater-M0702802-01.jpgWindstreaks inside Becquerel Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)206 visitenessun commentoMareKromium55555
(4 voti)
Craters-Unnamed_Crater_in_Terra_Sabaea-02.jpg
Craters-Unnamed_Crater_in_Terra_Sabaea-02.jpgUnnamed Crater in Terra Sabaea (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)230 visiteCaption originale:"This MGS-MOC image shows a 1,5 mt (~5 feet) per pixel view of an Impact Crater that is approximately 3 Km (about 9840 ft) in diameter. It is located in South-Western Terra Sabaea".

Location near: 21,9 South Lat. and 338,6 West Long.
Image width: ~3 km (~1,9 mi)
Illumination from: upper left
Season: Southern Summer
MareKromium55555
(4 voti)
Craters-Becquerel_Crater-Layers-01.jpg
Craters-Becquerel_Crater-Layers-01.jpgBeautiful Layers inside Becquerel Crater: Human Vision (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)165 visiteOriginal caption:"This MGS-MOC image shows light-toned, layered, Sedimentary Rock Outcrops in Becquerel Crater , located in the Western Arabia Terra Region. The Crater may once have hosted a lake, into which these sediments were deposited. Although the fine, detailed layering in Becquerel was not known until the MGS-MOC first began to image these materials in 1999, the presence of a grossly-layered, light-toned feature was known from Viking orbiter images and was speculated from those data to possibly represent evidence for the presence of a former lake".

Location near: 21,5 North Lat. and 8,2 West Long.
Image width: ~3 Km (~1,9 mi)
Season: Northern Winter
MareKromium55555
(4 voti)
Craters-Becquerel_Crater-Layers-02.jpg
Craters-Becquerel_Crater-Layers-02.jpgBeautiful Layers inside Becquerel Crater: Camera Vision (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)168 visiteOriginal caption:"This MGS-MOC image shows light-toned, layered, Sedimentary Rock Outcrops in Becquerel Crater , located in the Western Arabia Terra Region. The Crater may once have hosted a lake, into which these sediments were deposited. Although the fine, detailed layering in Becquerel was not known until the MGS-MOC first began to image these materials in 1999, the presence of a grossly-layered, light-toned feature was known from Viking orbiter images and was speculated from those data to possibly represent evidence for the presence of a former lake".

Location near: 21,5 North Lat. and 8,2 West Long.
Image width: ~3 Km (~1,9 mi)
Season: Northern Winter
MareKromium55555
(4 voti)
Craters-Spallanzani_Crater-MGS-01.jpg
Craters-Spallanzani_Crater-MGS-01.jpgLayered "Mesa" inside Spallanzani Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)206 visiteCaption NASA originale:"This MGS-MOC image shows a layered, light-toned Mesa among other Layered Materials exposed in a mound that covers much of the Floor of Spallanzani Crater".

Location near: 58,3 South Lat. and 273,9 West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: upper left
Season: Southern Summer
MareKromium55555
(4 voti)
Craters-Unnamed_Crater_with_Windstreak-PIA07508-01.jpg
Craters-Unnamed_Crater_with_Windstreak-PIA07508-01.jpgUnnamed Crater wth Windstreak (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)244 visiteCaption NASA originale:"This MGS-MOC image shows a 1,2 Km North Mid-Latitude Unnamed Crater with a bright Windstreak".

Location near: 30,8 North Lat. and 131,8 West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Northern Summer
MareKromium55555
(4 voti)
Craters-Unnamed_Crater_in_Terra_Cimmeria-MGS-PCF-LXTT.jpg
Craters-Unnamed_Crater_in_Terra_Cimmeria-MGS-PCF-LXTT.jpgUnnamed Impact Crater wth Gullies (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)219 visiteCaption NASA originale:"This MGS-MOC image shows a 1,5 mt (~5 feet) per pixel view of an Unnamed Crater in the Terra Cimmeria Region of Mars. Several Gullies extend from near the top of the Crater Rim, downslope toward the Floor of the Crater. Liquid water might have played a role in their genesis".

Location near: 37,7 South Lat. and 191,6 West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: upper left
Season: Southern Summer
MareKromium55555
(4 voti)
Craters-Unnamed_Crater_in_Terra_Tyrrhena-MGS-04.jpg
Craters-Unnamed_Crater_in_Terra_Tyrrhena-MGS-04.jpgUnnamed Crater and Dunes in Terra Tyrrhena (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team152 visitenessun commentoMareKromium55555
(4 voti)
Craters-Unnamed_Crater_in_Terra_Tyrrhena-02.jpg
Craters-Unnamed_Crater_in_Terra_Tyrrhena-02.jpgUnnamed Crater and Dunes in Terra Tyrrhena (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)151 visiteCaption originale:"This MGS-MOC image shows a portion of a Field of Dark Sand Dunes superposed on the light-toned Floor of an Unnamed Crater in Eastern Tyrrhena Terra. The orientation of the Dunes with the steep faces toward the South suggests that winds generally blew from North to South at the time the Dunes were formed".

Location near: 14,6 South Lat. and 262,3 West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Southern Summer
MareKromium55555
(4 voti)
Craters-Unnamed_Crater-PIA06699-PCF-LXTT.jpg
Craters-Unnamed_Crater-PIA06699-PCF-LXTT.jpgDark Slope Streaks (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)148 visiteCaption NASA:"Dark Slope Streaks are a common feature on the Slopes thickly-mantled by Dust in the Tharsis, Arabia, and Western Amazonis Planitia egions of Mars. Less common are light-toned Slope Streaks, which often occur in the same area as Dark Streaks. They are most common in Arabia Terra, and some are shown in this MGS image. Slope Streaks are probably the result of sudden Avalanches of extremely dry Dust. The behavior of the avalanching dust is somewhat fluid-like and it is a phenomenon often observed during the Martian year.

MareKromium55555
(4 voti)
Phlegra_Montes-PIA08743-1-PCF-LXTT.jpg
Phlegra_Montes-PIA08743-1-PCF-LXTT.jpgFeatures of Phlegra Montes (2 - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)205 visiteImage information: VIS instrument;
Latitude: 45,6 North;
Longitude: 168,7 East;
Resolution: 19 meter/pixel.
MareKromium55555
(4 voti)
Phlegra_Montes-PIA08743-2-PCF-LXTT.jpg
Phlegra_Montes-PIA08743-2-PCF-LXTT.jpgFeatures of Phlegra Montes (1 - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)206 visiteImage information: VIS instrument;
Latitude: 45,6 North;
Longitude: 168,7 East;
Resolution: 19 meter/pixel.
MareKromium55555
(4 voti)
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