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Salt and Sufates? - Sol 787
While driving eastward toward the northwestern flank of McCool Hill, the wheels of NASA's MER Spirit churned up the largest amount of bright soil discovered so far in the mission. This image from Spirit's NavCam, taken on the Rover's 787th Sol of exploration (March 21, 2006), shows the strikingly light tone and large extent of the deposit. A few days earlier, Spirit's wheels unearthed a small patch of light-toned material informally named Tyrone. In images from Spirit's PanCam, Tyrone strongly resembled both Arad and Paso Robles, such as 2 patches of light-toned soils discovered earlier in the mission. Spirit found Paso Robles in 2005 while climbing Cumberland Ridge, on the western slope of Husband Hill. In early January 2006, Sptirit discovered Arad on the basin floor just south of Husband Hill. Spirit's instruments confirmed that those soils had a salty chemistry dominated by iron-bearing sulfates. Spirit's miniature thermal emission spectrometer is analyzing this most recent discovery, and researchers will compare it with those other deposits. 

These discoveries indicate that light-toned soil deposits might be widely distributed on the flanks and valley floors of the "Columbia Hills" region in Gusev Crater on Mars. The salts may record the past presence of water, as they are easily mobilized and concentrated in liquid solution.

Parole chiave: Martian Surface - possible salt and carbonate underground deposits

Salt and Sufates? - Sol 787

While driving eastward toward the northwestern flank of McCool Hill, the wheels of NASA's MER Spirit churned up the largest amount of bright soil discovered so far in the mission. This image from Spirit's NavCam, taken on the Rover's 787th Sol of exploration (March 21, 2006), shows the strikingly light tone and large extent of the deposit. A few days earlier, Spirit's wheels unearthed a small patch of light-toned material informally named Tyrone. In images from Spirit's PanCam, Tyrone strongly resembled both Arad and Paso Robles, such as 2 patches of light-toned soils discovered earlier in the mission. Spirit found Paso Robles in 2005 while climbing Cumberland Ridge, on the western slope of Husband Hill. In early January 2006, Sptirit discovered Arad on the basin floor just south of Husband Hill. Spirit's instruments confirmed that those soils had a salty chemistry dominated by iron-bearing sulfates. Spirit's miniature thermal emission spectrometer is analyzing this most recent discovery, and researchers will compare it with those other deposits.

These discoveries indicate that light-toned soil deposits might be widely distributed on the flanks and valley floors of the "Columbia Hills" region in Gusev Crater on Mars. The salts may record the past presence of water, as they are easily mobilized and concentrated in liquid solution.

OPP-SOL763-1N195920309EDN65RXP1585L0M1~0.jpg OPP-SOL764-1P196011637ESF65RXP2553L2M1.jpg OPP-SOL762-1R195835445EFF65RXP1311L0M1.jpg OPP-SOL767-1R196278545EFF66DTP1311L0M1.jpg SOL788-2N196326151EFFAQB6P1911L0M1.jpg
Informazioni sul file
Nome del file:SOL787-PIA08012.jpg
Nome album:Walking on Mars with Spirit and Opportunity
Valutazione (5 voti):55555(Mostra dettagli)
Parole chiave:Martian / Surface / - / possible / salt / and / carbonate / underground / deposits
Copyright:NASA - Spirit Rover Mission
Dimensione del file:163 KiB
Data di inserimento:Mar 23, 2006
Dimensioni:1024 x 1024 pixels
Visualizzato:54 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=10335
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