eric44
Anomaly Finder
Posts: 53
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Post by eric44 on Apr 19, 2014 5:38:27 GMT -5
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Post by Marsrocks on Apr 20, 2014 20:45:21 GMT -5
Neat. Several interesting fragments nearby also that look to have artificially suggestive shapes.
Take a look into the wall behind it, and you will see another round - bowl like fragment in the wall.
These forms were considered by the geology guys as possible lava formed silica bubbles - having burst.
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eric44
Anomaly Finder
Posts: 53
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Post by eric44 on Apr 21, 2014 5:53:13 GMT -5
The bubble explanation is interesting but if it were bubbles, we should have rocks with round holes (like chees) but here we have an object with sharp edges and a thin wall
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Post by Marsrocks on Apr 21, 2014 13:21:14 GMT -5
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Post by Marsrocks on Apr 21, 2014 13:47:46 GMT -5
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Post by Marsrocks on Apr 21, 2014 13:54:48 GMT -5
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eric44
Anomaly Finder
Posts: 53
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Post by eric44 on Apr 21, 2014 15:34:13 GMT -5
Thanks for the search, great pictures !
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Post by Marsrocks on May 24, 2014 16:16:27 GMT -5
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Post by Marsrocks on May 26, 2014 7:40:50 GMT -5
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Post by Marsrocks on May 26, 2014 8:06:01 GMT -5
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Post by Marsrocks on May 26, 2014 8:15:43 GMT -5
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Post by Marsrocks on May 26, 2014 10:43:00 GMT -5
We do know there are clay materials in the Gale crater (Curiosity) area. The presence of clay was one of the reasons this site was selected. One of the key reasons of the selection of Gale crater as the MSL landing site is the presence of clay minerals in several thin beds of its lower member (Milliken et al. 2010). The presence of sulfate-bearing beds below and above the clay-bearings beds however makes the origin of clay minerals at Gale ambiguous. Previous and ongoing analyses of CRISM and OMEGA show that the Martian clay minerals have very diverse compositions and geological settings. We will present new evidences of clay mineral formation cycles during early Mars, which have similarities with the present Earth clay cycles. We will thus connect the aqueous-related characteristics of Gale to the Martian global clay cycle in order to better constrain the formation processes of clays at Gale and to relate the future MSL observations to planetary scale processes relevant to past habitability. adsabs.harvard.edu/abs/2011AGUFM.P33C1774PMaybe there is another reason the origin of the clay material on the surface at Gale crater is not easily explained by geology. Revealing the story that the clay tells us at Gale crater is a primary objective of this mission. marsoweb.nas.nasa.gov/landingsites/msl/workshops/5th_workshop/talks/Tuesday_AM/Vaniman_May_2011_Landing_Site_Workshop.pdf
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Post by Marsrocks on Jul 8, 2014 14:35:47 GMT -5
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Post by Marsrocks on Jan 12, 2015 17:17:56 GMT -5
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