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Post by Marsrocks on Dec 17, 2011 21:23:57 GMT -5
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Post by Marsrocks on Dec 17, 2011 21:25:43 GMT -5
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Post by Marsrocks on Dec 17, 2011 21:26:52 GMT -5
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Post by Marsrocks on Dec 18, 2011 9:47:22 GMT -5
Sol 698 nav - Spirit looks at comanche up close:
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Post by Marsrocks on Dec 18, 2011 9:51:00 GMT -5
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Post by Marsrocks on Dec 18, 2011 10:13:46 GMT -5
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Post by Marsrocks on Dec 18, 2011 10:43:05 GMT -5
GE Sciencewww.sciencemag.org Prev | Table of Contents | Next Science 19 December 2008: Vol. 322 no. 5909 pp. 1828-1832 DOI: 10.1126/science.1164759 * Report Orbital Identification of Carbonate-Bearing Rocks on Mars Abstract Geochemical models for Mars predict carbonate formation during aqueous alteration. Carbonate-bearing rocks had not previously been detected on Mars' surface, but Mars Reconnaissance Orbiter mapping reveals a regional rock layer with near-infrared spectral characteristics that are consistent with the presence of magnesium carbonate in the Nili Fossae region. The carbonate is closely associated with both phyllosilicate-bearing and olivine-rich rock units and probably formed during the Noachian or early Hesperian era from the alteration of olivine by either hydrothermal fluids or near-surface water. The presence of carbonate as well as accompanying clays suggests that waters were neutral to alkaline at the time of its formation and that acidic weathering, proposed to be characteristic of Hesperian Mars, did not destroy these carbonates and thus did not dominate all aqueous environments. www.sciencemag.org/content/322/5909/1828.full
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Post by Marsrocks on Dec 26, 2011 9:32:34 GMT -5
Spectra of martian dust taken by the Mars Exploration Rover Spirit's mini-thermal emission spectrometer are compared to that of the orbital Mars Global Surveyor's thermal emission spectrometer. The graph shows that the two instruments are in excellent agreement. Graphing silicates, CO2 and carbonates: photojournal.jpl.nasa.gov/catalog/PIA05030
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Post by Marsrocks on Nov 23, 2012 7:27:34 GMT -5
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