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Alpha Particle X-ray Spectrometer and Crater from 2004
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'Clovis' in Color
PIA06772
Sol (our sun)
Alpha Particle X-ray Spectro
| Title |
'Clovis' in Color |
| Original Caption Released with Image |
Figure 1 This approximate true-color image taken by the Mars Exploration Rover Spirit shows the rock outcrop dubbed "Clovis." The rock was discovered to be softer than other rocks studied so far at Gusev Crater after the rover easily ground a hole into it with its rock abrasion tool. This image was taken by the 750-, 530- and 480-nanometer filters of the rover's panoramic camera on sol 217(August 13, 2004). "Elemental Trio Found in 'Clovis'" Figure 1 above shows that the interior of the rock dubbed "Clovis" contains higher concentrations of sulfur, bromine and chlorine than basaltic, or volcanic, rocks studied so far at Gusev Crater. The data were taken by the Mars Exploration Rover Spirit's alpha particle X-ray spectrometer after the rover dug into Clovis with its rock abrasion tool. The findings might indicate that this rock was chemically altered, and that fluids once flowed through the rock depositing these elements. |
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'Clovis' in Color
PIA06772
Sol (our sun)
Alpha Particle X-ray Spectro
| Title |
'Clovis' in Color |
| Original Caption Released with Image |
Figure 1 This approximate true-color image taken by the Mars Exploration Rover Spirit shows the rock outcrop dubbed "Clovis." The rock was discovered to be softer than other rocks studied so far at Gusev Crater after the rover easily ground a hole into it with its rock abrasion tool. This image was taken by the 750-, 530- and 480-nanometer filters of the rover's panoramic camera on sol 217(August 13, 2004). "Elemental Trio Found in 'Clovis'" Figure 1 above shows that the interior of the rock dubbed "Clovis" contains higher concentrations of sulfur, bromine and chlorine than basaltic, or volcanic, rocks studied so far at Gusev Crater. The data were taken by the Mars Exploration Rover Spirit's alpha particle X-ray spectrometer after the rover dug into Clovis with its rock abrasion tool. The findings might indicate that this rock was chemically altered, and that fluids once flowed through the rock depositing these elements. |
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Spirit Sees Salty Soil
PIA06043
Sol (our sun)
Alpha Particle X-ray Spectro
| Title |
Spirit Sees Salty Soil |
| Original Caption Released with Image |
This graph compares amounts of magnesium and sulfur in the soil lining the trenches dug by the Mars Exploration Rover Spirit on sols 114 and 140 (April 28 and May 25, 2004) at Gusev Crater. Measurements were taken of the soil at the surface, floor and walls of the trench dug on sol 140 (squares), and at the surface and floor of the trench dug on sol 114 (diamonds). Non-trenched soil samples from Gusev Crater are represented as dots. The more recently made trench is located near the base of the "Columbia Hills." Because concentrations of magnesium and sulfur occur in the same ratio throughout the trench dug on sol 140, scientists believe the soil there contains the salt magnesium sulfate. The walls of this trench appear to contain the highest concentrations of the salt. The trench from sol 114 may also possess magnesium sulfate, but the data is less clear. These data were taken by Spirit's alpha particle X-ray spectrometer. One possible explanation for these findings is that water percolated through underground material and dissolved out minerals, then as the water evaporated near the surface, it left concentrated salts behind. |
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Smooth Side of 'Route 66'
PIA05761
Sol (our sun)
Microscopic Imager
| Title |
Smooth Side of 'Route 66' |
| Original Caption Released with Image |
This image was taken by the microscopic imager onboard NASA's Mars Exploration Rover Spirit on sol 99 (April 13, 2004). It is a close-up look at a portion of the rock called "Route 66," which was brushed by the rover's rock abrasion tool. This image intrigues scientists because it looks very different from the microscopic images taken of other brushed rocks at the Gusev Crater location. The surface of Route 66 is very shiny and specularly reflective, which may indicate a glassy surface, or perhaps a very smooth, discontinuous coating. The unique coating appears mottled and may be multi-layered. Other interesting features in this brushed area of Route 66 are the very thin, arc-shaped lines that are visible in the upper left quadrant of the image. An initial hypothesis suggests that these arcs may have been caused by the rock abrasion tool when the instrument made its initial contact with the surface. Scientists will use the combined data from the rover's Moessbauer spectrometer and alpha particle X-ray spectrometer along with color versions of this image to try to reach stronger conclusions about what they are seeing and what processes caused the features. |
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Window to 'Clovis's' Altered
PIA06781
Sol (our sun)
Navigation Camera
| Title |
Window to 'Clovis's' Altered Past |
| Original Caption Released with Image |
This image taken by the Mars Exploration Rover Spirit shows a rock outcrop dubbed "Clovis." The rock was discovered to be softer than other rocks studied so far at Gusev Crater after the rover easily ground a hole (center) into it with its rock abrasion tool. An analysis of the interior of the hole with the rover's alpha particle X-ray spectrometer found higher concentrations of sulfur, bromine and chlorine compared to basaltic, or volcanic, rocks at Gusev. This might indicate that Clovis was chemically altered, and that fluids once flowed through the rock depositing these elements. Spirit's solar panels can be seen in the foreground. This image was taken by the rover's navigation camera on sol 205 (July 31, 2004). |
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Soft Rock Yields Clues to Ma
PIA06771
Sol (our sun)
Navigation Camera
| Title |
Soft Rock Yields Clues to Mars' Past |
| Original Caption Released with Image |
Figure 1 This image taken by the Mars Exploration Rover Spirit shows the rock outcrop dubbed "Clovis." The rock was discovered to be softer than other rocks studied so far at Gusev Crater after the rover easily ground a hole into it with its rock abrasion tool. Spirit's solar panels can be seen in the foreground. This image was taken by the rover's navigation camera on sol 205 (July 31, 2004). "Elemental Trio Found in 'Clovis'" Figure 1 above shows that the interior of the rock dubbed "Clovis" contains higher concentrations of sulfur, bromine and chlorine than basaltic, or volcanic, rocks studied so far at Gusev Crater. The data were taken by the Mars Exploration Rover Spirit's alpha particle X-ray spectrometer after the rover dug into Clovis with its rock abrasion tool. The findings might indicate that this rock was chemically altered, and that fluids once flowed through the rock depositing these elements. |
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