File:PIA18396-MarsCuriosityRover-WinnipesaukeeRock-20140625.jpg
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摘要
描述PIA18396-MarsCuriosityRover-WinnipesaukeeRock-20140625.jpg |
English: 06.25.2014
Martian Rock and Dust Filling Studied with Laser and Camera http://mars.jpl.nasa.gov/msl/multimedia/images/?ImageID=6428 Scientists used the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity Mars rover in June 2014 to examine a Martian rock "shell" about one inch (two to three centimeters) across, embedded in fine-grained bedrock and with a dust-filled hollow interior. This graphic combines an image of the target, called "Winnipesaukee," with spectrographic results from using ChemCam's laser on a row of points including the rock, the matrix around it and the material filling it. The image merges a high-resolution, black-and-white image from ChemCam's remote micro-imager and a color image form the telephoto-lens camera of Curiosity's Mast Camera (Mastcam). The ChemCam laser and camera atop of Curiosity's remote sensing mast were about 9 feet, 10 inches (3 meter) from Winnipesaukee when the instrument examined Winnipesaukee on the 654th Martian day, or sol, of the rover's work on Mars (June 8, 2014). Similar-appearing features have been seen previously in the mission, but this time ChemCam was able to provide chemical analysis of the structure. The instrument fired 30 laser shots at each of 10 locations indicated by black, red and green circles on the image. Three distinct types of materials were analyzed: the bedrock on each side of the structure, the "shell" material itself and the dust inside the void space. The colors of the lines on the graph below the image correspond to the colors of the circles marking the laser-shot locations. Analysis of spectra from the bedrock (black circles) identified high abundances of oxides of silicon, aluminum and sodium, typical of a feldspathic composition. The material forming the "shell" (red circles) has a more basaltic or mafic composition, with higher iron and magnesium content. The dust (green circles) is almost certainly airborne material that accumulated in the void space. This dust contains a relatively high hydrogen (water) signature compared to other Martian materials, which is generally characteristic of the ubiquitous dust that forms a thin mantle on much of the surface. Scientists are considering multiple hypotheses for how this hollow feature formed. Formation as a bubble or carapace of rock that was embedded in the surrounding sediment cannot be ruled out. One alternative considered more likely is that transport of fluids through the bedrock could produce pipe-like structures with a wall consisting of bedrock that either has reacted with the fluids or has been coated with other material. Another is that the feature formed due to cracks penetrating the bedrock, then a mineral cement filling the cracks, then wind erosion removing material from the center. ChemCam is one of 10 instruments in Curiosity's science payload. The U.S. Department of Energy's Los Alamos National Laboratory, Los Alamos, N.M., developed ChemCam in partnership with scientists and engineers funded by the French national space agency, CNES, the University of Toulouse and research agency, CNRS. More information about ChemCam is available at http://www.msl-chemcam.com . The rover's MastCam was built by and is operated by Malin Space Science Systems, San Diego. |
日期 | |
来源 | http://mars.jpl.nasa.gov/msl/images/PIA18396_ccam-mcam_winnipesaukee-full.jpg |
作者 | NASA/JPL-Caltech/LANL/CNES/IRAP/LPGNantes/CNRS/IAS/MSSS |
许可协议
Public domainPublic domainfalsefalse |
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本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zh、NASA版权方针页面或JPL图片使用方针。) | ![]() |
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11 6 2014
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宽度 | 1,344 px |
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高度 | 1,200 px |
每色彩组分位数 |
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像素构成 | RGB |
方向 | 正常 |
色彩组分数 | 3 |
水平分辨率 | 72 dpi |
垂直分辨率 | 72 dpi |
使用软件 | Adobe Photoshop CS6 (Windows) |
文件修改日期时间 | 2014年6月17日 (二) 16:19 |
Exif版本 | 2.21 |
色彩空间 | 未标定 |
原始文件唯一ID | FC969D7194125231EE05830F6E1FDCFF |
数字化日期时间 | 2014年6月11日 (三) 20:02 |
元数据最后修改日期 | 2014年6月17日 (二) 18:19 |
IIM版本 | 64,402 |