WMS Planetary WMS service hosted by Astrogeology, USGS 4096 4096 text/xml image/png image/jpeg image/png; mode=8bit image/vnd.jpeg-png image/vnd.jpeg-png8 application/x-pdf image/svg+xml image/tiff application/json text/plain application/vnd.ogc.gml text/xml image/png image/jpeg image/png; mode=8bit image/vnd.jpeg-png image/vnd.jpeg-png8 text/xml XML INIMAGE BLANK Mars_Simple_Cylindrical_Rasters Planetary WMS service hosted by Astrogeology, USGS EPSG:4326 IAU_2015:49900 -180.000000 360.000000 -90.000000 90.000000 MOLA_THEMIS_blend MOLA Colorized DEM blended with the THEMIS IR Day 100m Global Mosaic v12. NASA's Goddard Space Flight Center used their Mars Orbiter Laser Altimeter topographic data (~640 million elevation measurements) to create a near-global digital elevation model (DEM). This DEM was used to create a colorized shaded relief at 128ppd (463m/p). Because the 128ppd version did not cover the poles, the global 64ppd DEM was used for those regions (above 88 latitude and below -88 latitude). Purple is low and white is high. Total global elevation range is approximately -8,200 meters minimum and 21,229 meters maximum. Elevations above 9000 meters are found only on the larger volcanos. Mars Odyssey THEMIS IR Day image mosaic was created by Arizona State University at 100 m/p and released in Aug. 2014. It is semi-controlled and thus may not match perfectly to the MOLA hillshade. -180.000000 359.999226 -89.999180 90.000000 text/xml THEMIS Mars Odyssey THEMIS IR Day image mosaic was created by Arizona State University at 100 m/p and released in Aug. 2014. It is semi-controlled and thus may not match perfectly to the MOLA controlled hillshade. -180.000000 359.983395 -89.996152 90.000000 text/xml THEMIS_controlled Mars Odyssey THEMIS IR Day near-global controlled mosaic was created by Astrogeology at 100m/p using data originally from Arizona State University (and NASA's Mars Odyssey mission). This represents all tiles that were completed as of Oct. 2018. It is fully-controlled and should closely align to the MOLA DEM/hillshade. This mosaic only covers from -65 to 65 latitude. For more background please see: https://astrogeology.usgs.gov/maps/mars-themis-controlled-mosaics-and-final-smithed-kernels -180.000000 359.999156 -65.000609 65.000844 text/xml THEMIS_night Mars Odyssey THEMIS IR Night near-global controlled mosaic was created by Astrogeology at 100 m/p and released in Oct. 2018. Data is originally from Arizona State University (and NASA's Mars Odyssey mission). It is fully-controlled and should closely align to the MOLA DEM/hillshade. This mosaic only covers from -65 to 65 latitude. For more background please see: https://astrogeology.usgs.gov/maps/mars-themis-controlled-mosaics-and-final-smithed-kernels -180.000000 359.999156 -65.000609 65.000844 text/xml MDIM21 Viking Mars Digital Image Mosaic (MDIM) version 2.1 was registered to the MOLA control network and created by the USGS at 256 pixel/degree (231m/p). -180.000000 360.000000 -90.000000 90.000000 text/xml MDIM20 Viking Mars Digital Image Mosaic version 2.0 created by the USGS at 256 pixel/degree (231m/p). The mosaic was released prior to the MOLA topographic control network and thus does not register well to more current image mosaics. This base has been superseded by MDIM version 2.1. -180.000000 360.000000 -90.000000 90.000000 text/xml MDIM21_color Viking Mars Digital Image Mosaic (MDIM) version 2.1 was registered to the MOLA control network and created by the USGS at 256 pixel/degree (231m/p). It was then colorized by NASA AMES using a warped colorized MDIM 1.0 -180.000000 360.000000 -90.000000 90.000000 text/xml MOLA_color NASA's Goddard Space Flight Center used their Mars Orbiter Laser Altimeter topographic data (~640 million elevation measurements) to create a near-global digital elevation model (DEM). This DEM was used to create a colorized shaded relief at 128ppd (463m/p). Because the 128ppd version did not cover the poles, the global 64ppd DEM was used for those regions (above 88 latitude and below -88 latitude). Purple is low and white is high. Total global elevation range is approximately -8,200 meters minimum and 21,229 meters maximum. Elevations above 9000 meters are found only on the larger volcanos. -180.000000 360.000000 -90.000000 90.000000 text/xml MOLA_bw NASA's Goddard Space Flight Center used their Mars Orbiter Laser Altimeter topographic data (~640 million elevation measurements) to create a near-global digital elevation model (DEM). This DEM was used to create a grayscale hillshade (shaded relief) at 128ppd (463m/p). Because the 128ppd version did not cover the poles, the global 64ppd DEM was used for those regions (above 88 latitude and below -88 latitude). Total global elevation range is approximately -8,200 meters minimum and 21,229 meters maximum. Elevations above 9000 meters are found only on the larger volcanos. -180.000000 360.000030 -90.000010 90.000000 text/xml HRSC_MOLA_Blend_Hillshade This data product, now at version 2, is a shaded relief created from blend of digital elevation model (DEM/DTM) data derived from the Mars Orbiter Laser Altimeter (MOLA), an instrument aboard NASAs Mars Global Surveyor spacecraft (MGS), and the High-Resolution Stereo Camera (HRSC), an instrument aboard the European Space Agencys Mars Express spacecraft. Total global elevation range is approximately -8,200 meters minimum and 21,229 meters maximum. Elevations above 9000 meters are found only on the larger volcanos. -180.000000 359.997672 -89.999224 90.000000 text/xml Mars5M_Quads Outlines and labels for the Mars 5M quad charts -180.000000 360.000000 -90.000000 90.000000 text/xml Mars2M_Quads Outlines and labels for the Mars 2M quad charts -180.000000 360.000000 -90.000000 90.000000 text/xml Mars500K_Quads Outlines and labels for the Mars 500K quad charts -180.000000 360.000000 -90.000000 90.000000 text/xml