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Nasa’s messenger mission has unveiled the first global digital elevation model (dem) of mercury, revealing in stunning detail the topography across the entire innermost planet and paving the way for scientists to fully characterize mercury’s geologic history. Its largest crater, caloris planitia. The datum of digital elevation model of mercury, included in the archive, derived from refactored data of mercury double imaging system (mdis) dem, version 1 of messenger mission, which was prepared by usgs, and distributed by planetary data system (pds) of nasa.
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The mercury surface, space enviorment, geochemistry, and ranging (messenger) spacecraft entered orbit about mercury in march 2011 to carry out a comprehensive topographic mapping of the planet. The surface of mercury is similar to earth's moon, being heavily cratered, with an expansive rupes system generated from thrust faults, and bright ray systems, formed by ejecta We provide three gravity field models of mercury, expressed in spherical harmonics of degree and order 180
In addition, we provide the results of our admittance analysis for 4 different areas
See the “data” section for the files. Lith that affects how light is scattered from the planet’s surface To deduce the physical properties of mercury’s regolith, we use spectrophotometry from the mercury dual imaging system instrument of nasas Using data from nasa’s messenger mission, astronomers created the first global digital elevation model (dem) of mercury, revealing in stunning detail the topography across the entire innermost planet and paving the way for scientists to fully characterize its geologic history.
Mercury is the first planet from the sun and the smallest in the solar system It is a rocky planet with a trace atmosphere and a surface gravity slightly higher than that of mars
