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Lessons
Remote Sensing Ices on MarsTarget Grade Level: 8-10 Target Curriculum: Earth Science, Physical Science Students analyze data collected by Mars spacecraft using three different energies of light – visible light, infrared light, and gamma rays – to investigate the composition and distribution of ices at the high latitude regions of Mars. This Socratic-Dialogue Inducing activity guides students to understand that seasonal carbon dioxide ice covers buried water ice during the winter season and that the permanent ice caps in the northern and southern hemispheres are made of different types of ice. In an extension activity, students use a computer simulation illustrating how gamma rays can be used to determine the composition of the Martian surface. |
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The Phoenix Mission is led by Principal Investigator Peter H. Smith of The University of Arizona, supported by a science team of CO-Is, with project management at NASA's Jet Propulsion Laboratory and development partnership with Lockheed Martin Space Systems. International contributions are provided by the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus Denmark; the Max Planck Institute, Germany; and the Finnish Meteorological Institute. Additional information on Phoenix is online at here and here. JPL, a division of the California Institute of Technology in Pasadena, manages Mars Odyssey and Mars Reconnaissance Orbiter for the NASA Science Mission Directorate, Washington. Additional information on NASA's Mars program is online at here.
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In remembrance of Diane Michelangeli
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