In the mid 1980s NASA began deploying the Tracking and Data Relay Satellite System (TDRSS) into geostationary orbit. The purpose of these satellites is to relay data to ground stations. Because of their high orbits and their widely spaced station points over Earth's equator, the TDRSS satellites serve as relay points for lower satellites and the Space Shuttle. The system provides nearly continuous contact with spacecraft as they orbit Earth. TDRSS satellites relay data to a receiver at White Sands, New Mexico. From there, the data travel via telephone lines, fiber optic cable, or com-mercial communications satellites to its destination. Most astrophysics data travels from White Sands to the NASA Goddard Space Flight Center in Maryland for distribution to scientists.

Unit Objective

  • To demonstrate how astronomical satellites use technology to collect optical data, transmit that data to Earth, and reassemble it into images.
Teaching Strategy

The activities in this unit demonstrate the imaging process of astronomical satellites such as the Hubble Space Telescope. Use the Magic Wand and Persistence of Vision activities together or as alternates. The Magic Wand activity shows how images can be divided and reassembled. The Persis-tence of Vision activity does the same thing, but lets students actively participate by making their own tubes. The two activities on colorPColor Recognition and Colored ShadowsPshow how astronomy satellites collect color data and how that data can be reassembled on the ground. The Binary Number and Paint By The Number activities familiarize students with the process of data transmission to Earth and its reassembly into images.

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Last modified prior to September, 2000 by the Windows Team

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