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Understand the two design methodologies for space systems - 'Bottom-up' vs. 'Top-down' approaches, interaction matrix for satellite subsystems, modes of interaction, Challenges for LISA project including electrical charging, radiation pressure, and more. Explore power generation, thermal management, attitude determination, data handling, and communication subsystems in satellite design. Discover the critical role of structure, launch vehicles, and ground control in successful space missions.
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S/C System Design Overview Robert G. Melton Department of Aerospace Engineering
Bottom-up method Top-down method System Product C A B subsystems C A B components interactions • design up from component level • interactions not handled well • costs:short-term – low • long-term – high • (low reliability) • design down from system reqmnts • consider interactions at each step • costs:short-term – high • long-term – lower • (high reliability) Designing a Satellite
Interaction Matrix Satellite Subsystems • Scientific instruments • Power • Thermal • Attitude • Command & Data Handling • Communications • Structure • Launch vehicle • Ground control • Propulsion Designers must fill in all the squares! Modes of Interaction • spatial (shadowing, motion restraints) • mechanical (vibrations) • thermal • electrical • magnetic • electromagnetic • radiative (ionizing radiation) • informational (data flow) • biological (contamination)
The Key Point blah ssszzzz blah blah blah . . . EVERY subsystem affects EVERY other subsystem . . . blah blah sszzzzzsstt blah blah ssszzzzz zzzssszzzzzz zzzzzssss
LIONSATLocal IONospheric Measurements SATellite • will measure ion distrib. in ram and wake of satellite in low orbit • student-run project • (funded by Air Force, NASA and AIAA) • www.psu.edu/dept/aerospace/lionsat
LionSat (exploded view) Created by Christopher Borella and Rachel Larson for LionSat
LISA (Laser Interferometer Space Antenna) Space-based detector of gravity waves from black hole binaries Formation will orbit Sun, but 20o behind Earth 3 spacecraft separated by l = 5 x 106 km Will detect spatial strain of l/ l = 10-23 l = 5 x 10-14 m. (both images from lisa.jpl.nasa.gov)
The LISA orbits simulation by W. Folkner, JPL
- - - - Challenges for LISA • Electrical charging • Radiation pressure from sunlight • Self-gravity • New technology thrusters (micro-Newton) + thrusters mirror
Hubble Space Telescope http://www.stsci.edu/hst/proposing/documents/cp_cy12/primer_cyc12.pdf
Power • Solar array: sunlight electrical power • max. efficiency = 17% (231 W/m2 of array) • degrade due to radiation damage 0.5%/year • best for missions 1.53 AU (Mars’ dist. from Sun) • Radioisotope Thermoelectric Generator (RTG): nuclear decay heat electrical power • max. efficiency = 8% (lots of waste heat!) • best for missions to outer planets • political problems (protests about launching 238PuO2) • Batteries – good for a few hours, then recharge
Thermal • Passive • Coatings (control amt of heat absorbed & emitted) • can include louvers • Multi-layer insulation (MLI) blankets • Heat pipes (phase transition) • Active (use power) • Refrigerant loops • Heater coils
satellite wheel motor Attitude Determination and Control y Earth sensor • Sensors • Earth sensor (0.1o to 1o) • Sun sensor (0.005o to 3o) • star sensors (0.0003o to0.01o) • magnetometers (0.5o to 3o) • Inertial measurement unit (gyros) • Active control (< 0.001o) • thrusters (pairs) • gyroscopic devices • reaction & momentum wheels • magnetic torquers (interact with Earth’s magnetic field) • Passive control (1o to 5o) • Spin stabilization (spin entire sat.) • Gravity gradient effect x field of view photocells rotation • Motor applies torque to wheel (red) • Reaction torque on motor (green) causes satellite to rotate
Command and Data Handling • Commands • Validates • Routes uplinked commands to subsystems • Data • Stores temporarily (as needed) • Formats for transmission to ground • Routes to other subsystems (as needed) • Example: thermal data routed to thermal controller, copy downlinked to ground for monitoring
Communications • Transmits data to ground or to relay satellite (e.g. TDRS) • Receives commands from ground or relay satellite Interconnections! • Data rate power available attitude ctrl. • Data rate antenna size structural support • Data rate pointing accuracy attitude ctrl.
Structure • Not just a coat-rack! • Unifies subsystems • Supports them during launch • (accel. and vibrational loads) • Protects them from space debris, dust, etc.
Launch Vehicle • Boosts satellite from Earth’s surface to space • May have upper stage to transfer satellite to higher orbit • Provides power and active thermal control before launch and until satellite deployment Creates high levels of accel. and vibrational loading
Ground Control • MOCC (Mission Operations Control Center) • Oversees all stages of the mission (changes in orbits, deployment of subsatellites, etc.) • SOCC (Spacecraft Operations Control Center) • Monitors housekeeping (engineering) data from sat. • Uplinks commands for vehicle operations • POCC (Payload Operations Control Center) • Processes (and stores) data from payload (telescope instruments, Earth resource sensors, etc.) • Routes data to users • Prepares commands for uplink to payload • Ground station – receives downlink and transmits uplink
Propulsion • Provides force needed to change satellite’s orbit • Includes thrusters and propellant
Effects of Power on Attitude Control • Provide properly regulated, adequate levels of electrical power for sensors and actuators • Failure to meet these requirements could result in incorrect satellite orientation (which affects astron. observations!)
Effects of Attitude Control on Power • Proper attitude (orientation) needed for solar arrays • some arrays track sun independently but still depend upon overall satellite orientation control • Spin-stabilized satellites require electrically switched arrays • high spin rates faster switching (cheaper attitude ctrl) (more complex electronics)