REG NASA-LLIS-0364-1994 Lessons Learned - Galileo Retro Propulsion Module and Pyro Power System Interaction.pdf
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1、Lessons Learned Entry: 0364Lesson Info:a71 Lesson Number: 0364a71 Lesson Date: 1994-12-22a71 Submitting Organization: JPLa71 Submitted by: B. LarmanSubject: Galileo Retro Propulsion Module and Pyro Power System Interaction Abstract: Galileo design optimizations over the years exacerbated interaction
2、s between spacecraft power and the propellant tanks. During the cruise phase, high power and heat dissipation near the propellant tanks combined with an enhanced tank load to increase the tank pressure.A thorough analysis should be conducted before changes are made to one or more of the flight proje
3、ct elements that occur late in the development cycle or well into the test program. Description of Driving Event: Over a period of several years, design optimizations were made to the Galileo Spacecraft system including the increase in the Retro Propulsion Module (RPM) tank load from 84% to 94%. Thi
4、s was to assure adequate propellant to accomplish the mission objectives and was done late in the spacecraft development cycle. However, the change resulted in a high degree of coupling between the RPM tank pressure and the spacecraft system power demand due to the spacecraft power dissipation mecha
5、nism. During the cruise phase, the spacecraft power demand will be low and the excess electrical power is to be dissipated by shunt heaters located near the RPM tanks. The power dissipation increases the RPM tanks temperature with a concomitant rise in the RPM tank pressure. The RPM design is such t
6、hat relatively small temperature increases combined with the low ullage (tanks nearly full), will cause a dangerous increase in the internal RPM tank pressure. The shunt heater circuit already had a requirement for a minimum dissipation level in order to assure adequate power margin for blowing fuse
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