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The International Ultraviolet Explorer (IUE) is a large astronomical observatory which was launched on January 26, 1978. The observatory was placed into a three-axis stabilized, eccentric synchronous orbit with an inclination of about 29 degrees. Although it was designed for a 3-year lifetime, it is currently still operational. This paper will briefly review the thermal design which consists of multilayer insulation, ammonia-filled grooved heat pipes, bimetallic actuated louvers, and assorted commandable heaters. It will discuss the 15 years of thermal data and compare the results with prelaunch predictions. This paper will also briefly discuss the more significant flight anomalies. Finally, an attempt will be made to discuss any anomalous thermal behavior with an emphasis on the temperature increase of the hydrazine auxiliary propulsion system.

The international Ultraviolet Explorer (IUE) is a large astronomical observatory which was launched on January 26, 1978. The observatory was placed into a three-axis stabilized, eccentric synchronous orbit with an inclination of about 29 degrees. It was designed for a three year lifetime, but is currently still operational. This paper will briefly review the thermal design which consists of multilayer insulation, ammonia-filled grooved heat pipes, bimetallic actuated louvers, and assorted command-able heaters. It will then discuss the seven years of thermal data and compare the results with prelaunch predictions. Finally an attempt will be made to explain the unexpected and continuing rise in temperature of the hydrazine auxiliary propulsion system which has increased over twenty degrees centigrade since launch.

The FWDBCK time step, which is usually chosen intuitively to achieve adequate accuracy at reasonable computational costs, can in fact lead to large errors. NASA observed such errors in solving cryogenic problems on the COBE spacecraft, but a similar error is also demonstrated for a single node radiating to space. An algorithm has been developed for selecting the time step during the course of the simulation. The error incurred when the time derivative is replaced by the FWDBCK time difference can be estimated from the Taylor-Series expression for the temperature. The algorithm selects the time step to keep this error small. The efficacy of the method is demonstrated on the COBE and single-node problems.