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Voyager 1 Batterie

The Voyager 1 and 2 Missions: Fueled by Radioisotope Power Systems

Radioisotope Power Systems: A Safe and Reliable Source of Energy for Spacecraft

Radioisotope Power Systems (RPS) have played a crucial role in powering spacecraft for decades, providing a safe and reliable source of energy for missions that venture far from the Sun. Each RPS consists of three main components: a radioisotope heat source, a thermoelectric converter, and a gas pressure venting system.

Radioisotope Heat Source

The radioisotope heat source is the heart of an RPS. It contains a radioactive material, such as plutonium-238, which undergoes radioactive decay, releasing heat energy. This heat energy is then used to power the thermoelectric converter.

Thermoelectric Converter

The thermoelectric converter converts the heat energy from the radioisotope heat source into electricity. It does this by using a series of thermocouples, which are devices that generate an electrical current when there is a temperature difference between their hot and cold junctions.

Gas Pressure Venting System

The gas pressure venting system is a safety feature that prevents the buildup of excess pressure within the RPS. It consists of a valve that opens when the pressure inside the system reaches a certain level, allowing excess gas to escape.

RPSs have been used to power a variety of spacecraft, including the Voyager 1 and 2 missions. Launched in 1977, Voyager 1 and 2 are the farthest spacecraft from Earth, exploring the outer regions of our solar system. The RPSs on these spacecraft have provided a continuous source of power for over 40 years, enabling them to transmit valuable data back to Earth.

The cost of the Voyager 1 and 2 missions, including launch, mission operations, and data analysis, is estimated to be around $865 million. This may seem like a significant investment, but it has paid off handsomely. The Voyager missions have provided us with invaluable insights into the outer planets and have helped to advance our understanding of the solar system.


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