About RPS

Radioisotope power systems — or RPS — provide electricity and heat that enable exploration in the darkest, dustiest, coldest and farthest regions of space.

A partially assembled Mars rover in the cleanroom at JPL. The rover's Radioisotope Thermoelectric Generator is jutting from the back of the rover.

What Is Radioisotope Power and Why Does NASA Use It?

Power to Explore

Power is the one thing a spacecraft cannot do without. Without the technology to reliably power space missions, our knowledge of the solar system would be only a fraction of what it is today. It might sound surprising, but there are currently only two practical options for providing a long-term source of electrical power for exploring space: the light of the sun or heat from a nuclear source such as a radioisotope.

Solar power is an excellent way to generate electricity for most Earth-orbiting spacecraft, and for certain missions to the moon and places beyond that offer sufficient sunlight and natural heat. However, many potential NASA missions given a high priority by the scientific community would visit some of the harshest, darkest, coldest locations in the solar system, and these missions could be impossible or extremely limited without the use of nuclear power.

Radioisotope power systems—abbreviated RPS—are a type of nuclear energy technology that uses heat to produce electric power for operating spacecraft systems and science instruments. That heat is produced by the natural radioactive decay of plutonium-238.

This technology has been a game changer in our exploration capabilities.

Nicola Fox

Nicola Fox

Associate Administrator of NASA's Science Mission Directorate

Choosing between solar and nuclear power for a space mission has everything to do with where a spacecraft needs to operate and what the mission must accomplish when it gets there. Radioisotope power is used only when it will enable or significantly enhance the ability of a mission to meet its science goals.

Critical Technology for Exploration

RPS offer several important benefits. They are compact, rugged and provide reliable power in harsh environments where solar arrays are not practical. For example, Saturn is about ten times farther from the sun than Earth, and the available sunlight there is only one hundredth, or one percent, of what we receive at Earth. At Pluto, the available sunlight is only six hundredths of a percent of the amount available at Earth. The ability to utilize radioisotope power is important for missions to these and other incredibly distant destinations, as the size of solar arrays required at such distances is impractically large with current technology.

RPS offer the key advantage of operating continuously over long-duration space missions, largely independent of changes in sunlight, temperature, charged particle radiation, or surface conditions like thick clouds or dust.

In addition, some of the excess heat produced by some radioisotope power systems can be used to enable spacecraft instruments and on-board systems to continue to operate effectively in extremely cold environments.

A 60-year Legacy

Radioisotope Power Systems are not a new part of the U.S. space program. They have made historic contributions to the United States' exploration of space for more than 60 years. NASA is directed by its original 1958 charter and by ongoing guidance from the White House and Congress to explore space for the peaceful benefit of all humankind. And RPS have enabled NASA's exploration of the solar system since the Apollo era of the late 1960s.

The missions that carry out this exploration are prioritized by a vigorous strategic planning process that incorporates the best ideas from internal and external scientific experts. These experts have consistently identified RPS as a fundamentally important technology.

An Evolving Technology

The latest RPS to be qualified for flight, called the Multi-Mission Radioisotope Thermoelectric Generator, provides both power and heat for the Mars Science Laboratory rover.

In 2011 the National Academy of Sciences completed a major study of the priorities for the next decade of U.S. exploration of the solar system, and several of the highest-ranked missions may require the use of an RPS.

As part of an ongoing partnership with the Department of Energy (DOE), NASA is conducting a mission-driven RPS program—a technology development effort that is strategically investing in nuclear power technologies that would maintain NASA's current space science capabilities and enable future space exploration missions.

NASA works in partnership with DOE to maintain the capability to produce the Multi-Mission Radioisotope Thermoelectric Generator (or MMRTG) and to develop higher-efficiency energy conversion technologies, such as more efficient thermoelectric converters as well as Stirling converter technology.

In the future, radioisotope power systems could continue to support missions to some of the most extreme environments in the solar system, probing the secrets of Jupiter's ocean moon Europa, floating in the liquid lakes of Saturn's moon Titan or touring the rings and moons of the ice giant planet Uranus. With this vital technological capability, the possibilities for exploration and discovery are limited only by our imaginations.

RPS Missions by Science Target

RPS-enabled missions have contributed to scientific knowledge across the solar system — and beyond.

Sun
Ulysses (1990-2009 orbit)
Venus
Cassini (2000 flyby)
Galileo (1990 flyby)
Earth
Cassini (1998 flyby )
Galileo (1990 and 1992 flybys )
Nimbus III (1969-1972)
Earth's Moon
Apollo 11-17 (Apollo Lunar Surface Experiment Package (1969-1977)
Mars
Perseverance Rover (2020 - Present)
Curiosity Rover (2012 - Present)
+Opportunity Rover (2004-2018)
+Spirit Rover (2004-2011)
+Sojourner Rover (1997)
Viking 2 Lander (1976-1982)
Viking 1 Lander (1976-1980)
Asteroids
Galileo (1991 and 1993 flybys)
Jupiter and its Moons
New Horizons (2007 Flyby)
Galileo (1995-2003 orbit) | +Galileo atmospheric probe (1995 descent)
Ulysses (1991 flyby, 2004 flyby)
Cassini (2000 Flyby)
Voyager 1 (1979 flyby)
Voyager 2 (1979 flyby)
Saturn and its Moons
Cassini-Huygens (2004-2017) | +Huygens Titan probe (2005)
Voyager 1 (1980)
Voyager 2 (1980)
Pioneer 11 (1973)
Uranus and its Moons
Voyager 2 (1986 flyby)
Neptune and its Moons
Voyager 2 (1989 flyby)
Pluto and its Moons
New Horizons (2015 flyby)
Kuiper Belt
New Horizons (2019 flyby)
Comets
Galileo (1994 observation)
Interstellar Space
Voyager 1 (2012-Present)
Voyager 2 (2018-Present)
Note: Pioneers 10 and 11 and New Horizons also are on interstellar trajectories.
+Solar- or battery-powered missions enabled by Radioisotope Heater Units (RHUs)