Circling Two Suns
On Earth, the daily rhythms of life sync to the sunrise and sunset of a single, bright star. But unlike our solar system, some planets have more than one sun. Using NASA's Kepler space observatory, scientists recently discovered a planetary system where two planets orbit two stars. The system, known as Kepler-47, provides the first evidence from Kepler that multiple planets can orbit a binary star—a star system consisting of two or more stars that circle each other. The outer planet, named Kepler-47c, orbits at an Earth-like distance from the larger and brighter of the two stars, residing in what astronomers call a habitable zone. This means the planet could support liquid water if it had terrestrial features, but scientists think Kepler-47c is likely made up entirely of gas. Watch the video to learn more about the discovery of this two-planet, two-star system.
Enjoy the sunset of your choice on the planets of Kepler-47.
The gaseous Kepler-47c (above) orbits a central star about the size of our sun every 303 days.
Kepler-47c (left) is about five times the size of Earth, while Kepler-47b (right) is three times the size of Earth.
The existence of a planet in the habitable zone of a binary star system expands the possibilities of finding Earth-like planets elsewhere.
Since its launch in 2009, Kepler drastically expanded the number of known planets and planetary systems beyond our solar system.
The Kepler observatory detects fluctuations in light when planets pass in front of stars. Its primary mirror is seen here before launch.
For More Information
See NASA.gov
Credits
Please give credit for this item to:
Science@NASA and NASA's Goddard Space Flight Center
Planet images courtesy of NASA/JPL-Caltech/T. Pyle
Planetary systems chart courtesy of NASA Ames/Jason Steffen, Fermilab Center for Particle Astrophysics
Primary mirror photo courtesy of NASA and Ball Aerospace
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Writer
- Patrick Lynch (Wyle Information Systems)
Release date
This page was originally published on Thursday, October 25, 2012.
This page was last updated on Wednesday, May 3, 2023 at 1:52 PM EDT.