Circumbinary planet - Video Learning - WizScience.com
A "circumbinary planet" is a planet that orbits two stars instead of one.
Because of the short orbits of some binary stars, the only way for planets to form is by forming outside the orbit of the two stars.
The first confirmed circumbinary extrasolar planet was found orbiting the system
PSR B1620-26, which contains a millisecond pulsar and a white dwarf and is located in the globular cluster M4. The existence of the third body was first reported in
1993, and was suggested to be a planet based on 5 years of observational data. In
2003 the planet was characterised as being 2.5 times the mass of
Jupiter in a low eccentricity orbit with a semimajor axis of 23 AU.
Announced in 2008, the eclipsing binary system
HW Virginis, comprising a subdwarf B star and a red dwarf, was found to also host a planetary system. The inner and outer planets have masses at least 8.47 and 19.23 times that of Jupiter respectively, and have orbital periods of 9 and 16 years. The outer planet is sufficiently massive that it may be considered to be a brown dwarf under some definitions of the term, but the discoverers argue that the orbital configuration implies it formed like a planet from a circumbinary disc. Both planets may have accreted additional mass when the primary star lost material during its red giant phase.
On
15 September 2011, astronomers announced the first partial-eclipse-based discovery of a circumbinary planet.
The planet, called Kepler-16b, is about
200 light years from
Earth, in the constellation
Cygnus, and is believed to be a frozen world of rock and gas, about the mass of
Saturn. It orbits two stars that are also circling each other, one about two-thirds the size of our sun, the other about a fifth the size of our sun. Each orbit of the stars by the planet takes 229 days, while the planet orbits the system's center of mass every 225 days; the stars eclipse each other every three weeks or so.
Scientists made the finding through
NASA's
Kepler spacecraft, which launched in 2009 and has been a driving force in the recent explosion in the discovery of distant planets.
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