Binary system

A binary system is a system of two objects in space (usually stars, but also brown dwarfs, planets, galaxies, or asteroids) which are so close that their gravitational interaction causes them to orbit about a common center of mass. Some definitions (e.g. that of double planet, but not that of binary star) require that this center of mass is not located within the interior of either object. A multiple system is like a binary system but consists of three or more objects.

Binary companion (minor planets)

When binary minor planets are similar in size, they may be called "binary companions" instead of referring to the smaller body as a satellite.^[1] Good examples of true binary companions are the 90 Antiope and the 79360 Sila–Nunam systems.

Close binary stars

A binary star that has an orbital period of less than 30 years implies that the two system components are less than about 10 AU apart. Because of this proximity, most close binaries are spectroscopic binaries and/or eclipsing binaries. Mass transfer occurs at some stage in most close binaries, profoundly affecting the evolution of the component stars. If the two components are in a close binary and do not fill their Roche lobes, the system is considered a detached binary. In a semidetached binary, one star fills its Roche lobe and mass transfer occurs. In a contact binary, both stars fill their Roche lobes. The evolution of close binaries depends on the initial masses of the two stars and their separation. When the more-massive star evolves into a red giant first and fills its Roche lobe, material will spill through the inner Lagrangian point onto its companion, thereby affecting its companion's evolution. Mass transfer can also alter the separation and orbital period of the binary star.

In binaries that are initially widely separated, material escaping from the Roche lobe of the evolved red giant immerses the system in material, creating a common-envelope binary that contains the core of the red giant (a white dwarf) and the companion star. Friction causes the two components to approach, and thus the orbital period to shorten. The common envelope is ejected and a cataclysmic variable star is left, wherein the mass transfer from the companion to the white dwarf causes the periodic outbursts seen in novae, recurrent novae, dwarf novae, and symbiotic novae.

If one component of a close binary is massive enough, it may become a neutron star or black hole instead of a white dwarf. Such binary systems are observed (see X-ray binary), but often a supernova explosion will blow the system apart into separate single stars.

In popular culture

• Binary suns and star systems are featured heavily in the Star Wars films and related material, the most notable example being the system in which the planet Tatooine is located.
• In the Discovery program Alien Planet, the planet Darwin IV orbits a binary system.
• In The Hitchhiker's Guide to the Galaxy, the planet Magrathea orbits a binary system
• In Spore, there are planetary systems with two suns.
• In Escape To Witch Mountain and Return From Witch Mountain, Tony and Tia's home planet orbits 2 suns.
• Futurama has an episode with three suns.
• In the Invader Zim episode "Planet Jackers", one of the aforementioned Jackers mentions a binary system.
• In Star Trek Voyager, there is a system with two suns.
• In Doctor Who, Gallifrey (the home planet of the Time Lords) has two suns in its planetary system.
• Binary sun systems are featured in the Mass Effect 2 game, these systems are in the Milky Way as explorable areas.
• In the Defiance TV series, the alien race Votans' home star system has two suns^[2]

See also

• Binary asteroid
• Binary star
• Contact binary
• Contact binary (asteroid)
• Double planet
• Rotational Brownian motion

References

Bibliography

• Astronomy: A Visual Guide by Mark A. Garlick