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Circumbinary Disk
Sig06 001

Credit: P. Marenfeld and NOAO/AURA/NSF

Artwork • January 10th, 2006 • sig06-001

sig06-001

This artist concept shows a debris disk that has been observed around an unusual class of interacting binary stars. The type of cataclysmic variable system being studied consists of a highly magnetic white dwarf star (a "dead" remnant star formed from the core of a star like our Sun when it exhausts the available fuel to support nuclear fusion) and a very low-mass, cool object similar to a brown dwarf. The two objects orbit so closely -- about the distance from Earth to the Moon -- that they make a complete revolution about each other in only 80-90 minutes. The white dwarf is Earth-sized but weighs about 60 percent of the mass of the Sun, while the companion star is Jupiter-sized but has about 40-50 times the mass of Jupiter.

About the Object

Name
Type
Star > Grouping > Binary
Star > Evolutionary Stage > White Dwarf
Star > Type > Brown Dwarf
Star > Circumstellar Material > Disk > Debris