The Sun Also Rises Twice
Astronomers with the McDonald Observatory Planet Search project have discovered the first planet orbiting a star in a close-in binary star system. The discovery has implications for the number of possible planets in our galaxy, because unlike the Sun, most stars are in binary systems. The team will announce their finding this week in a news conference at the American Astronomical Society's Division of Planetary Sciences meeting in Birmingham, Ala.
|Artist's conception of the planet in the gamma Cephei system (click to enlarge). Picture credit: Tim Jones/McDonald Observatory
Artie Hatzes (Thueringer Landessternwarte Tautenburg), Bill Cochran (UT-Austin McDonald Observatory), and colleagues found that the planet orbits the larger star of the binary system Gamma Cephei, about 45 light-years away in the constellation Cepheus. The primary star is 1.59 times as massive as the Sun. The planet is 1.76 times as massive as Jupiter. It orbits the star at about 2 Astronomical Units (A.U.), a little further than Mars' distance from the Sun. (An A.U. is the distance from Earth to the Sun.) The second, relatively small star is only 25 to 30 A.U. from the primary star about Uranus' distance from the Sun.
Two Sunrises, Two Shadows
Astronomers have found planets orbiting stars in binary systems before, but the stars in those binary systems were a hundred times farther apart than those of Gamma Cephei, Cochran said. "The stars were far enough apart to be essentially acting totally independently," he said. The twin stars would indeed cast two different shadows on the (hypothetical) rings of any planet by the light coming from the bright primary star, the orange K1 subgiant, and the much fainter secondary star (probably a red M-dwarf star).
Cochran's team began observing Gamma Cephei with the 2.7-meter Harlan J. Smith Telescope at McDonald Observatory in 1988. Prior to that, a Canadian team of astronomers used the Canada-France-Hawaii Telescope (CFHT) to study Gamma Cephei. Together, the observations total 20 years.
|The planet orbits 2 AU from the larger star in the Gamma Cephei system, while the secondary star is a mere 28-30 AU distant. Orbits drawn to scale; star and planet sizes NOT to scale. (Credit: McDonald Observatory) 123K jpeg
Two Decades of Observation
In the past, some astronomers thought that the 2.5-year variation in light output from the binary star could be caused by physical processes in the stars.
"We think this is a planet because the variation has been nice and steady for eight complete cycles," Cochran said. "The star itself would not be varying that nicely for eight cycles over 20 years. Our observing techniques include several good indicators of stellar variability, and we see no variations that we can attribute to the star itself. The only logical thing that's left is a planet."
A third-magnitude star, Gamma Cephei can be seen with the unaided eye. But even powerful telescopes cannot split the light from the system into two individual pinpoints.
|Gamma Cephei will be visible to the unaided eye in the northern sky, just above and to the east of Polaris. (Tim Jones/McDonald Observatory)
Future NASA and ESA missions for space-borne telescopes will attempt to resolve faint or nearly-positioned star-planet combinations. These missions include Darwin, various interferometers and the Terrestrial Planet Finder.
The McDonald Observatory Planet Search began in 1987. The team uses the 2.7-meter Harlan J. Smith Telescope to monitor about 180 nearby Sun-like stars for Jupiter-sized planets. In addition to Gamma Cephei, the team has found planets orbiting the stars 16 Cygni B and Epsilon Eridani. The program is supported by grants from the National Science Foundation and NASA.
Related Web Pages:
Abstract for the german AG meeting presentation (postscript file)
Abstract for 34th DPS meeting presentation (link to the DPS meeting website)
Gamma Cep fact sheet (including stellar parameters from K. Fuhrmann)
McDonald Observatory press release (9th.Oct.2002)
AG Tagung press release (in german)
TLS Tautenburg Observatory
Walker, G.A.H., Bohlender, D.A., Walker, A.R., Irwin, A.W., Stephenson, L.S., Larson, A., 1992, ApJ, 396, L91-94
Artie P. Hatzes (TLS Tautenburg)
William D. Cochran (McDonald Observatory)
Michael Endl (McDonald Observatory)
Diane Paulson (University of Texas at Austin)
Gordon A.H.Walker (University of British Columbia)
Barbara McArthur (University of Texas at Austin)
Bruce Campbell (BTEC Enterprises Ltd.)
S. Yang (University of British Columbia)