We introduce the Pan-Pacific Planet Search, a survey of 170 metal-rich Southern Hemisphere subgiants using the 3.9m Anglo-Australian Telescope. We report the first discovery from this program, a giant planet orbiting 7 CMa (HD 47205) with a period of 763 ± 17 days, eccentricity e = 0.14 ± 0.06, and msin i = 2.6 ± 0.6MJup. The host star is a K giant with a mass of 1.5 ± 0.3 M⊙ and metallicity [Fe/H] = 0.21 ± 0.10. The mass and period of 7 CMa b are typical of planets which have been found to orbit intermediate-mass stars (M * > 1.3 M ⊙). Hipparcos photometry shows this star to be stable to 0.0004mag on the radial-velocity period, giving confidence that this signal can be attributed to reflex motion caused by an orbiting planet. © 2011. The American Astronomical Society. All rights reserved.
CITATION STYLE
Wittenmyer, R. A., Endl, M., Wang, L., Johnson, J. A., Tinney, C. G., & O’Toole, S. J. (2011). The Pan-Pacific Planet Search. I. A giant planet orbiting 7 CMa. Astrophysical Journal, 743(2). https://doi.org/10.1088/0004-637X/743/2/184
Mendeley helps you to discover research relevant for your work.