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首页> 外文期刊>The Astrophysical journal >THE PAN-PACIFIC PLANET SEARCH. I. A GIANT PLANET ORBITING 7 CMa
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THE PAN-PACIFIC PLANET SEARCH. I. A GIANT PLANET ORBITING 7 CMa

机译:泛太平洋搜索。 I.巨型行星绕行7 CMa

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We introduce the Pan-Pacific Planet Search, a survey of 170 metal-rich Southern Hemisphere subgiants using the 3.9?m 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 ± 0.6?M Jup. 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 0.0004?mag on the radial-velocity period, giving confidence that this signal can be attributed to reflex motion caused by an orbiting planet.
机译:我们介绍了使用3.9?m的英澳望远镜对“泛太平洋行星搜索”进行的一项调查,该调查对170个富含金属的南半球亚族进行了调查。我们报告了该程序的第一个发现,它是一颗绕7 CMa(HD 47205)运转的巨型行星,周期为763±17天,偏心率e = 0.14±0.06,msin i = 2.6±0.6?M Jup。宿主恒星是质量为1.5±0.3 M☉且金属度[Fe / H] = 0.21±0.10的K巨星。 7 CMa b的质量和周期是典型的行星,已发现它们绕中间质量恒星(M *> 1.3 M☉)绕轨道运行。 Hipparcos光度法显示,该恒星在径向速度周期内稳定在0.0004?mag,这使该信号可以归因于行星运行引起的反射运动。

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