ar X iv : a st ro - p h / 06 10 17 9 v 1 6 O ct 2 00 6 A Long – period Jupiter – mass Planet Orbiting the Nearby M Dwarf GJ 849

نویسندگان

  • Paul Butler
  • John Asher Johnson
  • Geoffrey W. Marcy
  • Jason T. Wright
  • Steven S. Vogt
  • Debra A. Fischer
چکیده

We report precise Doppler measurements of GJ 849 (M3.5V) that reveal the presence of a planet with a minimum mass of 0.82 MJup in a 5.16 year orbit. At a = 2.35 AU, GJ 849 b is the first planet discovered around an M dwarf to orbit beyond 0.21 AU, and is only the second Jupiter mass planet discovered around a star less massive than 0.5 M⊙. This detection brings to 4 the number of M stars known to harbor planets. Based on the results of our survey of 1300 FGKM main–sequence stars we find that giant planets within 2.5 AU are ∼3 times more common around GK stars than around M stars. Due to the GJ 849’s proximity of 8.8 pc, the planet’s angular separation is 0. 27, making this system a prime target for high–resolution imaging using adaptive optics and future space–borne missions such as the Space Interferometry Mission. We also find evidence of a linear trend in the velocity time series, which may be indicative of an additional planetary companion. Subject headings: techniques: radial velocities—planetary systems: formation— stars: individual (GJ 849) 1 Based on observations obtained at the W.M. Keck Observatory, which is operated jointly by the University of California and the California Institute of Technology. Keck time has been granted by both NASA and the University of California. Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road NW, Washington D.C. USA 20015-1305 Department of Astronomy, University of California, Berkeley, CA USA 94720 Department of Physics and Astronomy, San Francisco State University, San Francisco, CA, USA 94132 UCO/Lick Observatory, University of California at Santa Cruz, Santa Cruz CA USA 95064

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : a st ro - p h / 06 10 17 9 v 2 2 6 O ct 2 00 6 A Long – period Jupiter – mass Planet Orbiting the Nearby M Dwarf GJ 849

We report precise Doppler measurements of GJ 849 (M3.5V) that reveal the presence of a planet with a minimum mass of 0.82 MJup in a 5.16 year orbit. At a = 2.35 AU, GJ 849 b is the first Doppler–detected planet discovered around an M dwarf orbiting beyond 0.21 AU, and is only the second Jupiter–mass planet discovered around a star less massive than 0.5 M⊙. This detection brings to 4 the number ...

متن کامل

ar X iv : a st ro - p h / 06 08 26 0 v 1 1 1 A ug 2 00 6 The M Dwarf GJ 436 and its Neptune - Mass Planet

We determine stellar parameters for the M dwarf GJ 436 that hosts a Neptunemass planet. We employ primarily spectral modeling at low and high resolution, examining the agreement between model and observed optical spectra of five comparison stars of type, M0-M3. Modeling high resolution optical spectra suffers from uncertainties in TiO transitions, affecting the predicted strengths of both atomi...

متن کامل

ar X iv : a st ro - p h / 05 10 50 8 v 1 1 8 O ct 2 00 5 A ∼ 7 . 5 Earth - Mass Planet Orbiting the Nearby Star , GJ 876

High precision, high cadence radial velocity monitoring over the past 8 years at the W. M. Keck Observatory reveals evidence for a third planet orbiting the nearby (4.69 pc) dM4 star GJ 876. The residuals of three-body Newtonian fits, which include GJ 876 and Jupiter mass companions b and c, show significant power at a periodicity of 1.9379 days. Self-consistently fitting the radial velocity da...

متن کامل

ar X iv : a st ro - p h / 05 10 50 8 v 2 1 8 O ct 2 00 5 A ∼ 7 . 5 Earth - Mass Planet Orbiting the Nearby Star , GJ 876

High precision, high cadence radial velocity monitoring over the past 8 years at the W. M. Keck Observatory reveals evidence for a third planet orbiting the nearby (4.69 pc) dM4 star GJ 876. The residuals of three-body Newtonian fits, which include GJ 876 and Jupiter mass companions b and c, show significant power at a periodicity of 1.9379 days. Self-consistently fitting the radial velocity da...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2006