HD 128311

HD 128311
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 14h 36m 00.56s[1]
Declination +09° 44′ 47.5″[1]
Apparent magnitude (V) 7.51
Characteristics
Spectral type K0V
U−B color index 0.78
B−V color index 0.99
Variable type BY Dra[2]
Astrometry
Radial velocity (Rv)-9.6 ± 0.4 km/s
Proper motion (μ) RA: 204.74 ± 0.74[1] mas/yr
Dec.: -249.98 ± 0.61[1] mas/yr
Parallax (π)60.60 ± 0.83[1] mas
Distance53.8 ± 0.7 ly
(16.5 ± 0.2 pc)
Absolute magnitude (MV)8.5
Details
Mass0.8 M☉
Radius0.73 R☉
Luminosity0.221 L☉
Surface gravity (log g)41.9 g cgs
Temperature4965 K
Metallicity108%
Age0.39 Gyr
Equatorial [ g ] 411 m/s2
Other designations
BD+10°2710, GC 19679, GJ3860, GSC 00910-00165, HIP 71395, HN Boötis, LTT 14312, SAO 120554.
Database references
SIMBADdata
ARICNSdata
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

HD 128311 or HN Boötis is an orange main-sequence star located approximately 54 light-years away in the constellation of Boötes. Two extrasolar planet candidates have been detected in orbit around this star.

Planetary system

In 2002, the discovery of the planet HD 128311 b was announced by Paul Butler.[3] In 2005, the discovery of a second planet HD 128311 c was announced by Steve Vogt.[4]

Most likely, the system has been formed in a very turbulent disc.[5] The authors were able to show with both analytic and numerical models that certain libration modes are readily excited by turbulence. It was initially thought that the system could have been resulted from planet planet scattering, but this is rather unlikely.

Time evolution of orbital elements in the system HD128311. This left panel in this plot shows the most likely formation scenario for the planetary system. The right panel shows the observed orbital configuration.
Time evolution of orbital elements in the system HD128311. This left panel in this plot shows the most likely formation scenario for the planetary system. The right panel shows the observed orbital configuration.
The HD 128311 planetary system[4]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b >2.18 ± 0.22 MJ 1.099 ± 0.04 458.6 ± 6.8 0.25 ± 0.10 — —
c >3.21 ± 0.30 MJ 1.76 ± 0.13 928.3 ± 18 0.17 ± 0.09 — —

See also

References

  1. 1 2 3 4 5 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. Bibcode:2007A&A...474..653V. arXiv:0708.1752 Freely accessible. doi:10.1051/0004-6361:20078357. Vizier catalog entry
  2. ↑ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  3. ↑ Butler, R. Paul; et al. (2003). "Seven New Keck Planets Orbiting G and K Dwarfs". The Astrophysical Journal. 582 (1): 455–466. Bibcode:2003ApJ...582..455B. doi:10.1086/344570.
  4. 1 2 Vogt, Steven S.; et al. (2005). "Five New Multicomponent Planetary Systems". The Astrophysical Journal. 632 (1): 638–658. Bibcode:2005ApJ...632..638V. doi:10.1086/432901.
  5. ↑ Rein, Hanno; Papaloizou, J. C. B. (2009). "On the evolution of mean motion resonances through stochastic forcing: Fast and slow libration modes and the origin of HD128311". Astronomy and Astrophysics. 497: 595–609. Bibcode:2009A&A...497..595R. arXiv:0811.1813 Freely accessible. doi:10.1051/0004-6361/200811330.

Coordinates: 14h 36m 00.5607s, +09° 44′ 47.466″

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.