2017년 1월 12일 목요일

HD 13931

HD 13931

HD 13931
Constellation Andromeda
Apparent magnitude (V) 7.61 (±0.03) [1]
Position
Epoch: J2000.0
Right ascension (RA,α) 02h 16m 47.4s [2]
Declination (Dec,δ) 43° 46′ 23″ [2]
Radial velocity (Rv) 33.7 (+-4.6) km/s [2]
Proper motion (μ) Right ascension: 99 milliseconds / year [2]
Declination: -184 milliseconds / year [2]
Annual parallax (π) 22.6 (+-0.7) a millisecond [1]
Distance 144 (±5) Light-year
44.2 (+-1.4) a parsec [1]
Absolute magnitude (MV) 4.32 (+-0.10)
Physical property
Radius 1.23 (+-0.06) R[1]
Mass 1.022 (+-0.02) M[1]
Surface gravity (log g) 4.30 (+-0.08) [1]
Rotation period Approximately 26 days [1]
Spectral class G0 [1] [2]
The intensity of light 1.57 (+-0.14) L[1]
Surface temperature 5829 (+-44) K [1]
Color index (B-V) 0.642 (±0.015) [1]
Quantity of metal [Fe/H] [Fe/H] 0.03 (+-0.04) [1]
Age 8,400 million (+-2,000,000,000) year [1]
The other name
The other name
HIP 10626, BD+43 459, SAO 37918 [2]
■Project ■ Template

HD 13931 is the fixed star of the G type at the approximately 144 light-year away position from the solar system in the direction of Andromeda. I cannot see the apparent magnitude by the naked eye in 7.6 and gloomy one. I am known to have one planet as of 2010.

Characteristic

HD 13931 is a fixed star of the spectral class G type same as the sun, and the metal quantity is observed with degree same as the sun, too, but, as for the intensity of light, there is greatly a radius around 1.57 times of the sun. Because I am slightly more spirited than the standard main sequence star of activity of the chromosphere being calm, and rotation speed being slow and the same spectral class, it is thought with a star aged than the sun (4,600 million years old), and the age is estimated with 10,400 million years old from 6,400 million [1].

In 2010, extrasolar planet HD 13931 b over this fixed star was reported. HD 13931 b revolves in circular orbit of radius 5.2AU on a huge planet of the mass 2 times as large as Jupiter for 11.5 years. Because this planet has the property of the solar system similar to the Jupiter; called "analog of the Jupiter" [1].

Planet of HD 13931
Name
(order near the fixed star)
Mass Orbit semimajor axis
Au
Revolution period
(Day)
Orbit eccentricity Orbit angle of inclination Radius
b >1.88 MJ 5.15 4218 0.02

References

  1. ^ a b c d e f g h i j k l m n o Howard, A. H. et al. (2010). It is arXiv: "The California Planet Survey I. Four New Giant Exoplanets" 1003.3488v1. 
  2. ^ a b c d e f g "SIMBAD query result". SIMBAD, CDS. March 25, 2010 reading.

Allied item

This article is taken from the Japanese Wikipedia HD 13931

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