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].
| 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
Allied item
This article is taken from the Japanese Wikipedia HD 13931
This article is distributed by cc-by-sa or GFDL license in accordance with the provisions of Wikipedia.
In addition, Tranpedia is simply not responsible for any show is only by translating the writings of foreign licenses that are compatible with CC-BY-SA license information.
0 개의 댓글:
댓글 쓰기