HIP 14810
HIP 14810 is a G type main sequence star at the position of approximately 170 light-year [1] in the direction of Aries.
Data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aries |
Right ascension | 03h 11m 14.23s [1] |
Declination | + 21° 05′ 50.5″ [1] |
Apparent magnitude (V) | 8.53 |
Characteristic | |
Spectral class | G5V |
B-V color index | 0.777 |
アストロメトリー | |
Proper motion (μ) | Right ascension: -3.66+-1.81[1]millisecond / year Declination: -53.44+-1.10[1]millisecond / year |
Annual parallax (π) | 18.71 +-1.26[1]millisecond |
Distance | 170 ± 10 Light-year (53 ± 4 Parsec) |
Absolute magnitude (MV) | 4.91 |
The details | |
Mass | 0.99 M☉ |
Radius | 1.1 R☉ |
Surface gravity (log g) | 4.31 |
The intensity of light | 1.2 L☉ |
Surface temperature | 5485 ± 44 K |
Quantity of metal | 0.23 +-0.3 |
Other names | |
BD+20 ° 518, SAO 75776, AG+20 283, TYC 1231-1727-1, GSC 01231-01727, PPM 92274, YZ 20 929 | |
Reference database | |
SIMBAD | data |
NStED | data |
Extrasolar Planets Encyclopaedia | data |
Table of contents
Planetary system
Three extrasolar planets revolve in the circumference of this fixed star. The article was published in 2007 when I discovered HIP 14810 b and HIP 14810 c [2]. On the other hand, the discovery of HIP 14810 d was published with the correction of the orbit parameter of HIP 14810 c in 2009 [3].
Name (order near the fixed star) | Mass | Orbit semimajor axis (Au) | Revolution period (Day) | Orbit eccentricity | Orbit angle of inclination | Radius |
---|---|---|---|---|---|---|
b | ≥3.88 ± 0.32 MJ | 0.0692+-0.0040 | 6.673855+-0.000019 | 0.14270+-0.00094 | — | — |
c | ≥1.28 ± 0.10 MJ | 0.545 +-0.031 | 147.730 +-0.065 | 0.164 +-0.012 | — | — |
d | ≥0.570 ± 0.052 MJ | 1.89 +-0.11 | 952+-15 | 0.173 +-0.037 | — | — |
Allied item
Source
- ^ a b c d e f van Leeuwen, F. (2007). "HIP 14810". Hipparcos, the New Reduction. January 27, 2010 reading.
- ^ Wright et al. (2007). "Four New Exoplanets and Hints of Additional Substellar Companions to Exoplanet Host Stars". The Astrophysical Journal 657 (1): 533?545. doi: 10.1086/51055 .
- ^ a b Jason T. Wright, Debra A. Fischer, Eric B. Ford, Dimitri Veras, Ji Wang, Gregory W. Henry, Geoff W. Marcy, Andrew W. Howard, John Asher Johnson. "A Third Giant Planet Orbiting HIP 14810". The Astrophysical Journal 699 (2): L97?L101. doi: 10.1088/0004-637X/699/2/L9 . (arXiv preprint)
Outside link
- Extrasolar Planet Interactions by Rory Barnes & Richard Greenberg, Lunar and Planetary Lab, University of Arizona
- Image HIP 14810
This article is taken from the Japanese Wikipedia HIP 14810
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