HD 4313
HD 4313 is a K-type subgiant located in the constellation of Pisces. It hosts an extrasolar planet, and is drifting away from the Solar System with a radial velocity of 14.67 km/s
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pisces |
Right ascension | 00h 45m 40.3578s[1] |
Declination | +07° 50′ 42.075″[1] |
Apparent magnitude (V) | 7.83[2] |
Characteristics | |
Spectral type | K2 IV |
Astrometry | |
Radial velocity (Rv) | 14.67[2] km/s |
Proper motion (μ) | RA: −6.281[1] mas/yr Dec.: 6.566[1] mas/yr |
Parallax (π) | 7.4492 ± 0.0259[1] mas |
Distance | 438 ± 2 ly (134.2 ± 0.5 pc) |
Details | |
Mass | 2.47±0.52[2] M☉ |
Radius | 5.14[2] R☉ |
Luminosity | +1.15±0.02[2] L☉ |
Surface gravity (log g) | 3.24[2] cgs |
Temperature | 4943[2] K |
Metallicity [Fe/H] | +0.14±0.10[2] dex |
Rotational velocity (v sin i) | 1.91±0.25[2] km/s |
Age | 1.72±0.37 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Physical properties
This is an aging star with a mass of twice the Sun, and radiating 1.15 times the luminosity. It also is a swollen star with 5.14 times the radius, and has a cool temperature of 4943 K. The "IV" in the spectral class means it's a K-type subgiant star which is starting to exhaust the hydrogen at its core, and cooling and expanding to become a red giant.
System
HD 4313 is a single star, which means it has no binary partners, but has a Jovian planet orbiting it. This planet was discovered in 2010.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 1.927±0.090 MJ | 1.157±0.097 | 356.21±0.88 | 0.147±0.047 | — | 1.2 RJ |
References
- Brown, A. G. A.; et al. (Gaia collaboration). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics (in press). arXiv:2012.01533. doi:10.1051/0004-6361/202039657. S2CID 227254300. Gaia EDR3 record for this source at VizieR.
- "Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 2020-12-11.
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