HD 27631
HD 27631 is a G-class yellow dwarf star located 164.3 ± 0.3 light-years from Earth.[1] It is smaller and cooler than the Sun, with 0.94 ± 0.04 of its mass and a surface temperature of 5737±36 K. It is thought to be 4.4 ± 3.6 billion years old.[3]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Horologium |
Right ascension | 04h 19m 45.46931s[1] |
Declination | –41° 57′ 36.9515″[1] |
Apparent magnitude (V) | 8.243±0.012[2] |
Characteristics | |
Spectral type | G3IV[2] |
B−V color index | 0.721±0.009[2] |
Astrometry | |
Proper motion (μ) | RA: –41.229 ± 0.054[1] mas/yr Dec.: –91.988 ± 0.067[1] mas/yr |
Parallax (π) | 19.8573 ± 0.0323[1] mas |
Distance | 164.3 ± 0.3 ly (50.36 ± 0.08 pc) |
Details[2] | |
Mass | 0.944±0.032 M☉ |
Radius | 0.923±0.033 R☉ |
Surface gravity (log g) | 4.455±0.038 cgs |
Temperature | 5,737±36 K |
Metallicity [Fe/H] | −0.12±0.05 dex |
Rotation | ~31 d |
Age | 4.010±2.892 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
Extrasolar Planets Encyclopaedia | data |
A survey in 2015 have ruled out the existence of any stellar companions at projected distances above 40 astronomical units.[4]
Planetary system
From 1998 to 2012, the star was under observance from "the CORALIE echelle spectrograph at La Silla Observatory".
In 2012, a long-period, wide-orbiting exoplanet was deduced by radial velocity. This was published in November.[3]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥ 1.494±0.042 MJ | 3.242+0.070 −0.068 |
2198.14+54.11 −50.34 |
0.141+0.062 −0.065 |
— | — |
References
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- Barbato, D.; et al. (August 2018). "Exploring the realm of scaled solar system analogues with HARPS". Astronomy & Astrophysics. 615: 21. arXiv:1804.08329. Bibcode:2018A&A...615A.175B. doi:10.1051/0004-6361/201832791. A175.
- Marmier, M.; et al. (2013). "The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets". Astronomy and Astrophysics. 551. A90. arXiv:1211.6444. Bibcode:2013A&A...551A..90M. doi:10.1051/0004-6361/201219639. S2CID 59467665.
- Mugrauer, M.; Ginski, C. (12 May 2015). "High-contrast imaging search for stellar and substellar companions of exoplanet host stars". Monthly Notices of the Royal Astronomical Society. 450 (3): 3127–3136. doi:10.1093/mnras/stv771. Retrieved 19 June 2020.
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