HD 166724

HD 166724
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Corona Australis
Right ascension 18h 13m 59.676s[1]
Declination –42° 34 31.35[1]
Apparent magnitude (V) +9.33
Characteristics
Spectral type K0IV
Astrometry
Proper motion (μ) RA: 36.60 ± 1.59[1] mas/yr
Dec.: –78.62 ± 0.99[1] mas/yr
Parallax (π)23.63 ± 1.21[1] mas
Distance138 ± 7 ly
(42 ± 2 pc)
Details
Mass0.81 ± 0.02 M
Radius0.81 ± 0.02 R
Luminosity0.31 L
Surface gravity (log g)4.41 ± 0.04 cgs
Temperature5362 ± 29 K
Metallicity [Fe/H]–0.09 ± 0.03 dex
Age4.0 ± 3.8 Gyr
Other designations
HIP 89354, CD–42 13019
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia
data

HD 166724 is a K-class dwarf star.

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 planet was deduced by radial velocity. This was published in November.

The discoverers noted that HD 166724 b is among "the three most eccentric planets with a period larger than 5 years" alongside HD 98649 b and HD 219077 b; but unlike them, too dim as a candidate for direct imaging with current technology. The reason for this eccentricity is unknown.[2]

The HD 166724 planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >3.53 ± 0.11 MJ 5.42 ± 0.43 5144+705
467
0.734 ± 0.020

References

  1. 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.Vizier catalog entry
  2. 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.
  3. "hd_166724_b".