Summary
HD 185269 is a stellar triple system[4] approximately 170 light-years away in the constellation Cygnus. It is easily visible to binoculars, but not the naked eye.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 37m 11.7411s[1] |
| Declination | +28° 29′ 59.5025″[1] |
| Apparent magnitude (V) | 6.67[2] |
| Characteristics | |
| Spectral type | G0IV[2] |
| B−V color index | 0.58[2] |
| Astrometry | |
| Proper motion (μ) | RA: −31.499±0.045[1] mas/yr Dec.: −80.782±0.046[1] mas/yr |
| Parallax (π) | 19.2049 ± 0.0309 mas[1] |
| Distance | 169.8 ± 0.3 ly (52.07 ± 0.08 pc) |
| Absolute magnitude (MV) | 3.29[2] |
| Absolute bolometric magnitude (Mbol) | 3.228[2] |
| Details[2] | |
| Mass | 1.33 ± 0.07 M☉ |
| Surface gravity (log g) | 4.05 ± 0.22 cgs |
| Temperature | 5983 ± 62 K |
| Metallicity [Fe/H] | 0.10 ± 0.08 dex |
| Rotational velocity (v sin i) | 5.5 km/s |
| Age | 4.0 ± 1.0 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
The primary star is a third more massive[2] and four times more luminous than the Sun.[citation needed] The spectrum of the star is G0IV.[2] About 4.5 arcseconds away are the two other stars, which are much less massive than the Sun. The primary has a mass of 0.165 M☉, while the secondary has a mass of 0.154 M☉.[4]
Planetary system edit
The Jupiter-mass hot Jupiter was independently discovered orbiting the primary star by two different teams using doppler spectroscopy. One group led by Claire Moutou used the ELODIE spectrograph at the Haute-Provence Observatory in France while John Asher Johnson and collaborators used the Coudé Auxiliary and C. Donald Shane telescopes at Lick Observatory in California.[2][5] The planet takes 6.8 days to orbit at 0.077 AU from the primary star in an eccentric orbit.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥1.010±0.014 MJ | 0.0770±0.0034 | 6.83776±0.00027 | 0.229±0.014 | — | — |
See also edit
References edit
- ^ a b c d e 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.
- ^ a b c d e f g h i Moutou, C.; et al. (2006). "ELODIE metallicity-biased search for transiting Hot Jupiters. III. A hot Jupiter orbiting the star HD 185269". Astronomy and Astrophysics. 458 (1): 327–329. arXiv:0707.0958. Bibcode:2006A&A...458..327M. doi:10.1051/0004-6361:20066029.
- ^ "HD 185269". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-09-19.
- ^ a b Ginski, C.; et al. (2016). "A lucky imaging multiplicity study of exoplanet host stars – II". Monthly Notices of the Royal Astronomical Society. 457 (2): 2173–2191. arXiv:1601.01524. Bibcode:2016MNRAS.457.2173G. doi:10.1093/mnras/stw049.
- ^ Johnson, John Asher; et al. (2006). "An Eccentric Hot Jupiter Orbiting the Subgiant HD 185269". The Astrophysical Journal. 652 (2): 1724–1728. arXiv:astro-ph/0608035. Bibcode:2006ApJ...652.1724J. doi:10.1086/508255.
- ^ Luhn, Jacob K.; et al. (2019). "Retired A Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts". The Astronomical Journal. 157 (4). 149. arXiv:1811.03043. Bibcode:2019AJ....157..149L. doi:10.3847/1538-3881/aaf5d0. S2CID 102486961.
External links edit
- "Notes for star HD 185269". Extrasolar Planets Encyclopaedia. Archived from the original on September 29, 2007.
- "HD 185269". Systemic. 20 April 2007.