HD 216770
| Observation data Epoch J2000 Equinox ICRS | |
|---|---|
| Constellation | Piscis Austrinus[1] |
| Right ascension | 22h 55m 53.708s[2] |
| Declination | –26° 39′ 31.54″[2] |
| Apparent magnitude (V) | 8.11[3] |
| Characteristics | |
| Spectral type | K0V[3] or G9VCN+1[4] |
| B−V color index | 0.821[3] |
| Astrometry | |
| Radial velocity (Rv) | 31.141±0.0004[5] km/s |
| Proper motion (μ) | RA: 226.237 mas/yr[2] Dec.: −177.985 mas/yr[2] |
| Parallax (π) | 27.2923±0.0245 mas[2] |
| Distance | 119.5 ± 0.1 ly (36.64 ± 0.03 pc) |
| Absolute magnitude (MV) | 5.22[3] |
| Details | |
| Mass | 0.74±0.07[6] M☉ |
| Radius | 0.93±0.02[6] R☉ |
| Luminosity | 0.79[3] L☉ |
| Surface gravity (log g) | 4.37±0.04[6] cgs |
| Temperature | 5,399±18[6] K |
| Metallicity [Fe/H] | 0.27[6] dex |
| Rotation | 35.6 d[3] |
| Rotational velocity (v sin i) | 1.4[3] km/s |
| Age | 3.1[3] Gyr |
| Other designations | |
| CD−27°16109, GC 31973, HIP 113238, SAO 191502, LTT 9276, NLTT 55283[7] | |
| Database references | |
| SIMBAD | data |
HD 216770 is a star with an orbiting exoplanet in the southern constellation of Piscis Austrinus. With an apparent visual magnitude of 8.11,[3] it is too faint to be visible to the naked eye. It is located at a distance of 120 light years from the Sun, as determined by parallax measurements, and is drifting further away with a radial velocity of 31.1 km/s.[5] The star shows a high proper motion, traversing the celestial sphere at an angular rate of 0.302 arcsec yr−1.[8]
The spectrum of HD 216770 presents as a late G-type main-sequence star, a yellow dwarf, with a stellar classification of G9VCN+1,[4] where the suffix notation indicates anomalously strong band of CN. The star is smaller than the Sun, with 74% of the Sun's mass and 93% of the Sun's radius.[6] It is about three billion years old and is spinning slowly with a rotation period of 35.6 days.[3] The abundance of iron, a measure of the metallicity of the star, is higher than solar. The star is radiating 79% of the luminosity of the Sun from its photosphere at an effective temperature of 5,399 K.[6]
In 2003 an exoplanet was announced orbiting it by the Geneva Extrasolar Planet Search team.[3] As the inclination of the orbital plane is unknown, only a lower bound on the mass of the object can be determined. It has at least 65% of the mass of Jupiter. The body has an eccentric orbit with a period of 118.5 days.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination (°) |
Radius |
|---|---|---|---|---|---|---|
| b | >0.65 MJ | 0.46 | 118.45 ± 0.55 | 0.37 ± 0.06 | — | — |
See also
[edit]References
[edit]- ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
- 1 2 3 4 5 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- 1 2 3 4 5 6 7 8 9 10 11 Mayor, M.; et al. (2004). "The CORALIE survey for southern extra-solar planets XII. Orbital solutions for 16 extra-solar planets discovered with CORALIE". Astronomy and Astrophysics. 415 (1): 391–402. arXiv:astro-ph/0310316. Bibcode:2004A&A...415..391M. doi:10.1051/0004-6361:20034250. S2CID 5233877.
- 1 2 Gray, R. O.; et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv:astro-ph/0603770. Bibcode:2006AJ....132..161G. doi:10.1086/504637. S2CID 119476992.
- 1 2 Soubiran, C.; et al. (2018). "Gaia Data Release 2. The catalogue of radial velocity standard stars". Astronomy and Astrophysics. 616: A7. arXiv:1804.09370. Bibcode:2018A&A...616A...7S. doi:10.1051/0004-6361/201832795. S2CID 52952408.
- 1 2 3 4 5 6 7 Stassun, Keivan G.; et al. (2017). "Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes". The Astronomical Journal. 153 (3): 136. arXiv:1609.04389. Bibcode:2017AJ....153..136S. doi:10.3847/1538-3881/aa5df3. S2CID 119219062.
- ↑ "HD 216770". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-06-25.
- ↑ Luyten, W. J. (June 1995). "NLTT Catalogue (Luyten, 1979)". VizieR Online Data Catalog. Bibcode:1995yCat.1098....0L.
External links
[edit]- "Notes for star HD 216770". Extrasolar Planets Encyclopaedia. Archived from the original on June 2, 2006.
