HD 191939
HD 191939 is a single yellow (G-type) main-sequence star, located approximately 174 light-years away in the constellation of Draco, taking its primary name from its Henry Draper Catalogue designation.
Location of HD 191939 in the night sky. The star is marked within the red diamond. | |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Draco |
| Right ascension | 20h 08m 05.75515s[1] |
| Declination | +66° 51′ 02.0766″[1] |
| Apparent magnitude (V) | 8.971[2] |
| Characteristics | |
| HD 191939 | |
| Evolutionary stage | main sequence |
| Spectral type | G9V[3] |
| Astrometry | |
| Radial velocity (Rv) | −9.23±0.16[1] km/s |
| Proper motion (μ) | RA: 150.194±0.015 mas/yr[1] Dec.: −63.988±0.017 mas/yr[1] |
| Parallax (π) | 18.6967 ± 0.0133 mas[1] |
| Distance | 174.4 ± 0.1 ly (53.49 ± 0.04 pc) |
| Absolute magnitude (MV) | 5.32 |
| Details[3] | |
| HD 191939 | |
| Mass | 0.81±0.04 M☉ |
| Radius | 0.94±0.02 R☉ |
| Luminosity (bolometric) | 0.65±0.02 L☉ |
| Surface gravity (log g) | 4.3±0.1 cgs |
| Temperature | 5348±100 K |
| Metallicity [Fe/H] | −0.15±0.06 dex |
| Rotational velocity (v sin i) | 0.6±0.5[4] km/s |
| Age | 7±3[4] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
| Extrasolar Planets Encyclopaedia | data |
Characteristics Edit
HD 191939 is a Sun-like G-type main-sequence star, likely older than the Sun and relatively depleted in metals.
Planetary system Edit
In 2020, an analysis carried out by a team of astronomers led by astronomer Mariona Badenas-Agusti of the TESS project confirmed the existence of three gaseous planets, all smaller than Neptune, in orbit around HD 191939.[4] Another non-transiting gas giant planet designated HD 191939 e was detected in 2021, along with a substellar object on a highly uncertain, 9 to 46 year orbit.[3] In 2022, a sixth planet, with a mass comparable to Uranus, was discovered in the system's habitable zone.[6] The 2021 study also suggested the possible presence of an additional non-transiting planet with a period of 17.7 days,[3] but the 2022 study did not support this.[6]
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 10.00±0.70 M🜨 | 0.0804+0.0025 −0.0023 | 8.8803256 | 0.031+0.010 −0.011 | 88.10+0.14 −0.10° | 3.410±0.075 R🜨 |
| c | 8.0±1.0 M🜨 | 0.1752+0.0055 −0.0050 | 28.579743 | 0.034+0.034 −0.013 | 89.10+0.06 −0.08° | 3.195±0.075 R🜨 |
| d | 2.80±0.60 M🜨 | 0.2132+0.0065 −0.0061 | 38.353037 | 0.031+0.018 −0.012 | 89.49+0.05 −0.08° | 2.995±0.070 R🜨 |
| e | ≥112.2±4.0 M🜨 | 0.407±0.012 | 101.12±0.13 | 0.031+0.008 −0.016 | 88.7±0.7[3]° | — |
| g | ≥13.5±2.0 M🜨 | 0.812±0.028 | 284+10 −8 | 0.030+0.025 −0.011 | — | — |
| f | >2.08 MJ | >3.2 | >2200 | — | — | — |
See also Edit
References Edit
- ^ a b c d e Vallenari, A.; et al. (Gaia Collaboration) (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. arXiv:2208.00211. doi:10.1051/0004-6361/202243940. Gaia DR3 record for this source at VizieR.
- ^ "HD 191939 - Star - SKY-MAP". news.sky-map.org.
- ^ a b c d e Lubin, Jack; et al. (2022). "TESS-Keck Survey. IX. Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian plus a Distant Substellar Companion". The Astronomical Journal. 163 (2): 101. arXiv:2108.02208. Bibcode:2022AJ....163..101L. doi:10.3847/1538-3881/ac3d38. S2CID 236924440.
- ^ a b c Badenas-Agusti, Mariona; Günther, Maximilian N.; Daylan, Tansu; Mikal-Evans, Thomas; Vanderburg, Andrew; Huang, Chelsea X.; Matthews, Elisabeth; Rackham, Benjamin V.; Bieryla, Allyson; Stassun, Keivan G.; Kane, Stephen R.; Shporer, Avi; Fulton, Benjamin J.; Hill, Michelle L.; Nowak, Grzegorz; Ribas, Ignasi; Pallé, Enric; Jenkins, Jon M.; Latham, David W.; Seager, Sara; Ricker, George R.; Vanderspek, Roland K.; Winn, Joshua N.; Abril-Pla, Oriol; Collins, Karen A.; Pere Guerra Serra; Niraula, Prajwal; Rustamkulov, Zafar; Barclay, Thomas; et al. (2020). "HD 191939: Three Sub-Neptunes Transiting a Sun-like Star Only 54 pc Away". The Astronomical Journal. 160 (3): 113. arXiv:2002.03958. Bibcode:2020AJ....160..113B. doi:10.3847/1538-3881/aba0b5. S2CID 211069628.
- ^ "HD 191939". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c Orell-Miquel, J.; Nowak, G.; Murgas, F.; Palle, E.; Morello, G.; Luque, R.; Badenas-Agusti, M.; Ribas, I.; Lafarga, M.; Espinoza, N.; Morales, J. C.; Zechmeister, M.; Alqasim, A.; Cochran, W. D.; Gandolfi, D.; Goffo, E.; Kabáth, P.; Korth, J.; Livingston, J.; Lam, K. W. F.; Muresan, A.; Persson, C. M.; Van Eylen, V. (2023). "HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone". Astronomy & Astrophysics. 669: A40. arXiv:2211.00667. Bibcode:2023A&A...669A..40O. doi:10.1051/0004-6361/202244120. S2CID 253197272.