Kepler-19
Kepler-19
Star in the constellation Lyra
Kepler-19 (TYC 3134-1549-1, 2MASS J19214099+3751064, GSC 03134-01549, KOI-84)[4] is a G7V star that is host to three known planets - Kepler-19b, Kepler-19c, and Kepler-19d. It is located about 720 light-years (220 parsecs) away in the constellation Lyra, five arcminutes northwest of the much more distant open cluster NGC 6791.
Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lyra |
Right ascension | 19h 21m 40.99950s[1] |
Declination | +37° 51′ 06.4373″[1] |
Apparent magnitude (V) | 12.04[2] |
Astrometry | |
Radial velocity (Rv) | −11.36±0.53[1] km/s |
Proper motion (μ) | RA: 25.349 mas/yr[1] Dec.: −30.792 mas/yr[1] |
Parallax (π) | 4.5296 ± 0.0087 mas[1] |
Distance | 720 ± 1 ly (220.8 ± 0.4 pc) |
Details | |
Mass | 0.936±0.04[3] M☉ |
Radius | 0.859±0.018[3] R☉ |
Surface gravity (log g) | 4.54[4] cgs |
Temperature | 5541±60[3] K |
Metallicity [Fe/H] | −0.13±0.06[3] dex |
Rotational velocity (v sin i) | 1.8±0.5[5] km/s |
Age | 1.9±1.7[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
KIC | data |
Close
There are three known planets in the Kepler-19 planetary system. Planet b was discovered by the transit method, c by transit-timing variations[6] and d by radial velocity measurements.[7]
More information Companion (in order from star), Mass ...
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 8.4+1.6 −1.5 M🜨 |
0.0846±0.0012 | 9.2869900 | 0.12±0.02 | 89.94+0.06 −0.44° |
2.209±0.048 R🜨 |
c | 13.1±2.7 M🜨 | — | 28.731+0.012 −0.005 |
0.21+0.05 −0.07 |
— | — |
d | 22.5+1.2 −5.6 M🜨 |
— | 62.95+0.04 −0.30 |
0.05+0.16 −0.01 |
— | — |
Close
- 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.
- Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H.
- Bonomo, A. S.; Dumusque, X.; et al. (April 2023). "Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems". Astronomy & Astrophysics. arXiv:2304.05773. doi:10.1051/0004-6361/202346211. S2CID 258078829.
- "KOI-84". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 January 2017.
- Buchhave, Lars A.; et al. (2012). "An abundance of small exoplanets around stars with a wide range of metallicities". Nature. 486 (7403): 375–377. Bibcode:2012Natur.486..375B. doi:10.1038/nature11121. PMID 22722196. S2CID 4427321.
- Ballard, Sarah; et al. (2011). "The Kepler-19 System: A Transiting 2.2R🜨 Planet and a Second Planet Detected Via Transit Timing Variations". The Astrophysical Journal. 743 (2). 200. arXiv:1109.1561. Bibcode:2011ApJ...743..200B. doi:10.1088/0004-637X/743/2/200.
- Malavolta, Luca; et al. (2017). "The Kepler-19 System: A Thick-envelope Super-Earth with Two Neptune-mass Companions Characterized Using Radial Velocities and Transit Timing Variations". The Astronomical Journal. 153 (5). 224. arXiv:1703.06885. Bibcode:2017AJ....153..224M. doi:10.3847/1538-3881/aa6897.
- NASA, Kepler mission, Table of Confirmed Planets
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