Kepler-19
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lyra |
Right ascension | 19h 21m 40.9996s[1] |
Declination | +37° 51′ 06.436″[1] |
Apparent magnitude (V) | 12.04[2] |
Astrometry | |
Proper motion (μ) | RA: ±0.033 25.284[1] mas/yr Dec.: ±0.037 −30.711[1] mas/yr |
Parallax (π) | 4.5465 ± 0.0202[1] mas |
Distance | 717 ± 3 ly (219.9 ± 1.0 pc) |
Details | |
Mass | ±0.04 0.936[3] M☉ |
Radius | ±0.018 0.85[3] R☉ |
Surface gravity (log g) | 4.54[4] cgs |
Temperature | ±60 5541[3] K |
Metallicity [Fe/H] | -0.13[4] dex |
Rotational velocity (v sin i) | ±0.5 1.8[5] km/s |
Age | ±1.7 1.9[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
KIC | data |
Kepler-19 (TYC 3134-1549-1, 2MASS J19214099+3751064, GSC 03134-01549, KOI-84)[4] is a G7V star that is host to planets Kepler-19b, Kepler-19c and Kepler-19d.
Planetary system
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]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | +1.6 −1.5 8.4 M⊕ |
— | 16+0.00004 −0.00006 9.287 |
±0.02 0.12 | 89.94° | ±0.048 2.209 R⊕ |
c | ±2.7 13.1 M⊕ | — | +0.012 −0.005 28.731 |
+0.05 −0.07 0.21 |
— | — |
d | +1.2 −5.6 22.5 M⊕ |
— | +0.04 −0.30 62.95 |
+0.16 −0.01 0.05 |
— | — |
References
- 1 2 3 4 5 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 Data Release 2 catalog entry
- ↑ 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.
- 1 2 3 4 "Notes on Kepler-19 b". Retrieved 21 January 2017.
- 1 2 3 4 "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.
- ↑ 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.
- 1 2 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.
External links
- NASA, Kepler mission, Table of Confirmed Planets
Coordinates:
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