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Kepler-19

Coordinates:Sky map19h 21m 41s, +37° 51′ 06″
From Wikipedia, the free encyclopedia
Star in the constellation Lyra
Kepler-19
Observation data
Epoch J2000      Equinox J2000
ConstellationLyra
Right ascension19h 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: 25.349mas/yr[1]
Dec.: −30.792mas/yr[1]
Parallax (π)4.5296±0.0087 mas[1]
Distance720 ± 1 ly
(220.8 ± 0.4 pc)
Details
Mass0.936±0.04[3] M
Radius0.859±0.018[3] R
Surface gravity (log g)4.54[4] cgs
Temperature5541±60[3] K
Metallicity [Fe/H]−0.13±0.06[3] dex
Rotational velocity (v sin i)1.8±0.5[5] km/s
Age1.9±1.7[3] Gyr
Other designations
KIC 2571238,KOI-84,TYC 3134-1549-1,GSC 03134-01549,2MASS J19214099+3751064, Gaia DR2 2051106987063242880[4]
Database references
SIMBADdata
KICdata

Kepler-19 (TYC 3134-1549-1,2MASS J19214099+3751064,GSC 03134-01549,KOI-84)[4] is a G7Vstar that is host to three knownplanets -Kepler-19b,Kepler-19c, andKepler-19d. It is located about 720light-years (220parsecs) away in the constellationLyra, five arcminutes northwest of the much more distantopen clusterNGC 6791.

Planetary system

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There are three known planets in the Kepler-19 planetary system. Planet b was discovered by thetransit method, c bytransit-timing variations[6] and d byradial velocity measurements.[7]

The Kepler-19 planetary system[7][3]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b8.4+1.6
−1.5
 M🜨
0.0846±0.00129.28699000.12±0.0289.94+0.06
−0.44
°
2.209±0.048 R🜨
c13.1±2.7 M🜨28.731+0.012
−0.005
0.21+0.05
−0.07
d22.5+1.2
−5.6
 M🜨
62.95+0.04
−0.30
0.05+0.16
−0.01

References

[edit]
  1. ^abcdeVallenari, 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 atVizieR.
  2. ^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.
  3. ^abcdefBonomo, 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.Bibcode:2023A&A...677A..33B.doi:10.1051/0004-6361/202346211.S2CID 258078829.
  4. ^abc"KOI-84".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved21 January 2017.
  5. ^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.
  6. ^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.
  7. ^abMalavolta, 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

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