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Kepler-67

From Wikipedia, the free encyclopedia
G-type star located in the open cluster NGC 6811 in the constellation Cygnus
Kepler-67
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus
Right ascension19h 36m 36.8094s[1]
Declination+46° 09′ 59.167″[1]
Apparent magnitude (V)16.4
Characteristics
Spectral typeG9V
Astrometry
Proper motion (μ)RA: −3.530(41)mas/yr[1]
Dec.: −8.741(39)mas/yr[1]
Parallax (π)0.8734±0.0344 mas[1]
Distance3,700 ± 100 ly
(1,140 ± 50 pc)
Details
Mass0.865 ± 0.034 M
Radius0.778 ± 0.031 R
Temperature5331 ± 63 K K
Metallicity [Fe/H]0.012 ± 0.003 dex
Rotation10.464±0.014 days[2]
Age1 ± 0.17 Gyr
Other designations
KOI-2115[3]
Database references
SIMBADdata

Kepler-67 is a star in theopen clusterNGC 6811[4] in theconstellationCygnus. It has slightly less mass than theSun and has one confirmed planet, slightly smaller thanNeptune, announced in 2013.[5]

Planetary system

[edit]
The Kepler-67 planetary system
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b0.31 ± 0.06 MJ0.1171 ± 0.001515.7259 ± 0.000110.26 ± 0.014 RJ

References

[edit]
  1. ^abcdVallenari, 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. ^McQuillan, A.; Mazeh, T.; Aigrain, S. (2013). "Stellar Rotation Periods of The Kepler objects of Interest: A Dearth of Close-In Planets Around Fast Rotators".The Astrophysical Journal Letters.775 (1). L11.arXiv:1308.1845.Bibcode:2013ApJ...775L..11M.doi:10.1088/2041-8205/775/1/L11.S2CID 118557681.
  3. ^"Kepler-67".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved15 January 2018.
  4. ^Maliuk, A.; Budaj, J. (2020), "Spatial distribution of exoplanet candidates based on Kepler and Gaia data",Astronomy & Astrophysics,635: A191,arXiv:2002.10823,Bibcode:2020A&A...635A.191M,doi:10.1051/0004-6361/201936692,S2CID 211296456
  5. ^Meibom, Søren; Torres, Guillermo; Fressin, Francois; Latham, David W.; Rowe, Jason F.; Ciardi, David R.; Bryson, Steven T.; Rogers, Leslie A.; Henze, Christopher E.; Janes, Kenneth; Barnes, Sydney A.; Marcy, Geoffrey W.; Isaacson, Howard; Fischer, Debra A.; Howell, Steve B.; Horch, Elliott P.; Jenkins, Jon M.; Schuler, Simon C.; Crepp, Justin (2013)."The same frequency of planets inside and outside open clusters of stars".Nature.499 (7456):55–58.arXiv:1307.5842.Bibcode:2013Natur.499...55M.doi:10.1038/nature12279.PMID 23803764.S2CID 4356893.

External links

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