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Kepler-67

From Wikipedia, the free encyclopedia
Kepler-67
Observation data
Epoch J2000      Equinox ICRS
Constellation Cygnus[1]
Right ascension 19h 36m 36.8094s[2]
Declination +46° 09 59.167[2]
Apparent magnitude (V) 16.4[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type G9V[3]
Astrometry
Proper motion (μ) RA: −3.530(41) mas/yr[2]
Dec.: −8.741(39) mas/yr[2]
Parallax (π)0.8734±0.0344 mas[2]
Distance3,700 ± 100 ly
(1,140 ± 50 pc)
Details
Mass0.865±0.034[3] M
Radius0.778±0.031[3] R
Surface gravity (log g)4.594±0.022[3] cgs
Temperature5,331±63[3] K
Metallicity [Fe/H]0.012±0.003[3] dex
Rotation10.464±0.014 days[4]
Age1±0.17[3] Gyr
Other designations
KOI-2115[5]
Database references
SIMBADdata

Kepler-67 is a star in the open cluster NGC 6811[6] in the constellation Cygnus. It has slightly less mass than the Sun and has one confirmed planet, slightly smaller than Neptune, announced in 2013.[3]

Planetary system

[edit]
The Kepler-67 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b 0.31±0.06 MJ 0.1171±0.0015 15.7259±0.00011 0.26±0.014 RJ

References

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  1. Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
  2. 1 2 3 4 5 6 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.
  3. 1 2 3 4 5 6 7 8 9 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.
  4. 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.
  5. "Kepler-67". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 15 January 2018.
  6. 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.
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