KIC 11026764
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 21m 24.6295s [1] |
| Declination | +48° 30′ 53.340″ [1] |
| Apparent magnitude (V) | 9.71[1] |
| Characteristics | |
| Evolutionary stage | subgiant star[2] |
| Spectral type | G1[3] |
| Astrometry | |
| Radial velocity (Rv) | -35.00[1] km/s |
| Proper motion (μ) | RA: -2466.98[1] mas/yr Dec.: 1180.09[1] mas/yr |
| Parallax (π) | 78.91 ± 2.60 mas |
| Distance | 41 ± 1 ly (12.7 ± 0.4 pc) |
| Details[4] | |
| Mass | 1.18±0.08[5] M☉ |
| Radius | 2.18 ± 0.05 R☉ |
| Luminosity | 3.56 ± 0.14 L☉ |
| Surface gravity (log g) | 3.884±0.009 cgs |
| Temperature | 5636±80[2] K |
| Metallicity [Fe/H] | 0.04[5] dex |
| Rotational velocity (v sin i) | 2.6[1] km/s |
| Age | 5.69±0.68[5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
KIC 11026764, nicknamed "Gemma" by Li et al.,[2] is a G-type main sequence star whose characteristics have been extensively measured by the Kepler spacecraft because of its similarity to the Sun. Its diameter is 2.18 times the Sun and is aged at 5.94 billion years, slightly older than the Sun.[4]
The star exhibits a weak quasi-periodic pulsations with frequency around 0.0009 Hz.[2]
References[edit]
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "KIC 11026764". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 27 November 2016.
- ↑ 2.0 2.1 2.2 2.3 Li, Yaguang; Bedding, Timothy R.; Li, Tanda; Bi, Shaolan; Stello, Dennis; Zhou, Yixiao; White, Timothy R. (2020), "Asteroseismology of 36 Kepler subgiants – I. Oscillation frequencies, linewidths, and amplitudes", Monthly Notices of the Royal Astronomical Society, 495 (2): 2363–2386, arXiv:2005.06460, doi:10.1093/mnras/staa1335
- ↑ Molenda-Żakowicz, J.; Sousa, S. G.; Frasca, A.; Uytterhoeven, K.; Briquet, M.; Van Winckel, H.; Drobek, D.; Niemczura, E.; Lampens, P.; Lykke, J.; Bloemen, S.; Gameiro, J. F.; Jean, C.; Volpi, D.; Gorlova, N.; Mortier, A.; Tsantaki, M.; Raskin, G. (2013). "Atmospheric parameters of 169 F-, G-, K- and M-type stars in the Kepler field". Monthly Notices of the Royal Astronomical Society. 434 (2): 1422. arXiv:1306.6011. Bibcode:2013MNRAS.434.1422M. doi:10.1093/mnras/stt1095. Unknown parameter
|s2cid=ignored (help) - ↑ 4.0 4.1 Metcalfe, T. S.; Monteiro, M. J. P. F. G.; Thompson, M. J.; Molenda-Żakowicz, J.; Appourchaux, T.; Chaplin, W. J.; Doğan, G.; Eggenberger, P.; Bedding, T. R.; Bruntt, H.; Creevey, O. L.; Quirion, P.-O.; Stello, D.; Bonanno, A.; Silva Aguirre, V.; Basu, S.; Esch, L.; Gai, N.; Di Mauro, M. P.; Kosovichev, A. G.; Kitiashvili, I. N.; Suárez, J. C.; Moya, A.; Piau, L.; García, R. A.; Marques, J. P.; Frasca, A.; Biazzo, K.; Sousa, S. G.; et al. (2010). "A Precise Asteroseismic Age and Radius for the Evolved Sun-Like Star Kic 11026764". The Astrophysical Journal. 723 (2): 1583–1598. arXiv:1010.4329. Bibcode:2010ApJ...723.1583M. doi:10.1088/0004-637X/723/2/1583. Unknown parameter
|s2cid=ignored (help) - ↑ 5.0 5.1 5.2 Li, Tanda; Bedding, Timothy R.; Christensen-Dalsgaard, Jørgen; Stello, Dennis; Li, Yaguang; Keen, Matthew A. (2020), "Asteroseismology of 36 Kepler subgiants – II. Determining ages from detailed modelling", Monthly Notices of the Royal Astronomical Society, 495 (3): 3431–3462, arXiv:2006.00901, doi:10.1093/mnras/staa1350
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