Kepler-43
| Observation data Epoch J2000 Equinox ICRS | |
|---|---|
| Constellation | Lyra[1] |
| Right ascension | 19h 00m 57.8034s[2] |
| Declination | +46° 40′ 05.666″[2] |
| Apparent magnitude (V) | 14.08[3] |
| Characteristics | |
| Evolutionary stage | subgiant[2] |
| Spectral type | G0V~G0IV[4] |
| Astrometry | |
| Proper motion (μ) | RA: −2.982(14) mas/yr[2] Dec.: 0.126(14) mas/yr[2] |
| Parallax (π) | 0.9846±0.0116 mas[2] |
| Distance | 3,310 ± 40 ly (1,020 ± 10 pc) |
| Details | |
| Mass | 1.32±0.09[4] M☉ |
| Radius | 1.42±0.07[4] R☉ |
| Luminosity | 1.95[5] L☉ |
| Surface gravity (log g) | 4.26±0.05[6] cgs |
| Temperature | 6,041±123[4] K |
| Metallicity [Fe/H] | 0.33±0.11[4] dex |
| Rotation | 12.851±0.053 days[7] |
| Rotational velocity (v sin i) | 5.5±1.5[4] km/s |
| Age | 2.8+1.0 −0.8[4] Gyr |
| Other designations | |
| Kepler-43, KOI-135, KIC 9818381 | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
| KIC | data |
Kepler-43, formerly known as KOI-135, is a star in the northern constellation of Lyra. At 14th magnitude, it is too faint to be seen with the naked eye.
Planetary system
[edit]The Kepler spacecraft detected a transiting planet candidate around this star that was confirmed by radial velocity measurements taken by the SOPHIE spectrograph mounted on the 1.93 m telescope at the Haute-Provence Observatory.[4]
The planet nightside temperature was measured to be 2,043+79
−352 K.[6]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination (°) |
Radius |
|---|---|---|---|---|---|---|
| b | 3.23±0.19 MJ | 0.0449 | 3.0240949±0.0000006 | — | — | — |
References
[edit]- ↑ 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.
- 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.
- ↑ Furlan, E.; Ciardi, D. R.; Everett, M. E.; Saylors, M.; Teske, J. K.; Horch, E. P.; Howell, S. B.; Van Belle, G. T.; Hirsch, L. A.; Gautier, T. N., III; Adams, E. R.; Barrado, D.; Cartier, K. M. S.; Dressing, C. D.; Dupree, A. K.; Gilliland, R. L.; Lillo-Box, J.; Lucas, P. W.; Wang, J. (2017). "The Kepler Follow-up Observation Program. I. A Catalog of Companions to Kepler Stars from High-Resolution Imaging". The Astronomical Journal. 153 (2): 71. arXiv:1612.02392. Bibcode:2017AJ....153...71F. doi:10.3847/1538-3881/153/2/71.
- 1 2 3 4 5 6 7 8 Bonomo, A. S.; et al. (2012). "SOPHIE velocimetry of Kepler transit candidates. V. The three hot Jupiters KOI-135b, KOI-204b, and KOI-203b (alias Kepler-17b)". Astronomy and Astrophysics. 538. A96. arXiv:1110.5462. Bibcode:2012A&A...538A..96B. doi:10.1051/0004-6361/201118323. S2CID 118528032.
- ↑ Wilson, Robert F.; Cañas, Caleb I.; Majewski, Steven R.; Cunha, Katia; Smith, Verne V.; Bender, Chad F.; Mahadevan, Suvrath; Fleming, Scott W.; Teske, Johanna; Ghezzi, Luan; Jönsson, Henrik; Beaton, Rachael L.; Hasselquist, Sten; Stassun, Keivan; Nitschelm, Christian; García-Hernández, D. A.; Hayes, Christian R.; Tayar, Jamie (2022). "The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets". The Astronomical Journal. 163 (3): 128. arXiv:2111.01753. Bibcode:2022AJ....163..128W. doi:10.3847/1538-3881/ac3a06.
- 1 2 3 4 Esteves, Lisa J.; Mooij, Ernst J. W. De; Jayawardhana, Ray (2014), "Changing Phases of Alien Worlds: Probing Atmospheres Ofkeplerplanets with High-Precision Photometry", The Astrophysical Journal, 804 (2): 150, arXiv:1407.2245, Bibcode:2015ApJ...804..150E, doi:10.1088/0004-637X/804/2/150, S2CID 117798959
- ↑ 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.