Kepler-411
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 10m 25.3471s[1] |
Declination | +49° 31′ 23.7119″[1] |
Apparent magnitude (V) | 12.55[1] |
Characteristics | |
Kepler-411 | |
Evolutionary stage | main-sequence star |
Spectral type | K3V |
Kepler-411B | |
Astrometry | |
Radial velocity (Rv) | -20.7±1.5[2] km/s |
Proper motion (μ) | RA: 13.611[2] mas/yr Dec.: 32.543[2] mas/yr |
Parallax (π) | 6.53126 ± 0.00796[2] mas |
Distance | 499.4 ± 0.6 ly (153.1 ± 0.2 pc) |
Position (relative to Kepler-411)[3] | |
Component | Kepler-411B |
Epoch of observation | 2012 |
Angular distance | 3.4±0.06″ |
Position angle | 331±3° |
Observed separation (projected) | 520 AU |
Details[4] | |
Surface gravity (log g) | 4.69±0.2 cgs |
Temperature | 4920±100 K |
Metallicity [Fe/H] | 0.11±0.1 dex |
Rotation | 10.52 d[5] |
Age | 0.212±0.031[6] Gyr |
Other designations | |
Kepler-411: Gaia EDR3 2132768956905956352 | |
Kepler-411B: Gaia EDR3 2132768956904826624 | |
Database references | |
SIMBAD | data |
Kepler-411 is a binary star system. Its primary star Kepler-411 is a K-type main-sequence star, orbited by the red dwarf star Kepler-411B on a wide orbit, discovered in 2012.[3]
The primary star's surface temperature is 4920±100 K. Kepler-411 is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of 0.11±0.1,[4] but is much younger at an age of 212±31 million years.[6]
Kepler-411 exhibits significant starspot activity, with starspots covering 1.7+0.3
−0.2% of the stellar surface.[7] Darker starspots are concentrated around the equator of the star. Kepler-411 exhibits differential rotation, but with smaller amount of differential shear compared to the Sun.[5]
Planetary system[]
In 2013, one planet, named , was discovered,[8] followed by planet in 2016, and planet in 2018. Three planets were discovered by the transit method, while was discovered in 2019[9] by the transit-timing variation and radial velocity method.[6]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
[10] | 0.08055±0.00818 MJ | 0.0375±0.0008 | 3.005156±0.000002 | 0.146+0.004 −0.005 |
87.4±0.1° | 0.214±0.005 RJ |
[11] | 0.08306±0.01856 MJ | 0.0739±0.001 | 7.834436247±0.000001137[12] | 0.108+0.003 −0.004 |
88.61±0.04° | 0.394±0.006 RJ |
[13] | 0.04782±0.01605 MJ | 0.279±0.004 | 58.02023116±0.00004203[12] | 0.128±0.003 | 89.43±0.02° | 0.296±0.009 RJ |
[14] | 0.03398±0.00346 MJ | 0.186±0.003 | 31.509728±0.000085 | 0.016+0.002 −0.001 |
88.04±0.02° | — |
References[]
- ^ a b c d "Kepler-411". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-22.
- ^ a b c d Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. Gaia EDR3 record for this source at VizieR.
- ^ a b Ziegler, Carl; Law, Nicholas M.; Baranec, Christoph; Riddle, Reed; Duev, Dmitry A.; Howard, Ward; Jensen-Clem, Rebecca; Kulkarni, S. R.; Morton, Tim; Salama, Maïssa (2017), "Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems", The Astronomical Journal, 155 (4): 161, arXiv:1712.04454, doi:10.3847/1538-3881/aab042, S2CID 119088873
- ^ a b Furlan, E.; Ciardi, D. R.; Cochran, W. D.; Everett, M. E.; Latham, D. W.; Marcy, G. W.; Buchhave, L. A.; Endl, M.; Isaacson, H.; Petigura, E. A.; Gautier, T. N.; Huber, D.; Bieryla, A.; Borucki, W. J.; Brugamyer, E.; Caldwell, C.; Cochran, A.; Howard, A. W.; Howell, S. B.; Johnson, M. C.; MacQueen, P. J.; Quinn, S. N.; Robertson, P.; Mathur, S.; Batalha, N. M. (2018), "The Kepler Follow-Up Observation Program. II. Stellar Parameters from Medium- and High-Resolution Spectroscopy", The Astrophysical Journal, 861 (2): 149, arXiv:1805.12089, Bibcode:2018ApJ...861..149F, doi:10.3847/1538-4357/aaca34, S2CID 119243987
- ^ a b Araújo, Alexandre; Valio, Adriana (2021), "Kepler-411 differential rotation from three transiting planets", The Astrophysical Journal, 907 (1): L5, arXiv:2101.07692, Bibcode:2021ApJ...907L...5A, doi:10.3847/2041-8213/abd3a7, S2CID 231639459
- ^ a b c Lillo-Box, J.; Lopez, T. A.; Santerne, A.; Nielsen, L. D.; Barros, S. C. C.; Deleuil, M.; Acuña, L.; Mousis, O.; Sousa, S. G.; Adibekyan, V.; Armstrong, D. J.; Barrado, D.; Bayliss, D.; Brown, D. J. A.; Demangeon, O. D. S.; Dumusque, X.; Figueira, P.; Hojjatpanah, S.; Osborn, H. P.; Santos, N. C.; Udry, S. (2020), "Masses for the seven planets in K2-32 and K2-233. Four diverse planets in resonant chain and the first young rocky worlds", Astronomy & Astrophysics, A48: 640, arXiv:2006.01102, Bibcode:2020A&A...640A..48L, doi:10.1051/0004-6361/202037896, S2CID 219176756
- ^ Morris, Brett M. (2020), "A relationship between stellar age and spot coverage", The Astrophysical Journal, 893 (1): 67, arXiv:2002.09135, Bibcode:2020ApJ...893...67M, doi:10.3847/1538-4357/ab79a0, S2CID 211252547
- ^ Wang, Ji; Xie, Ji-Wei; Barclay, Thomas; Fischer, Debra A. (2013), "Influence of Stellar Multiplicity On Planet Formation. I. Evidence of Suppressed Planet Formation Due to Stellar Companions Within 20 AU and Validation of Four Planets From the Kepler Multiple Planet Candidates", The Astrophysical Journal, 783: 4, arXiv:1309.7097, doi:10.1088/0004-637X/783/1/4, S2CID 119214390
- ^ Sun, L.; Ioannidis, P.; Gu, S.; Schmitt, J. H. M. M.; Wang, X.; Kouwenhoven, M. B. N. (2019), "Kepler-411: a four-planet system with an active host star", Astronomy & Astrophysics, 624: A15, arXiv:1902.09719, Bibcode:2019A&A...624A..15S, doi:10.1051/0004-6361/201834275, S2CID 102481339
- ^ Kepler-411b on exoplanet.eu
- ^ Kepler-411c on exoplanet.eu
- ^ a b Battley, Matthew P; et al. (10 March 2021). "Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data". Monthly Notices of the Royal Astronomical Society. 503 (3): 4092–4104. arXiv:2103.03259. Bibcode:2021MNRAS.503.4092B. doi:10.1093/mnras/stab701.
- ^ Kepler-411d on exoplanet.eu
- ^ Kepler-411e on exoplanet.eu
Coordinates: 19h 10m 25.3471s, +49° 31′ 23.7119″
- Cygnus (constellation)
- Planetary transit variables
- K-type main-sequence stars
- Planetary systems with four confirmed planets
- 2MASS objects
- Kepler objects of interest
- Binary stars