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Kepler-296

From Wikipedia, the free encyclopedia
Star in the constellation Draco
Kepler-296
Observation data
Epoch J2000      Equinox J2000
ConstellationDraco[1]
Right ascension19h 06m 09.60253s[2]
Declination+49° 26′ 14.3969″[2]
Characteristics
Spectral typeK7 V + M1 V[3]
Astrometry
Proper motion (μ)RA: 2.635mas/yr[2]
Dec.: −16.375mas/yr[2]
Parallax (π)4.5538±0.5562 mas[2]
Distanceapprox. 720 ly
(approx. 220 pc)
Details[4]
Kepler-296 A
Mass0.498+0.067
−0.087
 M
Radius0.480+0.066
−0.087
 R
Surface gravity (log g)4.774+0.091
−0.059
 cgs
Temperature3740±130 K
Metallicity[Fe/H]−0.08+0.28
−0.30
 dex
Kepler-296 B
Mass0.326+0.070
−0.079
 M
Radius0.322+0.060
−0.068
 R
Surface gravity (log g)4.993+0.087
−0.063
 cgs
Temperature3440±75 K
Metallicity[Fe/H]−0.08+0.28
−0.30
 dex
Other designations
Kepler-296,KOI-1422,KIC 11497958,2MASS J19060960+4926143[5]
Database references
SIMBADdata
Exoplanet Archivedata
KICdata

Kepler-296 is abinary star system[4] in the constellationDraco. The primary star appears to be a lateK-type main-sequence star, while the secondary is ared dwarf.[3]

Planetary system

[edit]
The following plot shows the approximate sizes of the planets in this system compared to planets in the Solar System.[6]

Fiveexoplanets have been detected around the system; all are believed to be orbiting the primary star rather than its dimmer companion.[4] Two planets in particular,Kepler-296e andKepler-296f, are likely located in thehabitable zone.[4] For the planetary system to remain stable, no additional giant planets can be located up to orbital radius 10.1AU.[7]

The Kepler-296 A planetary system[4]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
c0.0521+0.0088
−0.0086
5.8416366±0.000010<0.332.00+0.33
−0.32
 R🜨
b0.079±0.01310.864384+0.000051
−0.000046
<0.331.61+0.29
−0.27
 R🜨
d0.118±0.02019.850291+0.000061
−0.000057
<0.332.09+0.33
−0.32
 R🜨
e0.169+0.029
−0.028
34.14211±0.00025<0.331.53+0.27
−0.25
 R🜨
f0.255+0.043
−0.042
63.33627+0.00060
−0.00062
<0.331.80+0.31
−0.30
 R🜨

See also

[edit]

References

[edit]
  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 atVizieR.
  2. ^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.
  3. ^abLissauer, Jack J; Marcy, Geoffrey W; Bryson, Stephen T; Rowe, Jason F; Jontof-Hutter, Daniel; Agol, Eric; Borucki, William J; Carter, Joshua A; Ford, Eric B; Gilliland, Ronald L; Kolbl, Rea; Star, Kimberly M; Steffen, Jason H; Torres, Guillermo (2014). "Validation Ofkepler's Multiple Planet Candidates. Ii. Refined Statistical Framework and Descriptions of Systems of Special Interest".The Astrophysical Journal.784 (1): 44.arXiv:1402.6352.Bibcode:2014ApJ...784...44L.doi:10.1088/0004-637X/784/1/44.S2CID 119108651.
  4. ^abcdeBarclay, Thomas; Quintana, Elisa V; Adams, Fred C; Ciardi, David R; Huber, Daniel; Foreman-Mackey, Daniel; Montet, Benjamin T; Caldwell, Douglas (2015). "The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis".The Astrophysical Journal.809 (1): 7.arXiv:1505.01845.Bibcode:2015ApJ...809....7B.doi:10.1088/0004-637X/809/1/7.S2CID 37742564.
  5. ^"Kepler-296".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved26 November 2017.
  6. ^"Open Exoplanet Catalogue - Kepler-296 b".www.openexoplanetcatalogue.com. Retrieved2021-03-19.
  7. ^Becker, Juliette C.; Adams, Fred C. (2017), "Effects of Unseen Additional Planetary Perturbers on Compact Extrasolar Planetary Systems",Monthly Notices of the Royal Astronomical Society,468 (1):549–563,arXiv:1702.07714,Bibcode:2017MNRAS.468..549B,doi:10.1093/mnras/stx461,S2CID 119325005

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