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{{short description|G-type star in the constellation Cygnus}} |
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{{Starbox begin |
{{Starbox begin |
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| name = Kepler- |
| name = Kepler-27 |
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}} |
}} |
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<!-- {{Starbox image | |
<!-- {{Starbox image | |
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| image = |
| image = |
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| caption = A diagram of the Kepler- |
| caption = A diagram of the Kepler-27 System, compared to our Inner Solar System. |
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}} --> |
}} --> |
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{{Starbox observe |
{{Starbox observe |
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| title=The Constellations | publisher=[[International Astronomical Union]] |
| title=The Constellations | publisher=[[International Astronomical Union]] |
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| url=http://www.iau.org/public/constellations/#cyg |
| url=http://www.iau.org/public/constellations/#cyg |
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| |
| access-date=2011-12-15 }}</ref> |
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| ra = {{RA|19|28|56. |
| ra = {{RA|19|28|56.81962}}<ref name="Gaia DR3"/> |
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| dec = {{DEC|+41|05|09. |
| dec = {{DEC|+41|05|09.1405}}<ref name="Gaia DR3"/> |
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| appmag_v = 15.855<ref name=nasa_ames>{{citation |
| appmag_v = 15.855<ref name=nasa_ames>{{citation |
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| title=Kepler- |
| title=Kepler-27b |
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| publisher=[[NASA Ames Research Center]] |
| publisher=[[NASA Ames Research Center]] |
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| url=http://kepler.nasa.gov/Mission/discoveries/kepler30b/ |
| url=http://kepler.nasa.gov/Mission/discoveries/kepler30b/ |
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| archive-url=https://web.archive.org/web/20120503111252/http://kepler.nasa.gov/Mission/discoveries/kepler30b/ |
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| url-status=dead |
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| archive-date=2012-05-03 |
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}} |
}} |
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{{Starbox character |
{{Starbox character |
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|first1=Jean |
|first1=Jean |
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|last1=Schneider |
|last1=Schneider |
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|title=Star: Kepler- |
|title=Star: Kepler-27 |
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|publisher=Paris Observatory |
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|url-status=dead |
|url-status=dead |
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|archive-url=https://web.archive.org/web/20120426071816/http://exoplanet.eu/star.php?st=Kepler-27 |
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|archive-date=2012-04-26 |
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}}</ref><!-- NOTE: Please don't add a 'V' here until it is established as such by a reliable source. --> |
}}</ref><!-- NOTE: Please don't add a 'V' here until it is established as such by a reliable source. --> |
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| appmag_1_passband = <!-- Passband for first apparent magnitude (e.g., H, J, K, etc.) --> |
| appmag_1_passband = <!-- Passband for first apparent magnitude (e.g., H, J, K, etc.) --> |
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{{Starbox astrometry |
{{Starbox astrometry |
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| radial_v = |
| radial_v = |
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| prop_mo_ra = {{val|2. |
| prop_mo_ra = {{val|2.171|0.033}} |
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| prop_mo_dec = {{val| |
| prop_mo_dec = {{val|-0.324|0.031}} |
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| pm_footnote = <ref name="Gaia DR3"/> |
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| parallax = 0. |
| parallax = 0.9298 |
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| p_error = 0. |
| p_error = 0.0281 |
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| parallax_footnote = <ref name="Gaia |
| parallax_footnote = <ref name="Gaia DR3"/> |
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| absmag_v = |
| absmag_v = |
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}} |
}} |
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{{Starbox detail |
{{Starbox detail |
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| mass = {{ |
| mass = 0.9{{±|0.03|0.10}}<ref name=Hadden2016/> |
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| luminosity = {{nowrap|0.59}}<ref name=nasa_ames/> |
| luminosity = {{nowrap|0.59}}<ref name=nasa_ames/> |
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| temperature = {{nowrap|5400}}<ref name=nasa_ames/> |
| temperature = {{nowrap|5400}}<ref name=nasa_ames/> |
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| metal_fe = {{nowrap|0.41}}<ref name=nasa_ames/> |
| metal_fe = {{nowrap|0.41}}<ref name=nasa_ames/> |
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| radius = |
| radius = |
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| rotational_velocity = {{nowrap|0.6}}<ref name=nasa_ames/> |
| rotational_velocity = {{nowrap|0.6}}<ref name=nasa_ames/> |
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| age = |
| age = |
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}} |
}} |
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{{Starbox catalog |
{{Starbox catalog |
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| names = [[Kepler Object of Interest|KOI]]- |
| names = [[Kepler Object of Interest|KOI]]-841, [[Kepler Input Catalog|KIC]] 5792202, [[2MASS]] J19285682+4105091, Gaia DR2 2053586321364864640 |
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}} |
}} |
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{{Starbox reference |
{{Starbox reference |
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| Simbad = Kepler-27 |
| Simbad = Kepler-27 |
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| KIC = |
| KIC = 5792202 |
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}} |
}} |
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{{Starbox end}} |
{{Starbox end}} |
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'''Kepler-27''' is a [[star]] in the northern [[constellation]] of [[Cygnus (constellation)|Cygnus]], the swan |
'''Kepler-27''' is a [[star]] in the northern [[constellation]] of [[Cygnus (constellation)|Cygnus]], the swan. It is located at the [[celestial coordinates]]: Right Ascension {{RA|19|28|56.81962}}, Declination {{DEC|+41|05|09.1405}}.<ref name="Gaia DR3"/> With an [[apparent visual magnitude]] of 15.855,<ref name=nasa_ames/> this star is too faint to be seen with the naked eye. |
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==Planetary system== |
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The planetary system of Kepler-27 comprising two small gas giants on eccentric orbits<ref name=Hadden2016/> was discovered in late 2011.<ref name=Steffen2012/> The planets [[Kepler-27b]] and [[Kepler-27c]] have [[equilibrium temperature]]s of 610 [[Kelvin|K]] and 481 [[Kelvin|K]], respectively.<ref name=Furlan2017/> In 2021, a third, sub-Neptune-sized planet was confirmed, orbiting closer in than the other two planets.<ref name="Valizadegan2022"/><ref name="NASAExoplanetArchive"/> |
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{{OrbitboxPlanet begin |
{{OrbitboxPlanet begin |
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| table_ref = <ref name= |
| table_ref = <ref name=Furlan2017/><ref name="NASAExoplanetArchive"/> |
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}} |
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{{OrbitboxPlanet |
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| exoplanet = d |
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| mass = |
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| semimajor = |
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| period = 6.54629 |
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| radius = 0.2414 |
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}} |
}} |
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{{OrbitboxPlanet |
{{OrbitboxPlanet |
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| exoplanet = b |
| exoplanet = b |
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| mass = |
| mass = 0.1320{{±|0.018}} |
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| semimajor = 0.118 |
| semimajor = 0.118 |
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| period = 15.3348 |
| period = 15.3348 |
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| radius = 0.522{{±|0.024}} |
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| radius_earth = |
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}} |
}} |
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{{OrbitboxPlanet |
{{OrbitboxPlanet |
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| exoplanet = c |
| exoplanet = c |
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| mass = |
| mass = 0.0670{{±|0.011}} |
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| semimajor = 0.191 |
| semimajor = 0.191 |
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| period = 31.3309 |
| period = 31.3309 |
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| radius = 0.640{{±|0.029}} |
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| radius_earth = 4.1 |
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}} |
}} |
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{{Orbitbox end}} |
{{Orbitbox end}} |
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{{reflist|refs= |
{{reflist|refs= |
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<ref name="Gaia |
<ref name="Gaia DR3">{{Cite Gaia DR3|2053586321364864640}}</ref> |
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<ref name="NASAExoplanetArchive">{{cite web |title=Kepler-27 |url=https://exoplanetarchive.ipac.caltech.edu/overview/Kepler-27 |website=[[NASA Exoplanet Archive]] |accessdate=7 November 2022}}</ref> |
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<ref name=Steffen2012>{{citation|arxiv=1201.5412|title=Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations|year=2012|doi=10.1111/j.1365-2966.2012.20467.x|last1=Steffen|first1=Jason H.|last2=Fabrycky|first2=Daniel C.|last3=Ford|first3=Eric B.|last4=Carter|first4=Joshua A.|last5=Desert|first5=Jean-Michel|last6=Fressin|first6=Francois|last7=Holman|first7=Matthew J.|last8=Lissauer|first8=Jack J.|last9=Moorhead|first9=Althea V.|last10=Rowe|first10=Jason F.|last11=Ragozzine|first11=Darin|last12=Welsh|first12=William F.|last13=Batalha|first13=Natalie M.|last14=Borucki|first14=William J.|last15=Buchhave|first15=Lars A.|last16=Bryson|first16=Steve|last17=Caldwell|first17=Douglas A.|last18=Charbonneau|first18=David|last19=Ciardi|first19=David R.|last20=Cochran|first20=William D.|last21=Endl|first21=Michael|last22=Everett|first22=Mark E.|last23=Gautier III|first23=Thomas N.|last24=Gilliland|first24=Ron L.|last25=Girouard|first25=Forrest R.|last26=Jenkins|first26=Jon M.|last27=Horch|first27=Elliott|last28=Howell|first28=Steve B.|last29=Isaacson|first29=Howard|last30=Klaus|first30=Todd C.|doi-access=free |bibcode=2012MNRAS.421.2342S |s2cid=11898578|display-authors=29}}</ref> |
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<ref name=Hadden2016>{{citation|arxiv=1611.03516|doi=10.3847/1538-3881/aa71ef|last1=Hadden|first1=Sam|last2=Lithwick|first2=Yoram|title=Kepler Planet Masses and Eccentricities from TTV Analysis |journal=The Astronomical Journal|year=2017 |volume=154|issue=1 |page=5|bibcode=2017AJ....154....5H |s2cid=118936786 |doi-access=free }}</ref> |
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<ref name=Furlan2017>{{citation|arxiv=1707.01942|year=2017|doi=10.3847/1538-3881/aa7b70|last1=Furlan|first1=E.|last2=Howell|first2=S. B.|title=The Densities of Planets in Multiple Stellar Systems|journal=The Astronomical Journal|volume=154|issue=2|page=66|bibcode=2017AJ....154...66F |s2cid=28833730 |doi-access=free }}</ref> |
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<ref name="Valizadegan2022">{{cite journal |last1=Valizadegan |first1=Hamed |last2=Martinho |first2=Miguel J. S. |date=February 2022 |title=ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier That Validates 301 New Exoplanets |journal=[[The Astrophysical Journal]] |volume=926 |issue=2 |pages=120 |doi=10.3847/1538-4357/ac4399 |arxiv=2111.10009 |bibcode=2022ApJ...926..120V|s2cid=244954905 |doi-access=free }}</ref> |
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}} |
}} |
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{{Stars of Cygnus}} |
{{Stars of Cygnus}} |
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[[Category:Cygnus (constellation)]] |
[[Category:Cygnus (constellation)]] |
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[[Category:G-type main-sequence stars]] |
[[Category:G-type main-sequence stars]] |
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[[Category:Kepler objects of interest| |
[[Category:Kepler objects of interest|841]] |
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[[Category:Planetary transit variables]] |
[[Category:Planetary transit variables]] |
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[[Category:Planetary systems with three confirmed planets]] |
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[[Category:2MASS objects|J19285682+4105091]] |
Latest revision as of 05:24, 23 August 2024
Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Cygnus[1] |
Right ascension | 19h 28m 56.81962s[2] |
Declination | +41° 05′ 09.1405″[2] |
Apparent magnitude (V) | 15.855[3] |
Characteristics | |
Spectral type | G5[4] |
Astrometry | |
Proper motion (μ) | RA: 2.171±0.033 mas/yr[2] Dec.: −0.324±0.031 mas/yr[2] |
Parallax (π) | 0.9298 ± 0.0281 mas[2] |
Distance | 3,500 ± 100 ly (1,080 ± 30 pc) |
Details | |
Mass | 0.9+0.03 −0.10[5] M☉ |
Luminosity | 0.59[3] L☉ |
Temperature | 5400[3] K |
Metallicity [Fe/H] | 0.41[3] dex |
Rotational velocity (v sin i) | 0.6[3] km/s |
Other designations | |
Database references | |
SIMBAD | data |
KIC | data |
Kepler-27 is a star in the northern constellation of Cygnus, the swan. It is located at the celestial coordinates: Right Ascension 19h 28m 56.81962s, Declination +41° 05′ 09.1405″.[2] With an apparent visual magnitude of 15.855,[3] this star is too faint to be seen with the naked eye.
Planetary system
[edit]The planetary system of Kepler-27 comprising two small gas giants on eccentric orbits[5] was discovered in late 2011.[6] The planets Kepler-27b and Kepler-27c have equilibrium temperatures of 610 K and 481 K, respectively.[7] In 2021, a third, sub-Neptune-sized planet was confirmed, orbiting closer in than the other two planets.[8][9]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
d | — | — | 6.54629 | — | — | 0.2414 RJ |
b | 0.1320±0.018 MJ | 0.118 | 15.3348 | — | — | 0.522±0.024 RJ |
c | 0.0670±0.011 MJ | 0.191 | 31.3309 | — | — | 0.640±0.029 RJ |
References
[edit]- ^ "Cygnus – constellation boundary", The Constellations, International Astronomical Union, retrieved 2011-12-15
- ^ a b c d e 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.
- ^ a b c d e f Kepler-27b, NASA Ames Research Center, archived from the original on 2012-05-03, retrieved 2011-12-06
- ^ Schneider, Jean, "Star: Kepler-27", Extrasolar Planets Encyclopaedia, archived from the original on 2012-04-26, retrieved 2011-12-06
- ^ a b Hadden, Sam; Lithwick, Yoram (2017), "Kepler Planet Masses and Eccentricities from TTV Analysis", The Astronomical Journal, 154 (1): 5, arXiv:1611.03516, Bibcode:2017AJ....154....5H, doi:10.3847/1538-3881/aa71ef, S2CID 118936786
- ^ Steffen, Jason H.; Fabrycky, Daniel C.; Ford, Eric B.; Carter, Joshua A.; Desert, Jean-Michel; Fressin, Francois; Holman, Matthew J.; Lissauer, Jack J.; Moorhead, Althea V.; Rowe, Jason F.; Ragozzine, Darin; Welsh, William F.; Batalha, Natalie M.; Borucki, William J.; Buchhave, Lars A.; Bryson, Steve; Caldwell, Douglas A.; Charbonneau, David; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Gautier III, Thomas N.; Gilliland, Ron L.; Girouard, Forrest R.; Jenkins, Jon M.; Horch, Elliott; Howell, Steve B.; Isaacson, Howard; et al. (2012), Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations, arXiv:1201.5412, Bibcode:2012MNRAS.421.2342S, doi:10.1111/j.1365-2966.2012.20467.x, S2CID 11898578
- ^ a b Furlan, E.; Howell, S. B. (2017), "The Densities of Planets in Multiple Stellar Systems", The Astronomical Journal, 154 (2): 66, arXiv:1707.01942, Bibcode:2017AJ....154...66F, doi:10.3847/1538-3881/aa7b70, S2CID 28833730
- ^ Valizadegan, Hamed; Martinho, Miguel J. S. (February 2022). "ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier That Validates 301 New Exoplanets". The Astrophysical Journal. 926 (2): 120. arXiv:2111.10009. Bibcode:2022ApJ...926..120V. doi:10.3847/1538-4357/ac4399. S2CID 244954905.
- ^ a b "Kepler-27". NASA Exoplanet Archive. Retrieved 7 November 2022.