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Kepler-84

Kepler-84 is a Sun-like star 4,700 light-years from the Sun. It is a G-type star. The stellar radius measurement has a large uncertainty of 48% as in 2017, complicating the modelling of the star.[5] The Kepler-84 star has two suspected stellar companions. Four red dwarfs are few arcseconds away and at least one is probably gravitationally bound to Kepler-84.[6] Another (which is a background star with a probability 0.5%) is a yellow star of mass 0.855M on projected separations of 0.18±0.05″ or 0.26″ (213.6 AU).[7]

Kepler-84
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 01h 37m 40.87964s[1]
Declination +12° 04′ 42.1742″[1]
Characteristics
Spectral type G3[2]
Astrometry
Proper motion (μ) RA: −0.150 mas/yr
Dec.: −2.872 mas/yr
Parallax (π)0.6929 ± 0.7043 mas
Details
Mass1[2] M
Radius1.2 R
Temperature5,755[3] K
Metallicity [Fe/H]+0.09 ± 0.04[2] dex
Age4.9[4] Gyr
Other designations
Kepler-84, KOI-1589, Gaia DR2 2073776859551124992, KIC 5301750, 2MASS J19530049+4029458[1]
Database references
SIMBADdata
ARICNSdata

Planetary system edit

Kepler-84 is orbited by five known planets, four small gas giants and a Super-Earth. Planets Kepler-84b and Kepler-84c were confirmed in 2012[8] while the rest was confirmed in 2014.[9] To keep the known planetary system stable, no additional giant planets can be located within 7.4 AU from the parent stars.[10]

The Kepler-84 planetary system[11][12][13][14]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.126±0.038 MJ 0.083 8.725854±0.00006 0 88.24° 0.174±0.045 RJ
c 0.064±0.037 MJ 0.108 12.882525±0.000093 0 88.24° 0.184±0.047 RJ
d 0.052 4.224537±0.000042 0.123±0.024 RJ
e 0.181 27.434389±0.000224 0.232±0.044 RJ
f 0.25 44.552169±0.000812 0.196±0.038 RJ

References edit

  1. ^ a b c "Kepler-84". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved July 13, 2016.
  2. ^ a b c Vidotto, A. A; Gregory, S. G; Jardine, M; Donati, J. F; Petit, P; Morin, J; Folsom, C. P; Bouvier, J; Cameron, A. C; Hussain, G; Marsden, S; Waite, I. A; Fares, R; Jeffers, S; Do Nascimento, J. D (2014). "Stellar magnetism: Empirical trends with age and rotation" (PDF). Monthly Notices of the Royal Astronomical Society. 441 (3): 2361. arXiv:1404.2733. Bibcode:2014MNRAS.441.2361V. doi:10.1093/mnras/stu728. S2CID 43200119.
  3. ^ Gray, R. O; Corbally, C. J; Garrison, R. F; McFadden, M. T; Robinson, P. E (2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Northern Sample I". The Astronomical Journal. 126 (4): 2048. arXiv:astro-ph/0308182. Bibcode:2003AJ....126.2048G. doi:10.1086/378365. S2CID 119417105.
  4. ^ Melendez, Jorge; Dodds-Eden, Katie; Robles, Jose A (2006). "HD 98618: A Star Closely Resembling our Sun". The Astrophysical Journal. 641 (2): L133–L136. arXiv:astro-ph/0603219. Bibcode:2006ApJ...641L.133M. doi:10.1086/503898. S2CID 17479387.
  5. ^ Ramos, X. S.; Charalambous, C.; Benítez-Llambay, P.; Beaugé, C. (2017), "Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets", Astronomy & Astrophysics, 602: A101, arXiv:1704.06459, Bibcode:2017A&A...602A.101R, doi:10.1051/0004-6361/201629642, S2CID 119369796
  6. ^ Hirsch, Lea A.; Ciardi, David R.; Howard, Andrew W.; Everett, Mark E.; Furlan, Elise; Saylors, Mindy; Horch, Elliott P.; Howell, Steve B.; Teske, Johanna; Marcy, Geoffrey W. (2017), "ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST", The Astronomical Journal, 153 (3): 117, arXiv:1701.06577, Bibcode:2017AJ....153..117H, doi:10.3847/1538-3881/153/3/117, S2CID 39321033
  7. ^ Kraus, Adam L.; Ireland, Michael J.; Huber, Daniel; Mann, Andrew W.; Dupuy, Trent J. (2016), "The Impact of Stellar Multiplicity on Planetary Systems. I. The Ruinous Influence of Close Binary Companions", The Astronomical Journal, 152 (1): 8, arXiv:1604.05744, Bibcode:2016AJ....152....8K, doi:10.3847/0004-6256/152/1/8, S2CID 119110229
  8. ^ Xie, Ji-Wei (2012), "Transit Timing Variation of Near-Resonance Planetary Pairs: Confirmation of 12 Multiple-Planet Systems", The Astrophysical Journal Supplement Series, 208 (2): 22, arXiv:1208.3312, Bibcode:2013ApJS..208...22X, doi:10.1088/0067-0049/208/2/22, S2CID 17160267
  9. ^ openexoplanetcatalogue.com Kepler-84
  10. ^ 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
  11. ^ 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
  12. ^ Planet Kepler-84 d at exoplanets.eu
  13. ^ Planet Kepler-84 e at exoplanets.eu
  14. ^ Planet Kepler-84 f at exoplanets.eu

kepler, like, star, light, years, from, type, star, stellar, radius, measurement, large, uncertainty, 2017, complicating, modelling, star, star, suspected, stellar, companions, four, dwarfs, arcseconds, away, least, probably, gravitationally, bound, another, w. Kepler 84 is a Sun like star 4 700 light years from the Sun It is a G type star The stellar radius measurement has a large uncertainty of 48 as in 2017 complicating the modelling of the star 5 The Kepler 84 star has two suspected stellar companions Four red dwarfs are few arcseconds away and at least one is probably gravitationally bound to Kepler 84 6 Another which is a background star with a probability 0 5 is a yellow star of mass 0 855M on projected separations of 0 18 0 05 or 0 26 213 6 AU 7 Kepler 84 Observation dataEpoch J2000 Equinox J2000Constellation CygnusRight ascension 01h 37m 40 87964s 1 Declination 12 04 42 1742 1 CharacteristicsSpectral type G3 2 AstrometryProper motion m RA 0 150 mas yr Dec 2 872 mas yrParallax p 0 6929 0 7043 masDetailsMass1 2 M Radius1 2 R Temperature5 755 3 KMetallicity Fe H 0 09 0 04 2 dexAge4 9 4 GyrOther designationsKepler 84 KOI 1589 Gaia DR2 2073776859551124992 KIC 5301750 2MASS J19530049 4029458 1 Database referencesSIMBADdataARICNSdataPlanetary system editKepler 84 is orbited by five known planets four small gas giants and a Super Earth Planets Kepler 84b and Kepler 84c were confirmed in 2012 8 while the rest was confirmed in 2014 9 To keep the known planetary system stable no additional giant planets can be located within 7 4 AU from the parent stars 10 The Kepler 84 planetary system 11 12 13 14 Companion in order from star Mass Semimajor axis AU Orbital period days Eccentricity Inclination Radiusb 0 126 0 038 M J 0 083 8 725854 0 00006 0 88 24 0 174 0 045 R Jc 0 064 0 037 M J 0 108 12 882525 0 000093 0 88 24 0 184 0 047 R Jd 0 052 4 224537 0 000042 0 123 0 024 R Je 0 181 27 434389 0 000224 0 232 0 044 R Jf 0 25 44 552169 0 000812 0 196 0 038 R JReferences edit a b c Kepler 84 SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved July 13 2016 a b c Vidotto A A Gregory S G Jardine M Donati J F Petit P Morin J Folsom C P Bouvier J Cameron A C Hussain G Marsden S Waite I A Fares R Jeffers S Do Nascimento J D 2014 Stellar magnetism Empirical trends with age and rotation PDF Monthly Notices of the Royal Astronomical Society 441 3 2361 arXiv 1404 2733 Bibcode 2014MNRAS 441 2361V doi 10 1093 mnras stu728 S2CID 43200119 Gray R O Corbally C J Garrison R F McFadden M T Robinson P E 2003 Contributions to the Nearby Stars NStars Project Spectroscopy of Stars Earlier than M0 within 40 parsecs The Northern Sample I The Astronomical Journal 126 4 2048 arXiv astro ph 0308182 Bibcode 2003AJ 126 2048G doi 10 1086 378365 S2CID 119417105 Melendez Jorge Dodds Eden Katie Robles Jose A 2006 HD 98618 A Star Closely Resembling our Sun The Astrophysical Journal 641 2 L133 L136 arXiv astro ph 0603219 Bibcode 2006ApJ 641L 133M doi 10 1086 503898 S2CID 17479387 Ramos X S Charalambous C Benitez Llambay P Beauge C 2017 Planetary migration and the origin of the 2 1 and 3 2 near resonant population of close in exoplanets Astronomy amp Astrophysics 602 A101 arXiv 1704 06459 Bibcode 2017A amp A 602A 101R doi 10 1051 0004 6361 201629642 S2CID 119369796 Hirsch Lea A Ciardi David R Howard Andrew W Everett Mark E Furlan Elise Saylors Mindy Horch Elliott P Howell Steve B Teske Johanna Marcy Geoffrey W 2017 ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST The Astronomical Journal 153 3 117 arXiv 1701 06577 Bibcode 2017AJ 153 117H doi 10 3847 1538 3881 153 3 117 S2CID 39321033 Kraus Adam L Ireland Michael J Huber Daniel Mann Andrew W Dupuy Trent J 2016 The Impact of Stellar Multiplicity on Planetary Systems I The Ruinous Influence of Close Binary Companions The Astronomical Journal 152 1 8 arXiv 1604 05744 Bibcode 2016AJ 152 8K doi 10 3847 0004 6256 152 1 8 S2CID 119110229 Xie Ji Wei 2012 Transit Timing Variation of Near Resonance Planetary Pairs Confirmation of 12 Multiple Planet Systems The Astrophysical Journal Supplement Series 208 2 22 arXiv 1208 3312 Bibcode 2013ApJS 208 22X doi 10 1088 0067 0049 208 2 22 S2CID 17160267 openexoplanetcatalogue com Kepler 84 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 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 Planet Kepler 84 d at exoplanets eu Planet Kepler 84 e at exoplanets eu Planet Kepler 84 f at exoplanets eu nbsp This main sequence star related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title Kepler 84 amp oldid 1191214292, wikipedia, wiki, book, books, library,

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