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K2-58

K2-58 (also designated as EPIC 206026904) is G-type main-sequence star in the constellation of Aquarius, approximately 596 light-years from Solar System. The star is metal-rich, having 155% of Solar abundance of elements heavier than helium.[3] The star is located in the region allowing to see Venus transiting the Sun for hypothetical observer located in K2-58 system.[5]

K2-58
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 22h 15m 17.2364s[1]
Declination −14° 02′ 59.3151″[1]
Apparent magnitude (V) 12.13
Characteristics
Evolutionary stage Main sequence
Spectral type K2
Astrometry
Radial velocity (Rv)6.5±0.8 km/s
Proper motion (μ) RA: 4.67±0.02 mas/yr[2]
Dec.: -11.11±0.02 mas/yr[2]
Parallax (π)5.4932 ± 0.0194 mas[2]
Distance594 ± 2 ly
(182.0 ± 0.6 pc)
Details[3]
Mass0.858+0.022
−0.027
[4] M
Radius0.803+0.034
−0.020
[4] R
Surface gravity (log g)4.5 cgs
Temperature5038 K
Metallicity [Fe/H]0.25 dex
Rotational velocity (v sin i)2.2±0.5 km/s
Other designations
EPIC 206026904, 2MASS J22151722-1402593, Gaia DR2 2599975224481836672
Database references
SIMBADdata

Planetary system edit

The planetary system has three confirmed exoplanets (named as K2-58 b, K2-58 c, K2-58 d),[6][7][8] discovered in 2016.[9]

The K2-58 planetary system[9][4]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
K2-58c 0.0350 2.53726 86.1+2.8
−7.3
°
1.62 R🜨
K2-58b 0.0692 7.05254 88.9+0.8
−1.6
°
2.68 R🜨
K2-58d 0.1517 22.8827 89.43+0.41
−0.81
°
1.71 R🜨

References edit

  1. ^ a b "K2-58". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ a b 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. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  3. ^ a b Brewer, John M.; Fischer, Debra A. (2018), "Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest", The Astrophysical Journal Supplement Series, 237 (2): 38, arXiv:1804.00673, Bibcode:2018ApJS..237...38B, doi:10.3847/1538-4365/aad501, S2CID 119431797
  4. ^ a b c Mayo, Andrew W.; Vanderburg, Andrew; Latham, David W.; Bieryla, Allyson; Morton, Timothy D.; Buchhave, Lars A.; Dressing, Courtney D.; Beichman, Charles; Berlind, Perry; Calkins, Michael L.; Ciardi, David R.; Crossfield, Ian J. M.; Esquerdo, Gilbert A.; Everett, Mark E.; Gonzales, Erica J.; Hirsch, Lea A.; Horch, Elliott P.; Howard, Andrew W.; Howell, Steve B.; Livingston, John; Patel, Rahul; Petigura, Erik A.; Schlieder, Joshua E.; Scott, Nicholas J.; Schumer, Clea F.; Sinukoff, Evan; Teske, Johanna; Winters, Jennifer G. (2018), "275 Candidates and 149 Validated Planets Orbiting Bright Stars inK2 Campaigns 0–10", The Astronomical Journal, 155 (3): 136, arXiv:1802.05277, Bibcode:2018AJ....155..136M, doi:10.3847/1538-3881/aaadff, S2CID 85524387
  5. ^ Kruse, Ethan; Agol, Eric; Luger, Rodrigo; Foreman-Mackey, Daniel (2019), "Detection of Hundreds of New Planet Candidates and Eclipsing Binaries in K2 Campaigns 0–8", The Astrophysical Journal Supplement Series, 244 (1): 11, arXiv:1907.10806, Bibcode:2019ApJS..244...11K, doi:10.3847/1538-4365/ab346b, S2CID 198901606
  6. ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2019-07-16.
  7. ^ "EPIC 206026904". www.cfa.harvard.edu. Retrieved 2019-07-16.
  8. ^ "Open Exoplanet Catalogue - K2-58 b". www.openexoplanetcatalogue.com. Retrieved 2019-07-16.
  9. ^ a b Crossfield, Ian J. M.; et al. (2021), "197 CANDIDATES AND 104 VALIDATED PLANETS IN K2 's FIRST FIVE FIELDS", The Astrophysical Journal Supplement Series, 226: 7, arXiv:1607.05263, doi:10.3847/0067-0049/226/1/7, S2CID 56125109

also, designated, epic, 206026904, type, main, sequence, star, constellation, aquarius, approximately, light, years, from, solar, system, star, metal, rich, having, solar, abundance, elements, heavier, than, helium, star, located, region, allowing, venus, tran. K2 58 also designated as EPIC 206026904 is G type main sequence star in the constellation of Aquarius approximately 596 light years from Solar System The star is metal rich having 155 of Solar abundance of elements heavier than helium 3 The star is located in the region allowing to see Venus transiting the Sun for hypothetical observer located in K2 58 system 5 K2 58 Observation dataEpoch J2000 Equinox J2000Constellation AquariusRight ascension 22h 15m 17 2364s 1 Declination 14 02 59 3151 1 Apparent magnitude V 12 13CharacteristicsEvolutionary stage Main sequenceSpectral type K2AstrometryRadial velocity Rv 6 5 0 8 km sProper motion m RA 4 67 0 02 mas yr 2 Dec 11 11 0 02 mas yr 2 Parallax p 5 4932 0 0194 mas 2 Distance594 2 ly 182 0 0 6 pc Details 3 Mass0 858 0 022 0 027 4 M Radius0 803 0 034 0 020 4 R Surface gravity log g 4 5 cgsTemperature5038 KMetallicity Fe H 0 25 dexRotational velocity v sin i 2 2 0 5 km sOther designationsEPIC 206026904 2MASS J22151722 1402593 Gaia DR2 2599975224481836672Database referencesSIMBADdataPlanetary system editThe planetary system has three confirmed exoplanets named as K2 58 b K2 58 c K2 58 d 6 7 8 discovered in 2016 9 The K2 58 planetary system 9 4 Companion in order from star Mass Semimajor axis AU Orbital period days Eccentricity Inclination RadiusK2 58c 0 0350 2 53726 86 1 2 8 7 3 1 62 R K2 58b 0 0692 7 05254 88 9 0 8 1 6 2 68 R K2 58d 0 1517 22 8827 89 43 0 41 0 81 1 71 R References edit a b K2 58 SIMBAD Centre de donnees astronomiques de Strasbourg a b Brown A G A et al Gaia collaboration 2021 Gaia Early Data Release 3 Summary of the contents and survey properties Astronomy amp Astrophysics 649 A1 arXiv 2012 01533 Bibcode 2021A amp A 649A 1G doi 10 1051 0004 6361 202039657 S2CID 227254300 Erratum doi 10 1051 0004 6361 202039657e Gaia EDR3 record for this source at VizieR a b Brewer John M Fischer Debra A 2018 Spectral Properties of Cool Stars Extended Abundance Analysis of Kepler Objects of Interest The Astrophysical Journal Supplement Series 237 2 38 arXiv 1804 00673 Bibcode 2018ApJS 237 38B doi 10 3847 1538 4365 aad501 S2CID 119431797 a b c Mayo Andrew W Vanderburg Andrew Latham David W Bieryla Allyson Morton Timothy D Buchhave Lars A Dressing Courtney D Beichman Charles Berlind Perry Calkins Michael L Ciardi David R Crossfield Ian J M Esquerdo Gilbert A Everett Mark E Gonzales Erica J Hirsch Lea A Horch Elliott P Howard Andrew W Howell Steve B Livingston John Patel Rahul Petigura Erik A Schlieder Joshua E Scott Nicholas J Schumer Clea F Sinukoff Evan Teske Johanna Winters Jennifer G 2018 275 Candidates and 149 Validated Planets Orbiting Bright Stars inK2 Campaigns 0 10 The Astronomical Journal 155 3 136 arXiv 1802 05277 Bibcode 2018AJ 155 136M doi 10 3847 1538 3881 aaadff S2CID 85524387 Kruse Ethan Agol Eric Luger Rodrigo Foreman Mackey Daniel 2019 Detection of Hundreds of New Planet Candidates and Eclipsing Binaries in K2 Campaigns 0 8 The Astrophysical Journal Supplement Series 244 1 11 arXiv 1907 10806 Bibcode 2019ApJS 244 11K doi 10 3847 1538 4365 ab346b S2CID 198901606 Exoplanet catalog Exoplanet Exploration Planets Beyond our Solar System Retrieved 2019 07 16 EPIC 206026904 www cfa harvard edu Retrieved 2019 07 16 Open Exoplanet Catalogue K2 58 b www openexoplanetcatalogue com Retrieved 2019 07 16 a b Crossfield Ian J M et al 2021 197 CANDIDATES AND 104 VALIDATED PLANETS IN K2 s FIRST FIVE FIELDS The Astrophysical Journal Supplement Series 226 7 arXiv 1607 05263 doi 10 3847 0067 0049 226 1 7 S2CID 56125109 Retrieved from https en wikipedia org w index php title K2 58 amp oldid 1187564043, wikipedia, wiki, book, books, library,

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