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Chi Ceti

From Wikipedia, the free encyclopedia
Double star in the constellation Cetus
Chi Ceti
Location of χ Ceti (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCetus
HD 11171
Right ascension01h 49m 35.10277s[1]
Declination−10° 41′ 11.0719″[1]
Apparent magnitude (V)4.66[2]
HD 11131
Right ascension01h 49m 23.34886s[3]
Declination−10° 42′ 14.0839″[3]
Apparent magnitude (V)6.75[2]
Characteristics
HD 11171
Evolutionary stagemain sequence[4]
Spectral typeF3 III[5] or F0 V[6]
U−Bcolor index+0.04[2]
B−Vcolor index+0.33[2]
HD 11131
Evolutionary stagemain sequence[3]
Spectral typeG3 V[6]
U−Bcolor index+0.12[2]
B−Vcolor index+0.61[2]
Variable typeBY Dra[7]
Astrometry
HD 11171
Radial velocity (Rv)−1.8[5] km/s
Proper motion (μ)RA: −147.867[1]mas/yr
Dec.: −93.480[1]mas/yr
Parallax (π)42.5848±0.1249 mas[1]
Distance76.6 ± 0.2 ly
(23.48 ± 0.07 pc)
Absolute magnitude (MV)+2.83±0.01[8]
HD 11131
Radial velocity (Rv)−3.89±0.12[9] km/s
Proper motion (μ)RA: −159.846[3]mas/yr
Dec.: −70.666[3]mas/yr
Parallax (π)41.8±0.2579 mas[3]
Distance78.0 ± 0.5 ly
(23.9 ± 0.1 pc)
Absolute magnitude (MV)4.98[10]
Details
HD 11171
Mass1.26[11] M
Radius1.95[11] R
Luminosity5.6[11] L
Surface gravity (log g)3.96[11] cgs
Temperature6,342[11] K
Metallicity[Fe/H]−0.08[12] dex
Rotational velocity (v sin i)54.7[12] km/s
Age1.5[12] Gyr
HD 11131
Mass1.03[11] M
Radius1.00[11] R
Luminosity0.98[11] L
Surface gravity (log g)4.53[13] cgs
Temperature5,804[13] K
Metallicity[Fe/H]−0.09[13] dex
Rotation10 days[14]
Rotational velocity (v sin i)2.1[15] km/s
Age1.1[15] Gyr
Other designations
χ Cet,Gj 9061, ENG 8
χ Ceti A:53 Cet,HD 11171,BD−11°352,FK5 1051,HIP 8497,HR 531,SAO 148036[16]
χ Ceti B: EZ Cet, HD 11131, BD−11°351, HIP 8486, SAO 148033[17]
Database references
SIMBADχ Ceti
χ Ceti A
χ Ceti B

Chi Ceti (χ Ceti), is theBayer designation for adouble star in theequatorialconstellation ofCetus. They appear to becommon proper motion companions, sharing a similar motion through space.[18] The brighter component, HD 11171, is visible to thenaked eye with anapparent visual magnitude of 4.66, while the fainter companion, HD 11131, is magnitude 6.75.[2] Both lie at roughly the same distance, with the brighter component lying at an estimated distance of 76.6 light years from theSun based upon an annualparallax shift of42.58 mas.

Alight curve for EZ Ceti, plotted fromTESS data[19]

The primary, component A, is anevolvedK-typegiant star with astellar classification of F3 III.[5] However, Houk and Swift (1999) listed a classification of F0 V,[6] which would match anF-type main sequence star. It displays aninfrared excess at awavelength of 70 μm and thus is a candidate host of an orbitingdebris disk.[20]

The common proper motion companion, component B, is aG-type main sequence star with a classification of G3 V.[6] It is aBY Draconis variable with a periodicity of 8.92 days and avariable star designation of EZ Cet.[7]

References

[edit]
  1. ^abcdeVallenari, 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.
  2. ^abcdefgMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data: 0,Bibcode:1986EgUBV........0M.
  3. ^abcdefVallenari, 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.
  4. ^Hardegree-Ullman, Kevin K.; Apai, Dániel; Bergsten, Galen J.; Pascucci, Ilaria; López-Morales, Mercedes (2023)."Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets".The Astronomical Journal.165 (6): 267.arXiv:2304.12490.Bibcode:2023AJ....165..267H.doi:10.3847/1538-3881/acd1ec.
  5. ^abcLuck, R. Earle (September 2015), "Abundances in the Local Region. I. G and K Giants",The Astronomical Journal,150 (3): 23,arXiv:1507.01466,Bibcode:2015AJ....150...88L,doi:10.1088/0004-6256/150/3/88,S2CID 118505114, 88.
  6. ^abcdHouk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars",Michigan Spectral Survey,5: 0,Bibcode:1999MSS...C05....0H.
  7. ^abKazarovets, E. V.; et al. (2006), "The 78th Name-List of Variable Stars",Information Bulletin on Variable Stars,5721: 1,Bibcode:2006IBVS.5721....1K.
  8. ^Holmberg, J.; et al. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics",Astronomy and Astrophysics,501 (3):941–947,arXiv:0811.3982,Bibcode:2009A&A...501..941H,doi:10.1051/0004-6361/200811191,S2CID 118577511.
  9. ^de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  10. ^Porto de Mello, G. F.; et al. (March 2014), "A photometric and spectroscopic survey of solar twin stars within 50 parsecs of the Sun; I. Atmospheric parameters and color similarity to the Sun",Astronomy and Astrophysics,563: A52,arXiv:1312.7571,Bibcode:2014A&A...563A..52P,doi:10.1051/0004-6361/201322277,S2CID 119111150.
  11. ^abcdefghStassun, Keivan G.; et al. (2019)."The Revised TESS Input Catalog and Candidate Target List".The Astronomical Journal.158 (4): 138.arXiv:1905.10694.Bibcode:2019AJ....158..138S.doi:10.3847/1538-3881/ab3467.
  12. ^abcBorisov, Sviatoslav B.; Chilingarian, Igor V.; Rubtsov, Evgenii V.; Ledoux, Cédric; Melo, Claudio; Grishin, Kirill A.; Katkov, Ivan Yu.; Goradzhanov, Vladimir S.; Afanasiev, Anton V.; Kasparova, Anastasia V.; Saburova, Anna S. (2023)."New Generation Stellar Spectral Libraries in the Optical and Near-infrared. I. The Recalibrated UVES-POP Library for Stellar Population Synthesis".The Astrophysical Journal Supplement Series.266 (1): 11.arXiv:2211.09130.Bibcode:2023ApJS..266...11B.doi:10.3847/1538-4365/acc321.
  13. ^abcDatson, Juliet; et al. (February 2015), "Spectroscopic study of solar twins and analogues",Astronomy & Astrophysics,574: 12,arXiv:1412.8168,Bibcode:2015A&A...574A.124D,doi:10.1051/0004-6361/201425000,S2CID 53708062, A124.
  14. ^Isaacson, Howard; Fischer, Debra (2010). "Chromospheric Activity and Jitter Measurements for 2630 Stars on the California Planet Search".The Astrophysical Journal.725 (1): 875.arXiv:1009.2301.Bibcode:2010ApJ...725..875I.doi:10.1088/0004-637X/725/1/875.
  15. ^abLlorente De Andrés, F.; Chavero, C.; de la Reza, R.; Roca-Fàbrega, S.; Cifuentes, C. (2021). "The evolution of lithium in FGK dwarf stars. The lithium-rotation connection and the Li desert".Astronomy and Astrophysics.654.arXiv:2108.05852.Bibcode:2021A&A...654A.137L.doi:10.1051/0004-6361/202141339.
  16. ^"chi Cet",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2017-02-12.
  17. ^V* EZ Cet.
  18. ^Soderblom, David R.; Mayor, Michel (January 1993), "Stellar kinematic groups. I - The Ursa Major group",Astronomical Journal,105 (1):226–249,Bibcode:1993AJ....105..226S,doi:10.1086/116422.
  19. ^MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, retrieved8 December 2021.
  20. ^Koerner, D. W.; et al. (February 2010),"New Debris Disk Candidates Around 49 Nearby Stars"(PDF),The Astrophysical Journal Letters,710 (1):L26–L29,Bibcode:2010ApJ...710L..26K,doi:10.1088/2041-8205/710/1/L26,S2CID 122844702.

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