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7 Ceti

From Wikipedia, the free encyclopedia
Star in the constellation Cetus
7 Ceti

Alight curve for AE Ceti, plotted from data presented by Tabur,et al. (2009)[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationCetus
Right ascension00h 14m 38.41655s[2]
Declination−18° 55′ 58.3145″[2]
Apparent magnitude (V)4.44[3](4.26–4.46)[4]
Characteristics
Spectral typeM1 III[5]
B−Vcolor index1.640±0.044[3]
Variable typeLB:[4]
Astrometry
Radial velocity (Rv)−22.9±1.0[6] km/s
Proper motion (μ)RA: −26.15[2]mas/yr
Dec.: −73.58[2]mas/yr
Parallax (π)7.29±0.28 mas[2]
Distance450 ± 20 ly
(137 ± 5 pc)
Absolute magnitude (MV)–1.24[3]
Details
Radius54[7] R
Luminosity1019.14[8] L
Temperature3,800[8] K
Other designations
3 Cet,AE Ceti,BD−19°21,HD 1038,HIP 1170,HR 48,SAO 147169[9]
Database references
SIMBADdata

7 Ceti is a single,[10]variable star in theequatorialconstellation ofCetus. It has thevariable star designation AE Ceti.[1] The star is visible to thenaked eye with a baselineapparent visual magnitude of 4.44.[3] Based upon an annualparallax shift of only7.3 mas,[2] it is located roughly 450 light years away. It is moving closer to the Sun with a heliocentricradial velocity of −23 km/s.[6] Eggen (1965) listed it as a probable member of theWolf 630 group of co-moving stars.[11]

This is an agingred giant star with astellar classification of M1 III,[5] currently on theasymptotic giant branch.[12] In 1959,Alan William James Cousins announced the detection of variability in the brightness of 7 Ceti.[13] It was given its variable star designation in 1973.[14] Samus et al. (2017) has it classed as aslow irregular variable of type LB:, and ranges in magnitude from 4.26 down to 4.46.[4] Tabur et al. (2009) list it as asemiregular variable with four known periods ranging infrequency from 19.2 to 41.7 days.[1] Thestellar atmosphere of 7 Ceti has expanded to an estimated 54[7] times theSun's radius. It is radiating around 1,019[8] times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 3,800 K.[8]

Luminosity variation[1]
Period
(Days)
Amplitude
(Mag.)
19.20.018
19.60.020
27.10.018
41.70.017

References

[edit]
  1. ^abcdTabur, V.; et al. (December 2009), "Long-term photometry and periods for 261 nearby pulsating M giants",Monthly Notices of the Royal Astronomical Society,400 (4):1945–1961,arXiv:0908.3228,Bibcode:2009MNRAS.400.1945T,doi:10.1111/j.1365-2966.2009.15588.x,S2CID 15358380.
  2. ^abcdefvan Leeuwen, F. (2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
  3. ^abcdAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  4. ^abcSamus, N. N.; et al. (2017), "General Catalogue of Variable Stars",Astronomy Reports, 5.1,61 (1):80–88,Bibcode:2017ARep...61...80S,doi:10.1134/S1063772917010085,S2CID 125853869.
  5. ^abHouk, Nancy; Smith-Moore, M. (1978),Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 4, Ann Arbor: Dept. of Astronomy, University of Michigan,Bibcode:1988mcts.book.....H.
  6. ^abde 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.
  7. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (2) (Third ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  8. ^abcdMcDonald, I.; et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars",Monthly Notices of the Royal Astronomical Society,427 (1):343–357,arXiv:1208.2037,Bibcode:2012MNRAS.427..343M,doi:10.1111/j.1365-2966.2012.21873.x,S2CID 118665352.
  9. ^"7 Cet".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedDecember 26, 2018.
  10. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  11. ^Eggen, O. J. (October 1965), "The Wolf 630 group",The Observatory,85:191–195,Bibcode:1965Obs....85..191E,
  12. ^Eggen, O. J. (1992), "Asymptotic giant branch stars near the sun",The Astronomical Journal,104: 275,Bibcode:1992AJ....104..275E,doi:10.1086/116239.
  13. ^Cousins, A. W. J. (1959)."Measures of Bright Southern Stars on UBV System".Monthly Notes of the Astronomical Society of South Africa.18:46–47.Bibcode:1959MNSSA..18...46C. Retrieved24 January 2025.
  14. ^Kukarkin, B. V.; Kholopov, P. N.; Kukarkina, N. P.; Perova, N. B. (October 1973)."59th Name-List of Variable Stars"(PDF).Information Bulletin on Variable Stars.834:1–22.Bibcode:1973IBVS..834....1K. Retrieved24 January 2025.
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