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Phi2 Ceti

From Wikipedia, the free encyclopedia
Star in the constellation Cetus
For other stars with this Bayer designation, seeφ Ceti.
φ2 Ceti
Location of φ2 Ceti (circled in red)
Observation data
Epoch J2000      Equinox J2000
ConstellationCetus
Right ascension00h 50m 07.58896s[1]
Declination−10° 38′ 39.5839″[1]
Apparent magnitude (V)5.172[2]
Characteristics
Evolutionary stagemain sequence[1]
Spectral typeF7V[3]
U−Bcolor index+0.009[2]
B−Vcolor index+0.518[2]
Astrometry
Radial velocity (Rv)+8.21±0.12[1] km/s
Proper motion (μ)RA: −228.031[1]mas/yr
Dec.: −229.577[1]mas/yr
Parallax (π)62.8022±0.0951 mas[1]
Distance51.93 ± 0.08 ly
(15.92 ± 0.02 pc)
Absolute magnitude (MV)4.23[4]
Details
Mass1.19[5] M
Radius1.17+0.03
−0.01
[6] R
Luminosity1.852+0.006
−0.007
[6] L
Surface gravity (log g)4.45[5] cgs
Temperature6,352[5] K
Metallicity[Fe/H]−0.03[5] dex
Rotational velocity (v sin i)4.3[7] km/s
Age1.9[5] Gyr
Other designations
φ2 Cet,19 Cet,NSV 316,BD−11°153,GJ 37,HD 4813,HIP 3909,HR 235,SAO 147470
Database references
SIMBADdata

Phi2 Ceti,Latinized from φ2 Ceti), is astar located in the equatorialconstellation ofCetus. φ2 Ceti is also known as19 Ceti, andHD 4813. Based uponparallax measurements, it is located about 52 light years away. It has anapparent visual magnitude of +5.19, making it bright enough to be seen with the naked eye. The star is drifting further away with aradial velocity of +8 km/s.[1]

This is an ordinaryF-type main sequence star with astellar classification of F7V. The star is estimated to be 1.9[5] billion years old and is spinning with aprojected rotational velocity of 4.3 km/s.[7] It has 1.2[5] times the mass and 1.17[6] times the radius of the Sun. The star is radiating 1.85[6] times the luminosity of the Sun from itsphotosphere at aneffective temperature of 6,352 K.[5] It is a suspected variable star of unknown type, with a brightness that has been measured ranging from magnitude 5.15 down to 5.24.[8]

References

[edit]
  1. ^abcdefghVallenari, 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. ^abcGutierrez-Moreno, Adelina; et al. (1966), "A System of photometric standards",Publications of the Department of Astronomy University of Chile,1, Publicaciones Universidad de Chile, Department de Astronomy:1–17,Bibcode:1966PDAUC...1....1G.
  3. ^Gray, R. O.; et al. (2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample",The Astronomical Journal,132 (1):161–70,arXiv:astro-ph/0603770,Bibcode:2006AJ....132..161G,doi:10.1086/504637,S2CID 119476992.
  4. ^Paunzen, E.; et al. (July 2014), "Investigating the possible connection between λ Bootis stars and intermediate Population II type stars",Astronomy & Astrophysics,567: 8,arXiv:1406.3936,Bibcode:2014A&A...567A..67P,doi:10.1051/0004-6361/201423817,S2CID 56332289, A67.
  5. ^abcdefghBensby, T.; et al. (2014), "Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the solar neighbourhood",Astronomy & Astrophysics,562 (A71): 28,arXiv:1309.2631,Bibcode:2014A&A...562A..71B,doi:10.1051/0004-6361/201322631,S2CID 118786105.
  6. ^abcdBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  7. ^abSchröder, C.; Reiners, Ansgar; Schmitt, Jürgen H. M. M. (January 2009),"Ca II HK emission in rapidly rotating stars. Evidence for an onset of the solar-type dynamo"(PDF),Astronomy and Astrophysics,493 (3):1099–1107,Bibcode:2009A&A...493.1099S,doi:10.1051/0004-6361:200810377, archived fromthe original(PDF) on 2017-09-22, retrieved2018-11-04
  8. ^Samus, 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.
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