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Phi3 Hydrae

From Wikipedia, the free encyclopedia
Binary star system in the constellation Hydra
For other stars with thisBayer designation, seeφ Hydrae
Phi3 Hydrae
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationHydra
Right ascension10h 38m 34.95281s[1]
Declination−16° 52′ 35.6665″[1]
Apparent magnitude (V)4.90[2]
Characteristics
Evolutionary stagered clump[3]
Spectral typeG8 III[4]
B−Vcolor index0.912[5]
Astrometry
Radial velocity (Rv)+17.45±0.70[6] km/s
Proper motion (μ)RA: −98.92[1]mas/yr
Dec.: +25.84[1]mas/yr
Parallax (π)15.49±0.57 mas[1]
Distance211 ± 8 ly
(65 ± 2 pc)
Absolute magnitude (MV)+0.89[7]
Orbit[2]
Period (P)1200 d
Eccentricity (e)0.1
Periastronepoch (T)2420760 JD
Argument of periastron (ω)
(secondary)
270°
Semi-amplitude (K1)
(primary)
4.0 km/s
Details
φ3 Hya
Mass2.04[4] M
Radius9[5] R
Luminosity48[4] L
Surface gravity (log g)2.95[7] cgs
Temperature4,952±17[4] K
Metallicity [Fe/H]−0.22±0.12[7] dex
Rotational velocity (v sin i)3.6[5] km/s
Age1.17[4] Gyr
Other designations
φ3 Hya,BD−16°3100,FK5 2850,HD 92214,HIP 52085,HR 4171,SAO 156122[8]
Database references
SIMBADdata

Phi3 Hydrae (φ3 Hya) is abinary star[2] in the equatorialconstellation ofHydra. It originally received theFlamsteed designation of2 Crateris before being placed in the Hydra constellation.[9] Based upon an annualparallax shift of 15.49 mas as seen from Earth, it is located around 211 light years from theSun. It is visible to the naked eye with anapparent visual magnitude of 4.90.[2] It forms a triangle with the fainterφ1 Hydrae andφ2 Hydrae, betweenμ Hydrae andν Hydrae.

This is a single-linedspectroscopic binary star system with anorbital period of about 1,200 days and aneccentricity of 0.1.[2] The primary, component A, is anevolvedG-typegiant star with astellar classification of G8 III.[4] It is ared clump star,[3] which means it is generating energy through thefusion of helium at its core. The star has twice[4] themass of the Sun and has expanded to 9[5] times theSun's radius. It is 1.17[4] billion years old and is radiating 48[4] times thesolar luminosity from itsphotosphere at aneffective temperature of 4,952 K.[4]

References

[edit]
  1. ^abcdevan 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.
  2. ^abcdePourbaix, D.; et al. (September 2004), "SB9: The ninth catalogue of spectroscopic binary orbits",Astronomy and Astrophysics,424:727–732,arXiv:astro-ph/0406573,Bibcode:2004A&A...424..727P,doi:10.1051/0004-6361:20041213,S2CID 119387088.
  3. ^abLaney, C. D.; et al. (January 2012), "A new Large Magellanic Cloud K-band distance from precision measurements of nearby red clump stars",Monthly Notices of the Royal Astronomical Society,419 (2):1637–1641,arXiv:1109.4800,Bibcode:2012MNRAS.419.1637L,doi:10.1111/j.1365-2966.2011.19826.x,S2CID 117788450.
  4. ^abcdefghijLuck, 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.
  5. ^abcdMassarotti, Alessandro; et al. (January 2008), "Rotational and radial velocities for a sample of 761 HIPPARCOS giants and the role of binarity",The Astronomical Journal,135 (1):209–231,Bibcode:2008AJ....135..209M,doi:10.1088/0004-6256/135/1/209,S2CID 121883397.
  6. ^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.
  7. ^abcMcWilliam, Andrew (1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances",The Astrophysical Journal Supplement Series,74: 1075,Bibcode:1990ApJS...74.1075M,doi:10.1086/191527.
  8. ^"phi Hya".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-03-17.
  9. ^Wagman, M. (August 1987), "Flamsteed's Missing Stars",Journal for the History of Astronomy,18 (3): 216,Bibcode:1987JHA....18..209W,doi:10.1177/002182868701800305,S2CID 118445625.
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