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Zeta Mensae

Zeta Mensae, Latinized from ζ Mensae, is a solitary,[9] white-hued star in the southern constellation of Mensa. It is faintly visible to the naked eye, having an apparent visual magnitude of +5.64.[2] Based upon an annual parallax shift of 8.2879 mas as seen from GAIA, it is located around 394 light years from the Sun.[1] At that distance, the visual magnitude is diminished by an extinction factor of 0.088 due to interstellar dust.[4] Eggen (1995) listed it as a proper motion candidate for membership in the IC 2391 supercluster.[10]

Zeta Mensae
Location of ζ Mensae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Mensa
Right ascension 06h 40m 02.89197s[1]
Declination −80° 48′ 48.9391″[1]
Apparent magnitude (V) +5.64[2]
Characteristics
Spectral type A5 III[3][4]
U−B color index +0.15[2]
B−V color index +0.20[2]
Astrometry
Radial velocity (Rv)+7.0±7.4[5] km/s
Proper motion (μ) RA: −4.801[1] mas/yr
Dec.: +53.158[1] mas/yr
Parallax (π)8.2879 ± 0.0870 mas[1]
Distance394 ± 4 ly
(121 ± 1 pc)
Absolute magnitude (MV)+0.09[6]
Details
Radius4.65±0.27[1] R
Luminosity66.39±0.86[1] L
Temperature7,555±43[4] K
Rotational velocity (v sin i)200[7] km/s
Other designations
ζ Men, CPD−80° 196, FK5 264, HD 50506, HIP 31897, HR 2559, SAO 258451[8]
Database references
SIMBADdata

The stellar classification of A5 III[3] suggests this is an A-type giant star. It is spinning rapidly, showing a projected rotational velocity of 200 km/s,[7] giving the star an oblate shape with an equatorial bulge that is an estimated 26% larger than the polar radius.[3] The star is radiating about 69[11] times the Sun's luminosity from its photosphere at an effective temperature of around 7,555 K.[4] It displays a faint infrared excess at a wavelength of 18μm, indicating that it is being orbited by a debris disk.[12]

References Edit

  1. ^ a b c d e f g h Brown, 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 at VizieR.
  2. ^ a b c d Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99): 99, Bibcode:1966CoLPL...4...99J.
  3. ^ a b c Belle, G. T. (2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review, 20 (1): 51, arXiv:1204.2572, Bibcode:2012A&ARv..20...51V, doi:10.1007/s00159-012-0051-2, S2CID 119273474.
  4. ^ a b c d Paunzen, E.; et al. (October 2006), "An empirical temperature calibration for the Δ a photometric system. II. The A-type and mid F-type stars", Astronomy and Astrophysics, 458 (1): 293–296, arXiv:astro-ph/0607567, Bibcode:2006A&A...458..293P, doi:10.1051/0004-6361:20064889, S2CID 18219735.
  5. ^ 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.
  6. ^ Anderson, 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.
  7. ^ a b Levato, O. H. (August 1972). "Rotational Velocities and Spectral Types of Some A-Type Stars". Publications of the Astronomical Society of the Pacific. 84 (500): 584. Bibcode:1972PASP...84..584L. doi:10.1086/129336. eISSN 1538-3873. ISSN 0004-6280.
  8. ^ "zet Men". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-08-15.
  9. ^ 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.
  10. ^ Eggen, Olin J. (December 1995), "Reality Tests of Superclusters in the Young Disk Population", Astronomical Journal, 110: 2862, Bibcode:1995AJ....110.2862E, doi:10.1086/117734.
  11. ^ McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
  12. ^ Ishihara, Daisuke; et al. (May 2017), "Faint warm debris disks around nearby bright stars explored by AKARI and IRSF", Astronomy & Astrophysics, 601: 18, arXiv:1608.04480, Bibcode:2017A&A...601A..72I, doi:10.1051/0004-6361/201526215, S2CID 55234482, A72.

zeta, mensae, latinized, from, mensae, solitary, white, hued, star, southern, constellation, mensa, faintly, visible, naked, having, apparent, visual, magnitude, based, upon, annual, parallax, shift, 2879, seen, from, gaia, located, around, light, years, from,. Zeta Mensae Latinized from z Mensae is a solitary 9 white hued star in the southern constellation of Mensa It is faintly visible to the naked eye having an apparent visual magnitude of 5 64 2 Based upon an annual parallax shift of 8 2879 mas as seen from GAIA it is located around 394 light years from the Sun 1 At that distance the visual magnitude is diminished by an extinction factor of 0 088 due to interstellar dust 4 Eggen 1995 listed it as a proper motion candidate for membership in the IC 2391 supercluster 10 Zeta MensaeLocation of z Mensae circled Observation dataEpoch J2000 0 Equinox J2000 0 ICRS Constellation MensaRight ascension 06h 40m 02 89197s 1 Declination 80 48 48 9391 1 Apparent magnitude V 5 64 2 CharacteristicsSpectral type A5 III 3 4 U B color index 0 15 2 B V color index 0 20 2 AstrometryRadial velocity Rv 7 0 7 4 5 km sProper motion m RA 4 801 1 mas yr Dec 53 158 1 mas yrParallax p 8 2879 0 0870 mas 1 Distance394 4 ly 121 1 pc Absolute magnitude MV 0 09 6 DetailsRadius4 65 0 27 1 R Luminosity66 39 0 86 1 L Temperature7 555 43 4 KRotational velocity v sin i 200 7 km sOther designationsz Men CPD 80 196 FK5 264 HD 50506 HIP 31897 HR 2559 SAO 258451 8 Database referencesSIMBADdataThe stellar classification of A5 III 3 suggests this is an A type giant star It is spinning rapidly showing a projected rotational velocity of 200 km s 7 giving the star an oblate shape with an equatorial bulge that is an estimated 26 larger than the polar radius 3 The star is radiating about 69 11 times the Sun s luminosity from its photosphere at an effective temperature of around 7 555 K 4 It displays a faint infrared excess at a wavelength of 18mm indicating that it is being orbited by a debris disk 12 References Edit a b c d e f g h Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b c d Johnson H L et al 1966 UBVRIJKL photometry of the bright stars Communications of the Lunar and Planetary Laboratory 4 99 99 Bibcode 1966CoLPL 4 99J a b c Belle G T 2012 Interferometric observations of rapidly rotating stars The Astronomy and Astrophysics Review 20 1 51 arXiv 1204 2572 Bibcode 2012A amp ARv 20 51V doi 10 1007 s00159 012 0051 2 S2CID 119273474 a b c d Paunzen E et al October 2006 An empirical temperature calibration for the D a photometric system II The A type and mid F type stars Astronomy and Astrophysics 458 1 293 296 arXiv astro ph 0607567 Bibcode 2006A amp A 458 293P doi 10 1051 0004 6361 20064889 S2CID 18219735 de Bruijne J H J Eilers A C October 2012 Radial velocities for the HIPPARCOS Gaia Hundred Thousand Proper Motion project Astronomy amp Astrophysics 546 14 arXiv 1208 3048 Bibcode 2012A amp A 546A 61D doi 10 1051 0004 6361 201219219 S2CID 59451347 A61 Anderson 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 a b Levato O H August 1972 Rotational Velocities and Spectral Types of Some A Type Stars Publications of the Astronomical Society of the Pacific 84 500 584 Bibcode 1972PASP 84 584L doi 10 1086 129336 eISSN 1538 3873 ISSN 0004 6280 zet Men SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2017 08 15 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 Eggen Olin J December 1995 Reality Tests of Superclusters in the Young Disk Population Astronomical Journal 110 2862 Bibcode 1995AJ 110 2862E doi 10 1086 117734 McDonald I et al 2012 Fundamental Parameters and Infrared Excesses of Hipparcos Stars Monthly Notices of the Royal Astronomical Society 427 1 343 57 arXiv 1208 2037 Bibcode 2012MNRAS 427 343M doi 10 1111 j 1365 2966 2012 21873 x S2CID 118665352 Ishihara Daisuke et al May 2017 Faint warm debris disks around nearby bright stars explored by AKARI and IRSF Astronomy amp Astrophysics 601 18 arXiv 1608 04480 Bibcode 2017A amp A 601A 72I doi 10 1051 0004 6361 201526215 S2CID 55234482 A72 Retrieved from https en wikipedia org w index php title Zeta Mensae amp oldid 1141323270, wikipedia, wiki, book, books, library,

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