Star in the constellation of Scorpius
N Scorpii Location of N Scorpii on the map
Observation dataEpoch J2000 Equinox J2000 Constellation Scorpius Right ascension 16h 31m 22.93300s [ 1] Declination −34° 42′ 15.7146″[ 1] Apparent magnitude (V)4.23[ 2] Characteristics Spectral type B2 III-IV[ 3] U−Bcolor index −0.76[ 2] B−Vcolor index −0.17[ 2] Variable type candidateβ Cephei [ 4] Astrometry Radial velocity (Rv )0.8± 1.5[ 5] km/s Proper motion (μ)RA: −12.05± 0.20mas /yr [ 1] Dec.: −18.16± 0.13mas /yr [ 1] Parallax (π)5.88± 0.19 mas [ 1] Distance 550 ± 20 ly (170 ± 5 pc ) Absolute magnitude (MV )−1.91[ 6] Details Mass 7.8± 0.1[ 7] M ☉ Radius 6.25[ 8] R ☉ Luminosity (bolometric) 6,918[ 9] L ☉ Surface gravity (log g )4.0[ 9] cgs Temperature 21,877[ 9] K Metallicity [Fe/H] +0.01[ 10] dex Rotational velocity (v sin i )70± 8[ 11] km/s Age 22± 4[ 7] Myr Other designations N Scorpii ,72 G. Scorpii [ 12] ,CD −34°11044 ,CPD −34°6528 ,FK5 1431 ,GC 22195 ,HD 148703 ,HIP 80911 ,HR 6143 ,SAO 207732[ 13] Database references SIMBAD data
N Scorpii , also known asHD 148703 , is a solitary,[ 14] bluish-white huedstar located in the southernconstellation Scorpius . It has anapparent magnitude of 4.23, making it readily visible to thenaked eye . N Scorpii was initially given theBayer designation Alpha Normae byLacaille but it was later moved fromNorma to Scorpius.[ 15] N Scorpii is currently located 550light years away based onparallax measurements from theHipparcos satellite and is part of the Upper Scorpius–Centaurus region of theScorpius–Centaurus association .[ 16]
N Scorpii has been given severalstellar classifications over the years. It has been given theluminosity class of amain sequence star (V),[ 17] asubgiant (IV),[ 18] an evolvedgiant star (III),[ 19] or a blend between the last two classes (III-IV).[ 3] It is generally classified as either a B2 or B3 star several times hotter than theSun . HD 148703 is a candidateβ Cephei variable [ 4] and its variability was first noticed in 1983 by C. Sterken.[ 20] Further observations were made by Abt et al. (2002) by observing itsprojected rotational velocity .[ 21] It was identified as a candidate in 2002 in a survey for non-radial pulsations inB-type stars .[ 22]
The object has two generally accepted classes: B2 III-IV and B2 IV. It has 7.8 times themass of the Sun [ 7] and 6.25 times itssize .[ 8] It has abolometric luminosity 6,918 times greater than the Sun from itsphotosphere at aneffective temperature of 21,877 K .[ 9] N Scorpii is estimated to be 22million years old,[ 7] which is twice the average age of the aforementioned association. Like most hot stars, N Scorpii spins rapidly, having aprojected rotational velocity of 70 km/s .[ 11]
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"Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system".Astronomy Letters .32 (11):759– 771.arXiv :1606.08053 .Bibcode :2006AstL...32..759G .doi :10.1134/S1063773706110065 .eISSN 1562-6873 .ISSN 1063-7737 .S2CID 119231169 . ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters .38 (5):331– 346.arXiv :1108.4971 .Bibcode :2012AstL...38..331A .doi :10.1134/S1063773712050015 .eISSN 1562-6873 .ISSN 1063-7737 .S2CID 119257644 . ^a b c d Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (October 12, 2010)."A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun" .Monthly Notices of the Royal Astronomical Society .410 (1). Oxford University Press (OUP):190– 200.arXiv :1007.4883 .Bibcode :2011MNRAS.410..190T .doi :10.1111/j.1365-2966.2010.17434.x .ISSN 0035-8711 . ^a b Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022)."Stellar and substellar companions fromGaia EDR3" .Astronomy & Astrophysics .657 : A7.arXiv :2109.10912 .Bibcode :2022A&A...657A...7K .doi :10.1051/0004-6361/202142146 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b c d Sartori, M. J.; Lépine, J. R. D.; Dias, W. S. (June 2003)."Formation scenarios for the young stellar associations between galactic longitudesl = 280° - 360° " .Astronomy & Astrophysics .404 (3):913– 926.arXiv :astro-ph/0304426 .Bibcode :2003A&A...404..913S .doi :10.1051/0004-6361:20030581 .eISSN 1432-0746 .ISSN 0004-6361 . ^ Anders, F.; et al. (August 2019)."Photo-astrometric distances, extinctions, and astrophysical parameters forGaia DR2 stars brighter thanG = 18" .Astronomy & Astrophysics .628 : A94.arXiv :1904.11302 .Bibcode :2019A&A...628A..94A .doi :10.1051/0004-6361/201935765 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b Brown, A. G. A.; Verschueren, W. (March 1997). "High S/N Echelle spectroscopy in young stellar groups. II. Rotational velocities of early-type stars in SCO OB2".Astronomy & Astrophysics .319 :811– 838.arXiv :astro-ph/9608089 .Bibcode :1997A&A...319..811B .ISSN 0004-6361 . ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas".Resultados del Observatorio Nacional Argentino .1 .Bibcode :1879RNAO....1.....G . ^ "N Scorpii" .SIMBAD .Centre de données astronomiques de Strasbourg . RetrievedOctober 17, 2022 .^ Eggleton, P. P.; Tokovinin, A. A. (11 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 .eISSN 1365-2966 .ISSN 0035-8711 . ^ "Norma Constellation (the Level): Stars, Story, Facts... | Constellation Guide" .www.constellation-guide.com . Retrieved11 October 2021 .^ Rizzuto, A. C.; Ireland, M. J.; Robertson, J. G. (18 August 2011)."Multidimensional Bayesian membership analysis of the Sco OB2 moving group" .Monthly Notices of the Royal Astronomical Society .416 (4):3108– 3117.arXiv :1106.2857 .Bibcode :2011MNRAS.416.3108R .doi :10.1111/j.1365-2966.2011.19256.x .ISSN 0035-8711 . ^ de Vaucouleurs, A. (1 August 1957)."Spectral Types and Luminosities of B, A and F Southern Stars" .Monthly Notices of the Royal Astronomical Society .117 (4):449– 462.Bibcode :1957MNRAS.117..449D .doi :10.1093/mnras/117.4.449 .eISSN 1365-2966 .ISSN 0035-8711 . ^ Buscombe, W. (1 May 1969)."Line Strengths for Southern OB stars--II: Observations with Moderate Dispersion" .Monthly Notices of the Royal Astronomical Society .144 (1):31– 39.Bibcode :1969MNRAS.144...31B .doi :10.1093/mnras/144.1.31 .ISSN 0035-8711 . ^ Hiltner, W. A.; Garrison, R. F.; Schild, R. E. (July 1969)."MK Spectral Types for Bright Southern OB Stars" .The Astrophysical Journal .157 : 313.Bibcode :1969ApJ...157..313H .doi :10.1086/150069 .eISSN 1538-4357 .ISSN 0004-637X . ^ Sterken, C.; Jerzykiewicz, M. (1983). "Search for beta Cephei stars south of declination -20 II. Photometric and spectrographic observations of early B giants and subgiants - Winter objects".Acta Astronomica .33 :89– 111.Bibcode :1983AcA....33...89S .ISSN 0001-5237 . ^ Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002)."Rotational Velocities of B Stars" .The Astrophysical Journal .573 (1):359– 365.Bibcode :2002ApJ...573..359A .doi :10.1086/340590 .ISSN 0004-637X . ^ Schrijvers, C.; Telting, J. H.; De Ridder, J. (2002). "A Spectroscopic Search for Non-Radial Pulsations in Early B-Type Stars".IAU Colloq. 185: Radial and Nonradial Pulsationsn as Probes of Stellar Physics .259 : 204.Bibcode :2002ASPC..259..204S .