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Alpha Apodis

From Wikipedia, the free encyclopedia
Star in the constellation Apus
α Apodis
Diagram showing star positions and boundaries of the Apus constellation and its surroundings
Location of α Apodis (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationApus
Right ascension14h 47m 51.71203s[1]
Declination−79° 02′ 41.1032″[1]
Apparent magnitude (V)3.825[2]
Characteristics
Spectral typeK2.5III[2]
U−Bcolor index+1.68[3]
B−Vcolor index+1.43[3]
R−Icolor index+0.53[4]
Astrometry
Radial velocity (Rv)−1.1[5] km/s
Proper motion (μ)RA: −7.395[6]mas/yr
Dec.: −15.726[6]mas/yr
Parallax (π)7.5519±0.3237 mas[6]
Distance430 ± 20 ly
(132 ± 6 pc)
Absolute magnitude (MV)−1.67[7]
Details
Mass4.46[8] M
Radius65 ± 5[9][a] R
Luminosity1,072±22[9] L
Temperature4,090±80[9] K
Metallicity [Fe/H]-0.3[9] dex
Other designations
α Aps, Alpha Apodis, Alpha Aps,CPD−78°893,FK5 542,HD 129078,HIP 72370,HR 5470,SAO 257193.[2]
Database references
SIMBADdata

Alpha Apodis (Alpha Aps, α Apodis, α Aps) is the brighteststar in the southerncircumpolar constellation ofApus, with anapparent magnitude of approximately 3.825.[10] It had the Greek alpha designation as part of the constellation whichJohann Bayer called Apis Indica in his 1603Uranometria star atlas.[11] With a declination of –79°, this is acircumpolar star for much of the southern hemisphere. It can be identified on the night sky by drawing an imaginary line throughAlpha Centauri andAlpha Circini then extending it toward the south celestial pole.[12]

This is agiant star with astellar classification of K2.5III,[2] indicating that this star has consumed the hydrogen at its core and hasevolved away from themain sequence. It has expanded to an estimated radius of about 65 times theradius of the Sun and is emitting 1,000 times theSun's luminosity. Thephotosphere has aneffective temperature of 4,090 K,[9] giving the star the characteristic orange hue of a K-type star.[13] Based uponparallax measurements, this star is 430 ± 20light-years from theEarth.[6] It is not known to have a companion.[14]

Naming

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InChinese caused by adaptation of the European southern hemisphere constellations into the Chinese system,異雀 (Yì Què), meaningExotic Bird, refers to an asterism consisting of α Apodis,ζ Apodis,ι Apodis,β Apodis,γ Apodis,δ Octantis,δ1 Apodis,η Apodis, andε Apodis. Consequently, α Apodis itself is known as異雀八 (Yì Què bā, English:the Eighth Star of Exotic Bird.)[15]

Notes

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  1. ^ Applying theStefan–Boltzmann law with a nominalsolareffective temperature of 5,772 K:
    (5,7724,090)4103.03=65.19 R{\displaystyle {\sqrt {{\biggl (}{\frac {5,772}{4,090}}{\biggr )}^{4}\cdot 10^{3.03}}}=65.19\ R_{\odot }}.

References

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  1. ^abvan Leeuwen, F. (November 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. ^abcd"alf Aps -- Star",SIMBAD,Centre de Données astronomiques de Strasbourg, retrieved2011-12-23.
  3. ^abJohnson, 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.
  4. ^HR 5470, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr.,CDS IDV/50. Accessed online October 3, 2008.
  5. ^Evans, D. S. (June 20–24, 1966), Batten, Alan Henry; Heard, John Frederick (eds.), "The Revision of the General Catalogue of Radial Velocities",Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto:International Astronomical Union, p. 57,Bibcode:1967IAUS...30...57E.
  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.
  7. ^Cardini, D. (January 2005), "Mg II chromospheric radiative loss rates in cool active and quiet stars",Astronomy and Astrophysics,430 (1):303–311,arXiv:astro-ph/0409683,Bibcode:2005A&A...430..303C,doi:10.1051/0004-6361:20041440,S2CID 12136256.
  8. ^Kervella, Pierre; Arenou, Frédéric; Mignard, François; Thévenin, Frédéric (2019-03-01)."Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly".Astronomy and Astrophysics.623: A72.arXiv:1811.08902.Bibcode:2019A&A...623A..72K.doi:10.1051/0004-6361/201834371.ISSN 0004-6361.
  9. ^abcdeCharbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (2020-01-01)."Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era".Astronomy and Astrophysics.633: A34.arXiv:1910.12732.Bibcode:2020A&A...633A..34C.doi:10.1051/0004-6361/201936360.ISSN 0004-6361.
  10. ^Kaler, James B.,"Alpha Aps",Stars,University of Illinois, archived fromthe original on 2008-12-02, retrieved2011-12-23.
  11. ^Ridpath, Ian,"Apus, the bird of paradise",Ian Ridpath's Star Tales, retrieved2011-12-25.
  12. ^Moore, Patrick (2000),Exploring the night sky with binoculars (4th ed.),Cambridge University Press, p. 113,ISBN 0-521-79390-4.
  13. ^"The Colour of Stars",Australia Telescope, Outreach and Education,Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived fromthe original on February 22, 2012, retrieved2012-01-16.
  14. ^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.
  15. ^(in Chinese)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 29 日Archived 2011-05-22 at theWayback Machine
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