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{{Sky|21|40|05.5|-|16|39|44|139}}
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{{Starbox begin
| name=γ Capricorni
}}
{{Starbox image
| image = [[File:Capricornus constellation map.png|250px]]
| caption = Gamma Capricorni is at left center.
}}
{{Starbox observe
| epoch=[[J2000.0]]
| equinox=[[J2000.0]] ([[International Celestial Reference System|ICRS]])
| constell=[[Capricornus]]
| ra={{RA|21|40|05.4563}}<ref name="hipparcos">{{cite journal
  | author=Perryman, M. A. C. ''et al''
  | title=The HIPPARCOS Catalogue
  | journal=Astronomy & Astrophysics | volume=323
  | pages=L49–L52 |date=July 1997
  | bibcode=1997A&A...323L..49P }}</ref>
| dec={{DEC|−16|39|44.308}}<ref name="hipparcos" />
| appmag_v=+3.69
}}
{{Starbox character
| class=A7mp<ref name="SIMBAD" />
| b-v=+0.32<ref name="clpl4">{{cite journal
  | author=Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewskj, W. Z.
  | title=UBVRIJKL photometry of the bright stars
  | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | year=1966
  | bibcode=1966CoLPL...4...99J }}</ref>
| u-b=+0.22<ref name="clpl4" />
| variable=
}}
{{Starbox astrometry
| radial_v=−31.2<ref>{{cite book
  | last=Wilson | first=Ralph Elmer | year=1953
  | title=General catalogue of stellar radial velocities
  | publisher=Carnegie Institution of Washington
  | url=http://adsabs.harvard.edu/abs/1953QB901.W495.....
  | accessdate=2007-05-14 }}</ref>
| prop_mo_ra=187.39<ref name="hipparcos" />
| prop_mo_dec=−22.33<ref name="hipparcos" />
| parallax=23.48
| p_error=1.10
| parallax_footnote=<ref name="hipparcos" />
| absmag_v=
}}
{{Starbox detail
| age=
| metal=<math>\begin{smallmatrix}\left[\frac{Fe}{H}\right]\ =\ 0.5\end{smallmatrix}</math><ref name="aaa249" />
| mass=
| radius=
| rotational_velocity=40<ref>{{cite journal
  | author=Royer, F.; Grenier, S.; Baylac, M.-O.; Gómez, A. E.; Zorec, J. | title=Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i
  | journal=Astronomy and Astrophysics | volume=393
  | pages=897–911 |date=October 2002
  | doi=10.1051/0004-6361:20020943
  | bibcode=2002A&A...393..897R |arxiv = astro-ph/0205255 }}</ref>
| luminosity_bolometric=
| temperature=7,520<ref name="aaa249">{{cite journal
  | author=Burkhart, C.; Coupry, M. F. | title=The A and Am-Fm stars. I - The abundances of Li, Al, Si, and Fe
  | journal=Astronomy and Astrophysics | volume=249
   | issue=1 |date=September 1991 | pages=205−216
  | bibcode=1991A&A...249..205B }}</ref>
| gravity=3.95<ref name="aaa249" />
}}
{{Starbox catalog
| names = Nashira, 40 Capricorni, [[Harvard Revised catalogue|HR]] 8278, [[Henry Draper Catalogue|HD]] 206088, [[Gliese-Jahreiss catalogue|NN]] 4209, [[Bonner Durchmusterung|BD]]−17°6340, [[Fifth Fundamental Catalogue|FK5]] 812, [[Hipparcos catalogue|HIP]] 106985, [[Smithsonian Astrophysical Observatory catalogue|SAO]] 164560.<ref name="SIMBAD">{{cite web
  | work=SIMBAD | url =http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+206088
  | title=HD 206088 -- Variable Star of alpha2 CVn type
  | publisher=Centre de Données astronomiques de Strasbourg
  | accessdate=2009-11-12 }}</ref>
}}
{{Starbox end}}
'''Gamma Capricorni''' (γ Cap, γ Capricorni) is a [[giant star]] in the [[constellation]] [[Capricornus]]. It has the traditional name '''Nashira''', which comes from the [[Arabic language|Arabic]] '''سعد ناشرة''' - ''sa'd nashirah'' for "the lucky one" or "bearer of good news". 
 
In [[Chinese language|Chinese]], {{lang|zh|壘壁陣}} ({{lang|zh-Latn|Lěi Bì Zhèn}}), meaning ''[[Encampment (Chinese constellation)|Line of Ramparts]]'', refers to an asterism consisting of γ Capricorni, [[Kappa Capricorni|κ Capricorni]], [[Epsilon Capricorni|ε Capricorni]], [[Delta Capricorni|δ Capricorni]], [[Iota Aquarii|ι Aquarii]], [[Sigma Aquarii|σ Aquarii]], [[Lambda Aquarii|λ Aquarii]], [[Phi Aquarii|φ Aquarii]], [[27 Piscium]], [[29 Piscium]], [[33 Piscium]] and [[30 Piscium]].<ref>{{zh icon}} ''中國星座神話'', written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.</ref> Consequently, γ Capricorni itself is known as {{lang|zh|壘壁陣三}} ({{lang|zh-Latn|Lěi Bì Zhèn sān}}, {{lang-en|the Third Star of Line of Ramparts}}.)<ref>{{zh icon}} [http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/c_research_chinengstars_n_r.htm 香港太空館 - 研究資源 - 亮星中英對照表], Hong Kong Space Museum. Accessed on line November 23, 2010.</ref>
 
Because it is near the [[ecliptic]], γ Capricorni can be [[occultation|occulted]] by the [[Moon]], and (rarely) by [[planet]]s.
 
γ Capricorni is a blue-white [[stellar classification|A-type (A7III)]] [[sequence|giant star]] with a mean [[apparent magnitude]] of +3.69.  It is approximately 139 [[light years]] from [[Earth]].  It is classified as an [[Alpha² Canum Venaticorum variable|Alpha2 Canum Venaticorum type]] [[variable star]] and its brightness varies by 0.03 magnitudes.
 
==Nashira as the name==
[[Nashira (AK-85)]] is once of [[United States]] navy ship.
 
==References==
{{reflist}}
 
{{Stars of Capricornus}}
 
[[Category:Alpha2 Canum Venaticorum variables]]
[[Category:Bayer objects|Capricorni, Gamma]]
[[Category:Capricornus (constellation)]]
[[Category:F-type main-sequence stars]]
[[Category:Stars with proper names]]
 
 
{{var-star-stub}}

Revision as of 04:15, 22 February 2014

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