Gamma Arae
{{Short description|Star in the constellation Ara}}
{{Starbox begin
| name=γ Arae
}}
{{Starbox image
| image=
{{Location mark
|image=Ara constellation map.svg|alt=|float=center|width=240
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=γ Arae
|x=524|y=720
}}
|caption=Location of γ Arae (circled)
}}
{{Starbox observe
| epoch = J2000
| dec = {{DEC|−56|22|39.8148}}
| constell = Ara
}}
{{Starbox character
| variable =
}}
{{Starbox astrometry
| prop_mo_ra = −0.44
| prop_mo_dec = −15.77
| parallax = 2.93
| p_error = 0.16
}}
{{Starbox detail
| mass = {{solar mass|12.5}}
19
| temperature = {{val|21240|212|fmt=commas}}
| metal_fe =
| rotational_velocity = {{val|269|11}}
| rotation = 4.8 days
}}
{{Starbox catalog
| names = {{odlist | B=γ Ara | CPD=−56°8225 | HD=157246 | HIP=85267 | HR=6462 | SAO=244726 | 2E=3895 | WDS=J17254-5623A | GC=23517 | PPM=345992 }}
}}
{{Starbox reference
| Simbad=HD+157246
| ARICNS =
}}
{{Starbox end}}
Gamma Arae is a massive star in the southern constellation of Ara. Its name is a Bayer designation that is Latinized from γ Arae, and abbreviated Gamma Ara or γ Ara. With an apparent visual magnitude of 3.3, it is the fourth-brightest star in the constellation and is readily visible to the naked eye. From parallax measurements made during the Hipparcos mission, the distance to this star can be estimated as {{Convert|1110|ly|pc|abbr=off|lk=on}} from Earth.
The proper motion of this star traces back to the Scorpius region of the Galactic Plane, about 20–25°
away. Gamma Arae has an optical companion located at an angular separation of 17.9 arcseconds, which is an A-type main sequence star with an apparent magnitude of 10.5.
Properties
This is a enormous star with 14 times the radius of the Sun. It is radiating 120,000 as much energy as the Sun from its outer envelope at an effective temperature of 21,240 K. This heat gives the star the blue-white glow of a B-type star. The spectrum shows it to match a stellar classification of B1 Ib, with the luminosity class of 'Ib' indicating this is a lower luminosity supergiant star. It is a relatively young body, with an estimated age of around 15.7 million years.
Gamma Arae is rotating rapidly with a projected rotational velocity of 269 km s−1, causing it to complete a full rotation about every 4.8 days. In the spectrum of this star, this high rate of spin is causing absorption lines to blend together because of the Doppler effect, making them more difficult to analyze. It is a periodically variable star that undergoes non-radial pulsations with a primary period of 1.1811 days and a secondary period of 0.1281 days.{{Dubious|Not a variable|date=April 2025}}
There is some disagreement about the mass of this star in the literature. Tetzlaff et al. (2011) estimate the mass as {{val|12.5|0.6}} solar masses, while Fraser et al. (2010) give a mass of around 19 and Lefever et al. (2007) lists a value of 25. It is shedding mass through its stellar wind at the rate of {{val|3.0|e=−8|u=solar masses per year}}, which is equivalent to losing the mass of the Sun every 33 million years. The wind is being affected by the star's rapid rotation, resulting in an enhanced outflow along the equator.
References
{{Reflist|refs=
| title=gam Ara
| access-date=2025-04-25
| postscript=. | mode = cs2 }}
{{citation | postscript=. | last=Evans | first=D. S. | date=June 20–24, 1966 | editor1-last=Batten | editor1-first=Alan Henry | editor2-last=Heard | editor2-first=John Frederick | contribution=The Revision of the General Catalogue of Radial Velocities | volume=30 | page=57 | title=Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30 | location=University of Toronto | publisher=International Astronomical Union | bibcode=1967IAUS...30...57E }}
{{citation | postscript=. | display-authors=1 | last1=Fraser | first1=M. | last2=Dufton | first2=P. L. | last3=Hunter | first3=I. | last4=Ryans | first4=R. S. I. | title=Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants | journal=Monthly Notices of the Royal Astronomical Society | volume=404 | issue=3 | pages=1306–1320 |date=May 2010 | doi=10.1111/j.1365-2966.2010.16392.x | doi-access=free | bibcode=2010MNRAS.404.1306F |arxiv = 1001.3337 | s2cid=118674151 }}
{{citation | postscript=. |title=The Colour of Stars |date=December 21, 2004 |work=Australia Telescope, Outreach and Education |publisher=Commonwealth Scientific and Industrial Research Organisation |url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html |access-date=2012-01-16 |url-status=dead |archive-url=https://web.archive.org/web/20120318151427/http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html |archive-date=2012-03-18 }}
| title=Stellar parameters and H α line profile variability of Be stars in the BeSOS survey
| last1=Arcos | first1=C. | last2=Kanaan | first2=S.
| last3=Chávez | first3=J. | last4=Vanzi | first4=L.
| last5=Araya | first5=I. | last6=Curé | first6=M.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=474 |issue=4 |pages=5287–5299
| display-authors=1 | date=January 3, 2018
| doi=10.1093/mnras/stx3075 | doi-access=free
| issn=0035-8711|arxiv=1711.08675 | bibcode=2018MNRAS.474.5287A }}
| title=Search for Galactic runaway stars using Gaia Data Release 1 and HIPPARCOS proper motions
| last1=Maíz Apellániz | first1=J. | last2=Pantaleoni González | first2=M.
| last3=Barbá | first3=R. H. | last4=Simón-Díaz | first4=S.
| last5=Negueruela | first5=I. | last6=Lennon | first6=D. J.
| last7=Sota | first7=A. | last8=Trigueros Páez | first8=E.
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=616 | id=A149 | pages=20 | date=August 2018
| arxiv=1804.06915 | bibcode=2018A&A...616A.149M
| doi=10.1051/0004-6361/201832787 | s2cid=55004808 }}
}}
External links
- [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%206462 HR 6462]
- [http://aladin.u-strasbg.fr/AladinPreview?-c=*+gam+Ara&ident=*+gam+Ara&submit=Aladin+previewer Image Gamma Arae]
{{Stars of Ara}}
{{DEFAULTSORT:Gamma Arae}}
Category:A-type main-sequence stars