W Sagittarii
{{short description|Star in the constellation Sagittarius}}
{{about|γ1 Sagittarii|other stars with this Bayer designation|gamma Sagittarii{{!}}γ Sagittarii}}
{{Starbox begin
| name = W Sagittarii
}}
{{Starbox image
| image=
{{Location mark
|image=Sagittarius constellation map.svg|float=center
|alt=|label=|position=right|width=280
|mark=Red circle.svg|mark_width=10|mark_link=W Sagittarii
|x=668|y=524
}}
|caption=Location of W Sgr (circled)
}}
{{Starbox observe
| epoch = J2000
| dec = {{DEC|-29|34|48.3222}}
| appmag_v = {{nowrap|4.29 - 5.14}}
| constell = Sagittarius
}}
{{Starbox character
| component = Aa1
| variable = δ Cep{{cite journal|bibcode=2009yCat....102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}
}}
{{Starbox character|no_heading=y
| component = Aa2
| b-v =
| u-b =
| variable =
}}
{{Starbox character|no_heading=y
| component = Ab
}}
{{Starbox astrometry
| parallax = 2.365
| p_error = 0.1765
| parallax_footnote = {{cite Gaia EDR3|4050309195613114624}}
| dist_pc =
}}
{{Starbox orbit
| primary = Aa1
| name = Aa2
| period = {{val|4.33|0.01}}
| period_unitless =
| axis = 12.9 ± 0.3
| axis_unitless = 5.67 ± 0.13 AU
| eccentricity = 0.41 ± 0.02
| inclination = 7.0 ± 0.8
| node = 68.4 ± 4.0
| periastron = 2004.16 ± 0.01
| periarg = 328.0 ± 1.3
| k1 =
| k2 =
}}
{{Starbox orbit|no_heading=y
| primary = Aa
| name = Ab
| period = 172.9
| period_unitless =
| axis =
| axis_unitless = 63 AU
| eccentricity =
| inclination =
| node =
| periastron =
| periarg =
| periarg_primary =
| k1 =
| k2 =
}}
{{Starbox detail
| component1 = Aa
| rotational_velocity =
| component2 = Aa2
| radius2 =
| luminosity2 =
| temperature2=
| metal_fe2 =
| gravity2 =
| rotational_velocity2 =
| age_myr2 =
}}
{{Starbox detail|no_heading=y
| component1 = Ab
| radius =
| luminosity =
| temperature =
| metal_fe =
| gravity =
| rotational_velocity =
| age_myr =
}}
{{Starbox catalog
| names= γ1 Sgr, W Sagittarii, HR 6742, HD 164975, SAO 186237, HIP 88567, ADS 11029, CCDM 18050-2935
}}
{{Starbox reference
| Simbad=W+Sgr
}}
{{Starbox end}}
W Sagittarii (W Sgr, Gamma1 Sagittarii (γ1 Sgr)) is a multiple star system star in the constellation Sagittarius, and a Cepheid variable star.
W Sagittarii is an optical line-of-sight companion nearly a degree from the much brighter γ2 Sgr (Al Nasl) which marks the nozzle or spout of the teapot asterism.
System
W Sgr is listed as component A of a multiple star system catalogued as ADS 11029 and WDS J18050-2935. Components B and C are at 33" and 46" respectively and both are 13th magnitude. They are purely optical companions, not physically associated with W Sgr.{{cite journal|bibcode=2009AJ....137.3700E|arxiv=0902.3281|title=Massive Star Multiplicity: The Cepheid W Sgr|journal=The Astronomical Journal|volume=137|issue=3|pages=3700|last1=Evans|first1=Nancy Remage|last2=Massa|first2=Derck|last3=Proffitt|first3=Charles|year=2009|doi=10.1088/0004-6256/137/3/3700|s2cid=3112765}}
Component A, W Sgr, is itself a triple star system, with the components referred to as W Sgr Aa1, Aa2, and Ab.{{cite journal|bibcode= 2001AJ....122.3466M|title= The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog|journal= The Astronomical Journal|volume= 122|issue= 6|pages= 3466–3471|last1= Mason|first1= Brian D.|last2= Wycoff|first2= Gary L.|last3= Hartkopf|first3= William I.|last4= Douglass|first4= Geoffrey G.|last5= Worley|first5= Charles E.|year= 2001|doi= 10.1086/323920|doi-access= free}} These have also been referred to as components Aa, Ab, and B respectively. The outer companion Ab has been resolved at a separation of 0.14" and is over 5 magnitudes fainter than the primary supergiant. The inner components can only be identified spectroscopically by their radial velocity variations. The primary is a {{solar mass|6}} yellow supergiant, while the secondary is an early F main sequence star with a mass less than {{solar mass|1.4}}.
Variability
File:WSgrLightCurve.png for W Sagittarii, plotted from TESS data]]
The supergiant component W Sgr Aa1 is a variable star which pulsates regularly between magnitudes 4.3 and 5.1 every 7.59 days. During the pulsations, that temperature and spectral type also vary. It is classified as a Classical Cepheid (δ Cephei) variable.
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References
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{{Stars of Sagittarius}}
{{DEFAULTSORT:W Sagittarii}}
Category:Sagittarius (constellation)
Category:Classical Cepheid variables
Category:Spectroscopic binaries
Category:F-type main-sequence stars