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词条 Gamma Sagittae
释义

  1. Naming

  2. References

  3. External links

{{Starbox begin
| name = γ Sagittae
}}{{Starbox image
| image={{Location mark
|image=Sagitta constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=12|mark_link=γ Sge
|x=284|y=218
}}
|caption=Location of γ Sagittae (circled)
}}{{Starbox observe
| epoch = J2000.0
| equinox = J2000.0 (ICRS)
| constell = Sagitta
| ra = {{RA|19|58|45.42863}}[1]
| dec = {{DEC|+19|29|31.7281}}[1]
| appmag_v = +3.47[3]
}}{{Starbox character
| type = Red Giant
| class = M0 III[5][6]
| b-v = +1.57[3]
| u-b = +1.93[3]
}}{{Starbox astrometry
| radial_v = {{Val|−34.0|0.2}}[9]
| prop_mo_ra = {{Val|66.21|0.14}}[1]
| prop_mo_dec = {{Val|22.22|0.12}}[1]
| parallax = 12.62
| p_error = 0.18
| parallax_footnote = [1]
| absmag_v = −1.11[13]
}}{{Starbox detail
| mass = 1.37[14]
| radius = {{Val|55.13|3.29}}[15]
| luminosity_bolometric = {{Val|562|75}}[15]
| temperature = {{Val|3862|40|fmt=commas}}[5]
| metal_fe = −0.14[15]
| gravity = 1.71[19]
| rotation =
| age_gyr = 2.35[5]
}}{{Starbox catalog
| names = {{odlist | B=β Sge | F=12 Sagittae | BD=+19° 4229 | FK5=752 | HD=189319 | HIP=98337 | HR=7635 | SAO=105500 | GC=27672 | PPM=137344 }}
}}{{Starbox reference
| Simbad = Gamma+Sge
}}{{Starbox end}}Gamma Sagittae, Latinized from γ Sagittae, is the brightest star in northern constellation of Sagitta. A single star,[21] it is visible to the naked eye with an apparent visual magnitude of +3.47.[3] Based upon an annual parallax shift of 12.62 mas as seen from Earth, it is located about 258 light years from the Sun. It is moving closer to the Sun with a radial velocity of −34 km/s.[9]

This is an evolved red giant star with a stellar classification of M0 III.[24] It is around 2.35[5] billion years old with an estimated 1.37[14] times the mass of the Sun and roughly 55[15] times the Sun's radius. The star is radiating about 562[15] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,862 K.[5]

Naming

In Chinese, {{lang|zh|左旗}} ({{lang|zh-Latn|Zuǒ Qí}}), meaning Left Flag, refers to an asterism consisting of γ Sagittae, α Sagittae, β Sagittae, δ Sagittae, ζ Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and ρ Aquilae. Consequently, γ Sagittae itself is known as {{lang|zh|左旗五}} ({{lang|zh-Latn|Zuǒ Qí wǔ}}, {{lang-en|the Fifth Star of Left Flag}}.)[1]

References

1. ^{{zh icon}} AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 3 日
2. ^{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E | arxiv=0806.2878 | postscript=. }}
3. ^{{citation | title=Tests of stellar model atmospheres by optical interferometry. III. NPOI and VINCI interferometry of the M0 giant γ Sagittae covering 0.5-2.2 μm | last1=Wittkowski | first1=M. | last2=Hummel | first2=C. A. | last3=Aufdenberg | first3=J. P. | last4=Roccatagliata | first4=V. | journal=Astronomy and Astrophysics | volume=460 | issue=3 | date=December 2006 | pages=843–853 | doi=10.1051/0004-6361:20065853 | bibcode=2006A&A...460..843W | arxiv=astro-ph/0610149 | postscript=. }}
4. ^{{citation | title=Precise radial velocity measurements of G and K giants. Multiple systems and variability trend along the Red Giant Branch | last1=Setiawan | first1=J. | last2=Pasquini | first2=L. | last3=da Silva | first3=L. | last4=Hatzes | first4=A. P. | last5=von der Lühe | first5=O. | last6=Girardi | first6=L. | last7=de Medeiros | first7=J. R. | last8=Guenther | first8=E. | journal=Astronomy and Astrophysics | volume=421 | pages=241–254 | date=July 2004 | doi=10.1051/0004-6361:20041042-1 | bibcode=2004A&A...421..241S | display-authors=1 | postscript=. }}
5. ^{{cite journal | title=Abundances in the Local Region. I. G and K Giants | last1=Luck | first1=R. Earle | journal=Astronomical Journal | volume=150 | issue=3 | at=88 | year=2015 | bibcode=2015AJ....150...88L | doi=10.1088/0004-6256/150/3/88 | arxiv=1507.01466 }}
6. ^{{cite journal | first=F. | last=van Leeuwen | title=Validation of the New Hipparcos Reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–64 | date=2007 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | arxiv=0708.1752}}
7. ^{{cite journal|author1=Piau, L. |author2=Kervella, P. |author3=Dib, S. |author4=Hauschildt, P. |date=2011|title=Surface convection and red-giant radius measurements|journal=Astronomy and Astrophysics|volume=526|id=A100|pages=12|doi=10.1051/0004-6361/201014442 |bibcode=2011A&A...526A.100P|arxiv = 1010.3649 }}
8. ^{{cite journal|bibcode=2014yCat....1.2023S|title=VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2016)|journal=VizieR On-line Data Catalog: B/mk. Originally published in: Lowell Observatory (October 2014)|volume=1|author1=Skiff|first1=B. A.|year=2014}}
9. ^{{cite journal|bibcode=2005A&A...430..165F|title=Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters|journal=Astronomy and Astrophysics|volume=430|pages=165|author1=Famaey|first1=B.|last2=Jorissen|first2=A.|last3=Luri|first3=X.|last4=Mayor|first4=M.|last5=Udry|first5=S.|last6=Dejonghe|first6=H.|last7=Turon|first7=C.|year=2005|doi=10.1051/0004-6361:20041272|arxiv = astro-ph/0409579 }}
10. ^{{cite journal|bibcode=2002yCat.2237....0D |title=VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system |journal=CDS/ADC Collection of Electronic Catalogues |volume=2237 |author1=Ducati |first1=J. R. |year=2002 }}
11. ^{{cite journal|bibcode=2016A&A...593A.133B|title=New spectroscopic binary companions of giant stars and updated metallicity distribution for binary systems|journal=Astronomy & Astrophysics|volume=593|pages=A133|author1=Bluhm|first1=P.|last2=Jones|first2=M. I.|last3=Vanzi|first3=L.|last4=Soto|first4=M. G.|last5=Vos|first5=J.|last6=Wittenmyer|first6=R. A.|last7=Drass|first7=H.|last8=Jenkins|first8=J. S.|last9=Olivares|first9=F.|last10=Mennickent|first10=R. E.|last11=Vučković|first11=M.|last12=Rojo|first12=P.|last13=Melo|first13=C. H. F.|year=2016|doi=10.1051/0004-6361/201628459|arxiv = 1608.08260 }}
12. ^{{cite journal|bibcode=2015A&A...574A.116R|title=Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity|journal=Astronomy & Astrophysics|volume=574|pages=A116|author1=Reffert|first1=Sabine|last2=Bergmann|first2=Christoph|last3=Quirrenbach|first3=Andreas|last4=Trifonov|first4=Trifon|last5=Künstler|first5=Andreas|year=2015|doi=10.1051/0004-6361/201322360|arxiv = 1412.4634 |hdl=10722/215277}}
[2][3][4][5][6][7][8][9][10][11][12]
}}

External links

  • {{cite web

| first1=James B. | last1=Kaler | work=STARS
| title=GAMMA SGE (Gamma Sagittae)
| publisher=University of Illinois
| url=http://stars.astro.illinois.edu/sow/gammasge.html
| accessdate=2017-11-30 }}{{Stars of Sagitta}}

9 : M-type giants|Suspected variables|Bayer objects|Sagitta (constellation)|Durchmusterung objects|Flamsteed objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects

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