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Epsilon Sagittae

Epsilon Sagittae (ε Sagittae) is a solitary,[7] yellow-hued star in the northern constellation of Sagitta. With an apparent visual magnitude of +5.64 to +5.67,[2] it is faintly visible to the naked eye on a dark night. It is a variable star with a small amplitude of 0.03 magnitudes. Based upon an annual parallax shift of 5.60 mas as seen from Earth,[8] it is located roughly 580 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.1 due to interstellar dust.[3]

Epsilon Sagittae
Location of ε Sagittae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Sagitta
Right ascension 19h 37m 17.39324s[1]
Declination +16° 27′ 46.0871″[1]
Apparent magnitude (V) +5.64 to +5.67[2]
Characteristics
Spectral type G8 IIIvar[3]
U−B color index +0.83[4]
B−V color index +1.00[4]
Astrometry
Radial velocity (Rv)−32.49±0.18[1] km/s
Proper motion (μ) RA: +16.382±0.164[1] mas/yr
Dec.: +14.364±0.135[1] mas/yr
Parallax (π)5.6067 ± 0.1173 mas[1]
Distance580 ± 10 ly
(178 ± 4 pc)
Absolute magnitude (MV)−0.84±0.03[1]
Details[5]
Mass3.09 M
Radius18.37+0.65
−0.88
[1] R
Luminosity184.9±4.6[1] L
Surface gravity (log g)2.44 cgs
Temperature4966+124
−85
[1] K
Metallicity [Fe/H]+0.03 dex
Rotational velocity (v sin i)3.2 km/s
Age331 Myr
Other designations
ε Sge, 4 Sge, BD+16°3918, HD 185194, HIP 96516, HR 7463, WDS J19373+1628A[6]
Database references
SIMBADdata

This is an evolved, G-type giant star with a stellar classification of G8 IIIvar,[3] where the 'var' suffix indicates a variable spectral feature. The star is about 331 million years old with three times the mass of the Sun.[5] It is radiating 185 times the Sun's luminosity from its photosphere at an effective temperature of 4,966 K.[1]

Epsilon Sagittae is an optical binary, with a companion of magnitude 8.35 at an angular separation of 87.3 arc seconds along a position angle of 82°, as of 2013.[9] The companion is actually a more distant giant star approximately 7,000 light-years from Earth, with a luminosity 1,800 times that of the Sun and also designated HD 232029.[10]

References Edit

  1. ^ a b c d e f g h i j k Brown, 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. Gaia DR2 record for this source at VizieR.
  2. ^ a b Details for NSV 12213, The International Variable Star Index, 17 December 2005, retrieved 14 September 2018
  3. ^ a b c Takeda, Yoichi; et al. (August 2008), "Stellar Parameters and Elemental Abundances of Late-G Giants", Publications of the Astronomical Society of Japan, 60 (4): 781–802, arXiv:0805.2434, Bibcode:2008PASJ...60..781T, doi:10.1093/pasj/60.4.781.
  4. ^ a b Argue, A. N. (1966), "UBV photometry of 550 F, G and K type stars", Monthly Notices of the Royal Astronomical Society, 133 (4): 475–493, Bibcode:1966MNRAS.133..475A, doi:10.1093/mnras/133.4.475.
  5. ^ a b Takeda, Yoichi; Tajitsu, Akito (2014), "Spectroscopic study on the beryllium abundances of red giant stars", Publications of the Astronomical Society of Japan, 66 (5): 91, arXiv:1406.7066, Bibcode:2014PASJ...66...91T, doi:10.1093/pasj/psu066.
  6. ^ "eps Sge". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-07-14.{{cite web}}: CS1 maint: postscript (link)
  7. ^ 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.
  8. ^ van Leeuwen, F. (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.
  9. ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode:2001AJ....122.3466M, doi:10.1086/323920.
  10. ^ Brown, 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. Gaia DR2 record for this source at VizieR.

epsilon, sagittae, sagittae, solitary, yellow, hued, star, northern, constellation, sagitta, with, apparent, visual, magnitude, faintly, visible, naked, dark, night, variable, star, with, small, amplitude, magnitudes, based, upon, annual, parallax, shift, seen. Epsilon Sagittae e Sagittae is a solitary 7 yellow hued star in the northern constellation of Sagitta With an apparent visual magnitude of 5 64 to 5 67 2 it is faintly visible to the naked eye on a dark night It is a variable star with a small amplitude of 0 03 magnitudes Based upon an annual parallax shift of 5 60 mas as seen from Earth 8 it is located roughly 580 light years from the Sun At that distance the visual magnitude of the star is diminished by an extinction factor of 0 1 due to interstellar dust 3 Epsilon SagittaeLocation of e Sagittae circled Observation dataEpoch J2000 0 Equinox J2000 0 ICRS Constellation SagittaRight ascension 19h 37m 17 39324s 1 Declination 16 27 46 0871 1 Apparent magnitude V 5 64 to 5 67 2 CharacteristicsSpectral type G8 IIIvar 3 U B color index 0 83 4 B V color index 1 00 4 AstrometryRadial velocity Rv 32 49 0 18 1 km sProper motion m RA 16 382 0 164 1 mas yr Dec 14 364 0 135 1 mas yrParallax p 5 6067 0 1173 mas 1 Distance580 10 ly 178 4 pc Absolute magnitude MV 0 84 0 03 1 Details 5 Mass3 09 M Radius18 37 0 65 0 88 1 R Luminosity184 9 4 6 1 L Surface gravity log g 2 44 cgsTemperature4966 124 85 1 KMetallicity Fe H 0 03 dexRotational velocity v sin i 3 2 km sAge331 MyrOther designationse Sge 4 Sge BD 16 3918 HD 185194 HIP 96516 HR 7463 WDS J19373 1628A 6 Database referencesSIMBADdataThis is an evolved G type giant star with a stellar classification of G8 IIIvar 3 where the var suffix indicates a variable spectral feature The star is about 331 million years old with three times the mass of the Sun 5 It is radiating 185 times the Sun s luminosity from its photosphere at an effective temperature of 4 966 K 1 Epsilon Sagittae is an optical binary with a companion of magnitude 8 35 at an angular separation of 87 3 arc seconds along a position angle of 82 as of 2013 9 The companion is actually a more distant giant star approximately 7 000 light years from Earth with a luminosity 1 800 times that of the Sun and also designated HD 232029 10 References Edit a b c d e f g h i j k Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b Details for NSV 12213 The International Variable Star Index 17 December 2005 retrieved 14 September 2018 a b c Takeda Yoichi et al August 2008 Stellar Parameters and Elemental Abundances of Late G Giants Publications of the Astronomical Society of Japan 60 4 781 802 arXiv 0805 2434 Bibcode 2008PASJ 60 781T doi 10 1093 pasj 60 4 781 a b Argue A N 1966 UBV photometry of 550 F G and K type stars Monthly Notices of the Royal Astronomical Society 133 4 475 493 Bibcode 1966MNRAS 133 475A doi 10 1093 mnras 133 4 475 a b Takeda Yoichi Tajitsu Akito 2014 Spectroscopic study on the beryllium abundances of red giant stars Publications of the Astronomical Society of Japan 66 5 91 arXiv 1406 7066 Bibcode 2014PASJ 66 91T doi 10 1093 pasj psu066 eps Sge SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2017 07 14 a href Template Cite web html title Template Cite web cite web a CS1 maint postscript link 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 van Leeuwen F 2007 Validation of the new Hipparcos reduction Astronomy and Astrophysics 474 2 653 664 arXiv 0708 1752 Bibcode 2007A amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 Mason B D et al 2014 The Washington Visual Double Star Catalog The Astronomical Journal 122 6 3466 Bibcode 2001AJ 122 3466M doi 10 1086 323920 Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR Retrieved from https en wikipedia org w index php title Epsilon Sagittae amp oldid 1154747740, wikipedia, wiki, book, books, library,

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