From Wikipedia, the free encyclopedia
(Redirected from Ι Sagittarii)
ι Sagittarii
Location of ι Sagittarii (circled)
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Sagittarius
Right ascension 19h 55m 15.69691s [1]
Declination −41° 52′ 05.8388″ [1]
Apparent magnitude (V) +4.118 [2]
Characteristics
Spectral type K0 II-III [3]
U−B color index +0.911 [2]
B−V color index +1.084 [2]
Astrometry
Radial velocity (Rv)+35.8 [3] km/s
Proper motion (μ) RA: +22.61 [1]  mas/ yr
Dec.: +51.40 [1]  mas/ yr
Parallax (π)17.94 ± 0.21  mas [1]
Distance182 ± 2  ly
(55.7 ± 0.7  pc)
Absolute magnitude (MV)+0.39 [4]
Details
Mass1.40 [3]  M
Radius14 [5]  R
Luminosity87 [3]  L
Surface gravity (log g)1.89 [6]  cgs
Temperature4,594±41 [3]  K
Metallicity [Fe/H]−0.26 [6]  dex
Age4.74 [3]  Gyr
Other designations
ι Sgr, CPD−42° 8944, FK5 1520, HD 188114, HIP 98032, HR 7581, SAO 229927 [7]
Database references
SIMBAD data

Iota Sagittarii (Iota Sgr, ι Sagittarii, ι Sgr) is a star in the zodiac constellation of Sagittarius. With an apparent visual magnitude of +4.118, it is bright enough to be viewed with the naked eye. [2] Based upon an annual parallax shift of 17.94  mas as seen from Earth, [1] this star is located 182  light years from the Sun. It is moving away from the Earth with a radial velocity of +35.8 km/s. [3]

This is a probable astrometric binary, [8] based upon proper motion data collected during the Hipparcos mission. [9] The visible component shows the spectrum of an evolved K-type giant or bright giant star with a stellar classification of K0 II-III. [3] The measured angular diameter, after correction for limb darkening, is 2.32±0.02  mas. [10] At an estimated distance of this star, this yields a physical size of about 14 times the radius of the Sun. [5] It has 1.4 [3] times the mass of the Sun and is radiating 87 [3] times the Sun's luminosity from its photosphere at an effective temperature of about 4,594 K. [3]

References

  1. ^ a b c d e f 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.
  2. ^ a b c d Cousins, A. W. J. (1973), "Revised zero points and UBV photometry of stars in the Harvard E and F regions", Memoirs of the Royal Astronomical Society, 77: 223–236, Bibcode: 1973MmRAS..77..223C.
  3. ^ a b c d e f g h i j k Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal, 150 (3): 88, arXiv: 1507.01466, Bibcode: 2015AJ....150...88L, doi: 10.1088/0004-6256/150/3/88, S2CID  118505114.
  4. ^ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID  119257644.
  5. ^ a b Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN  3-540-29692-1. The radius (R*) is given by:
  6. ^ a b Soubiran, C.; Le Campion, J.-F.; Cayrel de Strobel, G.; Caillo, A. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, arXiv: 1004.1069, Bibcode: 2010A&A...515A.111S, doi: 10.1051/0004-6361/201014247, S2CID  118362423.
  7. ^ "iot Sgr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-07-07.
  8. ^ 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.
  9. ^ Frankowski, A.; et al. (March 2007), "Proper-motion binaries in the Hipparcos catalogue. Comparison with radial velocity data", Astronomy and Astrophysics, 464 (1): 377–392, arXiv: astro-ph/0612449, Bibcode: 2007A&A...464..377F, doi: 10.1051/0004-6361:20065526, S2CID  14010423.
  10. ^ Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode: 2005A&A...431..773R, doi: 10.1051/0004-6361:20042039.
From Wikipedia, the free encyclopedia
(Redirected from Ι Sagittarii)
ι Sagittarii
Location of ι Sagittarii (circled)
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Sagittarius
Right ascension 19h 55m 15.69691s [1]
Declination −41° 52′ 05.8388″ [1]
Apparent magnitude (V) +4.118 [2]
Characteristics
Spectral type K0 II-III [3]
U−B color index +0.911 [2]
B−V color index +1.084 [2]
Astrometry
Radial velocity (Rv)+35.8 [3] km/s
Proper motion (μ) RA: +22.61 [1]  mas/ yr
Dec.: +51.40 [1]  mas/ yr
Parallax (π)17.94 ± 0.21  mas [1]
Distance182 ± 2  ly
(55.7 ± 0.7  pc)
Absolute magnitude (MV)+0.39 [4]
Details
Mass1.40 [3]  M
Radius14 [5]  R
Luminosity87 [3]  L
Surface gravity (log g)1.89 [6]  cgs
Temperature4,594±41 [3]  K
Metallicity [Fe/H]−0.26 [6]  dex
Age4.74 [3]  Gyr
Other designations
ι Sgr, CPD−42° 8944, FK5 1520, HD 188114, HIP 98032, HR 7581, SAO 229927 [7]
Database references
SIMBAD data

Iota Sagittarii (Iota Sgr, ι Sagittarii, ι Sgr) is a star in the zodiac constellation of Sagittarius. With an apparent visual magnitude of +4.118, it is bright enough to be viewed with the naked eye. [2] Based upon an annual parallax shift of 17.94  mas as seen from Earth, [1] this star is located 182  light years from the Sun. It is moving away from the Earth with a radial velocity of +35.8 km/s. [3]

This is a probable astrometric binary, [8] based upon proper motion data collected during the Hipparcos mission. [9] The visible component shows the spectrum of an evolved K-type giant or bright giant star with a stellar classification of K0 II-III. [3] The measured angular diameter, after correction for limb darkening, is 2.32±0.02  mas. [10] At an estimated distance of this star, this yields a physical size of about 14 times the radius of the Sun. [5] It has 1.4 [3] times the mass of the Sun and is radiating 87 [3] times the Sun's luminosity from its photosphere at an effective temperature of about 4,594 K. [3]

References

  1. ^ a b c d e f 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.
  2. ^ a b c d Cousins, A. W. J. (1973), "Revised zero points and UBV photometry of stars in the Harvard E and F regions", Memoirs of the Royal Astronomical Society, 77: 223–236, Bibcode: 1973MmRAS..77..223C.
  3. ^ a b c d e f g h i j k Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal, 150 (3): 88, arXiv: 1507.01466, Bibcode: 2015AJ....150...88L, doi: 10.1088/0004-6256/150/3/88, S2CID  118505114.
  4. ^ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID  119257644.
  5. ^ a b Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN  3-540-29692-1. The radius (R*) is given by:
  6. ^ a b Soubiran, C.; Le Campion, J.-F.; Cayrel de Strobel, G.; Caillo, A. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, arXiv: 1004.1069, Bibcode: 2010A&A...515A.111S, doi: 10.1051/0004-6361/201014247, S2CID  118362423.
  7. ^ "iot Sgr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-07-07.
  8. ^ 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.
  9. ^ Frankowski, A.; et al. (March 2007), "Proper-motion binaries in the Hipparcos catalogue. Comparison with radial velocity data", Astronomy and Astrophysics, 464 (1): 377–392, arXiv: astro-ph/0612449, Bibcode: 2007A&A...464..377F, doi: 10.1051/0004-6361:20065526, S2CID  14010423.
  10. ^ Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode: 2005A&A...431..773R, doi: 10.1051/0004-6361:20042039.

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