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33+pegasi Latitude and Longitude:
Sky map 22h 23m 39.564s, +20° 50′ 53.62″
From Wikipedia, the free encyclopedia
33 Pegasi
Observation data
Epoch J2000       Equinox J2000
Constellation Pegasus
Right ascension 22h 23m 39.565s [1]
Declination 20° 50′ 53.84″ [1]
Apparent magnitude (V) 6.203 [2] (6.391 + 9.287) [3]
Characteristics
Spectral type F7 V [4]
B−V color index 0.518±0.004 [5]
Astrometry
Radial velocity (Rv)23.8±0.4 [2] km/s
Proper motion (μ) RA: +333.057  mas/ yr [1]
Dec.: −10.827  mas/ yr [1]
Parallax (π)29.8125 ± 0.0436  mas [1]
Distance109.4 ± 0.2  ly
(33.54 ± 0.05  pc)
Absolute magnitude (MV)3.55 [2]
Details
33 Peg A
Mass1.28 [6]  M☉
Radius1.29+0.15
−0.14 [7]  R☉
Luminosity2.850+0.007
−0.008 [7]  L☉
Surface gravity (log g)4.29 [8]  cgs
Temperature6,169 [9]  K
Metallicity [Fe/H]–0.18 [9]  dex
Rotational velocity (v sin i)6 [2] km/s
Age4.1 [9]  Gyr
33 Peg B
Mass0.80 [6]  M☉
Other designations
33 Peg, BD–16 4196, HD 212395, HIP 110548, HR 8532, SAO 90462 [10]
Database references
SIMBAD data

33 Pegasi is the Flamsteed designation for a visual binary star in the northern constellation of Pegasus. It has an apparent visual magnitude of 6.2, [2] placing it near the limit of naked eye visibility. Measurements show an annual parallax shift of 0.0298125 ″, [1] which is equivalent to a distance of 109 ly (33 pc) from the Sun. It is drifting further away with a radial velocity of 24 km/s. [2]

The primary component of this system is a main sequence star with a visual magnitude of 6.4 [3] and a stellar classification of F7 V. [4] It is nearly as old as the Sun with an estimated age of 4.1 billion years, but has a lower abundance of elements other than hydrogen and helium. The star has 1.3 times the mass [6] and radius [7] of the Sun. The stellar atmosphere has an effective temperature of 6,169 K, [9] giving it the yellow-white glow of an F-type star. [11]

A faint, magnitude 9.3 companion star is located at an angular separation of 0.420  arc seconds along a position angle of 0.0°. [3] The pair have a projected separation of 15.6  AU [6] with an orbital period of about 250 years. [12]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b c d e f Nordström, B.; et al. (May 2004), "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs", Astronomy and Astrophysics, 418: 989–1019, arXiv: astro-ph/0405198, Bibcode: 2004A&A...418..989N, doi: 10.1051/0004-6361:20035959, S2CID  11027621.
  3. ^ a b c Fabricius, C.; Makarov, V. V. (April 2000), "Two-colour photometry for 9473 components of close Hipparcos double and multiple stars", Astronomy and Astrophysics, 356: 141–145, Bibcode: 2000A&A...356..141F.
  4. ^ a b Harlan, E. A.; Taylor, D. C. (March 1970), "MK classification for F- and G-type stars. II", Astronomical Journal, 75 (2): 165–166, Bibcode: 1970AJ.....75..165H, doi: 10.1086/110956.
  5. ^ 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.
  6. ^ a b c d Tokovinin, A.; Kiyaeva, O. (2015), "Eccentricity distribution of wide binaries", Monthly Notices of the Royal Astronomical Society, 456 (2): 2070, arXiv: 1512.00278, Bibcode: 2016MNRAS.456.2070T, doi: 10.1093/mnras/stv2825, S2CID  1615080.
  7. ^ a b c 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.
  8. ^ Boesgaard, Ann Merchant; et al. (2004), "The Correlation of Lithium and Beryllium in F and G Field and Cluster Dwarf Stars", The Astrophysical Journal, 613 (2): 1202–1212, Bibcode: 2004ApJ...613.1202B, doi: 10.1086/423194.
  9. ^ a b c d Casagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics, 530: A138, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID  56118016.
  10. ^ "* 33 Peg". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-12-31.
  11. ^ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the original on March 18, 2012, retrieved 2012-01-16.
  12. ^ Tokovinin, Andrei (April 2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal, 147 (4): 14, arXiv: 1401.6827, Bibcode: 2014AJ....147...87T, doi: 10.1088/0004-6256/147/4/87, S2CID  56066740, 87.
Retrieved from " https://en.wikipedia.org/?title=33_Pegasi&oldid=1235339252"

33+pegasi Latitude and Longitude:
Sky map 22h 23m 39.564s, +20° 50′ 53.62″
From Wikipedia, the free encyclopedia
33 Pegasi
Observation data
Epoch J2000       Equinox J2000
Constellation Pegasus
Right ascension 22h 23m 39.565s [1]
Declination 20° 50′ 53.84″ [1]
Apparent magnitude (V) 6.203 [2] (6.391 + 9.287) [3]
Characteristics
Spectral type F7 V [4]
B−V color index 0.518±0.004 [5]
Astrometry
Radial velocity (Rv)23.8±0.4 [2] km/s
Proper motion (μ) RA: +333.057  mas/ yr [1]
Dec.: −10.827  mas/ yr [1]
Parallax (π)29.8125 ± 0.0436  mas [1]
Distance109.4 ± 0.2  ly
(33.54 ± 0.05  pc)
Absolute magnitude (MV)3.55 [2]
Details
33 Peg A
Mass1.28 [6]  M☉
Radius1.29+0.15
−0.14 [7]  R☉
Luminosity2.850+0.007
−0.008 [7]  L☉
Surface gravity (log g)4.29 [8]  cgs
Temperature6,169 [9]  K
Metallicity [Fe/H]–0.18 [9]  dex
Rotational velocity (v sin i)6 [2] km/s
Age4.1 [9]  Gyr
33 Peg B
Mass0.80 [6]  M☉
Other designations
33 Peg, BD–16 4196, HD 212395, HIP 110548, HR 8532, SAO 90462 [10]
Database references
SIMBAD data

33 Pegasi is the Flamsteed designation for a visual binary star in the northern constellation of Pegasus. It has an apparent visual magnitude of 6.2, [2] placing it near the limit of naked eye visibility. Measurements show an annual parallax shift of 0.0298125 ″, [1] which is equivalent to a distance of 109 ly (33 pc) from the Sun. It is drifting further away with a radial velocity of 24 km/s. [2]

The primary component of this system is a main sequence star with a visual magnitude of 6.4 [3] and a stellar classification of F7 V. [4] It is nearly as old as the Sun with an estimated age of 4.1 billion years, but has a lower abundance of elements other than hydrogen and helium. The star has 1.3 times the mass [6] and radius [7] of the Sun. The stellar atmosphere has an effective temperature of 6,169 K, [9] giving it the yellow-white glow of an F-type star. [11]

A faint, magnitude 9.3 companion star is located at an angular separation of 0.420  arc seconds along a position angle of 0.0°. [3] The pair have a projected separation of 15.6  AU [6] with an orbital period of about 250 years. [12]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b c d e f Nordström, B.; et al. (May 2004), "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs", Astronomy and Astrophysics, 418: 989–1019, arXiv: astro-ph/0405198, Bibcode: 2004A&A...418..989N, doi: 10.1051/0004-6361:20035959, S2CID  11027621.
  3. ^ a b c Fabricius, C.; Makarov, V. V. (April 2000), "Two-colour photometry for 9473 components of close Hipparcos double and multiple stars", Astronomy and Astrophysics, 356: 141–145, Bibcode: 2000A&A...356..141F.
  4. ^ a b Harlan, E. A.; Taylor, D. C. (March 1970), "MK classification for F- and G-type stars. II", Astronomical Journal, 75 (2): 165–166, Bibcode: 1970AJ.....75..165H, doi: 10.1086/110956.
  5. ^ 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.
  6. ^ a b c d Tokovinin, A.; Kiyaeva, O. (2015), "Eccentricity distribution of wide binaries", Monthly Notices of the Royal Astronomical Society, 456 (2): 2070, arXiv: 1512.00278, Bibcode: 2016MNRAS.456.2070T, doi: 10.1093/mnras/stv2825, S2CID  1615080.
  7. ^ a b c 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.
  8. ^ Boesgaard, Ann Merchant; et al. (2004), "The Correlation of Lithium and Beryllium in F and G Field and Cluster Dwarf Stars", The Astrophysical Journal, 613 (2): 1202–1212, Bibcode: 2004ApJ...613.1202B, doi: 10.1086/423194.
  9. ^ a b c d Casagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics, 530: A138, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID  56118016.
  10. ^ "* 33 Peg". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-12-31.
  11. ^ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the original on March 18, 2012, retrieved 2012-01-16.
  12. ^ Tokovinin, Andrei (April 2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal, 147 (4): 14, arXiv: 1401.6827, Bibcode: 2014AJ....147...87T, doi: 10.1088/0004-6256/147/4/87, S2CID  56066740, 87.
Retrieved from " https://en.wikipedia.org/?title=33_Pegasi&oldid=1235339252"

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