From Wikipedia, the free encyclopedia
HD 32453
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Caelum
Right ascension 05h 01m 34.5225s [1]
Declination −39° 43′ 04.9641″ [1]
Apparent magnitude (V) 6.01±0.01 [2]
Characteristics
Spectral type G8 III [3]
B−V color index +0.88 [4]
Astrometry
Radial velocity (Rv)5.73±0.12 [1] km/s
Proper motion (μ) RA: −5.456 [1]  mas/ yr
Dec.: +32.717 [1]  mas/ yr
Parallax (π)8.0168 ± 0.0344  mas [1]
Distance407 ± 2  ly
(124.7 ± 0.5  pc)
Absolute magnitude (MV)+0.78 [5]
Details
Mass2.40 [6]  M
Radius10.03 [7] [8]  R
Luminosity50.1 [9]  L
Surface gravity (log g)3.18±0.14 [10]  cgs
Temperature5,032±61 [9]  K
Metallicity [Fe/H]−0.02±0.13 [10]  dex
Rotational velocity (v sin i)2±1.4 [11] km/s
Age700 [6]  Myr
Other designations
CD–39°1744, HD 32453, HIP 23377, HR 1631, SAO 195501
Database references
SIMBAD data

HD 32453 (HR 1631) is a solitary star located in the southern constellation Caelum. With an apparent magnitude of 6.01, [2] it's barely visible to the naked eye under ideal conditions. This star is located 407 light years away based on its parallax shift, but is drifting away at a rate of 5.73 km/s. [1]

HD 32453 has a classification of G8 III, [3] which states it is an evolved G-type star that exhausted hydrogen at its core and left the main sequence. At present it has 2.40 [6] times the Sun's mass, but at an age of 700 million years, [6] HD 32453 has expanded to 10 [7] times the latter's girth (radius detected from an angular diameter of 0.748 mas [8]). It radiates at 50 [9] solar luminosities from its enlarged photosphere at an effective temperature of 5,032 K, [9] which gives it a yellow hue. HD 32453 is slightly metal deficient, [10] and spins slowly with a projected rotational velocity of 2 km/s, [11] common for a giant star.

References

  1. ^ a b c d e f g 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 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H. ISSN  0004-6361.
  3. ^ a b Houk, N. (1 January 1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0. Bibcode: 1982mcts.book.....H.
  4. ^ Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1 January 1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode: 1966CoLPL...4...99J.
  5. ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. ISSN  1063-7737. S2CID  255204555.
  6. ^ a b c d Demarque, Pierre; Woo, Jong‐Hak; Kim, Yong‐Cheol; Yi, Sukyoung K. (December 2004). "Y 2 Isochrones with an Improved Core Overshoot Treatment". The Astrophysical Journal Supplement Series. 155 (2): 667–674. arXiv: astro-ph/0409024. Bibcode: 2004ApJS..155..667D. doi: 10.1086/424966. ISSN  1538-4357.
  7. ^ a b Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3 ed.), Birkhäuser, ISBN  3-540-29692-1. The radius (R*) is given by:
  8. ^ a b Stevens, Daniel J.; Stassun, Keivan G.; Gaudi, B. Scott (1 December 2017). "Empirical Bolometric Fluxes and Angular Diameters of 1.6 Million Tycho-2 Stars and Radii of 350,000 Stars with Gaia DR1 Parallaxes". The Astronomical Journal. 154 (6): 259. arXiv: 1708.05025. Bibcode: 2017AJ....154..259S. doi: 10.3847/1538-3881/aa957b. ISSN  0004-6256. S2CID  119191064.
  9. ^ a b c d Luck, R. Earle (25 August 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. ISSN  1538-3881.
  10. ^ a b c Alves, S.; Benamati, L.; Santos, N. C.; Adibekyan, V. Zh.; Sousa, S. G.; Israelian, G.; De Medeiros, J. R.; Lovis, C.; Udry, S. (11 April 2015). "Determination of the spectroscopic stellar parameters for 257 field giant stars★". Monthly Notices of the Royal Astronomical Society. 448 (3): 2749–2765. arXiv: 1503.02556. Bibcode: 2015MNRAS.448.2749A. doi: 10.1093/mnras/stv189. ISSN  1365-2966.
  11. ^ a b De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. ISSN  1432-0746.
From Wikipedia, the free encyclopedia
HD 32453
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Caelum
Right ascension 05h 01m 34.5225s [1]
Declination −39° 43′ 04.9641″ [1]
Apparent magnitude (V) 6.01±0.01 [2]
Characteristics
Spectral type G8 III [3]
B−V color index +0.88 [4]
Astrometry
Radial velocity (Rv)5.73±0.12 [1] km/s
Proper motion (μ) RA: −5.456 [1]  mas/ yr
Dec.: +32.717 [1]  mas/ yr
Parallax (π)8.0168 ± 0.0344  mas [1]
Distance407 ± 2  ly
(124.7 ± 0.5  pc)
Absolute magnitude (MV)+0.78 [5]
Details
Mass2.40 [6]  M
Radius10.03 [7] [8]  R
Luminosity50.1 [9]  L
Surface gravity (log g)3.18±0.14 [10]  cgs
Temperature5,032±61 [9]  K
Metallicity [Fe/H]−0.02±0.13 [10]  dex
Rotational velocity (v sin i)2±1.4 [11] km/s
Age700 [6]  Myr
Other designations
CD–39°1744, HD 32453, HIP 23377, HR 1631, SAO 195501
Database references
SIMBAD data

HD 32453 (HR 1631) is a solitary star located in the southern constellation Caelum. With an apparent magnitude of 6.01, [2] it's barely visible to the naked eye under ideal conditions. This star is located 407 light years away based on its parallax shift, but is drifting away at a rate of 5.73 km/s. [1]

HD 32453 has a classification of G8 III, [3] which states it is an evolved G-type star that exhausted hydrogen at its core and left the main sequence. At present it has 2.40 [6] times the Sun's mass, but at an age of 700 million years, [6] HD 32453 has expanded to 10 [7] times the latter's girth (radius detected from an angular diameter of 0.748 mas [8]). It radiates at 50 [9] solar luminosities from its enlarged photosphere at an effective temperature of 5,032 K, [9] which gives it a yellow hue. HD 32453 is slightly metal deficient, [10] and spins slowly with a projected rotational velocity of 2 km/s, [11] common for a giant star.

References

  1. ^ a b c d e f g 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 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H. ISSN  0004-6361.
  3. ^ a b Houk, N. (1 January 1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0. Bibcode: 1982mcts.book.....H.
  4. ^ Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1 January 1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode: 1966CoLPL...4...99J.
  5. ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. ISSN  1063-7737. S2CID  255204555.
  6. ^ a b c d Demarque, Pierre; Woo, Jong‐Hak; Kim, Yong‐Cheol; Yi, Sukyoung K. (December 2004). "Y 2 Isochrones with an Improved Core Overshoot Treatment". The Astrophysical Journal Supplement Series. 155 (2): 667–674. arXiv: astro-ph/0409024. Bibcode: 2004ApJS..155..667D. doi: 10.1086/424966. ISSN  1538-4357.
  7. ^ a b Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3 ed.), Birkhäuser, ISBN  3-540-29692-1. The radius (R*) is given by:
  8. ^ a b Stevens, Daniel J.; Stassun, Keivan G.; Gaudi, B. Scott (1 December 2017). "Empirical Bolometric Fluxes and Angular Diameters of 1.6 Million Tycho-2 Stars and Radii of 350,000 Stars with Gaia DR1 Parallaxes". The Astronomical Journal. 154 (6): 259. arXiv: 1708.05025. Bibcode: 2017AJ....154..259S. doi: 10.3847/1538-3881/aa957b. ISSN  0004-6256. S2CID  119191064.
  9. ^ a b c d Luck, R. Earle (25 August 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. ISSN  1538-3881.
  10. ^ a b c Alves, S.; Benamati, L.; Santos, N. C.; Adibekyan, V. Zh.; Sousa, S. G.; Israelian, G.; De Medeiros, J. R.; Lovis, C.; Udry, S. (11 April 2015). "Determination of the spectroscopic stellar parameters for 257 field giant stars★". Monthly Notices of the Royal Astronomical Society. 448 (3): 2749–2765. arXiv: 1503.02556. Bibcode: 2015MNRAS.448.2749A. doi: 10.1093/mnras/stv189. ISSN  1365-2966.
  11. ^ a b De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. ISSN  1432-0746.

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