Astronomy:HD 46568

From HandWiki
Short description: Star in the constellation of Columba
HD 46568
Observation data
Epoch J2000.0   Equinox (celestial coordinates)
Constellation Columba
Right ascension  06h 32m 21.3775s[1]
Declination −37° 41′ 48.2053″[1]
Apparent magnitude (V) 5.25±0.01[2]
Characteristics
Spectral type G8 III[3]
U−B color index +0.75[4]
B−V color index +0.98[5]
Astrometry
Radial velocity (Rv)39±1[6] km/s
Proper motion (μ) RA: +73.075[1] mas/yr
Dec.: −75.599[1] mas/yr
Parallax (π)11.4692 ± 0.0782[1] mas
Distance284 ± 2 ly
(87.2 ± 0.6 pc)
Absolute magnitude (MV)+0.64[7]
Details[8]
Mass1.94±0.11 M☉
Radius10.66±0.18 R☉
Luminosity60.7±1.4 L☉
Surface gravity (log g)2.69±0.07 cgs
Temperature4,935±29 K
Metallicity [Fe/H]−0.16±0.02 dex
Rotational velocity (v sin i)1.2±1.2[9] km/s
Age1.68[10] Gyr
Other designations
CD−37°2889, CPD−37°964, GC 8514, HD 46568, HIP 31165, HR 2399, SAO 196917[11][12]
Database references
SIMBADdata

HD 46568 (HR 2399) is a solitary[13] star in the southern constellation Columba. It is faintly visible to the naked eye with an apparent magnitude of 5.25.[2] Parallax measurements place the object at a distance of 284 light years[1] and is currently receding with a heliocentric radial velocity of 39 km/s.[6]

HD 46568 has a stellar classification of G8 III, indicating that it is a yellow giant. At present it has nearly twice the mass of the Sun[8] but at an age of 1.68 billion years[10] it has expanded to 10.66 times the radius of the Sun.[8] It has an effective temperature of 4,935 K,[8] giving it a yellow glow. However, the star's large radius yields a luminosity 60 times that of Sun.[8] HD 46568's metallicity is 69% that of the Sun[8] and it spins with a poorly constrained projected rotational velocity of 1.2 km/s.[9]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  2. ↑ 2.0 2.1 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H. 
  3. ↑ Houk, N. (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. ↑ Paunzen, E. (May 2022). "Catalogue of stars measured in the Geneva seven-colour photometric system". Astronomy & Astrophysics 661: A89. doi:10.1051/0004-6361/202142355. ISSN 0004-6361. Bibcode: 2022A&A...661A..89P. 
  5. ↑ Stoy, R. H. (1968). "Photoelectric Magnitudes and Colours for Bright Southern Stars". Monthly Notes of the Astronomical Society of South Africa 27: 119. ISSN 0024-8266. Bibcode: 1968MNSSA..27..119S. 
  6. ↑ 6.0 6.1 Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. ISSN 1063-7737. Bibcode: 2006AstL...32..759G. 
  7. ↑ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation" (in en). Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode: 2012AstL...38..331A. 
  8. ↑ 8.0 8.1 8.2 8.3 8.4 8.5 Ottoni, G.; Udry, S.; Ségransan, D.; Buldgen, G.; Lovis, C.; Eggenberger, P.; Pezzotti, C.; Adibekyan, V. et al. (January 2022). "CORALIE radial-velocity search for companions around evolved stars (CASCADES): I. Sample definition and first results: Three new planets orbiting giant stars". Astronomy & Astrophysics 657: A87. doi:10.1051/0004-6361/202040078. ISSN 0004-6361. Bibcode: 2022A&A...657A..87O. 
  9. ↑ 9.0 9.1 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. doi:10.1051/0004-6361/201220762. ISSN 0004-6361. Bibcode: 2014A&A...561A.126D. 
  10. ↑ 10.0 10.1 Gomes da Silva, J.; Santos, N. C.; Adibekyan, V.; Sousa, S. G.; Campante, T. L.; Figueira, P.; Bossini, D.; Delgado-Mena, E. et al. (February 2021). "Stellar chromospheric activity of 1674 FGK stars from the AMBRE-HARPS sample". Astronomy & Astrophysics 646: A77. doi:10.1051/0004-6361/202039765. ISSN 0004-6361. Bibcode: 2021A&A...646A..77G. 
  11. ↑ "HD 46568". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+46568. 
  12. ↑ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino 1. Bibcode: 1879RNAO....1.....G. 
  13. ↑ Eggleton, P. P.; Tokovinin, A. A. (11 September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society 389 (2): 869–879. doi:10.1111/j.1365-2966.2008.13596.x. ISSN 0035-8711. Bibcode: 2008MNRAS.389..869E. 



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:HD_46568&oldid=3670774"