HD 45866

Last updated
HD 45866
Camelopardalis constellation map.svg
Red circle.svg
Location of HD 45866 on the map (circled)
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Camelopardalis [1]
Right ascension 06h 40m 28.87701s [2]
Declination +77° 59 44.8179 [2]
Apparent magnitude  (V)5.72±0.01 [3]
Characteristics
Spectral type K5 III [4]
B−V color index +1.47 [5]
Astrometry
Radial velocity (Rv)−16.6±0.2 [6] km/s
Proper motion (μ)RA: +13.997 mas/yr [2]
Dec.: −5.701 mas/yr [2]
Parallax (π)4.4952±0.0455  mas [2]
Distance 726 ± 7  ly
(222 ± 2  pc)
Absolute magnitude  (MV)−0.89 [1]
Details
Mass 2.34±0.69 [7]   M
Radius 49.6±2.6 [8]   R
Luminosity 468±8 [2]   L
Surface gravity (log g)1.62±0.11 [7]   cgs
Temperature 4,207±140 [9]   K
Metallicity [Fe/H]−0.11±0.01 [10]   dex
Age 1.15+0.51
0.35
[7]   Gyr
Other designations
AG+78°144, BD+78°227, FK5 2507, GC 8574, HD 45866, HIP 31940, HR 2363, SAO 5919 [11]
Database references
SIMBAD data

HD 45866, also known as HR 2363 is a solitary star [12] located in the northern circumpolar constellation Camelopardalis. It is faintly visible to the naked eye as an orange-hued star with an apparent magnitude of 5.72. [3] Gaia DR3 parallax measurements place it 726 light years away and it is currently approaching the Solar System with a heliocentric radial velocity of −16.6  km/s . [6] At its current distance, HD 45866's brightness is diminished by 0.26 magnitudes due to interstellar dust. [13] It has an absolute magnitude of −0.89 [1]

This is an evolved red giant with a stellar classification of K5 III. [4] It has 2.34 times the mass of the Sun [7] but it has expanded to nearly 50 times the radius of the Sun [8] at an age of 1.15 billion years. [7] It radiates 468 times the luminosity of the Sun [2] from its photosphere at an effective temperature of 4,207  K . [9] It has an iron abundance 78% of the Sun's, [10] making it slightly metal deficient.

References

  1. 1 2 3 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. XHIP record for this object at VizieR.
  2. 1 2 3 4 5 6 7 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211 . Bibcode:2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940 . S2CID   244398875. Gaia DR3 record for this source at VizieR.
  3. 1 2 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.
  4. 1 2 Adams, Walter S.; Joy, Alfred H.; Humason, Milton L.; Brayton, Ada Margaret (April 1935). "The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars". The Astrophysical Journal. 81: 187. Bibcode:1935ApJ....81..187A. doi: 10.1086/143628 . eISSN   1538-4357. ISSN   0004-637X.
  5. Haggkvist, L.; Oja, T. (1970). "Results of BV photometry 1969-70 (Uppsala refractor)". Private Communication. Bibcode:1970Priv.........0H.
  6. 1 2 Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (January 2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters". Astronomy and Astrophysics. 430: 165. arXiv: astro-ph/0409579 . Bibcode:2005A&A...430..165F. doi: 10.1051/0004-6361:20041272 . eISSN   1432-0746. ISSN   0004-6361. S2CID   17804304.
  7. 1 2 3 4 5 Feuillet, Diane K.; Bovy, Jo; Holtzman, Jon; Girardi, Léo; MacDonald, Nick; Majewski, Steven R.; Nidever, David L. (20 January 2016). "Determining Ages of APOGEE Giants with Known Distances". The Astrophysical Journal. 817 (1): 40. arXiv: 1511.04088 . Bibcode:2016ApJ...817...40F. doi: 10.3847/0004-637X/817/1/40 . eISSN   1538-4357.
  8. 1 2 Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004). "The angular sizes of dwarf stars and subgiants". Astronomy & Astrophysics. 426 (1): 297–307. arXiv: astro-ph/0404180 . Bibcode:2004A&A...426..297K. doi: 10.1051/0004-6361:20035930 . eISSN   1432-0746. ISSN   0004-6361.
  9. 1 2 Bai, Yu; Liu, JiFeng; Bai, ZhongRui; Wang, Song; Fan, DongWei (2 August 2019). "Machine-learning Regression of Stellar Effective Temperatures in the Second Gaia Data Release". The Astronomical Journal. 158 (2): 93. arXiv: 1906.09695 . Bibcode:2019AJ....158...93B. doi: 10.3847/1538-3881/ab3048 . eISSN   1538-3881.
  10. 1 2 Sprague, Dani; et al. (8 March 2022). "APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars". The Astronomical Journal. 163 (4): 152. arXiv: 2201.03661 . Bibcode:2022AJ....163..152S. doi: 10.3847/1538-3881/ac4de7 . eISSN   1538-3881. ISSN   0004-6256.
  11. "HD 45866". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved January 19, 2023.
  12. 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. arXiv: 0806.2878 . Bibcode:2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x . eISSN   1365-2966. ISSN   0035-8711. S2CID   14878976.
  13. Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017). "Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars". Monthly Notices of the Royal Astronomical Society. 472 (4): 3805–3820. arXiv: 1709.01160 . Bibcode:2017MNRAS.472.3805G. doi: 10.1093/mnras/stx2219 . eISSN   1365-2966. ISSN   0035-8711.