HD 63399

Last updated
HD 63399
Observation data
Epoch J2000       Equinox J2000
Constellation Puppis
Right ascension 07h 47m 14.59403s [1]
Declination −36° 04′ 24.9619″ [1]
Apparent magnitude  (V)6.45±0.01 [2]
Characteristics
Evolutionary stage red giant branch [3]
Spectral type K1 III [4]
U−B color index +1.13 [5]
B−V color index +1.12 [5]
Astrometry
Radial velocity (Rv)28.5±0.2 [6] km/s
Proper motion (μ)RA: −35.000 mas/yr [1]
Dec.: +26.931 mas/yr [1]
Parallax (π)7.3283±0.0162  mas [1]
Distance 445.1 ± 1.0  ly
(136.5 ± 0.3  pc)
Absolute magnitude  (MV)+0.78 [7]
Details
Mass 1.29 [8] or 1.7+1.3
−0.8 [9]   M☉
Radius 10.79 [10]   R☉
Luminosity 54.8±0.3 [6]   L☉
Surface gravity (log g)2.47 [8]   cgs
Temperature 4,761±77 [11]   K
Metallicity [Fe/H]−0.06 [3]   dex
Other designations
CD−35°3874, CPD−35°1579, GC 10510, HD 63399, HIP 37996, SAO 198437 [12]
Database references
SIMBAD data

HD 63399 is an orange hued star located in the southern constellation Puppis, the poop deck. It has an apparent magnitude of 6.45, [2] placing it near the limit for naked eye visibility. Based on parallax measurements from Gaia DR3, [1] the object is estimated to be 445 light years distant. It appears to be receding with a spectroscopic radial velocity of 28.5  km/s . [6] At its current distance, HD 63399 is diminished by 0.29 magnitudes due to interstellar dust. [13]

HD 63399 is a red giant star that is currently on the red giant branch, [3] fusing hydrogen in a shell around its core. It has a stellar classification of K1 III. [4] At present it has a mass ranging from 1.3 to 1.7 times the mass of the Sun, [8] [9] depending on the study. HD 63399 has expanded to 10.8 times its girth [10] and now radiates 54.8 times the luminosity of the Sun [6] from its swollen photosphere at an effective temperature of 4,761  K . [11] The star has an iron abundance 13% below solar levels, making it slightly metal deficient. [3]

References

  1. 1 2 3 4 5 6 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.
  2. 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.
  3. 1 2 3 4 Cardiel, Nicolás; Zamorano, Jaime; Carrasco, Josep Manel; Masana, Eduard; Bará, Salvador; González, Rafael; Izquierdo, Jaime; Pascual, Sergio; Sánchez de Miguel, Alejandro (23 July 2021). "RGB photometric calibration of 15 million Gaia stars". Monthly Notices of the Royal Astronomical Society. 507 (1): 318–329. arXiv: 2107.08734 . Bibcode:2021MNRAS.507..318C. doi: 10.1093/mnras/stab2124 . eISSN   1365-2966. ISSN   0035-8711.
  4. 1 2 Houk, N. (1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations −40° to −26°. Bibcode:1982mcts.book.....H.
  5. 1 2 Pickles, A.; Depagne, É. (December 2010). "All-Sky Spectrally MatchedUBVRI - ZY and u′g′r′i′z′ Magnitudes for Stars in the Tycho2 Catalog". Publications of the Astronomical Society of the Pacific. 122 (898): 1437–1464. arXiv: 1011.2020 . Bibcode:2010PASP..122.1437P. doi: 10.1086/657947 . eISSN   1538-3873. ISSN   0004-6280.
  6. 1 2 3 4 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.
  7. ↑ 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. eISSN   1562-6873. ISSN   1063-7737. S2CID   119257644.
  8. 1 2 3 Anders, F.; et al. (February 2022). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia EDR3 stars brighter than G = 18.5". Astronomy & Astrophysics. 658: A91. arXiv: 2111.01860 . Bibcode:2022A&A...658A..91A. doi: 10.1051/0004-6361/202142369 . eISSN   1432-0746. ISSN   0004-6361.
  9. 1 2 Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy & Astrophysics. 633: A34. arXiv: 1910.12732 . Bibcode:2020A&A...633A..34C. doi: 10.1051/0004-6361/201936360 . eISSN   1432-0746. ISSN   0004-6361.
  10. 1 2 Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics. 657: A7. arXiv: 2109.10912 . Bibcode:2022A&A...657A...7K. doi: 10.1051/0004-6361/202142146 . eISSN   1432-0746. ISSN   0004-6361.
  11. 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.
  12. ↑ "HD 63399". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved June 1, 2014.
  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.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.