Astronomy:HD 63399
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Short description: Star in the constellation Puppis
| Observation data Epoch J2000.0 Equinox (celestial coordinates) | |
|---|---|
| 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[1] mas/yr Dec.: +26.931[1] mas/yr |
| Parallax (π) | 7.3283 ± 0.0162[1] mas |
| 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 | |
| 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 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
- ↑ 1.0 1.1 1.2 1.3 1.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 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.
- ↑ 3.0 3.1 3.2 3.3 Cardiel, Nicolás; Zamorano, Jaime; Carrasco, Josep Manel; Masana, Eduard; Bará, Salvador; González, Rafael; Izquierdo, Jaime; Pascual, Sergio et al. (23 July 2021). "RGB photometric calibration of 15 million Gaia stars". Monthly Notices of the Royal Astronomical Society 507 (1): 318–329. doi:10.1093/mnras/stab2124. ISSN 0035-8711. Bibcode: 2021MNRAS.507..318C.
- ↑ 4.0 4.1 Houk, N. (1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations −40° to −26°. Bibcode: 1982mcts.book.....H.
- ↑ 5.0 5.1 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. doi:10.1086/657947. ISSN 0004-6280. Bibcode: 2010PASP..122.1437P.
- ↑ 6.0 6.1 6.2 6.3 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode: 2012AstL...38..331A.
- ↑ 8.0 8.1 8.2 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. doi:10.1051/0004-6361/202142369. ISSN 0004-6361. Bibcode: 2022A&A...658A..91A.
- ↑ 9.0 9.1 Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R. et al. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy & Astrophysics 633: A34. doi:10.1051/0004-6361/201936360. ISSN 0004-6361. Bibcode: 2020A&A...633A..34C.
- ↑ 10.0 10.1 Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics 657: A7. doi:10.1051/0004-6361/202142146. ISSN 0004-6361. Bibcode: 2022A&A...657A...7K.
- ↑ 11.0 11.1 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. doi:10.3847/1538-3881/ab3048. Bibcode: 2019AJ....158...93B.
- ↑ "HD 63399". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+63399.
- ↑ 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. doi:10.1093/mnras/stx2219. ISSN 0035-8711. Bibcode: 2017MNRAS.472.3805G.
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