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HD 63332

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Coordinates: Sky map 07h 51m 05.7s, +54° 07′ 45.3″
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HD 63332
Observation data
Epoch J2000      Equinox J2000
Constellation Lynx[1]
Right ascension 07h 51m 05.71s[2]
Declination +54° 07′ 45.3″[2]
Apparent magnitude (V) 6.02±0.009[2]
Characteristics
Evolutionary stage F-type main-sequence star
Spectral type F6V[3]
Apparent magnitude (B) 6.493[2]
Apparent magnitude (G) 5.913[2]
Apparent magnitude (J) 5.116[2]
Apparent magnitude (H) 4.914[2]
Apparent magnitude (K) 4.861[2]
B−V color index 0.496±0.004[4]
Astrometry
Radial velocity (Rv)1.331±0.157[5] km/s
Proper motion (μ) RA: -39.538 mas/yr[5]
Dec.: 53.894 mas/yr[5]
Parallax (π)33.78 ± 0.39 mas[4]
Distance97 ± 1 ly
(29.6 ± 0.3 pc)[4]
Absolute magnitude (MV)3.66[6]
Details
Mass1.3[7] M☉
Radius1.375[4] R☉
Luminosity2.671[4] L☉
Surface gravity (log g)4.27[8] cgs
Temperature6,298[4] K
Metallicity [Fe/H]-0.12[6]–+0.09[8] dex
Rotational velocity (v sin i)9[9] km/s
Age2.1[8] or 3.1[6] Gyr
Other designations
BD+54 1177, Gaia DR2 984918228123275776, Gaia DR3 984918228123275776, HD 63332, HIP 38325, HR 3028, SAO 26535, PPM 31335, TIC 53336409, TYC 3783-1422-1, GSC 03783-01422, IRAS 07471+5415, 2MASS J07510571+5407452
Database references
SIMBADdata

HD 63332 is an F-type main-sequence star in the constellation Lynx. The star has an apparent brightness of 6.02,[2] meaning that it is faintly visible to the naked eye under dark skies.[10] Parallax measurements derive a distance of 29.6 parsecs (97 light-years) to HD 63332.[4] Considering the apparent magnitude and distance from Earth, the star's absolute magnitude is 3.66.[6] No debris disks or exoplanets were detected around it.[11][12]

Characteristics

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The star has a spectral classification of F6V,[3] meaning that is a F-type main-sequence star that is currently fusing hydrogen into helium in its core. It has 1.3 times the mass[7] and 1.375 times the radius of the Sun.[4] HD 63332 is 2.67 times more luminous than the Sun, emitting this energy from its photosphere at an effective temperature of 6,298 K, which is around 9% hotter than the Sun.[4] Its age is estimated at 2.1[8] or 3.1 billion years,[6] equivalent to 46% and 68% of the Solar System's age respectively,[a] and it rotates under its own axis at a velocity of 9 km/s.[9] The B-V color index of the star is 0.496, giving it the yellowish-white color of a late F-type star.[4][13]

HD 63332 is located in the northern hemisphere, 97 light-years from Earth,[4] within the constellation Lynx.[1] It has an apparent magnitude of 6.02, which makes it faintly visible to the naked eye, under dark skies.[10] The absolute magnitude, i.e. its brightness if it was seen at 10 pc (32.6 ly), is 3.66.[6] The star makes part of the thin disk population of the Milky Way,[11] being located at a maximum distance of 60 parsecs (200 ly) from the galactic plane.[6] Its orbit around the galaxy has a low eccentricity of 0.06.[6]

No debris disks have been detected around it as of 2016,[12] and no exoplanets were detected around it as of 2012.[11] It has a 27% possibility of hosting an exoplanet made up of volatiles, lithophiles, siderophiles and iron.[14] The habitable zone is located at a distance of 1.63 astronomical units from the star.[7]

Notes

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  1. ^ The Solar System's age is 4.568 billion years.

References

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  1. ^ a b Ford, Dominic. "HIP-38325 (Star)". In-The-Sky.org. Retrieved 2024-05-14.
  2. ^ a b c d e f g h i "HD 63332". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2024-05-14.
  3. ^ a b Piirola, V.; Berdyugin, A.; Frisch, P. C.; Kagitani, M.; Sakanoi, T.; Berdyugina, S.; Cole, A. A.; Harlingten, C.; Hill, K. (2020-03-01). "High-precision polarimetry of nearby stars (d < 50 pc). Mapping the interstellar dust and magnetic field inside the Local Bubble". Astronomy and Astrophysics. 635: A46. arXiv:2002.03682. Bibcode:2020A&A...635A..46P. doi:10.1051/0004-6361/201937324. ISSN 0004-6361. Data is available here in VizieR.
  4. ^ a b c d e f g h i j k Schofield, Mathew; Chaplin, William J.; Huber, Daniel; Campante, Tiago L.; Davies, Guy R.; Miglio, Andrea; Ball, Warrick H.; Appourchaux, Thierry; Basu, Sarbani; Bedding, Timothy R.; Christensen-Dalsgaard, Jørgen; Creevey, Orlagh; García, Rafael A.; Handberg, Rasmus; Kawaler, Steven D. (2019-03-01). "The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite". The Astrophysical Journal Supplement Series. 241 (1): 12. arXiv:1901.10148. Bibcode:2019ApJS..241...12S. doi:10.3847/1538-4365/ab04f5. ISSN 0067-0049. Data is available here in VizieR.
  5. ^ a b Brandt, Timothy D. (2021-06-01). "The Hipparcos-Gaia Catalog of Accelerations: Gaia EDR3 Edition". The Astrophysical Journal Supplement Series. 254 (2): 42. arXiv:2105.11662. Bibcode:2021ApJS..254...42B. doi:10.3847/1538-4365/abf93c. ISSN 0067-0049. Data is available here in VizieR.
  6. ^ a b c d e f g h Holmberg, J.; Nordström, B.; Andersen, J. (2009-07-01). "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics". Astronomy and Astrophysics. 501 (3): 941–947. arXiv:0811.3982. Bibcode:2009A&A...501..941H. doi:10.1051/0004-6361/200811191. ISSN 0004-6361. Data is available here in VizieR.
  7. ^ a b c Reiners, Ansgar; Zechmeister, Mathias (2020-03-01). "Radial Velocity Photon Limits for the Dwarf Stars of Spectral Classes F-M". The Astrophysical Journal Supplement Series. 247 (1): 11. arXiv:1912.04120. Bibcode:2020ApJS..247...11R. doi:10.3847/1538-4365/ab609f. ISSN 0067-0049. Data is available here in VizieR.
  8. ^ a b c d Ramírez, I.; Allende Prieto, C.; Lambert, D. L. (2013-02-01). "Oxygen Abundances in Nearby FGK Stars and the Galactic Chemical Evolution of the Local Disk and Halo". The Astrophysical Journal. 764 (1): 78. arXiv:1301.1582. Bibcode:2013ApJ...764...78R. doi:10.1088/0004-637X/764/1/78. hdl:2152/34757. ISSN 0004-637X. Data is available here in VizieR.
  9. ^ a b Nordström, B.; Mayor, M.; Andersen, J.; Holmberg, J.; Pont, F.; Jørgensen, B. R.; Olsen, E. H.; Udry, S.; Mowlavi, N. (2004-05-01). "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ∼14 000 F and G dwarfs". Astronomy and Astrophysics. 418: 989–1019. arXiv:astro-ph/0405198. Bibcode:2004A&A...418..989N. doi:10.1051/0004-6361:20035959. ISSN 0004-6361. Data is available here at VizieR.
  10. ^ a b "University Lowbrow Astronomers Naked Eye Observer's Guide". websites.umich.edu. Retrieved 2024-05-14.
  11. ^ a b c Ramírez, I.; Fish, J. R.; Lambert, D. L.; Allende Prieto, C. (2012-09-01). "Lithium Abundances in nearby FGK Dwarf and Subgiant Stars: Internal Destruction, Galactic Chemical Evolution, and Exoplanets". The Astrophysical Journal. 756 (1): 46. arXiv:1207.0499. Bibcode:2012ApJ...756...46R. doi:10.1088/0004-637X/756/1/46. hdl:2152/34872. ISSN 0004-637X. Data is available here in VizieR.
  12. ^ a b Gáspár, András; Rieke, George H.; Ballering, Nicholas (2016-08-01). "The Correlation between Metallicity and Debris Disk Mass". The Astrophysical Journal. 826 (2): 171. arXiv:1604.07403. Bibcode:2016ApJ...826..171G. doi:10.3847/0004-637X/826/2/171. ISSN 0004-637X. Data is available here in VizieR.
  13. ^ "The Colour of Stars". Australia Telescope National Facility. 6 March 2024. Retrieved May 14, 2024.
  14. ^ Hinkel, Natalie R.; Unterborn, Cayman; Kane, Stephen R.; Somers, Garrett; Galvez, Richard (2019-07-01). "A Recommendation Algorithm to Predict Giant Exoplanet Host Stars Using Stellar Elemental Abundances". The Astrophysical Journal. 880 (1): 49. arXiv:1805.12144. Bibcode:2019ApJ...880...49H. doi:10.3847/1538-4357/ab27c0. ISSN 0004-637X. Data about this star is available here in VizieR.
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