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HD 96819
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hydra[1] |
| Right ascension | 11h 08m 43.99011s[2] |
| Declination | −28° 04′ 50.3539″[2] |
| Apparent magnitude (V) | 5.43[3] |
| Characteristics | |
| Evolutionary stage | main sequence[4][2] |
| Spectral type | A1V[4] |
| U−B color index | +0.06[5] |
| B−V color index | +0.07[5] |
| Astrometry | |
| Radial velocity (Rv) | 16.0±7.4[6] km/s |
| Proper motion (μ) | RA: −69.211[2] mas/yr Dec.: −22.181[2] mas/yr |
| Parallax (π) | 18.3139±0.0752 mas[2] |
| Distance | 178.1 ± 0.7 ly (54.6 ± 0.2 pc) |
| Absolute magnitude (MV) | 1.61[3] |
| Details | |
| HD 96819 A | |
| Mass | 1.93[7] M☉ |
| Radius | 1.80[7] R☉ |
| Luminosity | 20.66[4] L☉ |
| Surface gravity (log g) | 4.22±0.08[3] cgs |
| Temperature | 8,954[4] K |
| Rotational velocity (v sin i) | 249[4] km/s |
| Age | 9±1[8] Myr |
| HD 96819 B | |
| Mass | 0.51[7] M☉ |
| Radius | 0.47[7] R☉ |
| Temperature | 3,792[7] K |
| Other designations | |
| NSV 5101, CD−27°7886, HD 96819, HIP 54477, HR 4334, SAO 179577[9] | |
| Database references | |
| SIMBAD | data |
HD 96819 is a star in the equatorial constellation of Hydra. It was formerly known by its designation 10 Crateris, but that name fell into disuse after constellations were redrawn and the star was no longer in Crater. It is visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 5.43.[3] Parallax measurements put it at a distance of 178 light years away from the Sun.[2] This is most likely (98.7% chance) a member of the TW Hydrae association.[8]
This is a rapidly rotating A-type main-sequence star that is about double the mass of the Sun. It emits 20.66 times as much energy as the Sun, at an effective temperature of 8,954 K. HD 96819 is currently 31.5% through its life as a main-sequence star: after that it will swell up as a red giant.[4] It is a young star of around nine million years age,[8] and is a suspected variable star.[10] Previously thought to be a single star,[11] in 2022 a companion star was discovered, making HD 96819 a binary star. The companion star has about half the mass of the Sun.[7]
References
[edit]- ^ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
- ^ a b c d e f g 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.
- ^ a b c d Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. arXiv:astro-ph/9911002. Bibcode:1999A&A...352..555A.
- ^ a b c d e f Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy & Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. S2CID 55586789.
- ^ a b Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99. Bibcode:1966CoLPL...4...99J.
- ^ Kharchenko, N. V.; et al. (2007). "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ~55000 stars and mean radial velocities of 516 Galactic open clusters and associations". Astronomische Nachrichten. 328 (9): 889. arXiv:0705.0878. Bibcode:2007AN....328..889K. doi:10.1002/asna.200710776. S2CID 119323941.
- ^ a b c d e f Waisberg, Idel; Klein, Ygal; Katz, Boaz (2023). "Binarity and beyond in a stars – I. Survey description and first results of VLTI/GRAVITY observations of VAST targets with high Gaia–Hipparcos accelerations". Monthly Notices of the Royal Astronomical Society. 521 (4): 5232–5254. arXiv:2206.05251. Bibcode:2023MNRAS.521.5232W. doi:10.1093/mnras/stad872.
- ^ a b c Gagné, Jonathan; et al. (February 2017), "BANYAN. IX. The Initial Mass Function and Planetary-mass Object Space Density of the TW HYA Association", The Astrophysical Journal Supplement Series, 228 (2): 51, arXiv:1612.02881, Bibcode:2017ApJS..228...18G, doi:10.3847/1538-4365/228/2/18, S2CID 118920136, 18.
- ^ "HD 96819". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 22 August 2017.
- ^ Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80−88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.
- ^ Eggleton, P. P.; Tokovinin, A. A. (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, S2CID 14878976.
