Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

HD 96819

From Wikipedia, the free encyclopedia
Star in the constellation Hydra
HD 96819
Observation data
EpochJ2000      EquinoxJ2000
ConstellationHydra[1]
Right ascension11h 08m 43.99011s[2]
Declination−28° 04′ 50.3539″[2]
Apparent magnitude (V)5.43[3]
Characteristics
Evolutionary stagemain sequence[4][2]
Spectral typeA1V[4]
U−Bcolor index+0.06[5]
B−Vcolor 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]
Distance178.1 ± 0.7 ly
(54.6 ± 0.2 pc)
Absolute magnitude (MV)1.61[3]
Details
HD 96819 A
Mass1.93[7] M
Radius1.80[7] R
Luminosity20.66[4] L
Surface gravity (log g)4.22±0.08[3] cgs
Temperature8,954[4] K
Rotational velocity (v sin i)249[4] km/s
Age9±1[8] Myr
HD 96819 B
Mass0.51[7] M
Radius0.47[7] R
Temperature3,792[7] K
Other designations
NSV 5101,CD−27°7886,HD 96819,HIP 54477,HR 4334,SAO 179577[9]
Database references
SIMBADdata

HD 96819 is astar in theequatorialconstellation ofHydra. It was formerly known by its designation10 Crateris, but that name fell into disuse after constellations were redrawn and the star was no longer inCrater. It is visible to the naked eye as a dim, white-hued star with anapparent 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 theTW Hydrae association.[8]

This is a rapidly rotatingA-type main-sequence star that is about double the mass of theSun. It emits 20.66 times as much energy as theSun, at aneffective temperature of 8,954 K. HD 96819 is currently 31.5% through its life as amain-sequence star: after that it will swell up as ared giant.[4] It is a young star of around nine million years age,[8] and is a suspectedvariable 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]
  1. ^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 atVizieR.
  2. ^abcdefgVallenari, 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 atVizieR.
  3. ^abcdAllende 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.
  4. ^abcdefZorec, 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.
  5. ^abJohnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars".Communications of the Lunar and Planetary Laboratory.4: 99.Bibcode:1966CoLPL...4...99J.
  6. ^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.
  7. ^abcdefWaisberg, 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 highGaia–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.
  8. ^abcGagné, 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.
  9. ^"HD 96819".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved22 August 2017.
  10. ^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.
  11. ^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.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
Messier
NGC
Other
Galaxy clusters
Astronomical events
Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_96819&oldid=1328190068"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp