Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

HD 72108

From Wikipedia, the free encyclopedia
Star system in the constellation Vela
This article is about A Velorum. For a Velorum, seeHD 75063.
HD 72108
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationVela[1]
Right ascension08h 29m 04.752s[2]
Declination−47° 55′ 44.12″[2]
Apparent magnitude (V)+5.33[citation needed]
Characteristics
Spectral typeB2IV + B2IV[3]
Astrometry
Radial velocity (Rv)29.00±3.7[4] km/s
Proper motion (μ)RA: −6.90±0.43[2]mas/yr
Dec.: +7.12±0.34[2]mas/yr
Parallax (π)1.53±0.34 mas[2]
Distanceapprox. 2,100 ly
(approx. 700 pc)
Absolute magnitude (MV)−1.06[citation needed]
Orbit[5]
PrimaryHD 72018 Aa
CompanionHD 72018 Ab
Period (P)340±50 yr
Semi-major axis (a)0.427±0.030
Eccentricity (e)0.748±0.030
Inclination (i)78.9±2.0°
Longitude of the node (Ω)114.7±2.0°
Periastronepoch (T)1947.7±2.0
Argument of periastron (ω)
(secondary)
300.0±5.0°
Details
HD 72018 Aa
Mass6.08±3.43[5] M
HD 72018 Ab
Mass5.45±3.08[5] M
Other designations
HR 3358,CD−47°4004,HIP 41616,SAO 219985,WDS J08291-4756AB[6]
Database references
SIMBADdata

HD 72108 (A Vel, A Velorum) is astar system in theconstellationVela. It is approximately 1640light years fromEarth.

The primary component,HD 72108 A, is a blue-whiteB-typesubgiant with anapparent magnitude of +5.33. It is aspectroscopic binary, whose components are separated by 0.176arcseconds. At a distance of 4arcseconds away is the third component, the magnitude +7.7HD 72108 B. The fourth component,HD 72108 C has an apparent magnitude of +9.3, and is 19arcseconds from the primary.

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. ^abcdevan Leeuwen, F. (2007)."Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  3. ^Docobo, J. A.; Andrade, M. (2013)."Dynamical and physical properties of 22 binaries discovered by W. S. Finsen".Monthly Notices of the Royal Astronomical Society.428 (1):321–339.Bibcode:2013MNRAS.428..321D.doi:10.1093/mnras/sts045.
  4. ^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.
  5. ^abcDocobo, J. A.; Andrade, M. (2013)."Dynamical and physical properties of 22 binaries discovered by W. S. Finsen".Monthly Notices of the Royal Astronomical Society.428 (1):321–339.Bibcode:2013MNRAS.428..321D.doi:10.1093/mnras/sts045.
  6. ^"HR 3358 -- Double or multiple star".SIMBAD Astronomical Database.Centre de données astronomiques de Strasbourg. Retrieved2014-12-02.
Stars
Bayer
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
NGC
Other
Galaxies
NGC
Galaxy clusters


Stub icon

This binary or multiple star system-related article is astub. You can help Wikipedia byadding missing information.

Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_72108&oldid=1293973737"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp