V1054 Ophiuchi

V1054 Ophiuchi

An ultraviolet band light curve for a flare on V1054 Ophiuchi, plotted from data published by Dal and Evren (2010)[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ophiuchus
Right ascension 16h 55m 25.2222456607s[2]
Declination −08° 19′ 21.296969682″[2]
Apparent magnitude (V) 9.74/10.34/10.84/11.74/16.80[3]
Characteristics
Spectral type M3 V[4] / M4 Ve[note 1] / M3.5 V[4] / M7.0 V[3]
Astrometry
Proper motion (μ) RA: −817.580±0.052[2] mas/yr
Dec.: −898.595±0.040[2] mas/yr
Parallax (π)153.8754 ± 0.0474 mas[2]
Distance21.196 ± 0.007 ly
(6.499 ± 0.002 pc)
Absolute magnitude (MV)10.69±0.02 / 11.29±0.05 / 11.79±0.05 / 12.69[3][note 2]
VB 8
Proper motion (μ) RA: −813.038±0.063[5] mas/yr
Dec.: −870.609±0.044[5] mas/yr
Parallax (π)153.9659 ± 0.0570 mas[5]
Distance21.184 ± 0.008 ly
(6.495 ± 0.002 pc)
Absolute magnitude (MV)17.75[3]
Orbit[4]
PrimaryV1054 Oph A
CompanionV1054 Oph B
Period (P)1.717267±0.000039[3] yr
Semi-major axis (a)0.2273±0.0004"
(1.46683 AU[note 3])
Eccentricity (e)0.042±0.001
Inclination (i)160.3±0.1°
Longitude of the node (Ω)−10.2±0.2°
Periastron epoch (T)MJD 53943±3
Argument of periastron (ω)
(secondary)
306.0±1.5°
Orbit[4]
PrimaryV1054 Oph Ba
CompanionV1054 Oph Bb
Period (P)2.965509±0.000006 d
Semi-major axis (a)0.00687[note 4]"
(0.04432 AU[note 5])
Eccentricity (e)0.0209±0.0008
Inclination (i)164.18±0.08°
Periastron epoch (T)MJD 50919.48±0.03
Argument of periastron (ω)
(secondary)
150.0±3.0°
Details
V1054 Oph AB
Mass0.4155±0.0057 / 0.3466±0.0047 / 0.3143±0.0040[4] M
Gliese 643
Mass0.19[3] M
Details
VB 8
Mass0.0914+0.0026
−0.0025
[6] M
Radius0.1214+0.0060
−0.0057
[6] R
Luminosity0.000645+0.000004
−0.000005
[6] L
Temperature2,640+65
−64
[6] K
Other designations
V1054 Oph, BD−08°4352, GJ 644, HD 152751, HIP 82817, SAO 141439, Wolf 630[7]
Database references
SIMBADThe system
ABab
A
Bab
GJ 643
C (vB 8)
vB 8B (artifact)

V1054 Ophiuchi, together with the star Gliese 643, is a nearby quintuple star system. In the constellation Ophiuchus at a distance of 21.19 light-years. It consists of five stars, all of which are red dwarfs. The alternative designation of Wolf 630 forms the namesake of a moving group of stars that share a similar motion through space.[8]

  1. ^ Cite error: The named reference Dal2010 was invoked but never defined (see the help page).
  2. ^ a b c d e Cite error: The named reference GaiaEDR3 was invoked but never defined (see the help page).
  3. ^ a b c d e f Cite error: The named reference Mazeh2001 was invoked but never defined (see the help page).
  4. ^ a b c d e Cite error: The named reference Ségransan2000 was invoked but never defined (see the help page).
  5. ^ a b c Cite error: The named reference GaiaEDR3-VB8 was invoked but never defined (see the help page).
  6. ^ a b c d Cite error: The named reference Pineda2021 was invoked but never defined (see the help page).
  7. ^ "HD 152751". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-03-25.
  8. ^ Bubar, Eric J.; King, Jeremy R. (August 2010). "Spectroscopic Abundances and Membership in the Wolf 630 Moving Group". The Astronomical Journal. 140 (2): 293–318. arXiv:1005.1205. Bibcode:2010AJ....140..293B. doi:10.1088/0004-6256/140/2/293. S2CID 118455341.


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