Tau2 Gruis

For other stars with this Bayer designation, see τ Gruis.
Tau2 Gruis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Grus
Right ascension 22h 55m 15.99534s[1]
Declination −48° 29′ 30.30277″[1]
Apparent magnitude (V) 6.71[2] (7.30+ 7.50)[3]
Characteristics
Spectral type F6/8 V:[4]
B−V color index +0.46[5]
Astrometry
Radial velocity (Rv)0.7±0.3[6] km/s
Proper motion (μ) RA: −225.658 mas/yr[1]
Dec.: +55.712 mas/yr[1]
Parallax (π)22.3461 ± 0.0241 mas[1]
Distance146.0 ± 0.2 ly
(44.75 ± 0.05 pc)
Absolute magnitude (MV)+3.43[7] (combined)
Details[8]
A
Mass1.21 M☉
B
Mass1.16 M☉
Other designations
τ2 Gru, 71 G. Gruis[9], CD−49° 13997, CPD−49°11676, GC 31952, HD 216656, HIP 113190, SAO 231353, WDS J22553-4828CD[10]
Database references
SIMBADdata

Tau2 Gruis, Latinized from τ2 Gruis is a binary star located in the constellation Grus. It has a combined apparent magnitude of 6.71,[2] making it a challenge to view with the naked eye, even under ideal conditions. The system is located relatively close at a distance of 146 light-years based on Gaia DR3 parallax measurements, but it is slowly receding with a heliocentric radial velocity of 0.7 km/s.[6] At its current distance, Tau2 Gruis' combined brightness is diminished by an interstellar extinction of 0.12 magnitudes[11] and it has a combined absolute magnitude of +3.43.[7]

The pair was first discovered by astronomer W.H. van den Bos in 1944.[12] The primary has an apparent magnitude of 7.30 while the secondary has an apparent magnitude of 7.50.[3] Their current separation is 0.114",[8] making it difficult to resolve their individual properties; the companion is located at a position angle of 267° as of 1964.[3] The period of Tau2 Gruis is not well known,[13] but it is estimated to be 7.423 years.[8] Subsequent observations suggest that the pair may be spurious.[13] This system is often confused with HD 216655, a slightly brighter binary system.[14] HD 216655 is located 93.9" away from Tau2 Gruis and they appear to share a common proper motion.[3]

The system has a blended stellar classification of F6/8 V:,[4] indicating that it is a F-type star with the characteristics of a F6 and F8 main sequence star. However, there is uncertainty about the luminosity class. The primary has 1.21 times the mass of the Sun while the companion has 1.16 times the mass of the Sun.[8]

  1. ^ a b c d Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  2. ^ a b Cite error: The named reference Tycho2000 was invoked but never defined (see the help page).
  3. ^ a b c d Cite error: The named reference Mason2001 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference Houk1978 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Cousins1962 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference Nordstrom2004 was invoked but never defined (see the help page).
  7. ^ a b Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
  8. ^ a b c d Cite error: The named reference Tokovinin20141 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Gould1879 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference Gontcharov2017 was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference van den Bos1947 was invoked but never defined (see the help page).
  13. ^ a b Cite error: The named reference Tokovinin2018 was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference wagman was invoked but never defined (see the help page).