BB Phoenicis

BB Phoenicis

A light curve for BB Phoenicis, plotted from TESS data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Phoenix
Right ascension 00h 30m 27.825s[2]
Declination −40° 56′ 22.51″[2]
Apparent magnitude (V) 6.18[3]
Characteristics
Spectral type F0/2III[4]
Variable type δ Scuti[3]
Astrometry
Radial velocity (Rv)−3.6[5] km/s
Proper motion (μ) RA: −3.40[2] mas/yr
Dec.: 16.95[2] mas/yr
Parallax (π)7.2816 ± 0.0397 mas[2]
Distance448 ± 2 ly
(137.3 ± 0.7 pc)
Absolute magnitude (MV)0.57±0.20[6]
Details[6]
Mass2.25±0.10 M☉
Radius4.7±0.3 R☉
Luminosity55.2+5.4
−9.3 L☉
Surface gravity (log g)3.44±0.03 cgs
Temperature7,200±100 K
Rotation2.17 days
Rotational velocity (v sin i)82±2 km/s
Other designations
BB Phe, CD−41°116, HD 2724, HIP 2388, HR 119, SAO 215120[7]
Database references
SIMBADdata

BB Phoenicis is a variable star in the constellation of Phoenix. It has an average visual apparent magnitude of 6.17,[3] being visible to the naked eye with excellent viewing conditions. From parallax measurements by the Gaia spacecraft, it is located at a distance of 448 light-years (137 parsecs) from Earth.[2] Its absolute magnitude is calculated at 0.6.[6]

BB Phoenicis is a Delta Scuti variable, and shows stellar pulsations that cause brightness variations with an amplitude of 0.04 magnitudes.[3] Its variability was discovered by accident in 1981, when the star was used as a comparison star for the eclipsing binary AG Phoenicis.[8] Photometric and spectroscopic data have allowed the detection of at least 13 modes of radial and non-radial pulsations, the strongest one having a period of 0.174 days and an amplitude of 11.1 milli-magnitudes. Observations in different epochs show evidence that the pulsations modes vary in amplitude, which is common among Delta Scuti variables. Pulsation models indicate that the stellar rotation axis is inclined by 50–70° in relation to the line of sight.[9]

This star is classified as an F-type giant with a spectral type of F0/2III.[4] It appears to be expanding after depleting all the nuclear hydrogen and leaving the main sequence.[6] BB Phoenicis has an estimated mass of 2.25 times the solar mass and a radius of 4.7 times the solar radius. It is radiating 55 times the Sun's luminosity from its photosphere at an effective temperature of 7,200 K.[6]

  1. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  2. ^ a b c d e f Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  3. ^ a b c d Cite error: The named reference GCVS 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 Gontcharov2006 was invoked but never defined (see the help page).
  6. ^ a b c d e Cite error: The named reference Bossi1998 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference Reipurth1981 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Mantegazza1999 was invoked but never defined (see the help page).