HD 4778

Star in the constellation Andromeda From Wikipedia, the free encyclopedia

HD 4778, also known as HR 234 and GO Andromedae, is a variable star in the constellation Andromeda. Its magnitude varies by 0.04 magnitudes from the median of 6.12 with a period of approximately 2.55 days.[11] The star is located 350 light years away, as determined from its annual parallax shift of 9.62 mas.[3]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 4778

A light curve for GO Andromedae, plotted from TESS data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda[2]
Right ascension 00h 50m 18.26532s[3]
Declination +45° 00 08.1355[3]
Apparent magnitude (V) 6.13[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A3VpSiSrCrEuKsn[4]
B−V color index 0.043±0.004[2]
Variable type α2 CVn[5]
Astrometry
Radial velocity (Rv)1.60[6] km/s
Proper motion (μ) RA: +65.570[3] mas/yr
Dec.: +4.662[3] mas/yr
Parallax (π)9.6184±0.0488 mas[3]
Distance339 ± 2 ly
(104.0 ± 0.5 pc)
Absolute magnitude (MV)1.18[7]
Details
Mass2.24±0.09[7] M
Radius2.36±0.12[8] R
Luminosity34.9±4.3[8] L
Surface gravity (log g)4.12±0.09[7] cgs
Temperature9,135±400[8] K
Rotation2.5616[7] days
Rotational velocity (v sin i)33[4] km/s
Age77[9] Myr
Other designations
GO Andromedae, BD+44° 176, FK5 2055, HD 4778, HIP 3919, HR 234, SAO 36702, PPM 43369[10]
Database references
SIMBADdata
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This is an Ap star with a stellar classification of A3VpSiSrCrEuKsn,[4] showing chemical peculiarities in its spectrum from strontium, chromium, and europium.[12] It is an Alpha2 Canum Venaticorum variable[5] with a magnetic field that varies across the range +1,400 to −1,100 G.[13] This rotation-modulated variability allows direct determination of the rotation rate of 2.5616 days.[7]

HD 4778 has 2.24[7] times the mass of the Sun and 2.36[8] times the Sun's radius. The star is radiating 35[8] times the Sun's luminosity from its photosphere at an effective temperature of 9,375 K.[7] It is about 77[9] million years old.

References

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