Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 00h 22m 23.14956s[2] |
Declination | +26° 59′ 45.73676″[2] |
Apparent magnitude (V) | 7.70 – 14.30 variable [3] |
Characteristics | |
Spectral type | M4e-M7.5e[3] |
B−V color index | 2.63[4] |
Variable type | Mira[3] |
Astrometry | |
Radial velocity (Rv) | −90±10[4] km/s |
Proper motion (μ) | RA: −7.108[2] mas/yr Dec.: −3.352[2] mas/yr |
Parallax (π) | 0.5913 ± 0.0815 mas[2] |
Distance | approx. 5,500 ly (approx. 1,700 pc) |
Details | |
Mass | 4.9[5] M☉ |
Luminosity | 8.928[6] L☉ |
Surface gravity (log g) | −0.51[5] cgs |
Temperature | 3,235[5] K |
Metallicity [Fe/H] | −0.39[5] dex |
Other designations | |
Database references | |
SIMBAD | data |
T Andromedae (T And) is a variable star of the Mira type in the constellation Andromeda. Like all the stars of this kind, T And is a cool asymptotic giant branch star of spectral type M4e-M7.5e. Its brightness varies periodically, completing a cycle in 281 days. The peak luminosity, however, is different every variability cycle, but can reach a peak magnitude mv=7.70.[3]
Thomas David Anderson discovered that T Andromedae is a variable star, in 1894.[7] The next year, Edward Charles Pickering examined archival photographic plates to derive a light curve for the star, and calculated a period of 281 days.[8]
Measurements of the angular size variations of T And made with the Palomar Testbed Interferometer show no clear correlation with the star's brightness variations.[9][10]
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