Alpha Trianguli

Alpha Trianguli (α Trianguli, abbreviated Alpha Tri, α Tri) is a spectroscopic binary star in the constellation of Triangulum. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 63.3 light-years (19.4 parsecs) distant from the Sun. The brighter or primary component is named Mothallah /məˈθælə/.

α Trianguli
Location of α Trianguli (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Triangulum
Right ascension 01h 53m 04.90710s
Declination +29° 34 43.7801
Apparent magnitude (V) +3.42
Characteristics
Spectral type F5III to F6IV + M
U−B color index +0.06
B−V color index +0.48
Variable type Ellipsoidal
Astrometry
Radial velocity (Rv)−12.6 km/s
Proper motion (μ) RA: 10.82 mas/yr
Dec.: −234.24 mas/yr
Parallax (π)51.50 ± 0.23 mas
Distance63.3 ± 0.3 ly
(19.42 ± 0.09 pc)
Absolute magnitude (MV)1.98
Orbit
Period (P)1.767 days
Eccentricity (e)0.065
Semi-amplitude (K1)
(primary)
10.64 km/s
Details
α Tri A
Mass1.70 M
Radius3.22 R
Surface gravity (log g)3.91 cgs
Temperature6,288 K
Metallicity [Fe/H]−0.09 to 0.00 dex
Rotational velocity (v sin i)81.6 km/s
Age1.6 Gyr
α Tri B
Mass0.11 M
Other designations
Mothallah, Ras al Muthallah, Caput Trianguli, α Trianguli, 2 Trianguli, HR 544, HD 11443, BD+28°312, FK5 64, HIP 8796, SAO 74996.
Database references
SIMBADdata
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