- Alpha Trianguli
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α Trianguli Observation data
Epoch J2000.0 Equinox J2000.0Constellation Triangulum Right ascension 01h 53m 04.9s Declination +29° 34' 44" Apparent magnitude (V) +3.41 Distance 64.1 ± 1.0 ly
(19.7 ± 0.3 pc)Spectral type F6IV Other designations Alpha Trianguli (α Tri, α Trianguli) is a binary star in the constellation Triangulum. It has the traditional names Mothallah or Ras al Muthallah (alternate spellings Mathallah, Metallah, Ras al Mothallah, Elmuthalleth), and Caput Trianguli, from the Arabic رأس المثلث ra’s al-muθallaθ "the head of the triangle" and its Latin translation.
Alpha Trianguli is a yellow-white F-type subgiant with a mean apparent magnitude of +3.41. Its mass is about 1.5 times that of the Sun and its diameter is about 3 times as large as the Sun's.
Mothallah is a spectroscopic binary whose components have an orbital period of only 1.74 days. The companion star is a mere 6 million km (3.7 million miles) from the main star. The whole system is approximately 64.1 light years from Earth.
α Tri is listed as UR.BAR.RA "The Wolf", bearing the epithet "the seeder of the plough" in the MUL.APIN, listed after "The Plough", the name for a constellation formed of Triangulum plus Gamma Andromedae[1].
References
- ^ Rogers, J. H. (February 1998). "Origins of the ancient constellations: I. The Mesopotamian traditions". Journal of the British Astronomical Association, no.1 108: 9–28. Bibcode 1998JBAA..108....9R.
External links
Star systems within 60–70 light-years from Earth with brightest member's absolute magnitude of +8.5 or brighter.Rho Puppis «Tureis» (62.7 ± 0.8 ly; 1 star)Theta Centauri «Menkent» (60.9 ± 0.9 ly; 1 star) • Aldebaran (65.1 ± 1.3 ly; 2 stars) • Epsilon Scorpii «Wei» (65.4 ± 1.1 ly; 1 star) • Alpha Arietis «Hamal» (65.9 ± 1.3 ly; 1 star, 1 planet: planet b)Beta Arietis «Sheratan» (59.6 ± 0.8 ly; 2 stars)‡ • Beta Pictoris (62.9 ± 0.6 ly; 1 star, 1 planet: planet b)Psi Velorum (59.7 ± 1.0 ly; 2 stars)‡ • Mu Virginis (60.9 ± 1.1 ly; 1 star)‡ • Alpha Chamaeleontis (63.5 ± 0.6 ly; 1 star) • Alpha Trianguli «Metallah» (64.1 ± 1.0 ly; 2 stars) • Eta Crucis (64.2 ± 0.6 ly; 2 stars) • Tau Cygni (66.4 ± 0.8 ly; 4 stars) • Theta Draconis (68.3 ± 0.8 ly; 2 stars) • Iota Virginis «Syrma» (69.8 ± 1.3 ly; 1 star)‡Chi Cancri (59.2 ± 1.0 ly; 1 star)‡ • Eta Corvi «Avis Satyra» (59.4 ± 0.7 ly; 1 star)‡ • Delta Equulei «Pherasauval» (60.0 ± 1.0 ly; 2 stars)‡ • Theta Cygni (60.7 ± 0.5 ly; 2 stars) • HR 1249 (62.7 ± 0.9 ly; 1 star) • 1 Centauri (62.8 ± 0.9 ly; 2 stars) • Omicron Aquilae (63.3 ± 0.9 ly; 3 stars) • c (45) Boötis (64.3 ± 1.0 ly; 2 stars) • Alpha Caeli (65.7 ± 0.7 ly; 2 stars) • Kappa Tucanae (66.04 ± 1.2 ly; 4 stars) • Gamma Doradus (66.2 ± 0.7 ly; 1 star) • Sigma² Ursae Majoris (66.7 ± 0.9 ly; 3 stars) • HR 1686 (68.4 ± 0.8 ly; 2 stars, 1 planet: planet b) • B Carinae (69.8 + 5.4/- 4.7 ly; 1 star)‡94 Aquarii (67.6 + 8.3/- 6.6 ly; 2 stars)‡ • Gliese 848.4 (69.4 ± 1.2 ly; 1 star, 1 planet: planet b)‡HD 217107 (64.3 ± 1.0 ly; 1 star, 2 planets: planet b • planet c) • 53 Aquarii (65.5 ± 3.5 ly; 2 stars) • GJ 3255 (67.4 ± 1.5 ly; 1 star, 1 planet: planet b) • 51 Arietis (69.0 ± 1.3 ly; 1 star)‡ • c (16) Cygni (69.8 ± 0.8 ly; 2 stars, 1 planet: planet Bb)‡Epsilon Reticuli (59.5 ± 0.5 ly; 1 star, 1 planet: planet b)‡ • Eta Serpentis «Tang» (61.8 ± 0.9 ly; 1 star) • Nu² Canis Majoris (64.7 ± 0.9 ly; 1 star, 1 planet: planet b)GJ 4130 (62.8 ± 1.1 ly; 2 stars, 1 planet: planet b) • Gliese 710 (63.0 ± 1.8 ly; 1 star) • HD 192263 (64.9 ± 1.5 ly; 1 star, 1 planet: planet b) • GJ 3769 (66.6 ± 1.5 ly; 1 star, 1 planet: planet b) • GJ 3651 (69.5 ± 1.5 ly; 1 star, 1 planet: planet b)‡ • GJ 4291 (70.2 ± 2.0 ly; 1 star, 1 planet: planet b)‡In left column are stellar classes of primary members of star systems. ‡Distance error margin extends out of declared distance interval. Italic are systems possibly located within declared distance interval, but probably not.Common proper name MetallahBayer Flamsteed Categories:- Bayer objects
- Triangulum constellation
- Spectroscopic binaries
- F-type subgiants
- Stars with proper names
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